---
_id: '2478'
abstract:
- lang: eng
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.
author:
- first_name: Elaine
full_name: Budreck, Elaine C
last_name: Budreck
- first_name: Oh
full_name: Kwon, Oh-Bin
last_name: Kwon
- first_name: Jung
full_name: Jung, Jung-Hoon
last_name: Jung
- first_name: Stéphane
full_name: Baudouin, Stéphane J
last_name: Baudouin
- first_name: Albert
full_name: Thommen, Albert
last_name: Thommen
- first_name: Hye
full_name: Kim, Hye-Sun
last_name: Kim
- first_name: Yugo
full_name: Fukazawa, Yugo
last_name: Fukazawa
- first_name: Harumi
full_name: Harumi Harada
id: 2E55CDF2-F248-11E8-B48F-1D18A9856A87
last_name: Harada
orcid: 0000-0001-7429-7896
- first_name: Katsuhiko
full_name: Tabuchi, Katsuhiko
last_name: Tabuchi
- first_name: Ryuichi
full_name: Ryuichi Shigemoto
id: 499F3ABC-F248-11E8-B48F-1D18A9856A87
last_name: Shigemoto
orcid: 0000-0001-8761-9444
- first_name: Peter
full_name: Scheiffele, Peter
last_name: Scheiffele
- first_name: Joung
full_name: Kim, Joung-Hun
last_name: Kim
citation:
ama: Budreck E, Kwon O, Jung J, et al. Neuroligin-1 controls synaptic abundance
of NMDA-type glutamate receptors through extracellular coupling. PNAS.
2013;110(2):725-730. doi:10.1073/pnas.1214718110
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. PNAS. National Academy of Sciences. https://doi.org/10.1073/pnas.1214718110
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.” PNAS. National Academy
of Sciences, 2013. https://doi.org/10.1073/pnas.1214718110.
ieee: E. Budreck et al., “Neuroligin-1 controls synaptic abundance of NMDA-type
glutamate receptors through extracellular coupling,” PNAS, vol. 110, no.
2. National Academy of Sciences, pp. 725–730, 2013.
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.
mla: Budreck, Elaine, et al. “Neuroligin-1 Controls Synaptic Abundance of NMDA-Type
Glutamate Receptors through Extracellular Coupling.” PNAS, vol. 110, no.
2, National Academy of Sciences, 2013, pp. 725–30, doi:10.1073/pnas.1214718110.
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.
date_created: 2018-12-11T11:57:54Z
date_published: 2013-01-08T00:00:00Z
date_updated: 2021-01-12T06:57:43Z
day: '08'
doi: 10.1073/pnas.1214718110
extern: 1
intvolume: ' 110'
issue: '2'
month: '01'
page: 725 - 730
publication: PNAS
publication_status: published
publisher: National Academy of Sciences
publist_id: '4423'
quality_controlled: 0
status: public
title: Neuroligin-1 controls synaptic abundance of NMDA-type glutamate receptors through
extracellular coupling
type: journal_article
volume: 110
year: '2013'
...
---
_id: '250'
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.
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.
author:
- first_name: Régis
full_name: de la Bretèche, Régis
last_name: De La Bretèche
- first_name: Timothy D
full_name: Timothy Browning
id: 35827D50-F248-11E8-B48F-1D18A9856A87
last_name: Browning
orcid: 0000-0002-8314-0177
citation:
ama: De La Bretèche R, Browning TD. Density of Châtelet surfaces failing the Hasse
principle. Proceedings of the London Mathematical Society. 2013;108(4):1030-1078.
doi:10.1112/plms/pdt060
apa: De La Bretèche, R., & Browning, T. D. (2013). Density of Châtelet surfaces
failing the Hasse principle. Proceedings of the London Mathematical Society.
Oxford University Press. https://doi.org/10.1112/plms/pdt060
chicago: De La Bretèche, Régis, and Timothy D Browning. “Density of Châtelet Surfaces
Failing the Hasse Principle.” Proceedings of the London Mathematical Society.
Oxford University Press, 2013. https://doi.org/10.1112/plms/pdt060.
ieee: R. De La Bretèche and T. D. Browning, “Density of Châtelet surfaces failing
the Hasse principle,” Proceedings of the London Mathematical Society, vol.
108, no. 4. Oxford University Press, pp. 1030–1078, 2013.
