[{"month":"01","year":"2013","publication_status":"published","quality_controlled":0,"day":"08","type":"journal_article","abstract":[{"text":"Despite the pivotal functions of the NMDA receptor (NMDAR) for neural circuit development and synaptic plasticity, the molecular mechanisms underlying the dynamics of NMDAR trafficking are poorly understood. The cell adhesion molecule neuroligin-1 (NL1) modifies NMDAR-dependent synaptic transmission and synaptic plasticity, but it is unclear whether NL1 controls synaptic accumulation or function of the receptors. Here, we provide evidence that NL1 regulates the abundance of NMDARs at postsynaptic sites. This function relies on extracellular, NL1 isoform-specific sequences that facilitate biochemical interactions between NL1 and the NMDAR GluN1 subunit. Our work uncovers NL1 isoform-specific cisinteractions with ionotropic glutamate receptors as a key mechanism for controlling synaptic properties.","lang":"eng"}],"issue":"2","extern":1,"date_created":"2018-12-11T11:57:54Z","status":"public","title":"Neuroligin-1 controls synaptic abundance of NMDA-type glutamate receptors through extracellular coupling","citation":{"ama":"Budreck E, Kwon O, Jung J, et al. Neuroligin-1 controls synaptic abundance of NMDA-type glutamate receptors through extracellular coupling. <i>PNAS</i>. 2013;110(2):725-730. doi:<a href=\"https://doi.org/10.1073/pnas.1214718110\">10.1073/pnas.1214718110</a>","ista":"Budreck E, Kwon O, Jung J, Baudouin S, Thommen A, Kim H, Fukazawa Y, Harada H, Tabuchi K, Shigemoto R, Scheiffele P, Kim J. 2013. Neuroligin-1 controls synaptic abundance of NMDA-type glutamate receptors through extracellular coupling. PNAS. 110(2), 725–730.","short":"E. Budreck, O. Kwon, J. Jung, S. Baudouin, A. Thommen, H. Kim, Y. Fukazawa, H. Harada, K. Tabuchi, R. Shigemoto, P. Scheiffele, J. Kim, PNAS 110 (2013) 725–730.","ieee":"E. Budreck <i>et al.</i>, “Neuroligin-1 controls synaptic abundance of NMDA-type glutamate receptors through extracellular coupling,” <i>PNAS</i>, vol. 110, no. 2. National Academy of Sciences, pp. 725–730, 2013.","apa":"Budreck, E., Kwon, O., Jung, J., Baudouin, S., Thommen, A., Kim, H., … Kim, J. (2013). Neuroligin-1 controls synaptic abundance of NMDA-type glutamate receptors through extracellular coupling. <i>PNAS</i>. National Academy of Sciences. <a href=\"https://doi.org/10.1073/pnas.1214718110\">https://doi.org/10.1073/pnas.1214718110</a>","chicago":"Budreck, Elaine, Oh Kwon, Jung Jung, Stéphane Baudouin, Albert Thommen, Hye Kim, Yugo Fukazawa, et al. “Neuroligin-1 Controls Synaptic Abundance of NMDA-Type Glutamate Receptors through Extracellular Coupling.” <i>PNAS</i>. National Academy of Sciences, 2013. <a href=\"https://doi.org/10.1073/pnas.1214718110\">https://doi.org/10.1073/pnas.1214718110</a>.","mla":"Budreck, Elaine, et al. “Neuroligin-1 Controls Synaptic Abundance of NMDA-Type Glutamate Receptors through Extracellular Coupling.” <i>PNAS</i>, vol. 110, no. 2, National Academy of Sciences, 2013, pp. 725–30, doi:<a href=\"https://doi.org/10.1073/pnas.1214718110\">10.1073/pnas.1214718110</a>."},"doi":"10.1073/pnas.1214718110","_id":"2478","publication":"PNAS","date_updated":"2021-01-12T06:57:43Z","volume":110,"publist_id":"4423","publisher":"National Academy of Sciences","page":"725 - 730","author":[{"full_name":"Budreck, Elaine C","first_name":"Elaine","last_name":"Budreck"},{"last_name":"Kwon","first_name":"Oh","full_name":"Kwon, Oh-Bin"},{"last_name":"Jung","full_name":"Jung, Jung-Hoon","first_name":"Jung"},{"last_name":"Baudouin","first_name":"Stéphane","full_name":"Baudouin, Stéphane J"},{"last_name":"Thommen","full_name":"Thommen, Albert","first_name":"Albert"},{"full_name":"Kim, Hye-Sun","first_name":"Hye","last_name":"Kim"},{"last_name":"Fukazawa","full_name":"Fukazawa, Yugo","first_name":"Yugo"},{"id":"2E55CDF2-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-7429-7896","last_name":"Harada","full_name":"Harumi Harada","first_name":"Harumi"},{"last_name":"Tabuchi","first_name":"Katsuhiko","full_name":"Tabuchi, Katsuhiko"},{"full_name":"Ryuichi Shigemoto","first_name":"Ryuichi","id":"499F3ABC-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-8761-9444","last_name":"Shigemoto"},{"first_name":"Peter","full_name":"Scheiffele, Peter","last_name":"Scheiffele"},{"last_name":"Kim","first_name":"Joung","full_name":"Kim, Joung-Hun"}],"date_published":"2013-01-08T00:00:00Z","intvolume":"       110"},{"date_created":"2018-12-11T11:45:26Z","extern":1,"issue":"4","type":"journal_article","acknowledgement":"While working on this paper, the first author was supported by an IUF Junior and ANR while the second author was supported by ERC grant 306457.","abstract":[{"lang":"eng","text":"Châtelet surfaces provide a rich source of geometrically rational surfaces that do not always satisfy the Hasse principle. Restricting attention to a special class of Châtelet surfaces, we investigate the frequency that such counter-examples arise over the rational numbers."}],"quality_controlled":0,"day":"29","month":"11","year":"2013","publication_status":"published","main_file_link":[{"url":"https://arxiv.org/abs/1210.4010","open_access":"1"}],"intvolume":"       108","author":[{"last_name":"De La Bretèche","first_name":"Régis","full_name":"de la Bretèche, Régis"},{"orcid":"0000-0002-8314-0177","last_name":"Browning","id":"35827D50-F248-11E8-B48F-1D18A9856A87","first_name":"Timothy D","full_name":"Timothy Browning"}],"page":"1030 - 1078","date_published":"2013-11-29T00:00:00Z","publisher":"Oxford University Press","date_updated":"2021-01-12T06:57:51Z","volume":108,"oa":1,"publist_id":"7652","citation":{"short":"R. De La Bretèche, T.D. Browning, Proceedings of the London Mathematical Society 108 (2013) 1030–1078.","ieee":"R. De La Bretèche and T. D. Browning, “Density of Châtelet surfaces failing the Hasse principle,” <i>Proceedings of the London Mathematical Society</i>, vol. 108, no. 4. Oxford University Press, pp. 1030–1078, 2013.","ama":"De La Bretèche R, Browning TD. Density of Châtelet surfaces failing the Hasse principle. <i>Proceedings of the London Mathematical Society</i>. 2013;108(4):1030-1078. doi:<a href=\"https://doi.org/10.1112/plms/pdt060\">10.1112/plms/pdt060</a>","ista":"De La Bretèche R, Browning TD. 2013. Density of Châtelet surfaces failing the Hasse principle. Proceedings of the London Mathematical Society. 108(4), 1030–1078.","apa":"De La Bretèche, R., &#38; Browning, T. D. (2013). Density of Châtelet surfaces failing the Hasse principle. <i>Proceedings of the London Mathematical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1112/plms/pdt060\">https://doi.org/10.1112/plms/pdt060</a>","chicago":"De La Bretèche, Régis, and Timothy D Browning. “Density of Châtelet Surfaces Failing the Hasse Principle.” <i>Proceedings of the London Mathematical Society</i>. Oxford University Press, 2013. <a href=\"https://doi.org/10.1112/plms/pdt060\">https://doi.org/10.1112/plms/pdt060</a>.","mla":"De La Bretèche, Régis, and Timothy D. Browning. “Density of Châtelet Surfaces Failing the Hasse Principle.” <i>Proceedings of the London Mathematical Society</i>, vol. 108, no. 4, Oxford University Press, 2013, pp. 1030–78, doi:<a href=\"https://doi.org/10.1112/plms/pdt060\">10.1112/plms/pdt060</a>."},"doi":"10.1112/plms/pdt060","_id":"250","publication":"Proceedings of the London Mathematical Society","status":"public","title":"Density of Châtelet surfaces failing the Hasse principle"},{"title":"Counter examples to the Hasse principle among certain coflasque tori","status":"public","publication":"Journal de Theorie des Nombres de Bordeaux","_id":"251","doi":"10.5802/jtnb.857","citation":{"apa":"De La Bretèche, R., &#38; Browning, T. D. (2013). Counter examples to the Hasse principle among certain coflasque tori. <i>Journal de Theorie Des Nombres de Bordeaux</i>. Universite de Bordeaux I. <a href=\"https://doi.org/10.5802/jtnb.857\">https://doi.org/10.5802/jtnb.857</a>","chicago":"De La Bretèche, Régis, and Timothy D Browning. “Counter Examples to the Hasse Principle among Certain Coflasque Tori.” <i>Journal de Theorie Des Nombres de Bordeaux</i>. Universite de Bordeaux I, 2013. <a href=\"https://doi.org/10.5802/jtnb.857\">https://doi.org/10.5802/jtnb.857</a>.","mla":"De La Bretèche, Régis, and Timothy D. Browning. “Counter Examples to the Hasse Principle among Certain Coflasque Tori.” <i>Journal de Theorie Des Nombres de Bordeaux</i>, vol. 26, no. 1, Universite de Bordeaux I, 2013, pp. 25–44, doi:<a href=\"https://doi.org/10.5802/jtnb.857\">10.5802/jtnb.857</a>.","ama":"De La Bretèche R, Browning TD. Counter examples to the Hasse principle among certain coflasque tori. <i>Journal de Theorie des Nombres de Bordeaux</i>. 2013;26(1):25-44. doi:<a href=\"https://doi.org/10.5802/jtnb.857\">10.5802/jtnb.857</a>","ista":"De La Bretèche R, Browning TD. 2013. Counter examples to the Hasse principle among certain coflasque tori. Journal de Theorie des Nombres de Bordeaux. 26(1), 25–44.","short":"R. De La Bretèche, T.D. Browning, Journal de Theorie Des Nombres de Bordeaux 26 (2013) 25–44.","ieee":"R. De La Bretèche and T. D. Browning, “Counter examples to the Hasse principle among certain coflasque tori,” <i>Journal de Theorie des Nombres de Bordeaux</i>, vol. 26, no. 1. Universite de Bordeaux I, pp. 25–44, 2013."},"publisher":"Universite de Bordeaux I","publist_id":"7651","volume":26,"date_updated":"2021-01-12T06:57:55Z","intvolume":"        26","date_published":"2013-05-14T00:00:00Z","page":"25 - 44","author":[{"last_name":"De La Bretèche","full_name":"de la Bretèche, Régis","first_name":"Régis"},{"id":"35827D50-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-8314-0177","last_name":"Browning","full_name":"Timothy Browning","first_name":"Timothy D"}],"publication_status":"published","month":"05","year":"2013","abstract":[{"lang":"eng","text":"We study the density of varieties in a certain family which do not satisfy the Hasse principle. This work relies on results recently obtained by Colliot-Thélène [3]."