[{"quality_controlled":"1","language":[{"iso":"eng"}],"publication_status":"published","extern":"1","status":"public","date_published":"2021-08-01T00:00:00Z","year":"2021","citation":{"chicago":"Reischauer, Susanne, and Bartholomäus Pieber. “Recyclable, Bifunctional Metallaphotocatalysts for C−S Cross‐coupling Reactions.” <i>ChemPhotoChem</i>. Wiley, 2021. <a href=\"https://doi.org/10.1002/cptc.202100062\">https://doi.org/10.1002/cptc.202100062</a>.","short":"S. Reischauer, B. Pieber, ChemPhotoChem 5 (2021) 716–720.","mla":"Reischauer, Susanne, and Bartholomäus Pieber. “Recyclable, Bifunctional Metallaphotocatalysts for C−S Cross‐coupling Reactions.” <i>ChemPhotoChem</i>, vol. 5, no. 8, Wiley, 2021, pp. 716–20, doi:<a href=\"https://doi.org/10.1002/cptc.202100062\">10.1002/cptc.202100062</a>.","apa":"Reischauer, S., &#38; Pieber, B. (2021). Recyclable, bifunctional metallaphotocatalysts for C−S cross‐coupling reactions. <i>ChemPhotoChem</i>. Wiley. <a href=\"https://doi.org/10.1002/cptc.202100062\">https://doi.org/10.1002/cptc.202100062</a>","ama":"Reischauer S, Pieber B. Recyclable, bifunctional metallaphotocatalysts for C−S cross‐coupling reactions. <i>ChemPhotoChem</i>. 2021;5(8):716-720. doi:<a href=\"https://doi.org/10.1002/cptc.202100062\">10.1002/cptc.202100062</a>","ieee":"S. Reischauer and B. Pieber, “Recyclable, bifunctional metallaphotocatalysts for C−S cross‐coupling reactions,” <i>ChemPhotoChem</i>, vol. 5, no. 8. Wiley, pp. 716–720, 2021.","ista":"Reischauer S, Pieber B. 2021. Recyclable, bifunctional metallaphotocatalysts for C−S cross‐coupling reactions. ChemPhotoChem. 5(8), 716–720."},"issue":"8","intvolume":"         5","author":[{"last_name":"Reischauer","first_name":"Susanne","full_name":"Reischauer, Susanne"},{"first_name":"Bartholomäus","id":"93e5e5b2-0da6-11ed-8a41-af589a024726","orcid":"0000-0001-8689-388X","full_name":"Pieber, Bartholomäus","last_name":"Pieber"}],"oa":1,"abstract":[{"lang":"eng","text":"Metallaphotocatalytic cross-coupling reactions are typically carried out by combining homogeneous or heterogeneous photocatalysts with a soluble nickel complex. Previous attempts to realize recyclable catalytic systems use immobilized iridium complexes to harvest light. We present bifunctional materials based on semiconductors for metallaphotocatalytic C−S cross-coupling reactions that can be reused without losing their catalytic activity. Key to the success is the permanent immobilization of a nickel complex on the surface of a heterogeneous semiconductor through phosphonic acid anchors. The optimized catalyst harvests a broad range of the visible light spectrum and requires a nickel loading of only ∼0.1 mol %."}],"publisher":"Wiley","date_created":"2022-08-25T08:31:11Z","publication":"ChemPhotoChem","title":"Recyclable, bifunctional metallaphotocatalysts for C−S cross‐coupling reactions","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1002/cptc.202100062"}],"date_updated":"2024-10-14T11:43:32Z","publication_identifier":{"eissn":["2367-0932"]},"doi":"10.1002/cptc.202100062","day":"01","volume":5,"_id":"11965","article_type":"letter_note","scopus_import":"1","page":"716-720","article_processing_charge":"No","oa_version":"Published Version","month":"08","type":"journal_article"},{"_id":"11972","volume":23,"day":"21","doi":"10.1039/d1gc01284c","publication_identifier":{"issn":["1463-9262"],"eissn":["1463-9270"]},"article_type":"original","article_processing_charge":"No","page":"4524-4530","scopus_import":"1","type":"journal_article","month":"06","oa_version":"Published Version","citation":{"short":"Z. Zhao, S. Reischauer, B. Pieber, M. Delbianco, Green Chemistry 23 (2021) 4524–4530.","chicago":"Zhao, Zhouxiang, Susanne Reischauer, Bartholomäus Pieber, and Martina Delbianco. “Carbon Dot/TiO₂ Nanocomposites as Photocatalysts for Metallaphotocatalytic Carbon-Heteroatom Cross-Couplings.” <i>Green Chemistry</i>. Royal Society of Chemistry, 2021. <a href=\"https://doi.org/10.1039/d1gc01284c\">https://doi.org/10.1039/d1gc01284c</a>.","ieee":"Z. Zhao, S. Reischauer, B. Pieber, and M. Delbianco, “Carbon dot/TiO₂ nanocomposites as photocatalysts for metallaphotocatalytic carbon-heteroatom cross-couplings,” <i>Green Chemistry</i>, vol. 23, no. 12. Royal Society of Chemistry, pp. 4524–4530, 2021.","ama":"Zhao Z, Reischauer S, Pieber B, Delbianco M. Carbon dot/TiO₂ nanocomposites as photocatalysts for metallaphotocatalytic carbon-heteroatom cross-couplings. <i>Green Chemistry</i>. 2021;23(12):4524-4530. doi:<a href=\"https://doi.org/10.1039/d1gc01284c\">10.1039/d1gc01284c</a>","apa":"Zhao, Z., Reischauer, S., Pieber, B., &#38; Delbianco, M. (2021). Carbon dot/TiO₂ nanocomposites as photocatalysts for metallaphotocatalytic carbon-heteroatom cross-couplings. <i>Green Chemistry</i>. Royal Society of Chemistry. <a href=\"https://doi.org/10.1039/d1gc01284c\">https://doi.org/10.1039/d1gc01284c</a>","ista":"Zhao Z, Reischauer S, Pieber B, Delbianco M. 2021. Carbon dot/TiO₂ nanocomposites as photocatalysts for metallaphotocatalytic carbon-heteroatom cross-couplings. Green Chemistry. 23(12), 4524–4530.","mla":"Zhao, Zhouxiang, et al. “Carbon Dot/TiO₂ Nanocomposites as Photocatalysts for Metallaphotocatalytic Carbon-Heteroatom Cross-Couplings.” <i>Green Chemistry</i>, vol. 23, no. 12, Royal Society of Chemistry, 2021, pp. 4524–30, doi:<a href=\"https://doi.org/10.1039/d1gc01284c\">10.1039/d1gc01284c</a>."},"date_published":"2021-06-21T00:00:00Z","year":"2021","status":"public","extern":"1","publication_status":"published","language":[{"iso":"eng"}],"quality_controlled":"1","author":[{"last_name":"Zhao","full_name":"Zhao, Zhouxiang","first_name":"Zhouxiang"},{"full_name":"Reischauer, Susanne","first_name":"Susanne","last_name":"Reischauer"},{"id":"93e5e5b2-0da6-11ed-8a41-af589a024726","full_name":"Pieber, Bartholomäus","orcid":"0000-0001-8689-388X","first_name":"Bartholomäus","last_name":"Pieber"},{"last_name":"Delbianco","first_name":"Martina","full_name":"Delbianco, Martina"}],"intvolume":"        23","issue":"12","publisher":"Royal Society of Chemistry","abstract":[{"lang":"eng","text":"Carbon dots have been previosly immobilized on titanium dioxide to generate photocatalysts for pollutant degradation and water splitting. Here we demonstrate that these nanocomposites are valuable photocatalysts for metallaphotocatalytic carbon–heteroatom cross-couplings. These sustainable materials show a large applicability, high photostability, excellent reusability, and broadly absorb across the visible-light spectrum."}],"oa":1,"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_updated":"2024-10-14T12:05:41Z","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1039/D1GC01284C"}],"title":"Carbon dot/TiO₂ nanocomposites as photocatalysts for metallaphotocatalytic carbon-heteroatom cross-couplings","publication":"Green Chemistry","date_created":"2022-08-25T10:25:46Z"},{"publication_identifier":{"eissn":["2589-0042"]},"doi":"10.1016/j.isci.2021.102209","day":"19","volume":24,"_id":"11974","article_type":"review","article_number":"102209","scopus_import":"1","article_processing_charge":"No","oa_version":"Published Version","month":"03","type":"journal_article","quality_controlled":"1","language":[{"iso":"eng"}],"publication_status":"published","extern":"1","status":"public","date_published":"2021-03-19T00:00:00Z","year":"2021","citation":{"short":"S. Reischauer, B. Pieber, IScience 24 (2021).","chicago":"Reischauer, Susanne, and Bartholomäus Pieber. “Emerging Concepts in Photocatalytic Organic Synthesis.” <i>IScience</i>. Elsevier, 2021. <a href=\"https://doi.org/10.1016/j.isci.2021.102209\">https://doi.org/10.1016/j.isci.2021.102209</a>.","ista":"Reischauer S, Pieber B. 2021. Emerging concepts in photocatalytic organic synthesis. iScience. 24(3), 102209.","apa":"Reischauer, S., &#38; Pieber, B. (2021). Emerging concepts in photocatalytic organic synthesis. <i>IScience</i>. Elsevier. <a href=\"https://doi.org/10.1016/j.isci.2021.102209\">https://doi.org/10.1016/j.isci.2021.102209</a>","ama":"Reischauer S, Pieber B. Emerging concepts in photocatalytic organic synthesis. <i>iScience</i>. 2021;24(3). doi:<a href=\"https://doi.org/10.1016/j.isci.2021.102209\">10.1016/j.isci.2021.102209</a>","ieee":"S. Reischauer and B. Pieber, “Emerging concepts in photocatalytic organic synthesis,” <i>iScience</i>, vol. 24, no. 3. Elsevier, 2021.","mla":"Reischauer, Susanne, and Bartholomäus Pieber. “Emerging Concepts in Photocatalytic Organic Synthesis.” <i>IScience</i>, vol. 24, no. 3, 102209, Elsevier, 2021, doi:<a href=\"https://doi.org/10.1016/j.isci.2021.102209\">10.1016/j.isci.2021.102209</a>."},"issue":"3","intvolume":"        24","author":[{"first_name":"Susanne","full_name":"Reischauer, Susanne","last_name":"Reischauer"},{"last_name":"Pieber","first_name":"Bartholomäus","orcid":"0000-0001-8689-388X","id":"93e5e5b2-0da6-11ed-8a41-af589a024726","full_name":"Pieber, Bartholomäus"}],"oa":1,"abstract":[{"text":"Visible light photocatalysis has become a powerful tool in organic synthesis that uses photons as traceless, sustainable reagents. Most of the activities in the field focus on the development of new reactions via common photoredox cycles, but recently a number of exciting new concepts and strategies entered less charted territories. We survey approaches that enable the use of longer wavelengths and show that the wavelength and intensity of photons are import parameters that enable tuning of the reactivity of a photocatalyst to control or change the selectivity of chemical reactions. In addition, we discuss recent efforts to substitute strong reductants, such as elemental lithium and sodium, by light and technological advances in the field.","lang":"eng"}],"publisher":"Elsevier","date_created":"2022-08-25T10:31:44Z","publication":"iScience","title":"Emerging concepts in photocatalytic organic synthesis","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1016/j.isci.2021.102209"}],"date_updated":"2024-10-14T12:05:29Z"},{"article_type":"letter_note","_id":"11981","volume":23,"publication_identifier":{"issn":["1523-7060"],"eissn":["1523-7052"]},"doi":"10.1021/acs.orglett.0c04026","day":"15","oa_version":"Published Version","type":"journal_article","month":"01","article_processing_charge":"No","scopus_import":"1","page":"514-518","intvolume":"        23","issue":"2","author":[{"last_name":"Cavedon","first_name":"Cristian","full_name":"Cavedon, Cristian"},{"first_name":"Eric T.","full_name":"Sletten, Eric T.","last_name":"Sletten"},{"full_name":"Madani, Amiera","first_name":"Amiera","last_name":"Madani"},{"last_name":"Niemeyer","full_name":"Niemeyer, Olaf","first_name":"Olaf"},{"full_name":"Seeberger, Peter H.","first_name":"Peter H.","last_name":"Seeberger"},{"id":"93e5e5b2-0da6-11ed-8a41-af589a024726","full_name":"Pieber, Bartholomäus","orcid":"0000-0001-8689-388X","first_name":"Bartholomäus","last_name":"Pieber"}],"date_published":"2021-01-15T00:00:00Z","year":"2021","publication_status":"published","extern":"1","status":"public","citation":{"short":"C. Cavedon, E.T. Sletten, A. Madani, O. Niemeyer, P.H. Seeberger, B. Pieber, Organic Letters 23 (2021) 514–518.","chicago":"Cavedon, Cristian, Eric T. Sletten, Amiera Madani, Olaf Niemeyer, Peter H. Seeberger, and Bartholomäus Pieber. “Visible-Light-Mediated Oxidative Debenzylation Enables the Use of Benzyl Ethers as Temporary Protecting Groups.” <i>Organic Letters</i>. American Chemical Society, 2021. <a href=\"https://doi.org/10.1021/acs.orglett.0c04026\">https://doi.org/10.1021/acs.orglett.0c04026</a>.","ista":"Cavedon C, Sletten ET, Madani A, Niemeyer O, Seeberger PH, Pieber B. 2021. Visible-light-mediated oxidative debenzylation enables the use of benzyl ethers as temporary protecting groups. Organic Letters. 