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.
mla: De La Bretèche, Régis, and Timothy D. Browning. “Density of Châtelet Surfaces
Failing the Hasse Principle.” Proceedings of the London Mathematical Society,
vol. 108, no. 4, Oxford University Press, 2013, pp. 1030–78, doi:10.1112/plms/pdt060.
short: R. De La Bretèche, T.D. Browning, Proceedings of the London Mathematical
Society 108 (2013) 1030–1078.
date_created: 2018-12-11T11:45:26Z
date_published: 2013-11-29T00:00:00Z
date_updated: 2021-01-12T06:57:51Z
day: '29'
doi: 10.1112/plms/pdt060
extern: 1
intvolume: ' 108'
issue: '4'
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1210.4010
month: '11'
oa: 1
page: 1030 - 1078
publication: Proceedings of the London Mathematical Society
publication_status: published
publisher: Oxford University Press
publist_id: '7652'
quality_controlled: 0
status: public
title: Density of Châtelet surfaces failing the Hasse principle
type: journal_article
volume: 108
year: '2013'
...
---
_id: '251'
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].
author:
- first_name: Régis
full_name: de la Bretèche, Régis
last_name: De La Bretèche
- first_name: Timothy D
full_name: Timothy Browning
id: 35827D50-F248-11E8-B48F-1D18A9856A87
last_name: Browning
orcid: 0000-0002-8314-0177
citation:
ama: De La Bretèche R, Browning TD. Counter examples to the Hasse principle among
certain coflasque tori. Journal de Theorie des Nombres de Bordeaux. 2013;26(1):25-44.
doi:10.5802/jtnb.857
apa: De La Bretèche, R., & Browning, T. D. (2013). Counter examples to the Hasse
principle among certain coflasque tori. Journal de Theorie Des Nombres de Bordeaux.
Universite de Bordeaux I. https://doi.org/10.5802/jtnb.857
chicago: De La Bretèche, Régis, and Timothy D Browning. “Counter Examples to the
Hasse Principle among Certain Coflasque Tori.” Journal de Theorie Des Nombres
de Bordeaux. Universite de Bordeaux I, 2013. https://doi.org/10.5802/jtnb.857.
ieee: R. De La Bretèche and T. D. Browning, “Counter examples to the Hasse principle
among certain coflasque tori,” Journal de Theorie des Nombres de Bordeaux,
vol. 26, no. 1. Universite de Bordeaux I, pp. 25–44, 2013.
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.
mla: De La Bretèche, Régis, and Timothy D. Browning. “Counter Examples to the Hasse
Principle among Certain Coflasque Tori.” Journal de Theorie Des Nombres de
Bordeaux, vol. 26, no. 1, Universite de Bordeaux I, 2013, pp. 25–44, doi:10.5802/jtnb.857.
short: R. De La Bretèche, T.D. Browning, Journal de Theorie Des Nombres de Bordeaux
26 (2013) 25–44.
date_created: 2018-12-11T11:45:26Z
date_published: 2013-05-14T00:00:00Z
date_updated: 2021-01-12T06:57:55Z
day: '14'
doi: 10.5802/jtnb.857
extern: 1
intvolume: ' 26'
issue: '1'
month: '05'
page: 25 - 44
publication: Journal de Theorie des Nombres de Bordeaux
publication_status: published
publisher: Universite de Bordeaux I
publist_id: '7651'
quality_controlled: 0
status: public
title: Counter examples to the Hasse principle among certain coflasque tori
type: journal_article
volume: 26
year: '2013'
...
---
_id: '2516'
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.'
article_processing_charge: No
author:
- first_name: Christoph
full_name: Lampert, Christoph
id: 40C20FD2-F248-11E8-B48F-1D18A9856A87
last_name: Lampert
orcid: 0000-0001-8622-7887
- first_name: Hannes
full_name: Nickisch, Hannes
last_name: Nickisch
- first_name: Stefan
full_name: Harmeling, Stefan
last_name: Harmeling
citation:
ama: Lampert C, Nickisch H, Harmeling S. Attribute-based classification for zero-shot
learning of object categories. IEEE Transactions on Pattern Analysis and Machine
Intelligence. 2013;36(3):453-465. doi:10.1109/TPAMI.2013.140
apa: 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. IEEE. https://doi.org/10.1109/TPAMI.2013.140
chicago: Lampert, Christoph, Hannes Nickisch, and Stefan Harmeling. “Attribute-Based
Classification for Zero-Shot Learning of Object Categories.” IEEE Transactions
on Pattern Analysis and Machine Intelligence. IEEE, 2013. https://doi.org/10.1109/TPAMI.2013.140.
ieee: C. Lampert, H. Nickisch, and S. Harmeling, “Attribute-based classification
for zero-shot learning of object categories,” IEEE Transactions on Pattern
Analysis and Machine Intelligence, vol. 36, no. 3. IEEE, pp. 453–465, 2013.