}],"type":"journal_article","day":"14","quality_controlled":0,"extern":1,"issue":"1","date_created":"2018-12-11T11:45:26Z"},{"isi":1,"issue":"3","date_created":"2018-12-11T11:58:08Z","scopus_import":"1","_id":"2516","article_processing_charge":"No","language":[{"iso":"eng"}],"publisher":"IEEE","page":"453 - 465","author":[{"first_name":"Christoph","full_name":"Lampert, Christoph","last_name":"Lampert","orcid":"0000-0001-8622-7887","id":"40C20FD2-F248-11E8-B48F-1D18A9856A87"},{"first_name":"Hannes","full_name":"Nickisch, Hannes","last_name":"Nickisch"},{"last_name":"Harmeling","first_name":"Stefan","full_name":"Harmeling, Stefan"}],"date_published":"2013-07-30T00:00:00Z","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","year":"2013","month":"07","publication_status":"published","type":"journal_article","abstract":[{"lang":"eng","text":"We study the problem of object recognition for categories for which we have no training examples, a task also called zero-data or zero-shot learning. This situation has hardly been studied in computer vision research, even though it occurs frequently: the world contains tens of thousands of different object classes and for only few of them image collections have been formed and suitably annotated. To tackle the problem we introduce attribute-based classification: objects are identified based on a high-level description that is phrased in terms of semantic attributes, such as the object's color or shape. Because the identification of each such property transcends the specific learning task at hand, the attribute classifiers can be pre-learned independently, e.g. from existing image datasets unrelated to the current task. Afterwards, new classes can be detected based on their attribute representation, without the need for a new training phase. In this paper we also introduce a new dataset, Animals with Attributes, of over 30,000 images of 50 animal classes, annotated with 85 semantic attributes. Extensive experiments on this and two more datasets show that attribute-based classification indeed is able to categorize images without access to any training images of the target classes."}],"quality_controlled":"1","day":"30","oa_version":"None","status":"public","external_id":{"isi":["000331450100005"]},"title":"Attribute-based classification for zero-shot learning of object categories","department":[{"_id":"ChLa"}],"citation":{"short":"C. Lampert, H. Nickisch, S. Harmeling, IEEE Transactions on Pattern Analysis and Machine Intelligence 36 (2013) 453–465.","ieee":"C. Lampert, H. Nickisch, and S. Harmeling, “Attribute-based classification for zero-shot learning of object categories,” <i>IEEE Transactions on Pattern Analysis and Machine Intelligence</i>, vol. 36, no. 3. IEEE, pp. 453–465, 2013.","ama":"Lampert C, Nickisch H, Harmeling S. Attribute-based classification for zero-shot learning of object categories. <i>IEEE Transactions on Pattern Analysis and Machine Intelligence</i>. 2013;36(3):453-465. doi:<a href=\"https://doi.org/10.1109/TPAMI.2013.140\">10.1109/TPAMI.2013.140</a>","ista":"Lampert C, Nickisch H, Harmeling S. 2013. Attribute-based classification for zero-shot learning of object categories. IEEE Transactions on Pattern Analysis and Machine Intelligence. 36(3), 453–465.","apa":"Lampert, C., Nickisch, H., &#38; Harmeling, S. (2013). Attribute-based classification for zero-shot learning of object categories. <i>IEEE Transactions on Pattern Analysis and Machine Intelligence</i>. IEEE. <a href=\"https://doi.org/10.1109/TPAMI.2013.140\">https://doi.org/10.1109/TPAMI.2013.140</a>","chicago":"Lampert, Christoph, Hannes Nickisch, and Stefan Harmeling. “Attribute-Based Classification for Zero-Shot Learning of Object Categories.” <i>IEEE Transactions on Pattern Analysis and Machine Intelligence</i>. IEEE, 2013. <a href=\"https://doi.org/10.1109/TPAMI.2013.140\">https://doi.org/10.1109/TPAMI.2013.140</a>.","mla":"Lampert, Christoph, et al. “Attribute-Based Classification for Zero-Shot Learning of Object Categories.” <i>IEEE Transactions on Pattern Analysis and Machine Intelligence</i>, vol. 36, no. 3, IEEE, 2013, pp. 453–65, doi:<a href=\"https://doi.org/10.1109/TPAMI.2013.140\">10.1109/TPAMI.2013.140</a>."},"doi":"10.1109/TPAMI.2013.140","publication":"IEEE Transactions on Pattern Analysis and Machine Intelligence","date_updated":"2025-09-29T14:09:57Z","publist_id":"4385","volume":36,"intvolume":"        36"},{"oa_version":"Submitted Version","publication_status":"published","month":"07","year":"2013","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","day":"01","quality_controlled":"1","abstract":[{"text":"Traditional formal methods are based on a Boolean satisfaction notion: a reactive system satisfies, or not, a given specification. We generalize formal methods to also address the quality of systems. As an adequate specification formalism we introduce the linear temporal logic LTL[F]. The satisfaction value of an LTL[F] formula is a number between 0 and 1, describing the quality of the satisfaction. The logic generalizes traditional LTL by augmenting it with a (parameterized) set F of arbitrary functions over the interval [0,1]. For example, F may contain the maximum or minimum between the satisfaction values of subformulas, their product, and their average. The classical decision problems in formal methods, such as satisfiability, model checking, and synthesis, are generalized to search and optimization problems in the quantitative setting. For example, model checking asks for the quality in which a specification is satisfied, and synthesis returns a system satisfying the specification with the highest quality. Reasoning about quality gives rise to other natural questions, like the distance between specifications. We formalize these basic questions and study them for LTL[F]. By extending the automata-theoretic approach for LTL to a setting that takes quality into an account, we are able to solve the above problems and show that reasoning about LTL[F] has roughly the same complexity as reasoning about traditional LTL.","lang":"eng"}],"type":"conference","publist_id":"4384","oa":1,"volume":7966,"date_updated":"2020-08-11T10:09:47Z","file":[{"file_id":"7860","checksum":"85afbf6c18a2c7e377c52c9410e2d824","relation":"main_file","creator":"dernst","file_size":363031,"access_level":"open_access","content_type":"application/pdf","date_created":"2020-05-15T11:16:12Z","date_updated":"2020-07-14T12:45:42Z","file_name":"2013_ICALP_Almagor.pdf"}],"intvolume":"      7966","department":[{"_id":"ToHe"}],"title":"Formalizing and reasoning about quality","status":"public","ec_funded":1,"doi":"10.1007/978-3-642-39212-2_3","citation":{"mla":"Almagor, Shaull, et al. <i>Formalizing and Reasoning about Quality</i>. Vol. 7966, no. Part 2, Springer, 2013, pp. 15–27, doi:<a href=\"https://doi.org/10.1007/978-3-642-39212-2_3\">10.1007/978-3-642-39212-2_3</a>.","chicago":"Almagor, Shaull, Udi Boker, and Orna Kupferman. “Formalizing and Reasoning about Quality.” Lecture Notes in Computer Science. Springer, 2013. <a href=\"https://doi.org/10.1007/978-3-642-39212-2_3\">https://doi.org/10.1007/978-3-642-39212-2_3</a>.","apa":"Almagor, S., Boker, U., &#38; Kupferman, O. (2013). Formalizing and reasoning about quality. Presented at the ICALP: Automata, Languages and Programming, Riga, Latvia: Springer. <a href=\"https://doi.org/10.1007/978-3-642-39212-2_3\">https://doi.org/10.1007/978-3-642-39212-2_3</a>","ieee":"S. Almagor, U. Boker, and O. Kupferman, “Formalizing and reasoning about quality,” vol. 7966, no. Part 2. Springer, pp. 15–27, 2013.","short":"S. Almagor, U. Boker, O. Kupferman, 7966 (2013) 15–27.","ista":"Almagor S, Boker U, Kupferman O. 2013. Formalizing and reasoning about quality. 7966(Part 2), 15–27.","ama":"Almagor S, Boker U, Kupferman O. Formalizing and reasoning about quality. 2013;7966(Part 2):15-27. doi:<a href=\"https://doi.org/10.1007/978-3-642-39212-2_3\">10.1007/978-3-642-39212-2_3</a>"},"issue":"Part 2","ddc":["000"],"date_created":"2018-12-11T11:58:08Z","file_date_updated":"2020-07-14T12:45:42Z","acknowledgement":"ERC Grant QUALITY. ","series_title":"Lecture Notes in Computer Science","has_accepted_license":"1","publisher":"Springer","language":[{"iso":"eng"}],"article_processing_charge":"No","date_published":"2013-07-01T00:00:00Z","page":"15 - 27","conference":{"name":"ICALP: Automata, Languages and Programming","start_date":"2013-07-08","end_date":"2013-07-12","location":"Riga, Latvia"},"author":[{"full_name":"Almagor, Shaull","first_name":"Shaull","last_name":"Almagor"},{"full_name":"Boker, Udi","first_name":"Udi","id":"31E297B6-F248-11E8-B48F-1D18A9856A87","last_name":"Boker"},{"last_name":"Kupferman","first_name":"Orna","full_name":"Kupferman, Orna"}],"scopus_import":1,"alternative_title":["LNCS"],"project":[{"grant_number":"S 11407_N23","call_identifier":"FWF","name":"Rigorous Systems Engineering","_id":"25832EC2-B435-11E9-9278-68D0E5697425"},{"call_identifier":"FP7","name":"Quantitative Reactive Modeling","_id":"25EE3708-B435-11E9-9278-68D0E5697425","grant_number":"267989"}],"_id":"2517"},{"main_file_link":[{"open_access":"1","url":"http://arxiv.org/abs/1207.7213"}],"date_created":"2018-12-11T11:58:08Z","issue":"1","_id":"2518","alternative_title":["LNCS"],"scopus_import":1,"page":"625 - 636","author":[{"last_name":"Kolmogorov","id":"3D50B0BA-F248-11E8-B48F-1D18A9856A87","first_name":"Vladimir","full_name":"Kolmogorov, Vladimir"}],"conference":{"location":"Riga, Latvia","end_date":"2013-07-12","start_date":"2013-07-08","name":"ICALP: Automata, Languages and Programming"},"date_published":"2013-07-01T00:00:00Z","language":[{"iso":"eng"}],"publisher":"Springer","type":"conference","abstract":[{"text":"A class of valued constraint satisfaction problems (VCSPs) is characterised by a valued constraint language, a fixed set of cost functions on a finite domain. An instance of the problem is specified by a sum of cost functions from the language with the goal to minimise the sum. We study which classes of finite-valued languages can be solved exactly by the basic linear programming relaxation (BLP). Thapper and Živný showed [20] that if BLP solves the language then the language admits a binary commutative fractional polymorphism. We prove that the converse is also true. This leads to a necessary and a sufficient condition which can be checked in polynomial time for a given language. In contrast, the previous necessary and sufficient condition due to [20] involved infinitely many inequalities. More recently, Thapper and Živný [21] showed (using, in particular, a technique introduced in this paper) that core languages that do not satisfy our condition are NP-hard. Taken together, these results imply that a finite-valued language can either be solved using Linear Programming or is NP-hard.","lang":"eng"}],"related_material":{"record":[{"status":"public","relation":"later_version","id":"2271"}]},"corr_author":"1","quality_controlled":"1","day":"01","user_id":"3E5EF7F0-F248-11E8-B48F-1D18A9856A87","year":"2013","month":"07","publication_status":"published","arxiv":1,"oa_version":"Preprint","citation":{"apa":"Kolmogorov, V. (2013). The power of linear programming for finite-valued CSPs: A constructive characterization (Vol. 7965, pp. 625–636). Presented at the ICALP: Automata, Languages and Programming, Riga, Latvia: Springer. <a href=\"https://doi.org/10.1007/978-3-642-39206-1_53\">https://doi.org/10.1007/978-3-642-39206-1_53</a>","chicago":"Kolmogorov, Vladimir. “The Power of Linear Programming for Finite-Valued CSPs: A Constructive Characterization,” 7965:625–36. Springer, 2013. <a href=\"https://doi.org/10.1007/978-3-642-39206-1_53\">https://doi.org/10.1007/978-3-642-39206-1_53</a>.","mla":"Kolmogorov, Vladimir. <i>The Power of Linear Programming for Finite-Valued CSPs: A Constructive Characterization</i>. Vol. 7965, no. 1, Springer, 2013, pp. 625–36, doi:<a href=\"https://doi.org/10.1007/978-3-642-39206-1_53\">10.1007/978-3-642-39206-1_53</a>.","short":"V. Kolmogorov, in:, Springer, 2013, pp. 625–636.","ieee":"V. Kolmogorov, “The power of linear programming for finite-valued CSPs: A constructive characterization,” presented at the ICALP: Automata, Languages and Programming, Riga, Latvia, 2013, vol. 7965, no. 1, pp. 625–636.","ama":"Kolmogorov V. The power of linear programming for finite-valued CSPs: A constructive characterization. In: Vol 7965. Springer; 2013:625-636. doi:<a href=\"https://doi.org/10.1007/978-3-642-39206-1_53\">10.1007/978-3-642-39206-1_53</a>","ista":"Kolmogorov V. 2013. The power of linear programming for finite-valued CSPs: A constructive characterization. ICALP: Automata, Languages and Programming, LNCS, vol. 7965, 625–636."