23(2), 514–518.","apa":"Cavedon, C., Sletten, E. T., Madani, A., Niemeyer, O., Seeberger, P. H., &#38; Pieber, B. (2021). Visible-light-mediated oxidative debenzylation enables the use of benzyl ethers as temporary protecting groups. <i>Organic Letters</i>. American Chemical Society. <a href=\"https://doi.org/10.1021/acs.orglett.0c04026\">https://doi.org/10.1021/acs.orglett.0c04026</a>","ieee":"C. Cavedon, E. T. Sletten, A. Madani, O. Niemeyer, P. H. Seeberger, and B. Pieber, “Visible-light-mediated oxidative debenzylation enables the use of benzyl ethers as temporary protecting groups,” <i>Organic Letters</i>, vol. 23, no. 2. American Chemical Society, pp. 514–518, 2021.","ama":"Cavedon C, Sletten ET, Madani A, Niemeyer O, Seeberger PH, Pieber B. Visible-light-mediated oxidative debenzylation enables the use of benzyl ethers as temporary protecting groups. <i>Organic Letters</i>. 2021;23(2):514-518. doi:<a href=\"https://doi.org/10.1021/acs.orglett.0c04026\">10.1021/acs.orglett.0c04026</a>","mla":"Cavedon, Cristian, et al. “Visible-Light-Mediated Oxidative Debenzylation Enables the Use of Benzyl Ethers as Temporary Protecting Groups.” <i>Organic Letters</i>, vol. 23, no. 2, American Chemical Society, 2021, pp. 514–18, doi:<a href=\"https://doi.org/10.1021/acs.orglett.0c04026\">10.1021/acs.orglett.0c04026</a>."},"quality_controlled":"1","external_id":{"pmid":["33400534"]},"language":[{"iso":"eng"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","pmid":1,"main_file_link":[{"url":"https://doi.org/10.1021/acs.orglett.0c04026","open_access":"1"}],"date_updated":"2024-10-14T12:05:18Z","date_created":"2022-08-25T11:13:05Z","title":"Visible-light-mediated oxidative debenzylation enables the use of benzyl ethers as temporary protecting groups","publication":"Organic Letters","publisher":"American Chemical Society","oa":1,"abstract":[{"text":"The cleavage of benzyl ethers by catalytic hydrogenolysis or Birch reduction suffers from poor functional group compatibility and limits their use as a protecting group. The visible-light-mediated debenzylation disclosed here renders benzyl ethers temporary protective groups, enabling new orthogonal protection strategies. Using 2,3-dichloro-5,6-dicyano-1,4-benzoquinone (DDQ) as a stoichiometric or catalytic photooxidant, benzyl ethers can be cleaved in the presence of azides, alkenes, and alkynes. The reaction time can be reduced from hours to minutes in continuous flow.","lang":"eng"}]},{"author":[{"last_name":"Cavedon","full_name":"Cavedon, Cristian","first_name":"Cristian"},{"first_name":"Sebastian","full_name":"Gisbertz, Sebastian","last_name":"Gisbertz"},{"first_name":"Sarah","full_name":"Vogl, Sarah","last_name":"Vogl"},{"full_name":"Richter, Noah","first_name":"Noah","last_name":"Richter"},{"full_name":"Schrottke, Stefanie","first_name":"Stefanie","last_name":"Schrottke"},{"full_name":"Teutloff, Christian","first_name":"Christian","last_name":"Teutloff"},{"last_name":"Seeberger","full_name":"Seeberger, Peter H.","first_name":"Peter H."},{"last_name":"Thomas","first_name":"Arne","full_name":"Thomas, Arne"},{"last_name":"Pieber","full_name":"Pieber, Bartholomäus","orcid":"0000-0001-8689-388X","id":"93e5e5b2-0da6-11ed-8a41-af589a024726","first_name":"Bartholomäus"}],"citation":{"ista":"Cavedon C, Gisbertz S, Vogl S, Richter N, Schrottke S, Teutloff C, Seeberger PH, Thomas A, Pieber B. Photocatalyst-free, visible-light-mediated nickel catalyzed carbon–heteroatom cross-couplings. <a href=\"https://doi.org/10.26434/chemrxiv-2021-kt2wr\">10.26434/chemrxiv-2021-kt2wr</a>.","apa":"Cavedon, C., Gisbertz, S., Vogl, S., Richter, N., Schrottke, S., Teutloff, C., … Pieber, B. (n.d.). Photocatalyst-free, visible-light-mediated nickel catalyzed carbon–heteroatom cross-couplings. ChemRxiv. <a href=\"https://doi.org/10.26434/chemrxiv-2021-kt2wr\">https://doi.org/10.26434/chemrxiv-2021-kt2wr</a>","ieee":"C. Cavedon <i>et al.</i>, “Photocatalyst-free, visible-light-mediated nickel catalyzed carbon–heteroatom cross-couplings.” ChemRxiv.","ama":"Cavedon C, Gisbertz S, Vogl S, et al. Photocatalyst-free, visible-light-mediated nickel catalyzed carbon–heteroatom cross-couplings. doi:<a href=\"https://doi.org/10.26434/chemrxiv-2021-kt2wr\">10.26434/chemrxiv-2021-kt2wr</a>","mla":"Cavedon, Cristian, et al. <i>Photocatalyst-Free, Visible-Light-Mediated Nickel Catalyzed Carbon–Heteroatom Cross-Couplings</i>. ChemRxiv, doi:<a href=\"https://doi.org/10.26434/chemrxiv-2021-kt2wr\">10.26434/chemrxiv-2021-kt2wr</a>.","short":"C. Cavedon, S. Gisbertz, S. Vogl, N. Richter, S. Schrottke, C. Teutloff, P.H. Seeberger, A. Thomas, B. Pieber, (n.d.).","chicago":"Cavedon, Cristian, Sebastian Gisbertz, Sarah Vogl, Noah Richter, Stefanie Schrottke, Christian Teutloff, Peter H. Seeberger, Arne Thomas, and Bartholomäus Pieber. “Photocatalyst-Free, Visible-Light-Mediated Nickel Catalyzed Carbon–Heteroatom Cross-Couplings.” ChemRxiv, n.d. <a href=\"https://doi.org/10.26434/chemrxiv-2021-kt2wr\">https://doi.org/10.26434/chemrxiv-2021-kt2wr</a>."},"year":"2021","_id":"12068","date_published":"2021-08-04T00:00:00Z","publication_status":"submitted","status":"public","extern":"1","doi":"10.26434/chemrxiv-2021-kt2wr","day":"04","language":[{"iso":"eng"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","main_file_link":[{"url":"https://doi.org/10.26434/chemrxiv-2021-kt2wr","open_access":"1"}],"date_updated":"2024-10-14T12:05:05Z","type":"preprint","title":"Photocatalyst-free, visible-light-mediated nickel catalyzed carbon–heteroatom cross-couplings","month":"08","oa_version":"Preprint","date_created":"2022-09-08T11:42:02Z","publisher":"ChemRxiv","article_processing_charge":"No","abstract":[{"text":"Metallaphotocatalysis typically requires a photocatalyst to harness the energy of visible-light and transfer it to a transition metal catalyst to trigger chemical reactions. The most prominent example is the merger of photo- and nickel catalysis that unlocked various cross-couplings. However, the high reactivity of excited photocatalyst can lead to unwanted side reactions thus limiting this approach. Here we show that a bipyridine ligand that is subtly decorated with two carbazole groups forms a nickel complex that absorbs visible-light and promotes several carbon–heteroatom cross-couplings in the absence of an exogenous photocatalysts. The ligand can be polymerized in a simple one-step procedure to afford a porous organic polymer that can be used for heterogeneous nickel catalysis in the same reactions. The material can be easily recovered and reused multiple times maintaining high catalytic activity and selectivity.","lang":"eng"}],"oa":1},{"main_file_link":[{"open_access":"1","url":"https://doi.org/10.26434/chemrxiv.13521527"}],"date_updated":"2022-09-08T11:49:16Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","month":"01","title":"Switching between enantiomers by combining chromoselective photocatalysis and biocatalysis","type":"preprint","date_created":"2022-09-08T11:46:45Z","oa_version":"Preprint","publisher":"ChemRxiv","article_processing_charge":"No","abstract":[{"text":"Controlling the selectivity of a chemical reaction with external stimuli is common in thermal processes, but rare in visible-light photocatalysis. Here we show that the redox potential of a carbon nitride photocatalyst (CN-OA-m) can be tuned by changing the irradiation wavelength to generate electron holes with different oxidation potentials. This tuning was the key to realizing photo-chemo-enzymatic cascades that give either the (S)- or the (R)-enantiomer of phenylethanol. In combination with an unspecific peroxygenase from Agrocybe aegerita, green light irradiation of CN-OA-m led to the enantioselective hydroxylation of ethylbenzene to (R)-1-phenylethanol (99% ee). In contrast, blue light irradiation triggered the photocatalytic oxidation of ethylbenzene to acetophenone, which in turn was enantioselectively reduced with an alcohol dehydrogenase from Rhodococcus ruber to form (S)-1-phenylethanol (93% ee).","lang":"eng"}],"oa":1,"author":[{"last_name":"Schmermund","first_name":"Luca","full_name":"Schmermund, Luca"},{"full_name":"Reischauer, Susanne","first_name":"Susanne","last_name":"Reischauer"},{"last_name":"Bierbaumer","full_name":"Bierbaumer, Sarah","first_name":"Sarah"},{"last_name":"Winkler","first_name":"Christoph","full_name":"Winkler, Christoph"},{"full_name":"Diaz-Rodriguez, Alba","first_name":"Alba","last_name":"Diaz-Rodriguez"},{"last_name":"Edwards","first_name":"Lee J.","full_name":"Edwards, Lee J."},{"full_name":"Kara, Selin","first_name":"Selin","last_name":"Kara"},{"first_name":"Tamara","full_name":"Mielke, Tamara","last_name":"Mielke"},{"first_name":"Jared","full_name":"Cartwright, Jared","last_name":"Cartwright"},{"last_name":"Grogan","first_name":"Gideon","full_name":"Grogan, Gideon"},{"first_name":"Bartholomäus","orcid":"0000-0001-8689-388X","id":"93e5e5b2-0da6-11ed-8a41-af589a024726","full_name":"Pieber, Bartholomäus","last_name":"Pieber"},{"last_name":"Kroutil","first_name":"Wolfgang","full_name":"Kroutil, Wolfgang"}],"citation":{"chicago":"Schmermund, Luca, Susanne Reischauer, Sarah Bierbaumer, Christoph Winkler, Alba Diaz-Rodriguez, Lee J. Edwards, Selin Kara, et al. “Switching between Enantiomers by Combining Chromoselective Photocatalysis and Biocatalysis.” ChemRxiv, n.d. <a href=\"https://doi.org/10.26434/chemrxiv.13521527\">https://doi.org/10.26434/chemrxiv.13521527</a>.","short":"L. Schmermund, S. Reischauer, S. Bierbaumer, C. Winkler, A. Diaz-Rodriguez, L.J. Edwards, S. Kara, T. Mielke, J. Cartwright, G. Grogan, B. Pieber, W. Kroutil, (n.d.).","mla":"Schmermund, Luca, et al. <i>Switching between Enantiomers by Combining Chromoselective Photocatalysis and Biocatalysis</i>. ChemRxiv, doi:<a href=\"https://doi.org/10.26434/chemrxiv.13521527\">10.26434/chemrxiv.13521527</a>.","apa":"Schmermund, L., Reischauer, S., Bierbaumer, S., Winkler, C., Diaz-Rodriguez, A., Edwards, L. J., … Kroutil, W. (n.d.). Switching between enantiomers by combining chromoselective photocatalysis and biocatalysis. ChemRxiv. <a href=\"https://doi.org/10.26434/chemrxiv.13521527\">https://doi.org/10.26434/chemrxiv.13521527</a>","ieee":"L. Schmermund <i>et al.</i>, “Switching between enantiomers by combining chromoselective photocatalysis and biocatalysis.” ChemRxiv.","ama":"Schmermund L, Reischauer S, Bierbaumer S, et al. Switching between enantiomers by combining chromoselective photocatalysis and biocatalysis. doi:<a href=\"https://doi.org/10.26434/chemrxiv.13521527\">10.26434/chemrxiv.13521527</a>","ista":"Schmermund L, Reischauer S, Bierbaumer S, Winkler C, Diaz-Rodriguez A, Edwards LJ, Kara S, Mielke T, Cartwright J, Grogan G, Pieber B, Kroutil W. Switching between enantiomers by combining chromoselective photocatalysis and biocatalysis. <a href=\"https://doi.org/10.26434/chemrxiv.13521527\">10.26434/chemrxiv.13521527</a>."