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.
mla: Lampert, Christoph, et al. “Attribute-Based Classification for Zero-Shot Learning
of Object Categories.” IEEE Transactions on Pattern Analysis and Machine Intelligence,
vol. 36, no. 3, IEEE, 2013, pp. 453–65, doi:10.1109/TPAMI.2013.140.
short: C. Lampert, H. Nickisch, S. Harmeling, IEEE Transactions on Pattern Analysis
and Machine Intelligence 36 (2013) 453–465.
date_created: 2018-12-11T11:58:08Z
date_published: 2013-07-30T00:00:00Z
date_updated: 2025-09-29T14:09:57Z
day: '30'
department:
- _id: ChLa
doi: 10.1109/TPAMI.2013.140
external_id:
isi:
- '000331450100005'
intvolume: ' 36'
isi: 1
issue: '3'
language:
- iso: eng
month: '07'
oa_version: None
page: 453 - 465
publication: IEEE Transactions on Pattern Analysis and Machine Intelligence
publication_status: published
publisher: IEEE
publist_id: '4385'
quality_controlled: '1'
scopus_import: '1'
status: public
title: Attribute-based classification for zero-shot learning of object categories
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 36
year: '2013'
...
---
_id: '2517'
abstract:
- lang: eng
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.'
acknowledgement: 'ERC Grant QUALITY. '
alternative_title:
- LNCS
article_processing_charge: No
author:
- first_name: Shaull
full_name: Almagor, Shaull
last_name: Almagor
- first_name: Udi
full_name: Boker, Udi
id: 31E297B6-F248-11E8-B48F-1D18A9856A87
last_name: Boker
- first_name: Orna
full_name: Kupferman, Orna
last_name: Kupferman
citation:
ama: Almagor S, Boker U, Kupferman O. Formalizing and reasoning about quality. 2013;7966(Part
2):15-27. doi:10.1007/978-3-642-39212-2_3
apa: 'Almagor, S., Boker, U., & Kupferman, O. (2013). Formalizing and reasoning
about quality. Presented at the ICALP: Automata, Languages and Programming, Riga,
Latvia: Springer. https://doi.org/10.1007/978-3-642-39212-2_3'
chicago: Almagor, Shaull, Udi Boker, and Orna Kupferman. “Formalizing and Reasoning
about Quality.” Lecture Notes in Computer Science. Springer, 2013. https://doi.org/10.1007/978-3-642-39212-2_3.
ieee: S. Almagor, U. Boker, and O. Kupferman, “Formalizing and reasoning about quality,”
vol. 7966, no. Part 2. Springer, pp. 15–27, 2013.
ista: Almagor S, Boker U, Kupferman O. 2013. Formalizing and reasoning about quality.
7966(Part 2), 15–27.
mla: Almagor, Shaull, et al. Formalizing and Reasoning about Quality. Vol.
7966, no. Part 2, Springer, 2013, pp. 15–27, doi:10.1007/978-3-642-39212-2_3.
short: S. Almagor, U. Boker, O. Kupferman, 7966 (2013) 15–27.
conference:
end_date: 2013-07-12
location: Riga, Latvia
name: 'ICALP: Automata, Languages and Programming'
start_date: 2013-07-08
date_created: 2018-12-11T11:58:08Z
date_published: 2013-07-01T00:00:00Z
date_updated: 2020-08-11T10:09:47Z
day: '01'
ddc:
- '000'
department:
- _id: ToHe
doi: 10.1007/978-3-642-39212-2_3
ec_funded: 1
file:
- access_level: open_access
checksum: 85afbf6c18a2c7e377c52c9410e2d824
content_type: application/pdf
creator: dernst
date_created: 2020-05-15T11:16:12Z
date_updated: 2020-07-14T12:45:42Z
file_id: '7860'
file_name: 2013_ICALP_Almagor.pdf
file_size: 363031
relation: main_file
file_date_updated: 2020-07-14T12:45:42Z
has_accepted_license: '1'
intvolume: ' 7966'
issue: Part 2
language:
- iso: eng
month: '07'
oa: 1
oa_version: Submitted Version
page: 15 - 27
project:
- _id: 25832EC2-B435-11E9-9278-68D0E5697425
call_identifier: FWF
grant_number: S 11407_N23
name: Rigorous Systems Engineering
- _id: 25EE3708-B435-11E9-9278-68D0E5697425
call_identifier: FP7
grant_number: '267989'
name: Quantitative Reactive Modeling
publication_status: published
publisher: Springer
publist_id: '4384'
quality_controlled: '1'
scopus_import: 1
series_title: Lecture Notes in Computer Science
status: public
title: Formalizing and reasoning about quality
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 7966
year: '2013'
...