},"doi":"10.1007/978-3-642-39206-1_53","status":"public","title":"The power of linear programming for finite-valued CSPs: A constructive characterization","external_id":{"arxiv":["1207.7213"]},"department":[{"_id":"VlKo"}],"intvolume":"      7965","date_updated":"2025-09-23T14:14:56Z","oa":1,"volume":7965,"publist_id":"4383"},{"oa_version":"Submitted Version","type":"conference","abstract":[{"text":"We propose a probabilistic model to infer supervised latent variables in\r\nthe Hamming space from observed data. Our model allows simultaneous\r\ninference of the number of binary latent variables, and their values. The\r\nlatent variables preserve neighbourhood structure of the data in a sense\r\nthat objects in the same semantic concept have similar latent values, and\r\nobjects in different concepts have dissimilar latent values. We formulate\r\nthe supervised infinite latent variable problem based on an intuitive\r\nprinciple of pulling objects together if they are of the same type, and\r\npushing them apart if they are not. We then combine this principle with a\r\nflexible Indian Buffet Process prior on the latent variables. We show that\r\nthe inferred supervised latent variables can be directly used to perform a\r\nnearest neighbour search for the purpose of retrieval.  We introduce a new\r\napplication of dynamically extending hash codes, and show how to\r\neffectively couple the structure of the hash codes with continuously\r\ngrowing structure of the neighbourhood preserving infinite latent feature\r\nspace.","lang":"eng"}],"quality_controlled":"1","day":"11","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","month":"07","year":"2013","publication_status":"published","file":[{"file_size":1117100,"creator":"system","access_level":"open_access","date_created":"2018-12-12T10:15:16Z","content_type":"application/pdf","date_updated":"2020-07-14T12:45:42Z","file_name":"IST-2013-137-v1+1_QuaShaKnoGha13.pdf","file_id":"5134","checksum":"325f20c4b926bd74d39006b97df572bd","relation":"main_file"}],"pubrep_id":"137","date_updated":"2023-02-23T10:46:36Z","publist_id":"4381","oa":1,"citation":{"mla":"Quadrianto, Novi, et al. “The Supervised IBP: Neighbourhood Preserving Infinite Latent Feature Models.” <i>Proceedings of the 29th Conference Uncertainty in Artificial Intelligence</i>, AUAI Press, 2013, pp. 527–36.","chicago":"Quadrianto, Novi, Viktoriia Sharmanska, David Knowles, and Zoubin Ghahramani. “The Supervised IBP: Neighbourhood Preserving Infinite Latent Feature Models.” In <i>Proceedings of the 29th Conference Uncertainty in Artificial Intelligence</i>, 527–36. AUAI Press, 2013.","apa":"Quadrianto, N., Sharmanska, V., Knowles, D., &#38; Ghahramani, Z. (2013). The supervised IBP: Neighbourhood preserving infinite latent feature models. In <i>Proceedings of the 29th conference uncertainty in Artificial Intelligence</i> (pp. 527–536). Bellevue, WA, United States: AUAI Press.","ista":"Quadrianto N, Sharmanska V, Knowles D, Ghahramani Z. 2013. The supervised IBP: Neighbourhood preserving infinite latent feature models. Proceedings of the 29th conference uncertainty in Artificial Intelligence. UAI: Uncertainty in Artificial Intelligence, 527–536.","ama":"Quadrianto N, Sharmanska V, Knowles D, Ghahramani Z. The supervised IBP: Neighbourhood preserving infinite latent feature models. In: <i>Proceedings of the 29th Conference Uncertainty in Artificial Intelligence</i>. AUAI Press; 2013:527-536.","ieee":"N. Quadrianto, V. Sharmanska, D. Knowles, and Z. Ghahramani, “The supervised IBP: Neighbourhood preserving infinite latent feature models,” in <i>Proceedings of the 29th conference uncertainty in Artificial Intelligence</i>, Bellevue, WA, United States, 2013, pp. 527–536.","short":"N. Quadrianto, V. Sharmanska, D. Knowles, Z. Ghahramani, in:, Proceedings of the 29th Conference Uncertainty in Artificial Intelligence, AUAI Press, 2013, pp. 527–536."},"publication":"Proceedings of the 29th conference uncertainty in Artificial Intelligence","status":"public","title":"The supervised IBP: Neighbourhood preserving infinite latent feature models","department":[{"_id":"ChLa"}],"file_date_updated":"2020-07-14T12:45:42Z","date_created":"2018-12-11T11:58:09Z","ddc":["000"],"publication_identifier":{"isbn":["9780974903996"]},"conference":{"name":"UAI: Uncertainty in Artificial Intelligence","location":"Bellevue, WA, United States","start_date":"2013-07-11","end_date":"2013-07-15"},"author":[{"last_name":"Quadrianto","first_name":"Novi","full_name":"Quadrianto, Novi"},{"last_name":"Sharmanska","orcid":"0000-0003-0192-9308","id":"2EA6D09E-F248-11E8-B48F-1D18A9856A87","first_name":"Viktoriia","full_name":"Sharmanska, Viktoriia"},{"first_name":"David","full_name":"Knowles, David","last_name":"Knowles"},{"first_name":"Zoubin","full_name":"Ghahramani, Zoubin","last_name":"Ghahramani"}],"page":"527 - 536","date_published":"2013-07-11T00:00:00Z","language":[{"iso":"eng"}],"publisher":"AUAI Press","has_accepted_license":"1","_id":"2520","scopus_import":1},{"publication_status":"published","year":"2013","month":"09","type":"journal_article","day":"06","quality_controlled":0,"extern":1,"issue":"1","date_created":"2018-12-11T11:45:27Z","title":"Counting rational points on cubic hypersurfaces: Corrigendum","status":"public","_id":"253","publication":"Mathematika","doi":"10.1112/S0025579313000132","citation":{"ieee":"T. D. Browning, “Counting rational points on cubic hypersurfaces: Corrigendum,” <i>Mathematika</i>, vol. 60, no. 1. Unknown, pp. 101–107, 2013.","short":"T.D. Browning, Mathematika 60 (2013) 101–107.","ista":"Browning TD. 2013. Counting rational points on cubic hypersurfaces: Corrigendum. Mathematika. 60(1), 101–107.","ama":"Browning TD. Counting rational points on cubic hypersurfaces: Corrigendum. <i>Mathematika</i>. 2013;60(1):101-107. doi:<a href=\"https://doi.org/10.1112/S0025579313000132\">10.1112/S0025579313000132</a>","mla":"Browning, Timothy D. “Counting Rational Points on Cubic Hypersurfaces: Corrigendum.” <i>Mathematika</i>, vol. 60, no. 1, Unknown, 2013, pp. 101–07, doi:<a href=\"https://doi.org/10.1112/S0025579313000132\">10.1112/S0025579313000132</a>.","chicago":"Browning, Timothy D. “Counting Rational Points on Cubic Hypersurfaces: Corrigendum.” <i>Mathematika</i>. Unknown, 2013. <a href=\"https://doi.org/10.1112/S0025579313000132\">https://doi.org/10.1112/S0025579313000132</a>.","apa":"Browning, T. D. (2013). Counting rational points on cubic hypersurfaces: Corrigendum. <i>Mathematika</i>. Unknown. <a href=\"https://doi.org/10.1112/S0025579313000132\">https://doi.org/10.1112/S0025579313000132</a>"},"publisher":"Unknown","volume":60,"publist_id":"7649","date_updated":"2021-01-12T06:58:03Z","intvolume":"        60","date_published":"2013-09-06T00:00:00Z","page":"101 - 107","author":[{"full_name":"Timothy Browning","first_name":"Timothy D","id":"35827D50-F248-11E8-B48F-1D18A9856A87","last_name":"Browning","orcid":"0000-0002-8314-0177"}]},{"date_created":"2018-12-11T11:53:41Z","extern":1,"issue":"8","type":"journal_article","acknowledgement":"This study was supported by grants from the Israel Science Foundation (ISF) [11/09 to C.K.]; the Association Francaise contre les Myopathies (AFM) [15642 to C.K.]; the German Research Foundation (DFG) [UN 34/27-1 to C.K.]; the UK Medical Research Council (MRC) [U117560541 to J.B. and A.K.]; Fondation Pour la Recherche Médicale (FRM) (post-doctoral fellowship to V.R.). Deposited in PMC for release after 6 months","abstract":[{"text":"The development of a functional tissue requires coordination of the amplification of progenitors and their differentiation into specific cell types. The molecular basis for this coordination during myotome ontogeny is not well understood. Dermomytome progenitors that colonize the myotome first acquire myocyte identity and subsequently proliferate as Pax7-expressing progenitors before undergoing terminal differentiation. We show that the dynamics of sonic hedgehog (Shh) signaling is crucial for this transition in both avian and mouse embryos. Initially, Shh ligand emanating from notochord/floor plate reaches the dermomyotome, where it both maintains the proliferation of dermomyotome cells and promotes myogenic differentiation of progenitors that colonized the myotome. Interfering with Shh signaling at this stage produces small myotomes and accumulation of Pax7-expressing progenitors. An in vivo reporter of Shh activity combined with mouse genetics revealed the existence of both activator and repressor Shh activities operating on distinct subsets of cells during the epaxial myotomal maturation. In contrast to observations in mice, in avians Shh promotes the differentiation of both epaxial and hypaxial myotome domains. Subsequently, myogenic progenitors become refractory to Shh; this is likely to occur at the level of, or upstream of, smoothened signaling. The end of responsiveness to Shh coincides with, and is thus likely to enable, the transition into the growth phase of the myotome.","lang":"eng"}],"quality_controlled":0,"day":"18","month":"04","year":"2013","publication_status":"published","intvolume":"       140","author":[{"full_name":"Kahane, Nitza","first_name":"Nitza","last_name":"Kahane"},{"full_name":"Ribes, Vanessa","first_name":"Vanessa","last_name":"Ribes"},{"last_name":"Kicheva","orcid":"0000-0003-4509-4998","id":"3959A2A0-F248-11E8-B48F-1D18A9856A87","first_name":"Anna","full_name":"Anna Kicheva"},{"full_name":"Briscoe, James","first_name":"James","last_name":"Briscoe"},{"full_name":"Kalcheim, Chaya","first_name":"Chaya","last_name":"Kalcheim"}],"page":"1740 - 1750","date_published":"2013-04-18T00:00:00Z","publisher":"Company of Biologists","date_updated":"2021-01-12T06:52:47Z","publist_id":"5402","volume":140,"doi":"10.1242/dev.092726","citation":{"short":"N. Kahane, V. Ribes, A. Kicheva, J. Briscoe, C. Kalcheim, Development 140 (2013) 1740–1750.","ieee":"N. Kahane, V. Ribes, A. Kicheva, J. Briscoe, and C. Kalcheim, “The transition from differentiation to growth during dermomyotome-derived myogenesis depends on temporally restricted hedgehog signaling,” <i>Development</i>, vol. 140, no. 8. Company of Biologists, pp. 1740–1750, 2013.","ama":"Kahane N, Ribes V, Kicheva A, Briscoe J, Kalcheim C. The transition from differentiation to growth during dermomyotome-derived myogenesis depends on temporally restricted hedgehog signaling. <i>Development</i>. 