},"extern":"1","publication_status":"submitted","status":"public","_id":"12070","date_published":"2021-01-06T00:00:00Z","year":"2021","language":[{"iso":"eng"}],"day":"06","doi":"10.26434/chemrxiv.13521527"},{"_id":"12071","volume":3,"tmp":{"short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png"},"doi":"10.1103/physrevresearch.3.023075","day":"27","publication_identifier":{"issn":["2643-1564"]},"article_number":"023075","article_type":"original","article_processing_charge":"No","scopus_import":"1","ddc":["530"],"type":"journal_article","month":"04","oa_version":"Published Version","file_date_updated":"2022-09-09T07:23:40Z","citation":{"chicago":"Sun, Zhixiang, Jose M. Guevara, Steffen Sykora, Ekaterina Paerschke, Kaustuv Manna, Andrey Maljuk, Sabine Wurmehl, Jeroen van den Brink, Bernd Büchner, and Christian Hess. “Evidence for a Percolative Mott Insulator-Metal Transition in Doped Sr₂IrO₄.” <i>Physical Review Research</i>. American Physical Society, 2021. <a href=\"https://doi.org/10.1103/physrevresearch.3.023075\">https://doi.org/10.1103/physrevresearch.3.023075</a>.","short":"Z. Sun, J.M. Guevara, S. Sykora, E. Paerschke, K. Manna, A. Maljuk, S. Wurmehl, J. van den Brink, B. Büchner, C. Hess, Physical Review Research 3 (2021).","mla":"Sun, Zhixiang, et al. “Evidence for a Percolative Mott Insulator-Metal Transition in Doped Sr₂IrO₄.” <i>Physical Review Research</i>, vol. 3, no. 2, 023075, American Physical Society, 2021, doi:<a href=\"https://doi.org/10.1103/physrevresearch.3.023075\">10.1103/physrevresearch.3.023075</a>.","ista":"Sun Z, Guevara JM, Sykora S, Paerschke E, Manna K, Maljuk A, Wurmehl S, van den Brink J, Büchner B, Hess C. 2021. Evidence for a percolative Mott insulator-metal transition in doped Sr₂IrO₄. Physical Review Research. 3(2), 023075.","ieee":"Z. Sun <i>et al.</i>, “Evidence for a percolative Mott insulator-metal transition in doped Sr₂IrO₄,” <i>Physical Review Research</i>, vol. 3, no. 2. American Physical Society, 2021.","apa":"Sun, Z., Guevara, J. M., Sykora, S., Paerschke, E., Manna, K., Maljuk, A., … Hess, C. (2021). Evidence for a percolative Mott insulator-metal transition in doped Sr₂IrO₄. <i>Physical Review Research</i>. American Physical Society. <a href=\"https://doi.org/10.1103/physrevresearch.3.023075\">https://doi.org/10.1103/physrevresearch.3.023075</a>","ama":"Sun Z, Guevara JM, Sykora S, et al. Evidence for a percolative Mott insulator-metal transition in doped Sr₂IrO₄. <i>Physical Review Research</i>. 2021;3(2). doi:<a href=\"https://doi.org/10.1103/physrevresearch.3.023075\">10.1103/physrevresearch.3.023075</a>"},"date_published":"2021-04-27T00:00:00Z","year":"2021","extern":"1","status":"public","publication_status":"published","language":[{"iso":"eng"}],"quality_controlled":"1","author":[{"full_name":"Sun, Zhixiang","first_name":"Zhixiang","last_name":"Sun"},{"first_name":"Jose M.","full_name":"Guevara, Jose M.","last_name":"Guevara"},{"first_name":"Steffen","full_name":"Sykora, Steffen","last_name":"Sykora"},{"full_name":"Paerschke, Ekaterina","id":"8275014E-6063-11E9-9B7F-6338E6697425","orcid":"0000-0003-0853-8182","first_name":"Ekaterina","last_name":"Paerschke"},{"full_name":"Manna, Kaustuv","first_name":"Kaustuv","last_name":"Manna"},{"first_name":"Andrey","full_name":"Maljuk, Andrey","last_name":"Maljuk"},{"last_name":"Wurmehl","full_name":"Wurmehl, Sabine","first_name":"Sabine"},{"last_name":"van den Brink","full_name":"van den Brink, Jeroen","first_name":"Jeroen"},{"first_name":"Bernd","full_name":"Büchner, Bernd","last_name":"Büchner"},{"last_name":"Hess","full_name":"Hess, Christian","first_name":"Christian"}],"intvolume":"         3","issue":"2","has_accepted_license":"1","publisher":"American Physical Society","abstract":[{"lang":"eng","text":"Despite many efforts to rationalize the strongly correlated electronic ground states in doped Mott insulators, the nature of the doping-induced insulator-to-metal transition is still a subject under intensive investigation. Here, we probe the nanoscale electronic structure of the Mott insulator Sr₂IrO₄δ with low-temperature scanning tunneling microscopy and find an enhanced local density of states (LDOS) inside the Mott gap at the location of individual defects which we interpret as defects at apical oxygen sites. A chiral behavior in the topography for those defects has been observed. We also visualize the local enhanced conductance arising from the overlapping of defect states which induces finite LDOS inside of the Mott gap. By combining these findings with the typical spatial extension of isolated defects of about 2 nm, our results indicate that the insulator-to-metal transition in Sr₂IrO₄−δ could be percolative in nature."}],"file":[{"date_created":"2022-09-09T07:23:40Z","file_id":"12075","success":1,"access_level":"open_access","date_updated":"2022-09-09T07:23:40Z","checksum":"73f1331b9716295849e87a7d3acd9323","relation":"main_file","content_type":"application/pdf","file_name":"2021_PhysicalRevResearch_Sun.pdf","file_size":4020901,"creator":"dernst"}],"oa":1,"date_updated":"2022-09-09T07:26:01Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","title":"Evidence for a percolative Mott insulator-metal transition in doped Sr₂IrO₄","publication":"Physical Review Research","date_created":"2022-09-08T15:01:16Z"},{"_id":"12186","volume":72,"doi":"10.1093/jxb/erab373","day":"13","publication_identifier":{"issn":["0022-0957","1460-2431"]},"article_type":"original","article_processing_charge":"No","department":[{"_id":"XiFe"}],"page":"7927-7941","scopus_import":"1","type":"journal_article","month":"08","oa_version":"None","citation":{"mla":"Ding, Pingtao, et al. “Chromatin Accessibility Landscapes Activated by Cell-Surface and Intracellular Immune Receptors.” <i>Journal of Experimental Botany</i>, vol. 72, no. 22, Oxford University Press, 2021, pp. 7927–41, doi:<a href=\"https://doi.org/10.1093/jxb/erab373\">10.1093/jxb/erab373</a>.","ista":"Ding P, Sakai T, Krishna Shrestha R, Manosalva Perez N, Guo W, Ngou BPM, He S, Liu C, Feng X, Zhang R, Vandepoele K, MacLean D, Jones JDG. 2021. Chromatin accessibility landscapes activated by cell-surface and intracellular immune receptors. Journal of Experimental Botany. 72(22), 7927–7941.","ama":"Ding P, Sakai T, Krishna Shrestha R, et al. Chromatin accessibility landscapes activated by cell-surface and intracellular immune receptors. <i>Journal of Experimental Botany</i>. 2021;72(22):7927-7941. doi:<a href=\"https://doi.org/10.1093/jxb/erab373\">10.1093/jxb/erab373</a>","ieee":"P. Ding <i>et al.</i>, “Chromatin accessibility landscapes activated by cell-surface and intracellular immune receptors,” <i>Journal of Experimental Botany</i>, vol. 72, no. 22. Oxford University Press, pp. 7927–7941, 2021.","apa":"Ding, P., Sakai, T., Krishna Shrestha, R., Manosalva Perez, N., Guo, W., Ngou, B. P. M., … Jones, J. D. G. (2021). Chromatin accessibility landscapes activated by cell-surface and intracellular immune receptors. <i>Journal of Experimental Botany</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/jxb/erab373\">https://doi.org/10.1093/jxb/erab373</a>","chicago":"Ding, Pingtao, Toshiyuki Sakai, Ram Krishna Shrestha, Nicolas Manosalva Perez, Wenbin Guo, Bruno Pok Man Ngou, Shengbo He, et al. “Chromatin Accessibility Landscapes Activated by Cell-Surface and Intracellular Immune Receptors.” <i>Journal of Experimental Botany</i>. Oxford University Press, 2021. <a href=\"https://doi.org/10.1093/jxb/erab373\">https://doi.org/10.1093/jxb/erab373</a>.","short":"P. Ding, T. Sakai, R. Krishna Shrestha, N. Manosalva Perez, W. Guo, B.P.M. Ngou, S. He, C. Liu, X. Feng, R. Zhang, K. Vandepoele, D. MacLean, J.D.G. Jones, Journal of Experimental Botany 72 (2021) 7927–7941."},"date_published":"2021-08-13T00:00:00Z","year":"2021","status":"public","publication_status":"published","extern":"1","external_id":{"pmid":["34387350"]},"language":[{"iso":"eng"}],"quality_controlled":"1","author":[{"first_name":"Pingtao","full_name":"Ding, Pingtao","last_name":"Ding"},{"last_name":"Sakai","first_name":"Toshiyuki","full_name":"Sakai, Toshiyuki"},{"first_name":"Ram","full_name":"Krishna Shrestha, Ram","last_name":"Krishna Shrestha"},{"full_name":"Manosalva Perez, Nicolas","first_name":"Nicolas","last_name":"Manosalva Perez"},{"last_name":"Guo","first_name":"Wenbin","full_name":"Guo, Wenbin"},{"last_name":"Ngou","full_name":"Ngou, Bruno Pok Man","first_name":"Bruno Pok Man"},{"last_name":"He","full_name":"He, Shengbo","first_name":"Shengbo"},{"full_name":"Liu, Chang","first_name":"Chang","last_name":"Liu"},{"last_name":"Feng","first_name":"Xiaoqi","full_name":"Feng, Xiaoqi","orcid":"0000-0002-4008-1234","id":"e0164712-22ee-11ed-b12a-d80fcdf35958"},{"first_name":"Runxuan","full_name":"Zhang, Runxuan","last_name":"Zhang"},{"first_name":"Klaas","full_name":"Vandepoele, Klaas","last_name":"Vandepoele"},{"last_name":"MacLean","full_name":"MacLean, Dan","first_name":"Dan"},{"last_name":"Jones","full_name":"Jones, Jonathan D G","first_name":"Jonathan D G"}],"intvolume":"        72","issue":"22","publisher":"Oxford University Press","abstract":[{"lang":"eng","text":"Activation of cell-surface and intracellular receptor-mediated immunity results in rapid transcriptional reprogramming that underpins disease resistance. However, the mechanisms by which co-activation of both immune systems lead to transcriptional changes are not clear. Here, we combine RNA-seq and ATAC-seq to define changes in gene expression and chromatin accessibility. Activation of cell-surface or intracellular receptor-mediated immunity, or both, increases chromatin accessibility at induced defence genes. Analysis of ATAC-seq and RNA-seq data combined with publicly available information on transcription factor DNA-binding motifs enabled comparison of individual gene regulatory networks activated by cell-surface or intracellular receptor-mediated immunity, or by both. These results and analyses reveal overlapping and conserved transcriptional regulatory mechanisms between the two immune systems."}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_updated":"2023-05-08T11:01:18Z","pmid":1,"title":"Chromatin accessibility landscapes activated by cell-surface and intracellular immune receptors","keyword":["Plant Science","Physiology"],"publication":"Journal of Experimental Botany","date_created":"2023-01-16T09:14:35Z","acknowledgement":"We thank the Gatsby Foundation (UK) for funding to the JDGJ laboratory. PD acknowledges support from the European Union’s Horizon 2020 Research and Innovation Program under Marie Skłodowska Curie Actions (grant agreement: 656243) and a Future Leader Fellowship from the Biotechnology and Biological Sciences Research Council (BBSRC) (grant agreement: BB/R012172/1). TS, RKS, DM, and JDGJ were supported by the Gatsby Foundation funding to the\r\nSainsbury Laboratory. NMP and KV were supported by a BOF grant from Ghent University (grant agreement: BOF24Y2019001901). WG and RZ were supported by the Scottish Government Rural and Environment Science and Analytical Services division (RESAS), and RZ also acknowledges the support from a BBSRC Bioinformatics and Biological Resources Fund (grant agreement: BB/S020160/1).BPMN was supported by the Norwich Research Park (NRP) Biosciences Doctoral Training Partnership (DTP) funded by the BBSRC (grant agreement: BB/M011216/1). SH and XF were supported by a BBSRC Responsive Mode grant (grant agreement: BB/S009620/1) and a European Research Council Starting grant ‘SexMeth’ (grant agreement: 804981). CL was supported by Deutsche Forschungsgemeinschaft (grant agreement: LI 2862/4). "},{"oa_version":"Published