---
_id: '2518'
abstract:
- lang: eng
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.
alternative_title:
- LNCS
arxiv: 1
author:
- first_name: Vladimir
full_name: Kolmogorov, Vladimir
id: 3D50B0BA-F248-11E8-B48F-1D18A9856A87
last_name: Kolmogorov
citation:
ama: 'Kolmogorov V. The power of linear programming for finite-valued CSPs: A constructive
characterization. In: Vol 7965. Springer; 2013:625-636. doi:10.1007/978-3-642-39206-1_53'
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. https://doi.org/10.1007/978-3-642-39206-1_53'
chicago: 'Kolmogorov, Vladimir. “The Power of Linear Programming for Finite-Valued
CSPs: A Constructive Characterization,” 7965:625–36. Springer, 2013. https://doi.org/10.1007/978-3-642-39206-1_53.'
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.'
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.'
mla: 'Kolmogorov, Vladimir. The Power of Linear Programming for Finite-Valued
CSPs: A Constructive Characterization. Vol. 7965, no. 1, Springer, 2013, pp.
625–36, doi:10.1007/978-3-642-39206-1_53.'
short: V. Kolmogorov, in:, Springer, 2013, pp. 625–636.
conference:
end_date: 2013-07-12
location: Riga, Latvia
name: 'ICALP: Automata, Languages and Programming'
start_date: 2013-07-08
corr_author: '1'
date_created: 2018-12-11T11:58:08Z
date_published: 2013-07-01T00:00:00Z
date_updated: 2025-09-23T14:14:56Z
day: '01'
department:
- _id: VlKo
doi: 10.1007/978-3-642-39206-1_53
external_id:
arxiv:
- '1207.7213'
intvolume: ' 7965'
issue: '1'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: http://arxiv.org/abs/1207.7213
month: '07'
oa: 1
oa_version: Preprint
page: 625 - 636
publication_status: published
publisher: Springer
publist_id: '4383'
quality_controlled: '1'
related_material:
record:
- id: '2271'
relation: later_version
status: public
scopus_import: 1
status: public
title: 'The power of linear programming for finite-valued CSPs: A constructive characterization'
type: conference
user_id: 3E5EF7F0-F248-11E8-B48F-1D18A9856A87
volume: 7965
year: '2013'
...
---
_id: '2520'
abstract:
- lang: eng
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."
author:
- first_name: Novi
full_name: Quadrianto, Novi
last_name: Quadrianto
- first_name: Viktoriia
full_name: Sharmanska, Viktoriia
id: 2EA6D09E-F248-11E8-B48F-1D18A9856A87
last_name: Sharmanska
orcid: 0000-0003-0192-9308
- first_name: David
full_name: Knowles, David
last_name: Knowles
- first_name: Zoubin
full_name: Ghahramani, Zoubin
last_name: Ghahramani
citation:
ama: 'Quadrianto N, Sharmanska V, Knowles D, Ghahramani Z. The supervised IBP: Neighbourhood
preserving infinite latent feature models. In: Proceedings of the 29th Conference
Uncertainty in Artificial Intelligence. AUAI Press; 2013:527-536.'
apa: 'Quadrianto, N., Sharmanska, V., Knowles, D., & Ghahramani, Z. (2013).
The supervised IBP: Neighbourhood preserving infinite latent feature models. In
Proceedings of the 29th conference uncertainty in Artificial Intelligence
(pp. 527–536). Bellevue, WA, United States: AUAI Press.'
chicago: 'Quadrianto, Novi, Viktoriia Sharmanska, David Knowles, and Zoubin Ghahramani.
“The Supervised IBP: Neighbourhood Preserving Infinite Latent Feature Models.”
In Proceedings of the 29th Conference Uncertainty in Artificial Intelligence,
527–36. AUAI Press, 2013.'
ieee: 'N. Quadrianto, V. Sharmanska, D. Knowles, and Z. Ghahramani, “The supervised
IBP: Neighbourhood preserving infinite latent feature models,” in Proceedings
of the 29th conference uncertainty in Artificial Intelligence, Bellevue, WA,
United States, 2013, pp. 527–536.'
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.'
mla: 'Quadrianto, Novi, et al. “The Supervised IBP: Neighbourhood Preserving Infinite
Latent Feature Models.” Proceedings of the 29th Conference Uncertainty in Artificial
Intelligence, AUAI Press, 2013, pp. 527–36.'