2013;140(8):1740-1750. doi:<a href=\"https://doi.org/10.1242/dev.092726\">10.1242/dev.092726</a>","ista":"Kahane N, Ribes V, Kicheva A, Briscoe J, Kalcheim C. 2013. The transition from differentiation to growth during dermomyotome-derived myogenesis depends on temporally restricted hedgehog signaling. Development. 140(8), 1740–1750.","apa":"Kahane, N., Ribes, V., Kicheva, A., Briscoe, J., &#38; Kalcheim, C. (2013). The transition from differentiation to growth during dermomyotome-derived myogenesis depends on temporally restricted hedgehog signaling. <i>Development</i>. Company of Biologists. <a href=\"https://doi.org/10.1242/dev.092726\">https://doi.org/10.1242/dev.092726</a>","chicago":"Kahane, Nitza, Vanessa Ribes, Anna Kicheva, James Briscoe, and Chaya Kalcheim. “The Transition from Differentiation to Growth during Dermomyotome-Derived Myogenesis Depends on Temporally Restricted Hedgehog Signaling.” <i>Development</i>. Company of Biologists, 2013. <a href=\"https://doi.org/10.1242/dev.092726\">https://doi.org/10.1242/dev.092726</a>.","mla":"Kahane, Nitza, et al. “The Transition from Differentiation to Growth during Dermomyotome-Derived Myogenesis Depends on Temporally Restricted Hedgehog Signaling.” <i>Development</i>, vol. 140, no. 8, Company of Biologists, 2013, pp. 1740–50, doi:<a href=\"https://doi.org/10.1242/dev.092726\">10.1242/dev.092726</a>."},"_id":"1726","publication":"Development","status":"public","title":"The transition from differentiation to growth during dermomyotome-derived myogenesis depends on temporally restricted hedgehog signaling"},{"publication":"Cold Spring Harbor Protocols","_id":"1727","doi":"10.1101/pdb.top074237","citation":{"mla":"Kicheva, Anna, et al. “Quantitative Imaging of Morphogen Gradients in Drosophila Imaginal Discs.” <i>Cold Spring Harbor Protocols</i>, vol. 8, no. 5, Cold Spring Harbor Laboratory Press, 2013, pp. 387–403, doi:<a href=\"https://doi.org/10.1101/pdb.top074237\">10.1101/pdb.top074237</a>.","chicago":"Kicheva, Anna, Laurent Holtzer, Ortrud Wartlick, Thomas Schmidt, and Marcos González Gaitán. “Quantitative Imaging of Morphogen Gradients in Drosophila Imaginal Discs.” <i>Cold Spring Harbor Protocols</i>. Cold Spring Harbor Laboratory Press, 2013. <a href=\"https://doi.org/10.1101/pdb.top074237\">https://doi.org/10.1101/pdb.top074237</a>.","apa":"Kicheva, A., Holtzer, L., Wartlick, O., Schmidt, T., &#38; González Gaitán, M. (2013). Quantitative imaging of morphogen gradients in drosophila imaginal discs. <i>Cold Spring Harbor Protocols</i>. Cold Spring Harbor Laboratory Press. <a href=\"https://doi.org/10.1101/pdb.top074237\">https://doi.org/10.1101/pdb.top074237</a>","ista":"Kicheva A, Holtzer L, Wartlick O, Schmidt T, González Gaitán M. 2013. Quantitative imaging of morphogen gradients in drosophila imaginal discs. Cold Spring Harbor Protocols. 8(5), 387–403.","ama":"Kicheva A, Holtzer L, Wartlick O, Schmidt T, González Gaitán M. Quantitative imaging of morphogen gradients in drosophila imaginal discs. <i>Cold Spring Harbor Protocols</i>. 2013;8(5):387-403. doi:<a href=\"https://doi.org/10.1101/pdb.top074237\">10.1101/pdb.top074237</a>","ieee":"A. Kicheva, L. Holtzer, O. Wartlick, T. Schmidt, and M. González Gaitán, “Quantitative imaging of morphogen gradients in drosophila imaginal discs,” <i>Cold Spring Harbor Protocols</i>, vol. 8, no. 5. Cold Spring Harbor Laboratory Press, pp. 387–403, 2013.","short":"A. Kicheva, L. Holtzer, O. Wartlick, T. Schmidt, M. González Gaitán, Cold Spring Harbor Protocols 8 (2013) 387–403."},"title":"Quantitative imaging of morphogen gradients in drosophila imaginal discs","status":"public","intvolume":"         8","date_published":"2013-05-01T00:00:00Z","page":"387 - 403","author":[{"last_name":"Kicheva","orcid":"0000-0003-4509-4998","id":"3959A2A0-F248-11E8-B48F-1D18A9856A87","first_name":"Anna","full_name":"Anna Kicheva"},{"last_name":"Holtzer","first_name":"Laurent","full_name":"Holtzer, Laurent"},{"full_name":"Wartlick, Ortrud","first_name":"Ortrud","last_name":"Wartlick"},{"last_name":"Schmidt","first_name":"Thomas","full_name":"Schmidt, Thomas S"},{"last_name":"González Gaitán","first_name":"Marcos","full_name":"González-Gaitán, Marcos A"}],"publisher":"Cold Spring Harbor Laboratory Press","publist_id":"5401","volume":8,"date_updated":"2021-01-12T06:52:47Z","abstract":[{"lang":"eng","text":"Cells at different positions in a developing tissue receive different concentrations of signaling molecules, called morphogens, and this influences their cell fate. Morphogen concentration gradients have been proposed to control patterning as well as growth in many developing tissues. Some outstanding questions about tissue patterning by morphogen gradients are the following: What are the mechanisms that regulate gradient formation and shape? Is the positional information encoded in the gradient sufficiently precise to determine the positions of target gene domain boundaries? What are the temporal dynamics of gradients and how do they relate to patterning and growth? These questions are inherently quantitative in nature and addressing them requires measuring morphogen concentrations in cells, levels of downstream signaling activity, and kinetics of morphogen transport. Here we first present methods for quantifying morphogen gradient shape in which the measurements can be calibrated to reflect actual morphogen concentrations. We then discuss using fluorescence recovery after photobleaching to study the kinetics of morphogen transport at the tissue level. Finally, we present particle tracking as a method to study morphogen intracellular trafficking."}],"type":"journal_article","day":"01","quality_controlled":0,"publication_status":"published","year":"2013","month":"05","date_created":"2018-12-11T11:53:41Z","extern":1,"issue":"5"},{"publication":"Physical Review Letters","_id":"1759","doi":"10.1103/PhysRevLett.110.046602","citation":{"ista":"Ares N, Golovach V, Katsaros G, Stoffel M, Fournel F, Glazman L, Schmidt O, De Franceschi S. 2013. Nature of tunable hole g factors in quantum dots. Physical Review Letters. 110(4).","ama":"Ares N, Golovach V, Katsaros G, et al. Nature of tunable hole g factors in quantum dots. <i>Physical Review Letters</i>. 2013;110(4). doi:<a href=\"https://doi.org/10.1103/PhysRevLett.110.046602\">10.1103/PhysRevLett.110.046602</a>","ieee":"N. Ares <i>et al.</i>, “Nature of tunable hole g factors in quantum dots,” <i>Physical Review Letters</i>, vol. 110, no. 4. American Physical Society, 2013.","short":"N. Ares, V. Golovach, G. Katsaros, M. Stoffel, F. Fournel, L. Glazman, O. Schmidt, S. De Franceschi, Physical Review Letters 110 (2013).","chicago":"Ares, Natalia, Vitaly Golovach, Georgios Katsaros, Mathieu Stoffel, Frank Fournel, Leonid Glazman, Oliver Schmidt, and Silvano De Franceschi. “Nature of Tunable Hole g Factors in Quantum Dots.” <i>Physical Review Letters</i>. American Physical Society, 2013. <a href=\"https://doi.org/10.1103/PhysRevLett.110.046602\">https://doi.org/10.1103/PhysRevLett.110.046602</a>.","mla":"Ares, Natalia, et al. “Nature of Tunable Hole g Factors in Quantum Dots.” <i>Physical Review Letters</i>, vol. 110, no. 4, American Physical Society, 2013, doi:<a href=\"https://doi.org/10.1103/PhysRevLett.110.046602\">10.1103/PhysRevLett.110.046602</a>.","apa":"Ares, N., Golovach, V., Katsaros, G., Stoffel, M., Fournel, F., Glazman, L., … De Franceschi, S. (2013). Nature of tunable hole g factors in quantum dots. <i>Physical Review Letters</i>. American Physical Society. <a href=\"https://doi.org/10.1103/PhysRevLett.110.046602\">https://doi.org/10.1103/PhysRevLett.110.046602</a>"},"title":"Nature of tunable hole g factors in quantum dots","status":"public","intvolume":"       110","date_published":"2013-01-23T00:00:00Z","author":[{"first_name":"Natalia","full_name":"Ares, Natalia","last_name":"Ares"},{"last_name":"Golovach","full_name":"Golovach, Vitaly N","first_name":"Vitaly"},{"last_name":"Katsaros","id":"38DB5788-F248-11E8-B48F-1D18A9856A87","first_name":"Georgios","full_name":"Georgios Katsaros"},{"full_name":"Stoffel, Mathieu","first_name":"Mathieu","last_name":"Stoffel"},{"last_name":"Fournel","first_name":"Frank","full_name":"Fournel, Frank"},{"full_name":"Glazman, Leonid I","first_name":"Leonid","last_name":"Glazman"},{"full_name":"Schmidt, Oliver G","first_name":"Oliver","last_name":"Schmidt"},{"first_name":"Silvano","full_name":"De Franceschi, Silvano","last_name":"De Franceschi"}],"publisher":"American Physical Society","oa":1,"volume":110,"publist_id":"5365","date_updated":"2021-01-12T06:53:01Z","abstract":[{"lang":"eng","text":"We report an electric-field-induced giant modulation of the hole g factor in SiGe nanocrystals. The observed effect is ascribed to a so-far overlooked contribution to the g factor that stems from the mixing between heavy- and light-hole wave functions. We show that the relative displacement between the confined heavy- and light-hole states, occurring upon application of the electric field, alters their mixing strength leading to a strong nonmonotonic modulation of the g factor."