Version","type":"journal_article","month":"10","article_processing_charge":"No","scopus_import":"1","page":"940-949","article_type":"original","_id":"13357","volume":13,"publication_identifier":{"eissn":["1755-4349"],"issn":["1755-4330"]},"doi":"10.1038/s41557-021-00752-9","day":"01","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","main_file_link":[{"url":"https://doi.org/10.1038/s41557-021-00752-9","open_access":"1"}],"pmid":1,"date_updated":"2024-10-14T12:11:57Z","date_created":"2023-08-01T09:34:54Z","title":"Electrostatic co-assembly of nanoparticles with oppositely charged small molecules into static and dynamic superstructures","keyword":["General Chemical Engineering","General Chemistry"],"publication":"Nature Chemistry","publisher":"Springer Nature","oa":1,"abstract":[{"lang":"eng","text":"Coulombic interactions can be used to assemble charged nanoparticles into higher-order structures, but the process requires oppositely charged partners that are similarly sized. The ability to mediate the assembly of such charged nanoparticles using structurally simple small molecules would greatly facilitate the fabrication of nanostructured materials and harnessing their applications in catalysis, sensing and photonics. Here we show that small molecules with as few as three electric charges can effectively induce attractive interactions between oppositely charged nanoparticles in water. These interactions can guide the assembly of charged nanoparticles into colloidal crystals of a quality previously only thought to result from their co-crystallization with oppositely charged nanoparticles of a similar size. Transient nanoparticle assemblies can be generated using positively charged nanoparticles and multiply charged anions that are enzymatically hydrolysed into mono- and/or dianions. Our findings demonstrate an approach for the facile fabrication, manipulation and further investigation of static and dynamic nanostructured materials in aqueous environments."}],"intvolume":"        13","issue":"10","author":[{"first_name":"Tong","full_name":"Bian, Tong","last_name":"Bian"},{"full_name":"Gardin, Andrea","first_name":"Andrea","last_name":"Gardin"},{"last_name":"Gemen","full_name":"Gemen, Julius","first_name":"Julius"},{"last_name":"Houben","first_name":"Lothar","full_name":"Houben, Lothar"},{"full_name":"Perego, Claudio","first_name":"Claudio","last_name":"Perego"},{"last_name":"Lee","first_name":"Byeongdu","full_name":"Lee, Byeongdu"},{"first_name":"Nadav","full_name":"Elad, Nadav","last_name":"Elad"},{"first_name":"Zonglin","full_name":"Chu, Zonglin","last_name":"Chu"},{"first_name":"Giovanni M.","full_name":"Pavan, Giovanni M.","last_name":"Pavan"},{"last_name":"Klajn","first_name":"Rafal","id":"8e84690e-1e48-11ed-a02b-a1e6fb8bb53b","full_name":"Klajn, Rafal"}],"year":"2021","date_published":"2021-10-01T00:00:00Z","extern":"1","publication_status":"published","status":"public","citation":{"chicago":"Bian, Tong, Andrea Gardin, Julius Gemen, Lothar Houben, Claudio Perego, Byeongdu Lee, Nadav Elad, Zonglin Chu, Giovanni M. Pavan, and Rafal Klajn. “Electrostatic Co-Assembly of Nanoparticles with Oppositely Charged Small Molecules into Static and Dynamic Superstructures.” <i>Nature Chemistry</i>. Springer Nature, 2021. <a href=\"https://doi.org/10.1038/s41557-021-00752-9\">https://doi.org/10.1038/s41557-021-00752-9</a>.","short":"T. Bian, A. Gardin, J. Gemen, L. Houben, C. Perego, B. Lee, N. Elad, Z. Chu, G.M. Pavan, R. Klajn, Nature Chemistry 13 (2021) 940–949.","mla":"Bian, Tong, et al. “Electrostatic Co-Assembly of Nanoparticles with Oppositely Charged Small Molecules into Static and Dynamic Superstructures.” <i>Nature Chemistry</i>, vol. 13, no. 10, Springer Nature, 2021, pp. 940–49, doi:<a href=\"https://doi.org/10.1038/s41557-021-00752-9\">10.1038/s41557-021-00752-9</a>.","ista":"Bian T, Gardin A, Gemen J, Houben L, Perego C, Lee B, Elad N, Chu Z, Pavan GM, Klajn R. 2021. Electrostatic co-assembly of nanoparticles with oppositely charged small molecules into static and dynamic superstructures. Nature Chemistry. 13(10), 940–949.","ieee":"T. Bian <i>et al.</i>, “Electrostatic co-assembly of nanoparticles with oppositely charged small molecules into static and dynamic superstructures,” <i>Nature Chemistry</i>, vol. 13, no. 10. Springer Nature, pp. 940–949, 2021.","ama":"Bian T, Gardin A, Gemen J, et al. Electrostatic co-assembly of nanoparticles with oppositely charged small molecules into static and dynamic superstructures. <i>Nature Chemistry</i>. 2021;13(10):940-949. doi:<a href=\"https://doi.org/10.1038/s41557-021-00752-9\">10.1038/s41557-021-00752-9</a>","apa":"Bian, T., Gardin, A., Gemen, J., Houben, L., Perego, C., Lee, B., … Klajn, R. (2021). Electrostatic co-assembly of nanoparticles with oppositely charged small molecules into static and dynamic superstructures. <i>Nature Chemistry</i>. Springer Nature. <a href=\"https://doi.org/10.1038/s41557-021-00752-9\">https://doi.org/10.1038/s41557-021-00752-9</a>"},"quality_controlled":"1","external_id":{"pmid":["34489564"]},"language":[{"iso":"eng"}]},{"quality_controlled":"1","language":[{"iso":"eng"}],"status":"public","publication_status":"published","extern":"1","year":"2021","date_published":"2021-03-08T00:00:00Z","citation":{"ama":"Ryssy J, Natarajan AK, Wang J, et al. Light‐responsive dynamic DNA‐origami‐based plasmonic assemblies. <i>Angewandte Chemie International Edition</i>. 2021;60(11):5859-5863. doi:<a href=\"https://doi.org/10.1002/anie.202014963\">10.1002/anie.202014963</a>","ieee":"J. Ryssy <i>et al.</i>, “Light‐responsive dynamic DNA‐origami‐based plasmonic assemblies,” <i>Angewandte Chemie International Edition</i>, vol. 60, no. 11. Wiley, pp. 5859–5863, 2021.","apa":"Ryssy, J., Natarajan, A. K., Wang, J., Lehtonen, A. J., Nguyen, M., Klajn, R., &#38; Kuzyk, A. (2021). Light‐responsive dynamic DNA‐origami‐based plasmonic assemblies. <i>Angewandte Chemie International Edition</i>. Wiley. <a href=\"https://doi.org/10.1002/anie.202014963\">https://doi.org/10.1002/anie.202014963</a>","ista":"Ryssy J, Natarajan AK, Wang J, Lehtonen AJ, Nguyen M, Klajn R, Kuzyk A. 2021. Light‐responsive dynamic DNA‐origami‐based plasmonic assemblies. Angewandte Chemie International Edition. 60(11), 5859–5863.","mla":"Ryssy, Joonas, et al. “Light‐responsive Dynamic DNA‐origami‐based Plasmonic Assemblies.” <i>Angewandte Chemie International Edition</i>, vol. 60, no. 11, Wiley, 2021, pp. 5859–63, doi:<a href=\"https://doi.org/10.1002/anie.202014963\">10.1002/anie.202014963</a>.","short":"J. Ryssy, A.K. Natarajan, J. Wang, A.J. Lehtonen, M. Nguyen, R. Klajn, A. Kuzyk, Angewandte Chemie International Edition 60 (2021) 5859–5863.","chicago":"Ryssy, Joonas, Ashwin K. Natarajan, Jinhua Wang, Arttu J. Lehtonen, Minh‐Kha Nguyen, Rafal Klajn, and Anton Kuzyk. “Light‐responsive Dynamic DNA‐origami‐based Plasmonic Assemblies.” <i>Angewandte Chemie International Edition</i>. Wiley, 2021. <a href=\"https://doi.org/10.1002/anie.202014963\">https://doi.org/10.1002/anie.202014963</a>."},"issue":"11","intvolume":"        60","author":[{"last_name":"Ryssy","full_name":"Ryssy, Joonas","first_name":"Joonas"},{"first_name":"Ashwin K.","full_name":"Natarajan, Ashwin K.","last_name":"Natarajan"},{"first_name":"Jinhua","full_name":"Wang, Jinhua","last_name":"Wang"},{"full_name":"Lehtonen, Arttu J.","first_name":"Arttu J.","last_name":"Lehtonen"},{"last_name":"Nguyen","first_name":"Minh‐Kha","full_name":"Nguyen, Minh‐Kha"},{"full_name":"Klajn, Rafal","id":"8e84690e-1e48-11ed-a02b-a1e6fb8bb53b","first_name":"Rafal","last_name":"Klajn"},{"full_name":"Kuzyk, Anton","first_name":"Anton","last_name":"Kuzyk"}],"oa":1,"abstract":[{"lang":"eng","text":"DNA nanotechnology offers a versatile toolbox for precise spatial and temporal manipulation of matter on the nanoscale. However, rendering DNA-based systems responsive to light has remained challenging. Herein, we describe the remote manipulation of native (non-photoresponsive) chiral plasmonic molecules (CPMs) using light. Our strategy is based on the use of a photoresponsive medium comprising a merocyanine-based photoacid. Upon exposure to visible light, the medium decreases its pH, inducing the formation of DNA triplex links, leading to a spatial reconfiguration of the CPMs. The process can be reversed simply by turning the light off and it can be repeated for multiple cycles. The degree of the overall chirality change in an ensemble of CPMs depends on the CPM fraction undergoing reconfiguration, which, remarkably, depends on and can be tuned by the intensity of incident light. Such a dynamic, remotely controlled system could aid in further advancing DNA-based devices and nanomaterials."}],"publisher":"Wiley","date_created":"2023-08-01T09:35:06Z","keyword":["General Chemistry","Catalysis"],"publication":"Angewandte Chemie International Edition","related_material":{"link":[{"url":"https://doi.org/10.1002/anie.202210394","relation":"erratum"}]},"title":"Light‐responsive dynamic DNA‐origami‐based plasmonic assemblies","main_file_link":[{"url":"https://doi.org/10.1002/anie.202014963","open_access":"1"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_updated":"2023-08-02T07:22:23Z","publication_identifier":{"eissn":["1521-3773"],"issn":["1433-7851"]},"day":"08","doi":"10.1002/anie.202014963","volume":60,"_id":"13358","article_type":"original","scopus_import":"1","page":"5859-5863","article_processing_charge":"No","oa_version":"Published Version","month":"03","type":"journal_article"},{"month":"01","type":"journal_article","oa_version":"Published Version","page":"23-37","scopus_import":"1","article_processing_charge":"No","article_type":"original","day":"14","doi":"10.1016/j.chempr.2020.11.025","publication_identifier":{"issn":["2451-9294"]},"volume":7,"_id":"13359","keyword":["Materials Chemistry","Biochemistry (medical)","General Chemical Engineering","Environmental Chemistry","Biochemistry","General Chemistry"],"publication":"Chem","title":"Dissipative self-assembly: Fueling with chemicals versus light","date_created":"2023-08-01T09:35:19Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_updated":"2024-10-14T12:12:18Z","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1016/j.chempr.2020.11.025"}],"abstract":[{"text":"Dissipative self-assembly is ubiquitous in nature, where it gives rise to complex structures and functions such as self-healing, homeostasis, and camouflage. These phenomena are enabled by the continuous conversion of energy stored in chemical fuels, such as ATP. Over the past decade, an increasing number of synthetic chemically driven systems have been reported that mimic the features of their natural counterparts. At the same time, it has been shown that dissipative self-assembly can also be fueled by light; these optically fueled systems have been developed in parallel to the chemically fueled ones. In this perspective, we critically compare these two classes of systems. Despite the complementarity and fundamental differences between these two modes of dissipative self-assembly, our analysis reveals that multiple analogies exist between chemically and light-fueled systems. We hope that these considerations will facilitate further development of the field of dissipative self-assembly.","lang":"eng"}],"oa":1,"publisher":"Elsevier","author":[{"first_name":"Maren","full_name":"Weißenfels, Maren","last_name":"Weißenfels"},{"last_name":"Gemen","full_name":"Gemen, Julius","first_name":"Julius"},{"last_name":"Klajn","first_name":"Rafal","full_name":"Klajn, Rafal","id":"8e84690e-1e48-11ed-a02b-a1e6fb8bb53b"}],"issue":"1","intvolume":"         7","language":[{"iso":"eng"}],"quality_controlled":"1","citation":{"ista":"Weißenfels M, Gemen J, Klajn R. 2021. Dissipative self-assembly: Fueling with chemicals versus light. Chem. 7(1), 23–37.","apa":"Weißenfels, M., Gemen, J., &#38; Klajn, R. (2021). Dissipative self-assembly: Fueling with chemicals versus light. <i>Chem</i>. Elsevier. <a href=\"https://doi.org/10.1016/j.chempr.2020.11.025\">https://doi.org/10.1016/j.chempr.2020.11.025</a>","ama":"Weißenfels M, Gemen J, Klajn R. Dissipative self-assembly: Fueling with chemicals versus light. <i>Chem</i>. 