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.
conference:
end_date: 2013-07-15
location: Bellevue, WA, United States
name: 'UAI: Uncertainty in Artificial Intelligence'
start_date: 2013-07-11
date_created: 2018-12-11T11:58:09Z
date_published: 2013-07-11T00:00:00Z
date_updated: 2023-02-23T10:46:36Z
day: '11'
ddc:
- '000'
department:
- _id: ChLa
file:
- access_level: open_access
checksum: 325f20c4b926bd74d39006b97df572bd
content_type: application/pdf
creator: system
date_created: 2018-12-12T10:15:16Z
date_updated: 2020-07-14T12:45:42Z
file_id: '5134'
file_name: IST-2013-137-v1+1_QuaShaKnoGha13.pdf
file_size: 1117100
relation: main_file
file_date_updated: 2020-07-14T12:45:42Z
has_accepted_license: '1'
language:
- iso: eng
month: '07'
oa: 1
oa_version: Submitted Version
page: 527 - 536
publication: Proceedings of the 29th conference uncertainty in Artificial Intelligence
publication_identifier:
isbn:
- '9780974903996'
publication_status: published
publisher: AUAI Press
publist_id: '4381'
pubrep_id: '137'
quality_controlled: '1'
scopus_import: 1
status: public
title: 'The supervised IBP: Neighbourhood preserving infinite latent feature models'
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2013'
...
---
_id: '253'
author:
- first_name: Timothy D
full_name: Timothy Browning
id: 35827D50-F248-11E8-B48F-1D18A9856A87
last_name: Browning
orcid: 0000-0002-8314-0177
citation:
ama: 'Browning TD. Counting rational points on cubic hypersurfaces: Corrigendum.
Mathematika. 2013;60(1):101-107. doi:10.1112/S0025579313000132'
apa: 'Browning, T. D. (2013). Counting rational points on cubic hypersurfaces: Corrigendum.
Mathematika. Unknown. https://doi.org/10.1112/S0025579313000132'
chicago: 'Browning, Timothy D. “Counting Rational Points on Cubic Hypersurfaces:
Corrigendum.” Mathematika. Unknown, 2013. https://doi.org/10.1112/S0025579313000132.'
ieee: 'T. D. Browning, “Counting rational points on cubic hypersurfaces: Corrigendum,”
Mathematika, vol. 60, no. 1. Unknown, pp. 101–107, 2013.'
ista: 'Browning TD. 2013. Counting rational points on cubic hypersurfaces: Corrigendum.
Mathematika. 60(1), 101–107.'
mla: 'Browning, Timothy D. “Counting Rational Points on Cubic Hypersurfaces: Corrigendum.”
Mathematika, vol. 60, no. 1, Unknown, 2013, pp. 101–07, doi:10.1112/S0025579313000132.'
short: T.D. Browning, Mathematika 60 (2013) 101–107.
date_created: 2018-12-11T11:45:27Z
date_published: 2013-09-06T00:00:00Z
date_updated: 2021-01-12T06:58:03Z
day: '06'
doi: 10.1112/S0025579313000132
extern: 1
intvolume: ' 60'
issue: '1'
month: '09'
page: 101 - 107
publication: Mathematika
publication_status: published
publisher: Unknown
publist_id: '7649'
quality_controlled: 0
status: public
title: 'Counting rational points on cubic hypersurfaces: Corrigendum'
type: journal_article
volume: 60
year: '2013'
...
---
_id: '1726'
abstract:
- lang: eng
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.
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
author:
- first_name: Nitza
full_name: Kahane, Nitza
last_name: Kahane
- first_name: Vanessa
full_name: Ribes, Vanessa
last_name: Ribes
- first_name: Anna
full_name: Anna Kicheva
id: 3959A2A0-F248-11E8-B48F-1D18A9856A87
last_name: Kicheva
orcid: 0000-0003-4509-4998
- first_name: James
full_name: Briscoe, James
last_name: Briscoe
- first_name: Chaya
full_name: Kalcheim, Chaya
last_name: Kalcheim
citation:
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. Development. 2013;140(8):1740-1750. doi:10.1242/dev.092726
apa: 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. Company
of Biologists. https://doi.org/10.1242/dev.092726
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.” Development. Company
of Biologists, 2013. https://doi.org/10.1242/dev.092726.
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,” Development, vol. 140, no.