}],"acknowledgement":"We acknowledge financial support from the Nanosciences Foundation (Grenoble, France), DOE under Contract No. DEFG02-08ER46482 (Yale), the Agence Nationale de la Recherche, and the European Starting Grant. G. K. acknowledges support from the European Commission via a Marie Curie Carrer Integration Grant and the FWF for a Lise-Meitner Fellowship","type":"journal_article","day":"23","quality_controlled":0,"publication_status":"published","year":"2013","month":"01","main_file_link":[{"url":"http://arxiv.org/abs/1208.0476","open_access":"1"}],"date_created":"2018-12-11T11:53:51Z","extern":1,"issue":"4"},{"intvolume":"       103","date_published":"2013-01-23T00:00:00Z","author":[{"last_name":"Ares","full_name":"Ares, Natalia","first_name":"Natalia"},{"full_name":"Georgios Katsaros","first_name":"Georgios","id":"38DB5788-F248-11E8-B48F-1D18A9856A87","last_name":"Katsaros"},{"full_name":"Golovach, Vitaly N","first_name":"Vitaly","last_name":"Golovach"},{"first_name":"Jianjun","full_name":"Zhang, Jianjun","last_name":"Zhang"},{"full_name":"Prager, Aaron A","first_name":"Aaron","last_name":"Prager"},{"first_name":"Leonid","full_name":"Glazman, Leonid I","last_name":"Glazman"},{"full_name":"Schmidt, Oliver G","first_name":"Oliver","last_name":"Schmidt"},{"last_name":"De Franceschi","first_name":"Silvano","full_name":"De Franceschi, Silvano"}],"publisher":"American Institute of Physics","oa":1,"volume":103,"publist_id":"5364","date_updated":"2021-01-12T06:53:02Z","_id":"1760","publication":"Applied Physics Letters","doi":"10.1063/1.4858959","citation":{"mla":"Ares, Natalia, et al. “SiGe Quantum Dots for Fast Hole Spin Rabi Oscillations.” <i>Applied Physics Letters</i>, vol. 103, no. 26, American Institute of Physics, 2013, doi:<a href=\"https://doi.org/10.1063/1.4858959\">10.1063/1.4858959</a>.","chicago":"Ares, Natalia, Georgios Katsaros, Vitaly Golovach, Jianjun Zhang, Aaron Prager, Leonid Glazman, Oliver Schmidt, and Silvano De Franceschi. “SiGe Quantum Dots for Fast Hole Spin Rabi Oscillations.” <i>Applied Physics Letters</i>. American Institute of Physics, 2013. <a href=\"https://doi.org/10.1063/1.4858959\">https://doi.org/10.1063/1.4858959</a>.","apa":"Ares, N., Katsaros, G., Golovach, V., Zhang, J., Prager, A., Glazman, L., … De Franceschi, S. (2013). SiGe quantum dots for fast hole spin Rabi oscillations. <i>Applied Physics Letters</i>. American Institute of Physics. <a href=\"https://doi.org/10.1063/1.4858959\">https://doi.org/10.1063/1.4858959</a>","ista":"Ares N, Katsaros G, Golovach V, Zhang J, Prager A, Glazman L, Schmidt O, De Franceschi S. 2013. SiGe quantum dots for fast hole spin Rabi oscillations. Applied Physics Letters. 103(26).","ama":"Ares N, Katsaros G, Golovach V, et al. SiGe quantum dots for fast hole spin Rabi oscillations. <i>Applied Physics Letters</i>. 2013;103(26). doi:<a href=\"https://doi.org/10.1063/1.4858959\">10.1063/1.4858959</a>","ieee":"N. Ares <i>et al.</i>, “SiGe quantum dots for fast hole spin Rabi oscillations,” <i>Applied Physics Letters</i>, vol. 103, no. 26. American Institute of Physics, 2013.","short":"N. Ares, G. Katsaros, V. Golovach, J. Zhang, A. Prager, L. Glazman, O. Schmidt, S. De Franceschi, Applied Physics Letters 103 (2013)."},"title":"SiGe quantum dots for fast hole spin Rabi oscillations","status":"public","date_created":"2018-12-11T11:53:52Z","extern":1,"issue":"26","acknowledgement":"We acknowledge the financial support from the Nanosciences Foundation (Grenoble, France), the Commission for a Marie Curie Carrer Integration Grant, the Austrian Science Fund (FWF) for a Lise-Meitner Fellowship (M1435-N30), the DOE under Contract No. DE-FG02-08ER46482 (Yale), the European Starting Grant program, and the Agence Nationale de la Recherche","abstract":[{"lang":"eng","text":"We report on hole g-factor measurements in three terminal SiGe self-assembled quantum dot devices with a top gate electrode positioned very close to the nanostructure. Measurements of both the perpendicular as well as the parallel g-factor reveal significant changes for a small modulation of the top gate voltage. From the observed modulations, we estimate that, for realistic experimental conditions, hole spins can be electrically manipulated with Rabi frequencies in the order of 100 MHz. This work emphasises the potential of hole-based nano-devices for efficient spin manipulation by means of the g-tensor modulation technique."}],"type":"journal_article","day":"23","quality_controlled":0,"publication_status":"published","year":"2013","month":"01","main_file_link":[{"open_access":"1","url":"http://arxiv.org/abs/1307.7196"}]},{"oa_version":"Preprint","arxiv":1,"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","month":"10","year":"2013","publication_status":"published","quality_controlled":"1","day":"18","type":"journal_article","abstract":[{"text":"A near-equal-mass binary black hole (BH) can clear a central cavity in a circumbinary accretion disc; however, previous works have revealed accretion streams entering this cavity. Here we use 2D hydrodynamical simulations to study the accretion streams and their periodic behaviour. In particular, we perform a suite of simulations, covering different binary mass ratios q = M2/M1 in the range 0.003 ≤ q ≤ 1. In each case, we follow the system for several thousand binary orbits, until it relaxes to a stable accretion pattern. We find the following results: (i) the binary is efficient in maintaining a low-density cavity. However, the time-averaged mass accretion rate into the cavity, through narrow coherent accretion streams, is suppressed by at most a factor of a few compared to a disc with a single BH with the same mass; (ii) for q ≳ 0.05, the accretion rate is strongly modulated by the binary, and depending on the precise value of q, the power spectrum of the accretion rate shows either one, two or three distinct periods; and (iii) for q ≲ 0.05, the accretion rate becomes steady, with no time variations. Most binaries produced in galactic mergers are expected to have q ≳ 0.05. If the luminosity of these binaries tracks their accretion rate, then a periodogram of their light curve could help in their identification, and to constrain their mass ratio and disc properties.","lang":"eng"}],"date_updated":"2024-09-24T08:47:58Z","volume":436,"oa":1,"article_type":"original","intvolume":"       436","status":"public","title":"Accretion into the central cavity of a circumbinary disc","external_id":{"arxiv":["1210.0536"]},"doi":"10.1093/mnras/stt1787","citation":{"apa":"D’Orazio, D. J., Haiman, Z., &#38; MacFadyen, A. (2013). Accretion into the central cavity of a circumbinary disc. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stt1787\">https://doi.org/10.1093/mnras/stt1787</a>","mla":"D’Orazio, Daniel J., et al. “Accretion into the Central Cavity of a Circumbinary Disc.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 436, no. 4, Oxford University Press, 2013, pp. 2997–3020, doi:<a href=\"https://doi.org/10.1093/mnras/stt1787\">10.1093/mnras/stt1787</a>.","chicago":"D’Orazio, Daniel J., Zoltán Haiman, and Andrew MacFadyen. “Accretion into the Central Cavity of a Circumbinary Disc.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2013. <a href=\"https://doi.org/10.1093/mnras/stt1787\">https://doi.org/10.1093/mnras/stt1787</a>.","short":"D.J. D’Orazio, Z. Haiman, A. MacFadyen, Monthly Notices of the Royal Astronomical Society 436 (2013) 2997–3020.","ieee":"D. J. D’Orazio, Z. Haiman, and A. MacFadyen, “Accretion into the central cavity of a circumbinary disc,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 436, no. 4. Oxford University Press, pp. 2997–3020, 2013.","ama":"D’Orazio DJ, Haiman Z, MacFadyen A. Accretion into the central cavity of a circumbinary disc. <i>Monthly Notices of the Royal Astronomical Society</i>. 2013;436(4):2997-3020. doi:<a href=\"https://doi.org/10.1093/mnras/stt1787\">10.1093/mnras/stt1787</a>","ista":"D’Orazio DJ, Haiman Z, MacFadyen A. 2013. Accretion into the central cavity of a circumbinary disc. Monthly Notices of the Royal Astronomical Society. 436(4), 2997–3020."},"publication":"Monthly Notices of the Royal Astronomical Society","issue":"4","extern":"1","date_created":"2024-09-05T13:53:11Z","main_file_link":[{"url":" https://doi.org/10.48550/arXiv.1210.0536","open_access":"1"}],"publication_identifier":{"issn":["1365-2966","0035-8711"]},"language":[{"iso":"eng"}],"article_processing_charge":"No","publisher":"Oxford University Press","page":"2997-3020","author":[{"last_name":"D'Orazio","full_name":"D'Orazio, Daniel J.","first_name":"Daniel J."},{"last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","first_name":"Zoltán","full_name":"Haiman, Zoltán"},{"last_name":"MacFadyen","first_name":"Andrew","full_name":"MacFadyen, Andrew"}],"date_published":"2013-10-18T00:00:00Z","scopus_import":"1","_id":"17624"},{"main_file_link":[{"open_access":"1","url":" https://doi.org/10.48550/arXiv.1306.0009"}],"publication_identifier":{"issn":["1745-3933","1745-3925"]},"extern":"1","issue":"1","date_created":"2024-09-05T14:00:29Z","scopus_import":"1","_id":"17631","publisher":"Oxford University Press","language":[{"iso":"eng"}],"article_processing_charge":"No","date_published":"2013-08-09T00:00:00Z","page":"L53-L57","author":[{"first_name":"Fabio","full_name":"Pacucci, Fabio","last_name":"Pacucci"},{"last_name":"Mesinger","first_name":"Andrei","full_name":"Mesinger, Andrei"},{"first_name":"Zoltán","full_name":"Haiman, Zoltán","last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36"}],"publication_status":"published","month":"08","year":"2013","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","abstract":[{"text":"We propose a novel use of high-redshift galaxies, discovered in deep Hubble Space Telescope (HST) fields around strong lensing clusters. These fields probe small comoving volumes (∼103 Mpc3) at high magnification (μ ≳ 10) and can detect otherwise inaccessible ultra-faint galaxies. Even a few galaxies found in such small volumes require a very high number density of collapsed dark matter (DM) haloes. This implies significant primordial power on small scales, allowing these observations to rule out popular alternatives to standard cold dark matter (CDM) models, such as warm dark matter (WDM). In this work, we analytically compute WDM halo mass functions at z = 10, including the effects of both particle free-streaming and residual velocity dispersion. We show that the two z ≈ 10 galaxies already detected by the Cluster Lensing And Supernova survey with Hubble (CLASH) survey are sufficient to constrain the WDM particle mass to mx > 1 (0.9) keV at 68 per cent (95 per cent) confidence limit (for a thermal relic relativistic at decoupling). This limit depends only on the WDM halo mass function and, unlike previous constraints on mx, is independent of any astrophysical modelling. The forthcoming HST Frontier Fields can significantly tighten these constraints.","lang":"eng"}],"type":"journal_article","day":"09","quality_controlled":"1","oa_version":"Preprint","arxiv":1,"external_id":{"arxiv":["1306.0009"]},"title":"Focusing on warm dark matter with lensed high-redshift galaxies","status":"public","publication":"Monthly Notices of the Royal Astronomical Society: Letters","doi":"10.1093/mnrasl/slt093","citation":{"apa":"Pacucci, F., Mesinger, A., &#38; Haiman, Z. (2013). Focusing on warm dark matter with lensed high-redshift galaxies. <i>Monthly Notices of the Royal Astronomical Society: Letters</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnrasl/slt093\">https://doi.org/10.1093/mnrasl/slt093</a>","mla":"Pacucci, Fabio, et al. “Focusing on Warm Dark Matter with Lensed High-Redshift Galaxies.” <i>Monthly Notices of the Royal Astronomical Society: Letters</i>, vol. 435, no. 1, Oxford University Press, 2013, pp. L53–57, doi:<a href=\"https://doi.org/10.1093/mnrasl/slt093\">10.1093/mnrasl/slt093</a>.","chicago":"Pacucci, Fabio, Andrei Mesinger, and Zoltán Haiman. “Focusing on Warm Dark Matter with Lensed High-Redshift Galaxies.” <i>Monthly Notices of the Royal Astronomical Society: Letters</i>. Oxford University Press, 2013. <a href=\"https://doi.org/10.1093/mnrasl/slt093\">https://doi.org/10.1093/mnrasl/slt093</a>.","ama":"Pacucci F, Mesinger A, Haiman Z. Focusing on warm dark matter with lensed high-redshift galaxies. <i>Monthly Notices of the Royal Astronomical Society: Letters</i>. 