2021;7(1):23-37. doi:<a href=\"https://doi.org/10.1016/j.chempr.2020.11.025\">10.1016/j.chempr.2020.11.025</a>","ieee":"M. Weißenfels, J. Gemen, and R. Klajn, “Dissipative self-assembly: Fueling with chemicals versus light,” <i>Chem</i>, vol. 7, no. 1. Elsevier, pp. 23–37, 2021.","mla":"Weißenfels, Maren, et al. “Dissipative Self-Assembly: Fueling with Chemicals versus Light.” <i>Chem</i>, vol. 7, no. 1, Elsevier, 2021, pp. 23–37, doi:<a href=\"https://doi.org/10.1016/j.chempr.2020.11.025\">10.1016/j.chempr.2020.11.025</a>.","short":"M. Weißenfels, J. Gemen, R. Klajn, Chem 7 (2021) 23–37.","chicago":"Weißenfels, Maren, Julius Gemen, and Rafal Klajn. “Dissipative Self-Assembly: Fueling with Chemicals versus Light.” <i>Chem</i>. Elsevier, 2021. <a href=\"https://doi.org/10.1016/j.chempr.2020.11.025\">https://doi.org/10.1016/j.chempr.2020.11.025</a>."},"publication_status":"published","extern":"1","status":"public","year":"2021","date_published":"2021-01-14T00:00:00Z"},{"author":[{"last_name":"Bian","full_name":"Bian, Tong","first_name":"Tong"},{"first_name":"Zonglin","full_name":"Chu, Zonglin","last_name":"Chu"},{"id":"8e84690e-1e48-11ed-a02b-a1e6fb8bb53b","full_name":"Klajn, Rafal","first_name":"Rafal","last_name":"Klajn"}],"publication_status":"published","extern":"1","status":"public","_id":"13360","date_published":"2021-04-19T00:00:00Z","year":"2021","citation":{"chicago":"Bian, Tong, Zonglin Chu, and Rafal Klajn. “Controlling Self‐Assembly of Nanoparticles Using Light.” In <i>Out‐of‐Equilibrium (Supra)Molecular Systems and Materials</i>, edited by Nicolas Giuseppone and Andreas Walther, 241–73. Wiley, 2021. <a href=\"https://doi.org/10.1002/9783527821990.ch9\">https://doi.org/10.1002/9783527821990.ch9</a>.","short":"T. Bian, Z. Chu, R. Klajn, in:, N. Giuseppone, A. Walther (Eds.), Out‐of‐Equilibrium (Supra)Molecular Systems and Materials, Wiley, 2021, pp. 241–273.","mla":"Bian, Tong, et al. “Controlling Self‐Assembly of Nanoparticles Using Light.” <i>Out‐of‐Equilibrium (Supra)Molecular Systems and Materials</i>, edited by Nicolas Giuseppone and Andreas Walther, Wiley, 2021, pp. 241–73, doi:<a href=\"https://doi.org/10.1002/9783527821990.ch9\">10.1002/9783527821990.ch9</a>.","apa":"Bian, T., Chu, Z., &#38; Klajn, R. (2021). Controlling Self‐Assembly of Nanoparticles Using Light. In N. Giuseppone &#38; A. Walther (Eds.), <i>Out‐of‐Equilibrium (Supra)molecular Systems and Materials</i> (pp. 241–273). Wiley. <a href=\"https://doi.org/10.1002/9783527821990.ch9\">https://doi.org/10.1002/9783527821990.ch9</a>","ieee":"T. Bian, Z. Chu, and R. Klajn, “Controlling Self‐Assembly of Nanoparticles Using Light,” in <i>Out‐of‐Equilibrium (Supra)molecular Systems and Materials</i>, N. Giuseppone and A. Walther, Eds. Wiley, 2021, pp. 241–273.","ama":"Bian T, Chu Z, Klajn R. Controlling Self‐Assembly of Nanoparticles Using Light. In: Giuseppone N, Walther A, eds. <i>Out‐of‐Equilibrium (Supra)Molecular Systems and Materials</i>. Wiley; 2021:241-273. doi:<a href=\"https://doi.org/10.1002/9783527821990.ch9\">10.1002/9783527821990.ch9</a>","ista":"Bian T, Chu Z, Klajn R. 2021.Controlling Self‐Assembly of Nanoparticles Using Light. In: Out‐of‐Equilibrium (Supra)molecular Systems and Materials. , 241–273."},"publication_identifier":{"eisbn":["9783527821990"],"isbn":["9783527346158"]},"quality_controlled":"1","language":[{"iso":"eng"}],"doi":"10.1002/9783527821990.ch9","day":"19","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_updated":"2024-10-14T12:09:48Z","oa_version":"None","date_created":"2023-08-01T09:35:35Z","month":"04","publication":"Out‐of‐Equilibrium (Supra)molecular Systems and Materials","type":"book_chapter","title":"Controlling Self‐Assembly of Nanoparticles Using Light","article_processing_charge":"No","editor":[{"last_name":"Giuseppone","full_name":"Giuseppone, Nicolas","first_name":"Nicolas"},{"first_name":"Andreas","full_name":"Walther, Andreas","last_name":"Walther"}],"publisher":"Wiley","scopus_import":"1","page":"241-273","abstract":[{"lang":"eng","text":"Inorganic nanoparticles (NPs) exhibit a wide range of fascinating physicochemical properties, many of which can be controlled by modulating the NP–NP coupling. Controlling the self-assembly of NPs using light has traditionally been achieved by functionalizing their surfaces with monolayers of photoswitchable molecules, which can be reversibly isomerized between two or more states upon exposure to different wavelengths of light. NPs whose assembly can be controlled by light in a reversible fashion can find interesting applications. The chapter deals with systems comprising mixtures of non-photoswitchable NPs and small-molecule photoacids and photobases. Examples of light-controlled self-assembly of NPs hitherto reported have been categorized into six distinct approaches. These are: functionalizing NPs with monolayers of photoswitchable molecules, light-controlled adsorption/desorption of photoswitchable molecules onto NPs, and light-induced electron transfer between the particle's inorganic core and the NP-bound ligands."}]},{"author":[{"last_name":"Renzo","full_name":"Renzo, M.","first_name":"M."},{"first_name":"Ylva Louise Linsdotter","full_name":"Götberg, Ylva Louise Linsdotter","orcid":"0000-0002-6960-6911","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","last_name":"Götberg"}],"issue":"2","intvolume":"       923","citation":{"chicago":"Renzo, M., and Ylva Louise Linsdotter Götberg. “Evolution of Accretor Stars in Massive Binaries: Broader Implications from Modeling ζ Ophiuchi.” <i>The Astrophysical Journal</i>. American Astronomical Society, 2021. <a href=\"https://doi.org/10.3847/1538-4357/ac29c5\">https://doi.org/10.3847/1538-4357/ac29c5</a>.","short":"M. Renzo, Y.L.L. Götberg, The Astrophysical Journal 923 (2021).","mla":"Renzo, M., and Ylva Louise Linsdotter Götberg. “Evolution of Accretor Stars in Massive Binaries: Broader Implications from Modeling ζ Ophiuchi.” <i>The Astrophysical Journal</i>, vol. 923, no. 2, 277, American Astronomical Society, 2021, doi:<a href=\"https://doi.org/10.3847/1538-4357/ac29c5\">10.3847/1538-4357/ac29c5</a>.","ieee":"M. Renzo and Y. L. L. Götberg, “Evolution of accretor stars in massive binaries: Broader implications from modeling ζ Ophiuchi,” <i>The Astrophysical Journal</i>, vol. 923, no. 2. American Astronomical Society, 2021.","apa":"Renzo, M., &#38; Götberg, Y. L. L. (2021). Evolution of accretor stars in massive binaries: Broader implications from modeling ζ Ophiuchi. <i>The Astrophysical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/1538-4357/ac29c5\">https://doi.org/10.3847/1538-4357/ac29c5</a>","ama":"Renzo M, Götberg YLL. Evolution of accretor stars in massive binaries: Broader implications from modeling ζ Ophiuchi. <i>The Astrophysical Journal</i>. 2021;923(2). doi:<a href=\"https://doi.org/10.3847/1538-4357/ac29c5\">10.3847/1538-4357/ac29c5</a>","ista":"Renzo M, Götberg YLL. 2021. Evolution of accretor stars in massive binaries: Broader implications from modeling ζ Ophiuchi. The Astrophysical Journal. 923(2), 277."},"publication_status":"published","extern":"1","status":"public","year":"2021","date_published":"2021-12-29T00:00:00Z","language":[{"iso":"eng"}],"external_id":{"arxiv":["2107.10933"]},"quality_controlled":"1","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/2107.10933"}],"arxiv":1,"date_updated":"2023-08-21T11:59:34Z","publication":"The Astrophysical Journal","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"title":"Evolution of accretor stars in massive binaries: Broader implications from modeling ζ Ophiuchi","date_created":"2023-08-03T10:10:48Z","publisher":"American Astronomical Society","abstract":[{"text":"Most massive stars are born in binaries close enough for mass transfer episodes. These modify the appearance, structure, and future evolution of both stars. We compute the evolution of a 100-day-period binary, consisting initially of a 25 M⊙ star and a 17 M⊙ star, which experiences stable mass transfer. We focus on the impact of mass accretion on the surface composition, internal rotation, and structure of the accretor. To anchor our models, we show that our accretor broadly reproduces the properties of ζ Ophiuchi, which has long been proposed to have accreted mass before being ejected as a runaway star when the companion exploded. We compare our accretor to models of single rotating stars and find that the later and stronger spin-up provided by mass accretion produces significant differences. Specifically, the core of the accretor retains higher spin at the end of the main sequence, and a convective layer develops that changes its density profile. Moreover, the surface of the accretor star is polluted by CNO-processed material donated by the companion. Our models show effects of mass accretion in binaries that are not captured in single rotating stellar models. This possibly impacts the further evolution (either in a binary or as single stars), the final collapse, and the resulting spin of the compact object.","lang":"eng"}],"oa":1,"article_number":"277","article_type":"original","volume":923,"_id":"13453","doi":"10.3847/1538-4357/ac29c5","day":"29","publication_identifier":{"issn":["0004-637X"],"eissn":["1538-4357"]},"month":"12","type":"journal_article","oa_version":"Preprint","article_processing_charge":"No","scopus_import":"1"},{"issue":"2","intvolume":"       922","author":[{"first_name":"Tin Long Sunny","full_name":"Wong, Tin Long Sunny","last_name":"Wong"},{"first_name":"Josiah","full_name":"Schwab, Josiah","last_name":"Schwab"},{"last_name":"Götberg","first_name":"Ylva Louise Linsdotter","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","orcid":"0000-0002-6960-6911","full_name":"Götberg, Ylva Louise Linsdotter"}],"status":"public","extern":"1","publication_status":"published","date_published":"2021-12-03T00:00:00Z","year":"2021","citation":{"chicago":"Wong, Tin Long Sunny, Josiah Schwab, and Ylva Louise Linsdotter Götberg. “Pre-Explosion Properties of Helium Star Donors to Thermonuclear Supernovae.” <i>The Astrophysical Journal</i>. American Astronomical Society, 2021. <a href=\"https://doi.org/10.3847/1538-4357/ac27ae\">https://doi.org/10.3847/1538-4357/ac27ae</a>.","short":"T.L.S. Wong, J. Schwab, Y.L.L. Götberg, The Astrophysical Journal 922 (2021).","mla":"Wong, Tin Long Sunny, et al. “Pre-Explosion Properties of Helium Star Donors to Thermonuclear Supernovae.” <i>The Astrophysical Journal</i>, vol. 922, no. 2, 241, American Astronomical Society, 2021, doi:<a href=\"https://doi.org/10.3847/1538-4357/ac27ae\">10.3847/1538-4357/ac27ae</a>.","ama":"Wong TLS, Schwab J, Götberg YLL. Pre-explosion properties of Helium star donors to thermonuclear supernovae. <i>The Astrophysical Journal</i>. 