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506 Publications


2023 | Thesis | IST-REx-ID: 12491 | OA
Ultrastructural characterization of natively preserved extracellular matrix by cryo-electron tomography
B. Zens, Ultrastructural Characterization of Natively Preserved Extracellular Matrix by Cryo-Electron Tomography, Institute of Science and Technology Austria, 2023.
[Published Version] View | Files available | DOI
 

2023 | Thesis | IST-REx-ID: 12809 | OA
Plasticity in the cerebellum: What molecular mechanisms are behind physiological learning
C. Alcarva, Plasticity in the Cerebellum: What Molecular Mechanisms Are behind Physiological Learning, Institute of Science and Technology Austria, 2023.
[Published Version] View | Files available | DOI
 

2022 | Journal Article | IST-REx-ID: 10758 | OA
1H NMR chemical exchange techniques reveal local and global effects of oxidized cytosine derivatives
R.C.A. Dubini, E. Korytiaková, T. Schinkel, P. Heinrichs, T. Carell, P. Rovo, ACS Physical Chemistry Au 2 (2022) 237–246.
[Published Version] View | Files available | DOI | PubMed | Europe PMC
 

2022 | Journal Article | IST-REx-ID: 11490 | OA
Deciphering stellar metallicities in the early universe: Case study of a young galaxy at z = 4.77 in the MUSE eXtremely Deep Field
J.J. Matthee, A. Feltre, M. Maseda, T. Nanayakkara, L. Boogaard, R. Bacon, A. Verhamme, F. Leclercq, H. Kusakabe, T. Urrutia, L. Wisotzki, Astronomy & Astrophysics 660 (2022).
[Published Version] View | DOI | Download Published Version (ext.) | arXiv
 

2022 | Journal Article | IST-REx-ID: 11509 | OA
EMPRESS. IV. Extremely metal-poor galaxies including very low-mass primordial systems with M∗= 10⁴-10⁵⊙ and 2%–3% (O/H): High (Fe/O) suggestive of metal enrichment by hypernovae/pair-instability supernovae
Isobe Y, Ouchi M, Suzuki A, Moriya TJ, Nakajima K, Nomoto K, Rauch M, Harikane Y, Kojima T, Ono Y, Fujimoto S, Inoue AK, Kim JH, Komiyama Y, Kusakabe H, Lee C-H, Maseda M, Matthee JJ, Michel-Dansac L, Nagao T, Nanayakkara T, Nishigaki M, Onodera M, Sugahara Y, Xu Y. 2022. EMPRESS. IV. Extremely metal-poor galaxies including very low-mass primordial systems with M∗= 104-105⊙ and 2%–3% (O/H): High (Fe/O) suggestive of metal enrichment by hypernovae/pair-instability supernovae. The Astrophysical Journal. 925(2), 111.
[Published Version] View | DOI | Download Published Version (ext.) | arXiv
 

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