2013;435(1):L53-L57. doi:<a href=\"https://doi.org/10.1093/mnrasl/slt093\">10.1093/mnrasl/slt093</a>","ista":"Pacucci F, Mesinger A, Haiman Z. 2013. Focusing on warm dark matter with lensed high-redshift galaxies. Monthly Notices of the Royal Astronomical Society: Letters. 435(1), L53–L57.","short":"F. Pacucci, A. Mesinger, Z. Haiman, Monthly Notices of the Royal Astronomical Society: Letters 435 (2013) L53–L57.","ieee":"F. Pacucci, A. Mesinger, and Z. Haiman, “Focusing on warm dark matter with lensed high-redshift galaxies,” <i>Monthly Notices of the Royal Astronomical Society: Letters</i>, vol. 435, no. 1. Oxford University Press, pp. L53–L57, 2013."},"article_type":"original","oa":1,"volume":435,"date_updated":"2024-09-24T09:59:26Z","intvolume":"       435"},{"title":"Electromagnetic signatures of supermassive black hole binaries resolved by PTAs","external_id":{"arxiv":["1309.2302"]},"status":"public","publication":"Classical and Quantum Gravity","citation":{"mla":"Tanaka, Takamitsu L., and Zoltán Haiman. “Electromagnetic Signatures of Supermassive Black Hole Binaries Resolved by PTAs.” <i>Classical and Quantum Gravity</i>, vol. 30, no. 22, 224012, IOP Publishing, 2013, doi:<a href=\"https://doi.org/10.1088/0264-9381/30/22/224012\">10.1088/0264-9381/30/22/224012</a>.","chicago":"Tanaka, Takamitsu L, and Zoltán Haiman. “Electromagnetic Signatures of Supermassive Black Hole Binaries Resolved by PTAs.” <i>Classical and Quantum Gravity</i>. IOP Publishing, 2013. <a href=\"https://doi.org/10.1088/0264-9381/30/22/224012\">https://doi.org/10.1088/0264-9381/30/22/224012</a>.","apa":"Tanaka, T. L., &#38; Haiman, Z. (2013). Electromagnetic signatures of supermassive black hole binaries resolved by PTAs. <i>Classical and Quantum Gravity</i>. IOP Publishing. <a href=\"https://doi.org/10.1088/0264-9381/30/22/224012\">https://doi.org/10.1088/0264-9381/30/22/224012</a>","ieee":"T. L. Tanaka and Z. Haiman, “Electromagnetic signatures of supermassive black hole binaries resolved by PTAs,” <i>Classical and Quantum Gravity</i>, vol. 30, no. 22. IOP Publishing, 2013.","short":"T.L. Tanaka, Z. Haiman, Classical and Quantum Gravity 30 (2013).","ista":"Tanaka TL, Haiman Z. 2013. Electromagnetic signatures of supermassive black hole binaries resolved by PTAs. Classical and Quantum Gravity. 30(22), 224012.","ama":"Tanaka TL, Haiman Z. Electromagnetic signatures of supermassive black hole binaries resolved by PTAs. <i>Classical and Quantum Gravity</i>. 2013;30(22). doi:<a href=\"https://doi.org/10.1088/0264-9381/30/22/224012\">10.1088/0264-9381/30/22/224012</a>"},"doi":"10.1088/0264-9381/30/22/224012","article_type":"original","oa":1,"volume":30,"date_updated":"2024-09-24T11:39:17Z","intvolume":"        30","publication_status":"published","month":"11","year":"2013","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","abstract":[{"lang":"eng","text":"Pulsar timing arrays (PTAs) may eventually be able to detect not only the stochastic gravitational-wave (GW) background of SMBH binaries, but also individual, particularly massive binaries whose signals stick out above the background. In this contribution, we discuss the possibility of identifying and studying such 'resolved' binaries through their electromagnetic emission. The host galaxies of such binaries are themselves expected to be also very massive and rare, so that out to redshifts z ≈ 0.2 a unique massive galaxy may be identified as the host. At higher redshifts, the PTA error boxes are larger and may contain as many as several hundred massive-galaxy interlopers. In this case, the true counterpart may be identified, if it is accreting gas efficiently, as an active galactic nucleus (AGN) with a peculiar spectrum and variable emission features. Specifically, the binary's tidal torques expel the gas from the inner part of the accretion disc, making it unusually dim in x-ray and UV bands and in broad optical emission lines. The tails of the broad wings of any FeKα emission line may also be 'clipped' and missing. The binary's orbital motion, as well as the gas motions it induces, may trigger quasiperiodic variations. These include coherent flux variability, such as luminous, multi-wavelength flares, as well as Doppler shifts of broad emission lines and 'see-saw' oscillations in the FeKα line. Additional features, such as evidence for a recent major merger or dual collimated jets, could also corroborate the counterpart. These properties would make resolved PTA sources stand out among AGN with similar overall luminosities and allow their identification."}],"type":"journal_article","day":"04","quality_controlled":"1","oa_version":"Preprint","arxiv":1,"scopus_import":"1","_id":"17638","article_number":"224012","publisher":"IOP Publishing","language":[{"iso":"eng"}],"article_processing_charge":"No","date_published":"2013-11-04T00:00:00Z","author":[{"first_name":"Takamitsu L","full_name":"Tanaka, Takamitsu L","last_name":"Tanaka"},{"last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","first_name":"Zoltán","full_name":"Haiman, Zoltán"}],"main_file_link":[{"open_access":"1","url":" https://doi.org/10.48550/arXiv.1309.2302"}],"publication_identifier":{"issn":["0264-9381","1361-6382"]},"extern":"1","issue":"22","date_created":"2024-09-06T07:16:12Z"},{"status":"public","title":"Constraints on warm dark matter models from high-redshift long gamma-ray bursts","citation":{"short":"R.S. de Souza, A. Mesinger, A. Ferrara, Z. Haiman, R. Perna, N. Yoshida, Monthly Notices of the Royal Astronomical Society 432 (2013) 3218–3227.","ieee":"R. S. de Souza, A. Mesinger, A. Ferrara, Z. Haiman, R. Perna, and N. Yoshida, “Constraints on warm dark matter models from high-redshift long gamma-ray bursts,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 432, no. 4. Oxford University Press, pp. 3218–3227, 2013.","ama":"de Souza RS, Mesinger A, Ferrara A, Haiman Z, Perna R, Yoshida N. Constraints on warm dark matter models from high-redshift long gamma-ray bursts. <i>Monthly Notices of the Royal Astronomical Society</i>. 2013;432(4):3218-3227. doi:<a href=\"https://doi.org/10.1093/mnras/stt674\">10.1093/mnras/stt674</a>","ista":"de Souza RS, Mesinger A, Ferrara A, Haiman Z, Perna R, Yoshida N. 2013. Constraints on warm dark matter models from high-redshift long gamma-ray bursts. Monthly Notices of the Royal Astronomical Society. 432(4), 3218–3227.","apa":"de Souza, R. S., Mesinger, A., Ferrara, A., Haiman, Z., Perna, R., &#38; Yoshida, N. (2013). Constraints on warm dark matter models from high-redshift long gamma-ray bursts. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stt674\">https://doi.org/10.1093/mnras/stt674</a>","chicago":"Souza, R. S. de, A. Mesinger, A. Ferrara, Zoltán Haiman, R. Perna, and N. Yoshida. “Constraints on Warm Dark Matter Models from High-Redshift Long Gamma-Ray Bursts.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2013. <a href=\"https://doi.org/10.1093/mnras/stt674\">https://doi.org/10.1093/mnras/stt674</a>.","mla":"de Souza, R. S., et al. “Constraints on Warm Dark Matter Models from High-Redshift Long Gamma-Ray Bursts.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 432, no. 4, Oxford University Press, 2013, pp. 3218–27, doi:<a href=\"https://doi.org/10.1093/mnras/stt674\">10.1093/mnras/stt674</a>."},"doi":"10.1093/mnras/stt674","publication":"Monthly Notices of the Royal Astronomical Society","date_updated":"2024-09-24T12:40:52Z","volume":432,"oa":1,"article_type":"original","intvolume":"       432","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","month":"05","year":"2013","publication_status":"published","quality_controlled":"1","day":"09","type":"journal_article","abstract":[{"lang":"eng","text":"Structures in Warm Dark Matter (WDM) models are exponentially suppressed below a certain scale, characterized by the dark matter particle mass, mx. Since structures form hierarchically, the presence of collapsed objects at high-redshifts can set strong lower limits on mx. We place robust constraints on mx using recent results from the {\\it Swift} database of high-redshift gamma-ray bursts (GRBs). We parameterize the redshift evolution of the ratio between the cosmic GRB rate and star formation rate (SFR) as ∝(1+z)α, thereby allowing astrophysical uncertainties to partially mimic the cosmological suppression of structures in WDM models. Using a maximum likelihood estimator on two different z>4 GRB subsamples (including two bursts at z>8), we constrain mx≳1.6-1.8 keV at 95% C.L., when marginalized over a flat prior in α. We further estimate that 5 years of a SVOM-like mission would tighten these constraints to mx≳2.3 keV. Our results show that GRBs are a powerful probe of high-redshift structures, providing robust and competitive constraints on mx."}],"oa_version":"Published Version","scopus_import":"1","_id":"17646","language":[{"iso":"eng"}],"article_processing_charge":"No","publisher":"Oxford University Press","page":"3218-3227","author":[{"first_name":"R. S.","full_name":"de Souza, R. S.","last_name":"de Souza"},{"last_name":"Mesinger","full_name":"Mesinger, A.","first_name":"A."},{"last_name":"Ferrara","full_name":"Ferrara, A.","first_name":"A."},{"full_name":"Haiman, Zoltán","first_name":"Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman"},{"last_name":"Perna","full_name":"Perna, R.","first_name":"R."