2021;922(2). doi:<a href=\"https://doi.org/10.3847/1538-4357/ac27ae\">10.3847/1538-4357/ac27ae</a>","ieee":"T. L. S. Wong, J. Schwab, and Y. L. L. Götberg, “Pre-explosion properties of Helium star donors to thermonuclear supernovae,” <i>The Astrophysical Journal</i>, vol. 922, no. 2. American Astronomical Society, 2021.","apa":"Wong, T. L. S., Schwab, J., &#38; Götberg, Y. L. L. (2021). Pre-explosion properties of Helium star donors to thermonuclear supernovae. <i>The Astrophysical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/1538-4357/ac27ae\">https://doi.org/10.3847/1538-4357/ac27ae</a>","ista":"Wong TLS, Schwab J, Götberg YLL. 2021. Pre-explosion properties of Helium star donors to thermonuclear supernovae. The Astrophysical Journal. 922(2), 241."},"quality_controlled":"1","external_id":{"arxiv":["2109.14817"]},"language":[{"iso":"eng"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_updated":"2023-08-21T11:52:05Z","main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/2109.14817"}],"arxiv":1,"date_created":"2023-08-03T10:10:58Z","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"publication":"The Astrophysical Journal","title":"Pre-explosion properties of Helium star donors to thermonuclear supernovae","publisher":"American Astronomical Society","oa":1,"abstract":[{"lang":"eng","text":"Helium star–carbon-oxygen white dwarf (CO WD) binaries are potential single-degenerate progenitor systems of thermonuclear supernovae. Revisiting a set of binary evolution calculations using the stellar evolution code MESA, we refine our previous predictions about which systems can lead to a thermonuclear supernova and then characterize the properties of the helium star donor at the time of explosion. We convert these model properties to near-UV/optical magnitudes assuming a blackbody spectrum and support this approach using a matched stellar atmosphere model. These models will be valuable to compare with pre-explosion imaging for future supernovae, though we emphasize the observational difficulty of detecting extremely blue companions. The pre-explosion source detected in association with SN 2012Z has been interpreted as a helium star binary containing an initially ultra-massive WD in a multiday orbit. However, extending our binary models to initial CO WD masses of up to 1.2 M⊙, we find that these systems undergo off-center carbon ignitions and thus are not expected to produce thermonuclear supernovae. This tension suggests that, if SN 2012Z is associated with a helium star–WD binary, then the pre-explosion optical light from the system must be significantly modified by the binary environment and/or the WD does not have a carbon-rich interior composition."}],"article_number":"241","article_type":"original","volume":922,"_id":"13454","publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"day":"03","doi":"10.3847/1538-4357/ac27ae","oa_version":"Preprint","month":"12","type":"journal_article","article_processing_charge":"No","scopus_import":"1"},{"title":"Different to the core: The pre-supernova structures of massive single and binary-stripped stars","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"publication":"Astronomy & Astrophysics","date_created":"2023-08-03T10:11:09Z","arxiv":1,"main_file_link":[{"open_access":"1","url":"https://doi.org/10.1051/0004-6361/202140506"}],"date_updated":"2025-01-14T14:11:32Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","abstract":[{"lang":"eng","text":"The majority of massive stars live in binary or multiple systems and will interact with a companion during their lifetimes, which helps to explain the observed diversity of core-collapse supernovae. Donor stars in binary systems can lose most of their hydrogen-rich envelopes through mass transfer. As a result, not only are the surface properties affected, but so is the core structure. However, most calculations of the core-collapse properties of massive stars rely on single-star models. We present a systematic study of the difference between the pre-supernova structures of single stars and stars of the same initial mass (11–21 M⊙) that have been stripped due to stable post-main-sequence mass transfer at solar metallicity. We present the pre-supernova core composition with novel diagrams that give an intuitive representation of the isotope distribution. As shown in previous studies, at the edge of the carbon-oxygen core, the binary-stripped star models contain an extended gradient of carbon, oxygen, and neon. This layer remains until core collapse and is more extended in mass for higher initial stellar masses. It originates from the receding of the convective helium core during core helium burning in binary-stripped stars, which does not occur in single-star models. We find that this same evolutionary phase leads to systematic differences in the final density and nuclear energy generation profiles. Binary-stripped star models have systematically higher total masses of carbon at the moment of core collapse compared to single-star models, which likely results in systematically different supernova yields. In about half of our models, the silicon-burning and oxygen-rich layers merge after core silicon burning. We discuss the implications of our findings for the “explodability”, supernova observations, and nucleosynthesis of these stars. Our models are publicly available and can be readily used as input for detailed supernova simulations."}],"oa":1,"publisher":"EDP Sciences","author":[{"full_name":"Laplace, E.","first_name":"E.","last_name":"Laplace"},{"last_name":"Justham","first_name":"S.","full_name":"Justham, S."},{"last_name":"Renzo","first_name":"M.","full_name":"Renzo, M."},{"id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","full_name":"Götberg, Ylva Louise Linsdotter","orcid":"0000-0002-6960-6911","first_name":"Ylva Louise Linsdotter","last_name":"Götberg"},{"full_name":"Farmer, R.","first_name":"R.","last_name":"Farmer"},{"full_name":"Vartanyan, D.","first_name":"D.","last_name":"Vartanyan"},{"full_name":"de Mink, S. E.","first_name":"S. E.","last_name":"de Mink"}],"intvolume":"       656","language":[{"iso":"eng"}],"external_id":{"arxiv":["2102.05036"]},"quality_controlled":"1","citation":{"mla":"Laplace, E., et al. “Different to the Core: The Pre-Supernova Structures of Massive Single and Binary-Stripped Stars.” <i>Astronomy &#38; Astrophysics</i>, vol. 656, A58, EDP Sciences, 2021, doi:<a href=\"https://doi.org/10.1051/0004-6361/202140506\">10.1051/0004-6361/202140506</a>.","ieee":"E. Laplace <i>et al.</i>, “Different to the core: The pre-supernova structures of massive single and binary-stripped stars,” <i>Astronomy &#38; Astrophysics</i>, vol. 656. EDP Sciences, 2021.","ama":"Laplace E, Justham S, Renzo M, et al. Different to the core: The pre-supernova structures of massive single and binary-stripped stars. <i>Astronomy &#38; Astrophysics</i>. 2021;656. doi:<a href=\"https://doi.org/10.1051/0004-6361/202140506\">10.1051/0004-6361/202140506</a>","apa":"Laplace, E., Justham, S., Renzo, M., Götberg, Y. L. L., Farmer, R., Vartanyan, D., &#38; de Mink, S. E. (2021). Different to the core: The pre-supernova structures of massive single and binary-stripped stars. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a href=\"https://doi.org/10.1051/0004-6361/202140506\">https://doi.org/10.1051/0004-6361/202140506</a>","ista":"Laplace E, Justham S, Renzo M, Götberg YLL, Farmer R, Vartanyan D, de Mink SE. 2021. Different to the core: The pre-supernova structures of massive single and binary-stripped stars. Astronomy &#38; Astrophysics. 656, A58.","chicago":"Laplace, E., S. Justham, M. Renzo, Ylva Louise Linsdotter Götberg, R. Farmer, D. Vartanyan, and S. E. de Mink. “Different to the Core: The Pre-Supernova Structures of Massive Single and Binary-Stripped Stars.” <i>Astronomy &#38; Astrophysics</i>. EDP Sciences, 2021. <a href=\"https://doi.org/10.1051/0004-6361/202140506\">https://doi.org/10.1051/0004-6361/202140506</a>.","short":"E. Laplace, S. Justham, M. Renzo, Y.L.L. Götberg, R. Farmer, D. Vartanyan, S.E. de Mink, Astronomy &#38; Astrophysics 656 (2021)."},"year":"2021","date_published":"2021-12-02T00:00:00Z","extern":"1","status":"public","publication_status":"published","type":"journal_article","month":"12","oa_version":"Published Version","scopus_import":"1","article_processing_charge":"No","article_type":"original","article_number":"A58","day":"02","doi":"10.1051/0004-6361/202140506","publication_identifier":{"eissn":["1432-0746"],"issn":["0004-6361"]},"_id":"13455","volume":656},{"oa":1,"abstract":[{"text":"While most simulations of the epoch of reionization have focused on single-stellar populations in star-forming dwarf galaxies, products of binary evolution are expected to significantly contribute to emissions of hydrogen-ionizing photons. Among these products are stripped stars (or helium stars), which have their envelopes stripped from interactions with binary companions, leaving an exposed helium core. Previous work has suggested these stripped stars can dominate the Lyman Continuum (LyC) photon output of high-redshift, low-luminosity galaxies post-starburst. Other sources of hard radiation in the early universe include zero-metallicity Population iii stars, which may have similar spectral energy distribution (SED) properties to galaxies with radiation dominated by stripped-star emissions. Here, we use four metrics (the power-law exponent over wavelength intervals 240–500 Å, 600–900 Å, and 1200–2000 Å, and the ratio of total luminosity in FUV wavelengths to LyC wavelengths) to compare the SEDs of simulated galaxies with only single-stellar evolution, galaxies containing stripped stars, and galaxies containing Population iii stars, with four different initial mass functions (IMFs). We find that stripped stars significantly alter SEDs in the LyC range of galaxies at the epoch of reionization. SEDs in galaxies with stripped stars have lower power-law indices in the LyC range and lower FUV to LyC luminosity ratios. These differences in SEDs are present at all considered luminosities (${M}_{\\mathrm{UV}}\\gt -15$, AB system), and are most pronounced for lower-luminosity galaxies. Intrinsic SEDs as well as those with interstellar medium absorption of galaxies with stripped stars and Population iii stars are found to be distinct for all tested Population iii IMFs.","lang":"eng"}],"publisher":"American Astronomical Society","date_created":"2023-08-03T10:11:24Z","title":"Spectral signatures of population III and envelope-stripped stars in galaxies at the epoch of reionization","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"publication":"The Astrophysical Journal","arxiv":1,"date_updated":"2023-08-21T11:44:50Z","main_file_link":[{"url":"https://doi.org/10.3847/1538-4357/ac0af6","open_access":"1"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","quality_controlled":"1","language":[{"iso":"eng"}],"external_id":{"arxiv":["2102.08408"]},"date_published":"2021-08-27T00:00:00Z","year":"2021","status":"public","publication_status":"published","extern":"1","citation":{"chicago":"Berzin, Elizabeth, Amy Secunda, Renyue Cen, Alexander Menegas, and Ylva Louise Linsdotter Götberg. “Spectral Signatures of Population III and Envelope-Stripped Stars in Galaxies at the Epoch of Reionization.” <i>The Astrophysical Journal</i>. American Astronomical Society, 2021. <a href=\"https://doi.org/10.3847/1538-4357/ac0af6\">https://doi.org/10.3847/1538-4357/ac0af6</a>.","short":"E. Berzin, A. Secunda, R. Cen, A. Menegas, Y.L.L. Götberg, The Astrophysical Journal 918 (2021).","mla":"Berzin, Elizabeth, et al. “Spectral Signatures of Population III and Envelope-Stripped Stars in Galaxies at the Epoch of Reionization.” <i>The Astrophysical Journal</i>, vol. 918, no. 1, 5, American Astronomical Society, 2021, doi:<a href=\"https://doi.org/10.3847/1538-4357/ac0af6\">10.3847/1538-4357/ac0af6</a>.","ista":"Berzin E, Secunda A, Cen R, Menegas A, Götberg YLL. 2021. Spectral signatures of population III and envelope-stripped stars in galaxies at the epoch of reionization. The Astrophysical Journal. 