8. Company of Biologists, pp. 1740–1750, 2013.
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.
mla: Kahane, Nitza, et al. “The Transition from Differentiation to Growth during
Dermomyotome-Derived Myogenesis Depends on Temporally Restricted Hedgehog Signaling.”
Development, vol. 140, no. 8, Company of Biologists, 2013, pp. 1740–50,
doi:10.1242/dev.092726.
short: N. Kahane, V. Ribes, A. Kicheva, J. Briscoe, C. Kalcheim, Development 140
(2013) 1740–1750.
date_created: 2018-12-11T11:53:41Z
date_published: 2013-04-18T00:00:00Z
date_updated: 2021-01-12T06:52:47Z
day: '18'
doi: 10.1242/dev.092726
extern: 1
intvolume: ' 140'
issue: '8'
month: '04'
page: 1740 - 1750
publication: Development
publication_status: published
publisher: Company of Biologists
publist_id: '5402'
quality_controlled: 0
status: public
title: The transition from differentiation to growth during dermomyotome-derived myogenesis
depends on temporally restricted hedgehog signaling
type: journal_article
volume: 140
year: '2013'
...
---
_id: '1727'
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.'
author:
- first_name: Anna
full_name: Anna Kicheva
id: 3959A2A0-F248-11E8-B48F-1D18A9856A87
last_name: Kicheva
orcid: 0000-0003-4509-4998
- first_name: Laurent
full_name: Holtzer, Laurent
last_name: Holtzer
- first_name: Ortrud
full_name: Wartlick, Ortrud
last_name: Wartlick
- first_name: Thomas
full_name: Schmidt, Thomas S
last_name: Schmidt
- first_name: Marcos
full_name: González-Gaitán, Marcos A
last_name: González Gaitán
citation:
ama: Kicheva A, Holtzer L, Wartlick O, Schmidt T, González Gaitán M. Quantitative
imaging of morphogen gradients in drosophila imaginal discs. Cold Spring Harbor
Protocols. 2013;8(5):387-403. doi:10.1101/pdb.top074237
apa: 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. Cold Spring Harbor Laboratory Press.
https://doi.org/10.1101/pdb.top074237
chicago: Kicheva, Anna, Laurent Holtzer, Ortrud Wartlick, Thomas Schmidt, and Marcos
González Gaitán. “Quantitative Imaging of Morphogen Gradients in Drosophila Imaginal
Discs.” Cold Spring Harbor Protocols. Cold Spring Harbor Laboratory Press,
2013. https://doi.org/10.1101/pdb.top074237.
ieee: A. Kicheva, L. Holtzer, O. Wartlick, T. Schmidt, and M. González Gaitán, “Quantitative
imaging of morphogen gradients in drosophila imaginal discs,” Cold Spring Harbor
Protocols, vol. 8, no. 5. Cold Spring Harbor Laboratory Press, pp. 387–403,
2013.
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.
mla: Kicheva, Anna, et al. “Quantitative Imaging of Morphogen Gradients in Drosophila
Imaginal Discs.” Cold Spring Harbor Protocols, vol. 8, no. 5, Cold Spring
Harbor Laboratory Press, 2013, pp. 387–403, doi:10.1101/pdb.top074237.
short: A. Kicheva, L. Holtzer, O. Wartlick, T. Schmidt, M. González Gaitán, Cold
Spring Harbor Protocols 8 (2013) 387–403.
date_created: 2018-12-11T11:53:41Z
date_published: 2013-05-01T00:00:00Z
date_updated: 2021-01-12T06:52:47Z
day: '01'
doi: 10.1101/pdb.top074237
extern: 1
intvolume: ' 8'
issue: '5'
month: '05'
page: 387 - 403
publication: Cold Spring Harbor Protocols
publication_status: published
publisher: Cold Spring Harbor Laboratory Press
publist_id: '5401'
quality_controlled: 0
status: public
title: Quantitative imaging of morphogen gradients in drosophila imaginal discs
type: journal_article
volume: 8
year: '2013'
...
---
_id: '1759'
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
author:
- first_name: Natalia
full_name: Ares, Natalia
last_name: Ares
- first_name: Vitaly
full_name: Golovach, Vitaly N
last_name: Golovach
- first_name: Georgios
full_name: Georgios Katsaros
id: 38DB5788-F248-11E8-B48F-1D18A9856A87
last_name: Katsaros
- first_name: Mathieu
full_name: Stoffel, Mathieu
last_name: Stoffel
- first_name: Frank
full_name: Fournel, Frank
last_name: Fournel
- first_name: Leonid
full_name: Glazman, Leonid I
last_name: Glazman
- first_name: Oliver
full_name: Schmidt, Oliver G
last_name: Schmidt
- first_name: Silvano
full_name: De Franceschi, Silvano
last_name: De Franceschi
citation:
ama: Ares N, Golovach V, Katsaros G, et al. Nature of tunable hole g factors in
quantum dots. Physical Review Letters. 2013;110(4). doi:10.1103/PhysRevLett.110.046602
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.