},{"full_name":"Yoshida, N.","first_name":"N.","last_name":"Yoshida"}],"date_published":"2013-05-09T00:00:00Z","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnras/stt674"}],"publication_identifier":{"issn":["0035-8711","1365-2966"]},"issue":"4","extern":"1","date_created":"2024-09-06T07:25:13Z"},{"oa_version":"Published Version","publication_status":"published","year":"2013","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","month":"09","abstract":[{"text":"Observations of quasars at redshifts z > 6 reveal that 10^9 Msol supermassive black holes (SMBHs) had already formed when the Universe was < 0.9 Gyr old. One hypothesis for the origins of these SMBHs is that they grew from the remnants of the first generation of massive stars, which formed in low-mass (~ 10^5 to 10^6 Msol) dark matter minihaloes at z > 20. This is the regime where baryonic streaming motions--the relative velocities of baryons with respect to dark matter in the early Universe--most strongly inhibit star formation by suppressing gas infall and cooling. We investigate the impact of this effect on the growth of the first SMBHs using a suite of high-fidelity, ellipsoidal-collapse Monte Carlo merger-tree simulations. We find that the suppression of seed BH formation by the streaming motions significantly reduces the number density of the most massive BHs at z > 15, but the residual effect at lower redshifts is essentially negligible. The streaming motions can reduce by a factor of few the number density of the most luminous quasars at z ~ 10-11, where such objects could be detected by the James Webb Space Telescope. We conclude, with minor theoretical caveats, that baryonic streaming motions are unlikely to pose a significant additional obstacle to the formation of the observed high-redshift quasar SMBHs. Nor do they appreciably affect the heating and reionization histories of the Universe or the merger rates of nuclear BHs in the mass and redshift ranges of interest for proposed gravitational-wave detectors.","lang":"eng"}],"type":"journal_article","day":"10","quality_controlled":"1","article_type":"original","volume":435,"oa":1,"date_updated":"2024-09-24T13:26:36Z","intvolume":"       435","title":"The effect of baryonic streaming motions on the formation of the first supermassive black holes","status":"public","publication":"Monthly Notices of the Royal Astronomical Society","doi":"10.1093/mnras/stt1553","citation":{"apa":"Tanaka, T. L., Li, M., &#38; Haiman, Z. (2013). The effect of baryonic streaming motions on the formation of the first supermassive black holes. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stt1553\">https://doi.org/10.1093/mnras/stt1553</a>","chicago":"Tanaka, Takamitsu L., Miao Li, and Zoltán Haiman. “The Effect of Baryonic Streaming Motions on the Formation of the First Supermassive Black Holes.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2013. <a href=\"https://doi.org/10.1093/mnras/stt1553\">https://doi.org/10.1093/mnras/stt1553</a>.","mla":"Tanaka, Takamitsu L., et al. “The Effect of Baryonic Streaming Motions on the Formation of the First Supermassive Black Holes.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 435, no. 4, Oxford University Press, 2013, pp. 3559–67, doi:<a href=\"https://doi.org/10.1093/mnras/stt1553\">10.1093/mnras/stt1553</a>.","ama":"Tanaka TL, Li M, Haiman Z. The effect of baryonic streaming motions on the formation of the first supermassive black holes. <i>Monthly Notices of the Royal Astronomical Society</i>. 2013;435(4):3559-3567. doi:<a href=\"https://doi.org/10.1093/mnras/stt1553\">10.1093/mnras/stt1553</a>","ista":"Tanaka TL, Li M, Haiman Z. 2013. The effect of baryonic streaming motions on the formation of the first supermassive black holes. Monthly Notices of the Royal Astronomical Society. 435(4), 3559–3567.","short":"T.L. Tanaka, M. Li, Z. Haiman, Monthly Notices of the Royal Astronomical Society 435 (2013) 3559–3567.","ieee":"T. L. Tanaka, M. Li, and Z. Haiman, “The effect of baryonic streaming motions on the formation of the first supermassive black holes,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 435, no. 4. Oxford University Press, pp. 3559–3567, 2013."},"extern":"1","issue":"4","date_created":"2024-09-06T07:31:32Z","main_file_link":[{"url":"https://doi.org/10.1093/mnras/stt1553","open_access":"1"}],"publication_identifier":{"issn":["1365-2966","0035-8711"]},"publisher":"Oxford University Press","language":[{"iso":"eng"}],"article_processing_charge":"No","date_published":"2013-09-10T00:00:00Z","author":[{"full_name":"Tanaka, Takamitsu L.","first_name":"Takamitsu L.","last_name":"Tanaka"},{"last_name":"Li","first_name":"Miao","full_name":"Li, Miao"},{"last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","first_name":"Zoltán","full_name":"Haiman, Zoltán"}],"page":"3559-3567","scopus_import":"1","_id":"17653"},{"intvolume":"       773","article_type":"original","volume":773,"oa":1,"date_updated":"2024-09-25T07:11:08Z","publication":"The Astrophysical Journal","citation":{"apa":"Rhoads, J. E., Malhotra, S., Stern, D., Dickinson, M., Pirzkal, N., Spinrad, H., … Yan, H. (2013). A Lyman break galaxy in the epoch of reionization from hubble space telescope grism spectroscopy. <i>The Astrophysical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.1088/0004-637x/773/1/32\">https://doi.org/10.1088/0004-637x/773/1/32</a>","mla":"Rhoads, James E., et al. “A Lyman Break Galaxy in the Epoch of Reionization from Hubble Space Telescope Grism Spectroscopy.” <i>The Astrophysical Journal</i>, vol. 773, no. 1, 32, American Astronomical Society, 2013, doi:<a href=\"https://doi.org/10.1088/0004-637x/773/1/32\">10.1088/0004-637x/773/1/32</a>.","chicago":"Rhoads, James E., Sangeeta Malhotra, Daniel Stern, Mark Dickinson, Norbert Pirzkal, Hyron Spinrad, Naveen Reddy, et al. “A Lyman Break Galaxy in the Epoch of Reionization from Hubble Space Telescope Grism Spectroscopy.” <i>The Astrophysical Journal</i>. American Astronomical Society, 2013. <a href=\"https://doi.org/10.1088/0004-637x/773/1/32\">https://doi.org/10.1088/0004-637x/773/1/32</a>.","short":"J.E. Rhoads, S. Malhotra, D. Stern, M. Dickinson, N. Pirzkal, H. Spinrad, N. Reddy, N. Hathi, N. Grogin, A. Koekemoer, M.A. Peth, S. Cohen, Z. Zheng, T. Budavari, I. Ferreras, J.P. Gardner, C. Gronwall, Z. Haiman, M. Kümmel, G. Meurer, L. Moustakas, N. Panagia, A. Pasquali, K. Sahu, S. di Serego Alighieri, R. Somerville, A. Straughn, J. Walsh, R. Windhorst, C. Xu, H. Yan, The Astrophysical Journal 773 (2013).","ieee":"J. E. Rhoads <i>et al.</i>, “A Lyman break galaxy in the epoch of reionization from hubble space telescope grism spectroscopy,” <i>The Astrophysical Journal</i>, vol. 773, no. 1. American Astronomical Society, 2013.","ama":"Rhoads JE, Malhotra S, Stern D, et al. A Lyman break galaxy in the epoch of reionization from hubble space telescope grism spectroscopy. <i>The Astrophysical Journal</i>. 2013;773(1). doi:<a href=\"https://doi.org/10.1088/0004-637x/773/1/32\">10.1088/0004-637x/773/1/32</a>","ista":"Rhoads JE, Malhotra S, Stern D, Dickinson M, Pirzkal N, Spinrad H, Reddy N, Hathi N, Grogin N, Koekemoer A, Peth MA, Cohen S, Zheng Z, Budavari T, Ferreras I, Gardner JP, Gronwall C, Haiman Z, Kümmel M, Meurer G, Moustakas L, Panagia N, Pasquali A, Sahu K, di Serego Alighieri S, Somerville R, Straughn A, Walsh J, Windhorst R, Xu C, Yan H. 2013. A Lyman break galaxy in the epoch of reionization from hubble space telescope grism spectroscopy. The Astrophysical Journal. 773(1), 32."},"doi":"10.1088/0004-637x/773/1/32","external_id":{"arxiv":["1302.7005"]},"title":"A Lyman break galaxy in the epoch of reionization from hubble space telescope grism spectroscopy","status":"public","arxiv":1,"oa_version":"Preprint","abstract":[{"lang":"eng","text":"We present observations of a luminous galaxy at z = 6.573—the end of the reionization epoch—which has been spectroscopically confirmed twice. The first spectroscopic confirmation comes from slitless Hubble Space Telescope Advanced Camera for Surveys grism spectra from the PEARS survey (Probing Evolution And Reionization Spectroscopically), which show a dramatic continuum break in the spectrum at rest frame 1216 Å. The second confirmation is done with Keck + DEIMOS. The continuum is not clearly detected with ground-based spectra, but high wavelength resolution enables the Lyα emission line profile to be determined. We compare the line profile to composite line profiles at z = 4.5. The Lyα line profile shows no signature of a damping wing attenuation, confirming that the intergalactic gas is ionized at z = 6.57. Spectra of Lyman breaks at yet higher redshifts will be possible using comparably deep observations with IR-sensitive grisms, even at redshifts where Lyα is too attenuated by the neutral intergalactic medium to be detectable using traditional spectroscopy from the ground."}],"type":"journal_article","day":"22","quality_controlled":"1","publication_status":"published","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","year":"2013","month":"07","date_published":"2013-07-22T00:00:00Z","author":[{"last_name":"Rhoads","full_name":"Rhoads, James E.","first_name":"James E."},{"last_name":"Malhotra","first_name":"Sangeeta","full_name":"Malhotra, Sangeeta"},{"last_name":"Stern","full_name":"Stern, Daniel","first_name":"Daniel"},{"full_name":"Dickinson, Mark","first_name":"Mark","last_name":"Dickinson"},{"last_name":"Pirzkal","first_name":"Norbert","full_name":"Pirzkal, Norbert"},{"last_name":"Spinrad","first_name":"Hyron","full_name":"Spinrad, Hyron"},{"first_name":"Naveen","full_name":"Reddy, Naveen","last_name":"Reddy"},{"last_name":"Hathi","first_name":"Nimish","full_name":"Hathi, Nimish"},{"full_name":"Grogin, Norman","first_name":"Norman","last_name":"Grogin"},{"first_name":"Anton","full_name":"Koekemoer, Anton","last_name":"Koekemoer"},{"last_name":"Peth","first_name":"Michael A.","full_name":"Peth, Michael A."},{"last_name":"Cohen","full_name":"Cohen, Seth","first_name":"Seth"},{"first_name":"Zhenya","full_name":"Zheng, Zhenya","last_name":"Zheng"},{"last_name":"Budavari","full_name":"Budavari, Tamas","first_name":"Tamas"},{"full_name":"Ferreras, Ignacio","first_name":"Ignacio","last_name":"Ferreras"},{"last_name":"Gardner","first_name":"Jonathan P.","full_name":"Gardner, Jonathan P."},{"last_name":"Gronwall","first_name":"Caryl","full_name":"Gronwall, Caryl"},{"full_name":"Haiman, Zoltán","first_name":"Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman"},{"first_name":"Martin","full_name":"Kümmel, Martin","last_name":"Kümmel"},{"full_name":"Meurer, Gerhardt","first_name":"Gerhardt","last_name":"Meurer"},{"first_name":"Leonidas","full_name":"Moustakas, Leonidas","last_name":"Moustakas"},{"full_name":"Panagia, Nino","first_name":"Nino","last_name":"Panagia"},{"first_name":"Anna","full_name":"Pasquali, Anna","last_name":"Pasquali"},{"last_name":"Sahu","first_name":"Kailash","full_name":"Sahu, Kailash"},{"last_name":"di Serego Alighieri","first_name":"Sperello","full_name":"di Serego Alighieri, Sperello"},{"last_name":"Somerville","first_name":"Rachel","full_name":"Somerville, Rachel"},{"last_name":"Straughn","first_name":"Amber","full_name":"Straughn, Amber"},{"first_name":"Jeremy","full_name":"Walsh, Jeremy","last_name":"Walsh"},{"last_name":"Windhorst","full_name":"Windhorst, Rogier","first_name":"Rogier"},{"last_name":"Xu","full_name":"Xu, Chun","first_name":"Chun"},{"last_name":"Yan","first_name":"Haojing","full_name":"Yan, Haojing"}],"publisher":"American Astronomical Society","language":[{"iso":"eng"}],"article_processing_charge":"No","_id":"17657","article_number":"32","scopus_import":"1","date_created":"2024-09-06T07:35:50Z","extern":"1","issue":"1","publication_identifier":{"issn":["0004-637X","1538-4357"]},"main_file_link":[{"open_access":"1","url":" https://doi.org/10.48550/arXiv.1302.7005"}]},{"extern":"1","issue":"1","date_created":"2024-09-06T07:47:50Z","main_file_link":[{"url":" https://doi.org/10.48550/arXiv.1301.0830","open_access":"1"}],"publication_identifier":{"issn":["0004-637X","1538-4357"]},"publisher":"American Astronomical Society","language":[{"iso":"eng"}],"article_processing_charge":"No","date_published":"2013-08-16T00:00:00Z","author":[{"first_name":"D.","full_name":"Bard, D.","last_name":"Bard"},{"full_name":"Kratochvil, J. M.","first_name":"J. M.","last_name":"Kratochvil"},{"first_name":"C.","full_name":"Chang, C.","last_name":"Chang"},{"full_name":"May, M.","first_name":"M.","last_name":"May"},{"last_name":"Kahn","full_name":"Kahn, S. M.","first_name":"S. M."