918(1), 5.","apa":"Berzin, E., Secunda, A., Cen, R., Menegas, A., &#38; Götberg, Y. L. L. (2021). Spectral signatures of population III and envelope-stripped stars in galaxies at the epoch of reionization. <i>The Astrophysical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/1538-4357/ac0af6\">https://doi.org/10.3847/1538-4357/ac0af6</a>","ama":"Berzin E, Secunda A, Cen R, Menegas A, Götberg YLL. Spectral signatures of population III and envelope-stripped stars in galaxies at the epoch of reionization. <i>The Astrophysical Journal</i>. 2021;918(1). doi:<a href=\"https://doi.org/10.3847/1538-4357/ac0af6\">10.3847/1538-4357/ac0af6</a>","ieee":"E. Berzin, A. Secunda, R. Cen, A. Menegas, and Y. L. L. Götberg, “Spectral signatures of population III and envelope-stripped stars in galaxies at the epoch of reionization,” <i>The Astrophysical Journal</i>, vol. 918, no. 1. American Astronomical Society, 2021."},"intvolume":"       918","issue":"1","author":[{"last_name":"Berzin","full_name":"Berzin, Elizabeth","first_name":"Elizabeth"},{"first_name":"Amy","full_name":"Secunda, Amy","last_name":"Secunda"},{"first_name":"Renyue","full_name":"Cen, Renyue","last_name":"Cen"},{"last_name":"Menegas","first_name":"Alexander","full_name":"Menegas, Alexander"},{"last_name":"Götberg","first_name":"Ylva Louise Linsdotter","orcid":"0000-0002-6960-6911","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","full_name":"Götberg, Ylva Louise Linsdotter"}],"scopus_import":"1","article_processing_charge":"No","oa_version":"Published Version","type":"journal_article","month":"08","publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"doi":"10.3847/1538-4357/ac0af6","day":"27","_id":"13456","volume":918,"article_type":"original","article_number":"5"},{"date_published":"2021-08-12T00:00:00Z","year":"2021","publication_status":"published","extern":"1","status":"public","citation":{"chicago":"Bodensteiner, J., H. Sana, C. Wang, N. Langer, L. Mahy, G. Banyard, A. de Koter, et al. “The Young Massive SMC Cluster NGC 330 Seen by MUSE. II. Multiplicity Properties of the Massive-Star Population.” <i>Astronomy &#38; Astrophysics</i>. EDP Sciences, 2021. <a href=\"https://doi.org/10.1051/0004-6361/202140507\">https://doi.org/10.1051/0004-6361/202140507</a>.","short":"J. Bodensteiner, H. Sana, C. Wang, N. Langer, L. Mahy, G. Banyard, A. de Koter, S.E. de Mink, C.J. Evans, Y.L.L. Götberg, L.R. Patrick, F.R.N. Schneider, F. Tramper, Astronomy &#38; Astrophysics 652 (2021).","mla":"Bodensteiner, J., et al. “The Young Massive SMC Cluster NGC 330 Seen by MUSE. II. Multiplicity Properties of the Massive-Star Population.” <i>Astronomy &#38; Astrophysics</i>, vol. 652, A70, EDP Sciences, 2021, doi:<a href=\"https://doi.org/10.1051/0004-6361/202140507\">10.1051/0004-6361/202140507</a>.","ista":"Bodensteiner J, Sana H, Wang C, Langer N, Mahy L, Banyard G, de Koter A, de Mink SE, Evans CJ, Götberg YLL, Patrick LR, Schneider FRN, Tramper F. 2021. The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population. Astronomy &#38; Astrophysics. 652, A70.","apa":"Bodensteiner, J., Sana, H., Wang, C., Langer, N., Mahy, L., Banyard, G., … Tramper, F. (2021). The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a href=\"https://doi.org/10.1051/0004-6361/202140507\">https://doi.org/10.1051/0004-6361/202140507</a>","ieee":"J. Bodensteiner <i>et al.</i>, “The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population,” <i>Astronomy &#38; Astrophysics</i>, vol. 652. EDP Sciences, 2021.","ama":"Bodensteiner J, Sana H, Wang C, et al. The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population. <i>Astronomy &#38; Astrophysics</i>. 2021;652. doi:<a href=\"https://doi.org/10.1051/0004-6361/202140507\">10.1051/0004-6361/202140507</a>"},"quality_controlled":"1","language":[{"iso":"eng"}],"external_id":{"arxiv":["2104.13409"]},"intvolume":"       652","author":[{"first_name":"J.","full_name":"Bodensteiner, J.","last_name":"Bodensteiner"},{"last_name":"Sana","first_name":"H.","full_name":"Sana, H."},{"last_name":"Wang","full_name":"Wang, C.","first_name":"C."},{"first_name":"N.","full_name":"Langer, N.","last_name":"Langer"},{"full_name":"Mahy, L.","first_name":"L.","last_name":"Mahy"},{"last_name":"Banyard","full_name":"Banyard, G.","first_name":"G."},{"full_name":"de Koter, A.","first_name":"A.","last_name":"de Koter"},{"last_name":"de Mink","full_name":"de Mink, S. E.","first_name":"S. E."},{"last_name":"Evans","full_name":"Evans, C. J.","first_name":"C. J."},{"orcid":"0000-0002-6960-6911","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","full_name":"Götberg, Ylva Louise Linsdotter","first_name":"Ylva Louise Linsdotter","last_name":"Götberg"},{"first_name":"L. R.","full_name":"Patrick, L. R.","last_name":"Patrick"},{"last_name":"Schneider","full_name":"Schneider, F. R. N.","first_name":"F. R. N."},{"first_name":"F.","full_name":"Tramper, F.","last_name":"Tramper"}],"publisher":"EDP Sciences","oa":1,"abstract":[{"lang":"eng","text":"Context. Observations of massive stars in open clusters younger than ∼8 Myr have shown that a majority of them are in binary systems, most of which will interact during their life. While these can be used as a proxy of the initial multiplicity properties, studying populations of massive stars older than ∼20 Myr allows us to probe the outcome of these interactions after a significant number of systems have experienced mass and angular momentum transfer and may even have merged.\r\n\r\nAims. Using multi-epoch integral-field spectroscopy, we aim to investigate the multiplicity properties of the massive-star population in the dense core of the ∼40 Myr old cluster NGC 330 in the Small Magellanic Cloud in order to search for possible imprints of stellar evolution on the multiplicity properties.\r\n\r\nMethods. We obtained six epochs of VLT/MUSE observations operated in wide-field mode with the extended wavelength setup and supported by adaptive optics. We extracted spectra and measured radial velocities for stars brighter than mF814W = 19. We identified single-lined spectroscopic binaries through significant RV variability with a peak-to-peak amplitude larger than 20 km s−1. We also identified double-lined spectroscopic binaries, and quantified the observational biases for binary detection. In particular, we took into account that binary systems with similar line strengths are difficult to detect in our data set.\r\n\r\nResults. The observed spectroscopic binary fraction among stars brighter than mF814W = 19 (approximately 5.5 M⊙ on the main sequence) is fSBobs = 13.2 ± 2.0%. Considering period and mass ratio ranges from log(P) = 0.15−3.5 (about 1.4 to 3160 d), q = 0.1−1.0, and a representative set of orbital parameter distributions, we find a bias-corrected close binary fraction of fcl = 34−7+8%. This fraction seems to decline for the fainter stars, which indicates either that the close binary fraction drops in the B-type domain, or that the period distribution becomes more heavily weighted toward longer orbital periods. We further find that both fractions vary strongly in different regions of the color-magnitude diagram, which corresponds to different evolutionary stages. This probably reveals the imprint of the binary history of different groups of stars. In particular, we find that the observed spectroscopic binary fraction of Be stars (fSBobs = 2 ± 2%) is significantly lower than that of B-type stars (fSBobs = 9 ± 2%).\r\n\r\nConclusions. We provide the first homogeneous radial velocity study of a large sample of B-type stars at a low metallicity ([Fe/H] ≲ −1.0). The overall bias-corrected close binary fraction (log(P) < 3.5 d) of the B-star population in NGC 330 is lower than the fraction reported for younger Galactic and Large Magellanic Cloud clusters in previous works. More data are needed, however, to establish whether the observed differences are caused by an age or a metallicity effect."}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","arxiv":1,"date_updated":"2023-08-21T11:49:36Z","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1051/0004-6361/202140507"}],"date_created":"2023-08-03T10:11:34Z","title":"The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"publication":"Astronomy & Astrophysics","_id":"13457","volume":652,"publication_identifier":{"issn":["0004-6361"],"eissn":["1432-0746"]},"doi":"10.1051/0004-6361/202140507","day":"12","article_number":"A70","article_type":"original","article_processing_charge":"No","scopus_import":"1","oa_version":"Published Version","type":"journal_article","month":"08"},{"intvolume":"       916","issue":"1","author":[{"full_name":"Vartanyan, David","first_name":"David","last_name":"Vartanyan"},{"full_name":"Laplace, Eva","first_name":"Eva","last_name":"Laplace"},{"last_name":"Renzo","first_name":"Mathieu","full_name":"Renzo, Mathieu"},{"first_name":"Ylva Louise Linsdotter","full_name":"Götberg, Ylva Louise Linsdotter","orcid":"0000-0002-6960-6911","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","last_name":"Götberg"},{"last_name":"Burrows","full_name":"Burrows, Adam","first_name":"Adam"},{"full_name":"de Mink, Selma E.","first_name":"Selma E.","last_name":"de Mink"}],"year":"2021","date_published":"2021-07-23T00:00:00Z","status":"public","extern":"1","publication_status":"published","citation":{"chicago":"Vartanyan, David, Eva Laplace, Mathieu Renzo, Ylva Louise Linsdotter Götberg, Adam Burrows, and Selma E. de Mink. “Binary-Stripped Stars as Core-Collapse Supernovae Progenitors.” <i>The Astrophysical Journal Letters</i>. American Astronomical Society, 2021. <a href=\"https://doi.org/10.3847/2041-8213/ac0b42\">https://doi.org/10.3847/2041-8213/ac0b42</a>.","short":"D. Vartanyan, E. Laplace, M. Renzo, Y.L.L. Götberg, A. Burrows, S.E. de Mink, The Astrophysical Journal Letters 916 (2021).","mla":"Vartanyan, David, et al. “Binary-Stripped Stars as Core-Collapse Supernovae Progenitors.” <i>The Astrophysical Journal Letters</i>, vol. 916, no. 1, L5, American Astronomical Society, 2021, doi:<a href=\"https://doi.org/10.3847/2041-8213/ac0b42\">10.3847/2041-8213/ac0b42</a>.","ama":"Vartanyan D, Laplace E, Renzo M, Götberg YLL, Burrows A, de Mink SE. Binary-stripped stars as core-collapse supernovae progenitors. <i>The Astrophysical Journal Letters</i>. 2021;916(1). doi:<a href=\"https://doi.org/10.3847/2041-8213/ac0b42\">10.3847/2041-8213/ac0b42</a>","ieee":"D. Vartanyan, E. Laplace, M. Renzo, Y. L. L. Götberg, A. Burrows, and S. E. de Mink, “Binary-stripped stars as core-collapse supernovae progenitors,” <i>The Astrophysical Journal Letters</i>, vol. 916, no. 1. American Astronomical Society, 2021.","apa":"Vartanyan, D., Laplace, E., Renzo, M., Götberg, Y. L. L., Burrows, A., &#38; de Mink, S. E. (2021). Binary-stripped stars as core-collapse supernovae progenitors. <i>The Astrophysical Journal Letters</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/2041-8213/ac0b42\">https://doi.org/10.3847/2041-8213/ac0b42</a>","ista":"Vartanyan D, Laplace E, Renzo M, Götberg YLL, Burrows A, de Mink SE. 2021. Binary-stripped stars as core-collapse supernovae progenitors. The Astrophysical Journal Letters. 