Physical Review Letters. American Physical Society. https://doi.org/10.1103/PhysRevLett.110.046602
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.” Physical Review Letters. American
Physical Society, 2013. https://doi.org/10.1103/PhysRevLett.110.046602.
ieee: N. Ares et al., “Nature of tunable hole g factors in quantum dots,”
Physical Review Letters, vol. 110, no. 4. American Physical Society, 2013.
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).
mla: Ares, Natalia, et al. “Nature of Tunable Hole g Factors in Quantum Dots.” Physical
Review Letters, vol. 110, no. 4, American Physical Society, 2013, doi:10.1103/PhysRevLett.110.046602.
short: N. Ares, V. Golovach, G. Katsaros, M. Stoffel, F. Fournel, L. Glazman, O.
Schmidt, S. De Franceschi, Physical Review Letters 110 (2013).
date_created: 2018-12-11T11:53:51Z
date_published: 2013-01-23T00:00:00Z
date_updated: 2021-01-12T06:53:01Z
day: '23'
doi: 10.1103/PhysRevLett.110.046602
extern: 1
intvolume: ' 110'
issue: '4'
main_file_link:
- open_access: '1'
url: http://arxiv.org/abs/1208.0476
month: '01'
oa: 1
publication: Physical Review Letters
publication_status: published
publisher: American Physical Society
publist_id: '5365'
quality_controlled: 0
status: public
title: Nature of tunable hole g factors in quantum dots
type: journal_article
volume: 110
year: '2013'
...
---
_id: '1760'
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.
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
author:
- first_name: Natalia
full_name: Ares, Natalia
last_name: Ares
- first_name: Georgios
full_name: Georgios Katsaros
id: 38DB5788-F248-11E8-B48F-1D18A9856A87
last_name: Katsaros
- first_name: Vitaly
full_name: Golovach, Vitaly N
last_name: Golovach
- first_name: Jianjun
full_name: Zhang, Jianjun
last_name: Zhang
- first_name: Aaron
full_name: Prager, Aaron A
last_name: Prager
- first_name: Leonid
full_name: Glazman, Leonid I
last_name: Glazman
- first_name: Oliver
full_name: Schmidt, Oliver G
last_name: Schmidt
- first_name: Silvano
full_name: De Franceschi, Silvano
last_name: De Franceschi
citation:
ama: Ares N, Katsaros G, Golovach V, et al. SiGe quantum dots for fast hole spin
Rabi oscillations. Applied Physics Letters. 2013;103(26). doi:10.1063/1.4858959
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.
Applied Physics Letters. American Institute of Physics. https://doi.org/10.1063/1.4858959
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.” Applied Physics Letters. American
Institute of Physics, 2013. https://doi.org/10.1063/1.4858959.
ieee: N. Ares et al., “SiGe quantum dots for fast hole spin Rabi oscillations,”
Applied Physics Letters, vol. 103, no. 26. American Institute of Physics,
2013.
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).
mla: Ares, Natalia, et al. “SiGe Quantum Dots for Fast Hole Spin Rabi Oscillations.”
Applied Physics Letters, vol. 103, no. 26, American Institute of Physics,
2013, doi:10.1063/1.4858959.
short: N. Ares, G. Katsaros, V. Golovach, J. Zhang, A. Prager, L. Glazman, O. Schmidt,
S. De Franceschi, Applied Physics Letters 103 (2013).
date_created: 2018-12-11T11:53:52Z
date_published: 2013-01-23T00:00:00Z
date_updated: 2021-01-12T06:53:02Z
day: '23'
doi: 10.1063/1.4858959
extern: 1
intvolume: ' 103'
issue: '26'
main_file_link:
- open_access: '1'
url: http://arxiv.org/abs/1307.7196
month: '01'
oa: 1
publication: Applied Physics Letters
publication_status: published
publisher: American Institute of Physics
publist_id: '5364'
quality_controlled: 0
status: public
title: SiGe quantum dots for fast hole spin Rabi oscillations
type: journal_article
volume: 103
year: '2013'
...