},{"first_name":"Y.","full_name":"AlSayyad, Y.","last_name":"AlSayyad"},{"first_name":"Z.","full_name":"Ahmad, Z.","last_name":"Ahmad"},{"full_name":"Bankert, J.","first_name":"J.","last_name":"Bankert"},{"first_name":"A.","full_name":"Connolly, A.","last_name":"Connolly"},{"last_name":"Gibson","full_name":"Gibson, R. R.","first_name":"R. R."},{"last_name":"Gilmore","full_name":"Gilmore, K.","first_name":"K."},{"full_name":"Grace, E.","first_name":"E.","last_name":"Grace"},{"full_name":"Haiman, Zoltán","first_name":"Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman"},{"full_name":"Hannel, M.","first_name":"M.","last_name":"Hannel"},{"full_name":"Huffenberger, K. M.","first_name":"K. M.","last_name":"Huffenberger"},{"last_name":"Jernigan","full_name":"Jernigan, J. G.","first_name":"J. G."},{"first_name":"L.","full_name":"Jones, L.","last_name":"Jones"},{"last_name":"Krughoff","full_name":"Krughoff, S.","first_name":"S."},{"full_name":"Lorenz, S.","first_name":"S.","last_name":"Lorenz"},{"last_name":"Marshall","full_name":"Marshall, S.","first_name":"S."},{"full_name":"Meert, A.","first_name":"A.","last_name":"Meert"},{"first_name":"S.","full_name":"Nagarajan, S.","last_name":"Nagarajan"},{"first_name":"E.","full_name":"Peng, E.","last_name":"Peng"},{"first_name":"J.","full_name":"Peterson, J.","last_name":"Peterson"},{"full_name":"Rasmussen, A. P.","first_name":"A. P.","last_name":"Rasmussen"},{"last_name":"Shmakova","full_name":"Shmakova, M.","first_name":"M."},{"first_name":"N.","full_name":"Sylvestre, N.","last_name":"Sylvestre"},{"last_name":"Todd","full_name":"Todd, N.","first_name":"N."},{"full_name":"Young, M.","first_name":"M.","last_name":"Young"}],"scopus_import":"1","_id":"17670","article_number":"49","oa_version":"Preprint","arxiv":1,"publication_status":"published","month":"08","year":"2013","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","abstract":[{"lang":"eng","text":"The statistics of peak counts in reconstructed shear maps contain information beyond the power spectrum, and can improve cosmological constraints from measurements of the power spectrum alone if systematic errors can be controlled. We study the effect of galaxy shape measurement errors on predicted cosmological constraints from the statistics of shear peak counts with the Large Synoptic Survey Telescope (LSST). We use the LSST image simulator in combination with cosmological N-body simulations to model realistic shear maps for different cosmological models. We include both galaxy shape noise and, for the first time, measurement errors on galaxy shapes. We find that the measurement errors considered have relatively little impact on the constraining power of shear peak counts for LSST."}],"type":"journal_article","day":"16","quality_controlled":"1","article_type":"original","oa":1,"volume":774,"date_updated":"2024-09-25T08:04:49Z","intvolume":"       774","external_id":{"arxiv":["1301.0830"]},"title":"Effect of measurement errors on predicted cosmological constraints from shear peak statistics with large synoptic survey telescope","status":"public","publication":"The Astrophysical Journal","citation":{"ama":"Bard D, Kratochvil JM, Chang C, et al. Effect of measurement errors on predicted cosmological constraints from shear peak statistics with large synoptic survey telescope. <i>The Astrophysical Journal</i>. 2013;774(1). doi:<a href=\"https://doi.org/10.1088/0004-637x/774/1/49\">10.1088/0004-637x/774/1/49</a>","ista":"Bard D, Kratochvil JM, Chang C, May M, Kahn SM, AlSayyad Y, Ahmad Z, Bankert J, Connolly A, Gibson RR, Gilmore K, Grace E, Haiman Z, Hannel M, Huffenberger KM, Jernigan JG, Jones L, Krughoff S, Lorenz S, Marshall S, Meert A, Nagarajan S, Peng E, Peterson J, Rasmussen AP, Shmakova M, Sylvestre N, Todd N, Young M. 2013. Effect of measurement errors on predicted cosmological constraints from shear peak statistics with large synoptic survey telescope. The Astrophysical Journal. 774(1), 49.","short":"D. Bard, J.M. Kratochvil, C. Chang, M. May, S.M. Kahn, Y. AlSayyad, Z. Ahmad, J. Bankert, A. Connolly, R.R. Gibson, K. Gilmore, E. Grace, Z. Haiman, M. Hannel, K.M. Huffenberger, J.G. Jernigan, L. Jones, S. Krughoff, S. Lorenz, S. Marshall, A. Meert, S. Nagarajan, E. Peng, J. Peterson, A.P. Rasmussen, M. Shmakova, N. Sylvestre, N. Todd, M. Young, The Astrophysical Journal 774 (2013).","ieee":"D. Bard <i>et al.</i>, “Effect of measurement errors on predicted cosmological constraints from shear peak statistics with large synoptic survey telescope,” <i>The Astrophysical Journal</i>, vol. 774, no. 1. American Astronomical Society, 2013.","apa":"Bard, D., Kratochvil, J. M., Chang, C., May, M., Kahn, S. M., AlSayyad, Y., … Young, M. (2013). Effect of measurement errors on predicted cosmological constraints from shear peak statistics with large synoptic survey telescope. <i>The Astrophysical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.1088/0004-637x/774/1/49\">https://doi.org/10.1088/0004-637x/774/1/49</a>","mla":"Bard, D., et al. “Effect of Measurement Errors on Predicted Cosmological Constraints from Shear Peak Statistics with Large Synoptic Survey Telescope.” <i>The Astrophysical Journal</i>, vol. 774, no. 1, 49, American Astronomical Society, 2013, doi:<a href=\"https://doi.org/10.1088/0004-637x/774/1/49\">10.1088/0004-637x/774/1/49</a>.","chicago":"Bard, D., J. M. Kratochvil, C. Chang, M. May, S. M. Kahn, Y. AlSayyad, Z. Ahmad, et al. “Effect of Measurement Errors on Predicted Cosmological Constraints from Shear Peak Statistics with Large Synoptic Survey Telescope.” <i>The Astrophysical Journal</i>. American Astronomical Society, 2013. <a href=\"https://doi.org/10.1088/0004-637x/774/1/49\">https://doi.org/10.1088/0004-637x/774/1/49</a>."},"doi":"10.1088/0004-637x/774/1/49"},{"publisher":"American Physical Society","article_processing_charge":"No","language":[{"iso":"eng"}],"date_published":"2013-05-30T00:00:00Z","author":[{"full_name":"Bartos, Imre","first_name":"Imre","last_name":"Bartos"},{"full_name":"Haiman, Zoltán","first_name":"Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman"},{"first_name":"Bence","full_name":"Kocsis, Bence","last_name":"Kocsis"},{"first_name":"Szabolcs","full_name":"Márka, Szabolcs","last_name":"Márka"}],"scopus_import":"1","article_number":"221102","_id":"17671","issue":"22","extern":"1","date_created":"2024-09-06T07:48:38Z","main_file_link":[{"url":" https://doi.org/10.48550/arXiv.1302.3220","open_access":"1"}],"publication_identifier":{"issn":["0031-9007","1079-7114"]},"oa":1,"volume":110,"date_updated":"2024-09-25T08:25:00Z","article_type":"original","intvolume":"       110","external_id":{"arxiv":["1302.3220"]},"title":"Gas cloud G2 can illuminate the black hole population near the galactic center","status":"public","publication":"Physical Review Letters","citation":{"ama":"Bartos I, Haiman Z, Kocsis B, Márka S. Gas cloud G2 can illuminate the black hole population near the galactic center. <i>Physical Review Letters</i>. 2013;110(22). doi:<a href=\"https://doi.org/10.1103/physrevlett.110.221102\">10.1103/physrevlett.110.221102</a>","ista":"Bartos I, Haiman Z, Kocsis B, Márka S. 2013. Gas cloud G2 can illuminate the black hole population near the galactic center. Physical Review Letters. 110(22), 221102.","short":"I. Bartos, Z. Haiman, B. Kocsis, S. Márka, Physical Review Letters 110 (2013).","ieee":"I. Bartos, Z. Haiman, B. Kocsis, and S. Márka, “Gas cloud G2 can illuminate the black hole population near the galactic center,” <i>Physical Review Letters</i>, vol. 110, no. 22. American Physical Society, 2013.","apa":"Bartos, I., Haiman, Z., Kocsis, B., &#38; Márka, S. (2013). Gas cloud G2 can illuminate the black hole population near the galactic center. <i>Physical Review Letters</i>. American Physical Society. <a href=\"https://doi.org/10.1103/physrevlett.110.221102\">https://doi.org/10.1103/physrevlett.110.221102</a>","mla":"Bartos, Imre, et al. “Gas Cloud G2 Can Illuminate the Black Hole Population near the Galactic Center.” <i>Physical Review Letters</i>, vol. 110, no. 22, 221102, American Physical Society, 2013, doi:<a href=\"https://doi.org/10.1103/physrevlett.110.221102\">10.1103/physrevlett.110.221102</a>.","chicago":"Bartos, Imre, Zoltán Haiman, Bence Kocsis, and Szabolcs Márka. “Gas Cloud G2 Can Illuminate the Black Hole Population near the Galactic Center.” <i>Physical Review Letters</i>. American Physical Society, 2013. <a href=\"https://doi.org/10.1103/physrevlett.110.221102\">https://doi.org/10.1103/physrevlett.110.221102</a>."},"doi":"10.1103/physrevlett.110.221102","oa_version":"Preprint","arxiv":1,"publication_status":"published","year":"2013","month":"05","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","day":"30","quality_controlled":"1","abstract":[{"text":"Galactic nuclei are expected to be densely populated with stellar and intermediate mass black holes. Exploring this population will have important consequences for the observation prospects of gravitational waves as well as understanding galactic evolution. The gas cloud G2 currently approaching Sgr A* provides an unprecedented opportunity to probe the black hole and neutron star population of the Galactic nucleus. We examine the possibility of a G2-black hole encounter and its detectability with current X-ray satellites, such as Chandra and NuSTAR. We find that multiple encounters are likely to occur close to the pericenter, which may be detectable upon favorable circumstances. This opportunity provides an additional, important science case for leading X-ray observatories to closely follow G2 on its way to the nucleus.","lang":"eng"}],"type":"journal_article"}]