916(1), L5."},"quality_controlled":"1","language":[{"iso":"eng"}],"external_id":{"arxiv":["2104.03317"]},"main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/2104.03317"}],"date_updated":"2023-08-21T11:37:48Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","arxiv":1,"date_created":"2023-08-03T10:11:45Z","title":"Binary-stripped stars as core-collapse supernovae progenitors","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"publication":"The Astrophysical Journal Letters","publisher":"American Astronomical Society","oa":1,"abstract":[{"text":"Most massive stars experience binary interactions in their lifetimes that can alter both the surface and core structure of the stripped star with significant effects on their ultimate fate as core-collapse supernovae. However, core-collapse supernovae simulations to date have focused almost exclusively on the evolution of single stars. We present a systematic simulation study of single and binary-stripped stars with the same initial mass as candidates for core-collapse supernovae (11–21 M⊙). Generally, we find that binary-stripped stars core tend to have a smaller compactness parameter, with a more prominent, deeper silicon/oxygen interface, and explode preferentially to the corresponding single stars of the same initial mass. Such a dichotomy of behavior between these two modes of evolution would have important implications for supernovae statistics, including the final neutron star masses, explosion energies, and nucleosynthetic yields. Binary-stripped remnants are also well poised to populate the possible mass gap between the heaviest neutron stars and the lightest black holes. Our work presents an improvement along two fronts, as we self-consistently account for the pre-collapse stellar evolution and the subsequent explosion outcome. Even so, our results emphasize the need for more detailed stellar evolutionary models to capture the sensitive nature of explosion outcome.","lang":"eng"}],"article_number":"L5","article_type":"original","_id":"13458","volume":916,"publication_identifier":{"eissn":["2041-8213"],"issn":["2041-8205"]},"day":"23","doi":"10.3847/2041-8213/ac0b42","oa_version":"Preprint","type":"journal_article","month":"07","article_processing_charge":"No","scopus_import":"1"},{"oa_version":"Preprint","type":"journal_article","month":"05","scopus_import":"1","article_processing_charge":"No","article_type":"original","article_number":"248","publication_identifier":{"eissn":["1538-3881"],"issn":["0004-6256"]},"doi":"10.3847/1538-3881/abf144","day":"04","_id":"13459","volume":161,"date_created":"2023-08-03T10:11:57Z","title":"The detection and characterization of Be+sdO binaries from HST/STIS FUV spectroscopy","publication":"The Astronomical Journal","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"arxiv":1,"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_updated":"2023-08-21T11:35:50Z","main_file_link":[{"url":"https://arxiv.org/abs/2103.13642","open_access":"1"}],"oa":1,"abstract":[{"lang":"eng","text":"The B emission-line stars are rapid rotators that were probably spun up by mass and angular momentum accretion through mass transfer in an interacting binary. Mass transfer will strip the donor star of its envelope to create a small and hot subdwarf remnant. Here we report on Hubble Space Telescope/STIS far-ultraviolet spectroscopy of a sample of Be stars that reveals the presence of the hot sdO companion through the calculation of cross-correlation functions of the observed and model spectra. We clearly detect the spectral signature of the sdO star in 10 of the 13 stars in the sample, and the spectral signals indicate that the sdO stars are hot, relatively faint, and slowly rotating as predicted by models. A comparison of their temperatures and radii with evolutionary tracks indicates that the sdO stars occupy the relatively long-lived, He-core burning stage. Only 1 of the 10 detections was a known binary prior to this investigation, which emphasizes the difficulty of finding such Be+sdO binaries through optical spectroscopy. However, these results and others indicate that many Be stars probably host hot subdwarf companions."}],"publisher":"American Astronomical Society","intvolume":"       161","issue":"5","author":[{"first_name":"Luqian","full_name":"Wang, Luqian","last_name":"Wang"},{"last_name":"Gies","full_name":"Gies, Douglas R.","first_name":"Douglas R."},{"last_name":"Peters","first_name":"Geraldine J.","full_name":"Peters, Geraldine J."},{"first_name":"Ylva Louise Linsdotter","orcid":"0000-0002-6960-6911","full_name":"Götberg, Ylva Louise Linsdotter","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","last_name":"Götberg"},{"last_name":"Chojnowski","full_name":"Chojnowski, S. Drew","first_name":"S. Drew"},{"last_name":"Lester","full_name":"Lester, Kathryn V.","first_name":"Kathryn V."},{"full_name":"Howell, Steve B.","first_name":"Steve B.","last_name":"Howell"}],"quality_controlled":"1","language":[{"iso":"eng"}],"external_id":{"arxiv":["2103.13642"]},"date_published":"2021-05-04T00:00:00Z","year":"2021","publication_status":"published","extern":"1","status":"public","citation":{"mla":"Wang, Luqian, et al. “The Detection and Characterization of Be+sdO Binaries from HST/STIS FUV Spectroscopy.” <i>The Astronomical Journal</i>, vol. 161, no. 5, 248, American Astronomical Society, 2021, doi:<a href=\"https://doi.org/10.3847/1538-3881/abf144\">10.3847/1538-3881/abf144</a>.","ama":"Wang L, Gies DR, Peters GJ, et al. The detection and characterization of Be+sdO binaries from HST/STIS FUV spectroscopy. <i>The Astronomical Journal</i>. 2021;161(5). doi:<a href=\"https://doi.org/10.3847/1538-3881/abf144\">10.3847/1538-3881/abf144</a>","ieee":"L. Wang <i>et al.</i>, “The detection and characterization of Be+sdO binaries from HST/STIS FUV spectroscopy,” <i>The Astronomical Journal</i>, vol. 161, no. 5. American Astronomical Society, 2021.","apa":"Wang, L., Gies, D. R., Peters, G. J., Götberg, Y. L. L., Chojnowski, S. D., Lester, K. V., &#38; Howell, S. B. (2021). The detection and characterization of Be+sdO binaries from HST/STIS FUV spectroscopy. <i>The Astronomical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/1538-3881/abf144\">https://doi.org/10.3847/1538-3881/abf144</a>","ista":"Wang L, Gies DR, Peters GJ, Götberg YLL, Chojnowski SD, Lester KV, Howell SB. 2021. The detection and characterization of Be+sdO binaries from HST/STIS FUV spectroscopy. The Astronomical Journal. 161(5), 248.","chicago":"Wang, Luqian, Douglas R. Gies, Geraldine J. Peters, Ylva Louise Linsdotter Götberg, S. Drew Chojnowski, Kathryn V. Lester, and Steve B. Howell. “The Detection and Characterization of Be+sdO Binaries from HST/STIS FUV Spectroscopy.” <i>The Astronomical Journal</i>. American Astronomical Society, 2021. <a href=\"https://doi.org/10.3847/1538-3881/abf144\">https://doi.org/10.3847/1538-3881/abf144</a>.","short":"L. Wang, D.R. Gies, G.J. Peters, Y.L.L. Götberg, S.D. Chojnowski, K.V. Lester, S.B. Howell, The Astronomical Journal 161 (2021)."}},{"issue":"49","intvolume":"         7","author":[{"last_name":"Heck","full_name":"Heck, Saijoscha","first_name":"Saijoscha"},{"last_name":"Baykusheva","first_name":"Denitsa Rangelova","full_name":"Baykusheva, Denitsa Rangelova","id":"71b4d059-2a03-11ee-914d-dfa3beed6530"},{"last_name":"Han","full_name":"Han, Meng","first_name":"Meng"},{"first_name":"Jia-Bao","full_name":"Ji, Jia-Bao","last_name":"Ji"},{"last_name":"Perry","first_name":"Conaill","full_name":"Perry, Conaill"},{"first_name":"Xiaochun","full_name":"Gong, Xiaochun","last_name":"Gong"},{"last_name":"Wörner","full_name":"Wörner, Hans Jakob","first_name":"Hans Jakob"}],"publication_status":"published","extern":"1","status":"public","year":"2021","date_published":"2021-12-03T00:00:00Z","citation":{"mla":"Heck, Saijoscha, et al. “Attosecond Interferometry of Shape Resonances in the Recoil Frame of CF4.” <i>Science Advances</i>, vol. 7, no. 49, abj8121, American Association for the Advancement of Science, 2021, doi:<a href=\"https://doi.org/10.1126/sciadv.abj8121\">10.1126/sciadv.abj8121</a>.","ista":"Heck S, Baykusheva DR, Han M, Ji J-B, Perry C, Gong X, Wörner HJ. 2021. Attosecond interferometry of shape resonances in the recoil frame of CF4. Science Advances. 7(49), abj8121.","ama":"Heck S, Baykusheva DR, Han M, et al. Attosecond interferometry of shape resonances in the recoil frame of CF4. <i>Science Advances</i>. 2021;7(49). doi:<a href=\"https://doi.org/10.1126/sciadv.abj8121\">10.1126/sciadv.abj8121</a>","apa":"Heck, S., Baykusheva, D. R., Han, M., Ji, J.-B., Perry, C., Gong, X., &#38; Wörner, H. J. (2021). Attosecond interferometry of shape resonances in the recoil frame of CF4. <i>Science Advances</i>. American Association for the Advancement of Science. <a href=\"https://doi.org/10.1126/sciadv.abj8121\">https://doi.org/10.1126/sciadv.abj8121</a>","ieee":"S. Heck <i>et al.</i>, “Attosecond interferometry of shape resonances in the recoil frame of CF4,” <i>Science Advances</i>, vol. 7, no. 49. American Association for the Advancement of Science, 2021.","chicago":"Heck, Saijoscha, Denitsa Rangelova Baykusheva, Meng Han, Jia-Bao Ji, Conaill Perry, Xiaochun Gong, and Hans Jakob Wörner. “Attosecond Interferometry of Shape Resonances in the Recoil Frame of CF4.” <i>Science Advances</i>. American Association for the Advancement of Science, 2021. <a href=\"https://doi.org/10.1126/sciadv.abj8121\">https://doi.org/10.1126/sciadv.abj8121</a>.","short":"S. Heck, D.R. Baykusheva, M. Han, J.-B. Ji, C. Perry, X. Gong, H.J. Wörner, Science Advances 7 (2021)."},"quality_controlled":"1","external_id":{"pmid":["34860540"]},"language":[{"iso":"eng"}],"main_file_link":[{"url":"https://doi.org/10.1126/sciadv.abj8121","open_access":"1"}],"date_updated":"2024-10-14T12:23:37Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","pmid":1,"date_created":"2023-08-09T13:09:02Z","publication":"Science Advances","keyword":["Multidisciplinary"],"title":"Attosecond interferometry of shape resonances in the recoil frame of CF4","publisher":"American Association for the Advancement of Science","oa":1,"abstract":[{"lang":"eng","text":"Shape resonances play a central role in many areas of science, but the real-time measurement of the associated many-body dynamics remains challenging. Here, we present measurements of recoil frame angle-resolved photoionization delays in the vicinity of shape resonances of CF4. This technique provides insights into the spatiotemporal photoionization dynamics of molecular shape resonances. We find delays of up to ∼600 as in the ionization out of the highest occupied molecular orbital (HOMO) with a strong dependence on the emission direction and a pronounced asymmetry along the dissociation axis. Comparison with quantum-scattering calculations traces the asymmetries to the interference of a small subset of partial waves at low kinetic energies and, additionally, to the interference of two overlapping shape resonances in the HOMO-1 channel. Our experimental and theoretical results establish a broadly applicable approach to space- and time-resolved photoionization dynamics in the molecular frame."}],"article_number":"abj8121","article_type":"original","volume":7,"_id":"13995","publication_identifier":{"eissn":["2375-2548"]},"doi":"10.1126/sciadv.abj8121","day":"03","oa_version":"Published Version","month":"12","type":"journal_article","article_processing_charge":"No","scopus_import":"1"}]