---
_id: '17624'
abstract:
- lang: eng
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.'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Daniel J.
full_name: D'Orazio, Daniel J.
last_name: D'Orazio
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
- first_name: Andrew
full_name: MacFadyen, Andrew
last_name: MacFadyen
citation:
ama: D’Orazio DJ, Haiman Z, MacFadyen A. Accretion into the central cavity of a
circumbinary disc. Monthly Notices of the Royal Astronomical Society. 2013;436(4):2997-3020.
doi:10.1093/mnras/stt1787
apa: D’Orazio, D. J., Haiman, Z., & MacFadyen, A. (2013). Accretion into the
central cavity of a circumbinary disc. Monthly Notices of the Royal Astronomical
Society. Oxford University Press. https://doi.org/10.1093/mnras/stt1787
chicago: D’Orazio, Daniel J., Zoltán Haiman, and Andrew MacFadyen. “Accretion into
the Central Cavity of a Circumbinary Disc.” Monthly Notices of the Royal Astronomical
Society. Oxford University Press, 2013. https://doi.org/10.1093/mnras/stt1787.
ieee: D. J. D’Orazio, Z. Haiman, and A. MacFadyen, “Accretion into the central cavity
of a circumbinary disc,” Monthly Notices of the Royal Astronomical Society,
vol. 436, no. 4. Oxford University Press, pp. 2997–3020, 2013.
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.
mla: D’Orazio, Daniel J., et al. “Accretion into the Central Cavity of a Circumbinary
Disc.” Monthly Notices of the Royal Astronomical Society, vol. 436, no.
4, Oxford University Press, 2013, pp. 2997–3020, doi:10.1093/mnras/stt1787.
short: D.J. D’Orazio, Z. Haiman, A. MacFadyen, Monthly Notices of the Royal Astronomical
Society 436 (2013) 2997–3020.
date_created: 2024-09-05T13:53:11Z
date_published: 2013-10-18T00:00:00Z
date_updated: 2024-09-24T08:47:58Z
day: '18'
doi: 10.1093/mnras/stt1787
extern: '1'
external_id:
arxiv:
- '1210.0536'
intvolume: ' 436'
issue: '4'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: ' https://doi.org/10.48550/arXiv.1210.0536'
month: '10'
oa: 1
oa_version: Preprint
page: 2997-3020
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
issn:
- 1365-2966
- 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: Accretion into the central cavity of a circumbinary disc
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 436
year: '2013'
...
---
_id: '17631'
abstract:
- lang: eng
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.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Fabio
full_name: Pacucci, Fabio
last_name: Pacucci
- first_name: Andrei
full_name: Mesinger, Andrei
last_name: Mesinger
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
citation:
ama: 'Pacucci F, Mesinger A, Haiman Z. Focusing on warm dark matter with lensed
high-redshift galaxies. Monthly Notices of the Royal Astronomical Society:
Letters. 2013;435(1):L53-L57. doi:10.1093/mnrasl/slt093'
apa: '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. Oxford University Press. https://doi.org/10.1093/mnrasl/slt093'
chicago: 'Pacucci, Fabio, Andrei Mesinger, and Zoltán Haiman. “Focusing on Warm
Dark Matter with Lensed High-Redshift Galaxies.” Monthly Notices of the Royal
Astronomical Society: Letters. Oxford University Press, 2013. https://doi.org/10.1093/mnrasl/slt093.'
ieee: 'F. Pacucci, A. Mesinger, and Z. Haiman, “Focusing on warm dark matter with
lensed high-redshift galaxies,” Monthly Notices of the Royal Astronomical Society:
Letters, vol. 435, no. 1. Oxford University Press, pp. L53–L57, 2013.'
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.'
mla: 'Pacucci, Fabio, et al. “Focusing on Warm Dark Matter with Lensed High-Redshift
Galaxies.” Monthly Notices of the Royal Astronomical Society: Letters,
vol. 435, no. 1, Oxford University Press, 2013, pp. L53–57, doi:10.1093/mnrasl/slt093.'
short: 'F. Pacucci, A. Mesinger, Z. Haiman, Monthly Notices of the Royal Astronomical
Society: Letters 435 (2013) L53–L57.'
date_created: 2024-09-05T14:00:29Z
date_published: 2013-08-09T00:00:00Z
date_updated: 2024-09-24T09:59:26Z
day: '09'
doi: 10.1093/mnrasl/slt093
extern: '1'
external_id:
arxiv:
- '1306.0009'
intvolume: ' 435'
issue: '1'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: ' https://doi.org/10.48550/arXiv.1306.0009'
month: '08'
oa: 1
oa_version: Preprint
page: L53-L57
publication: 'Monthly Notices of the Royal Astronomical Society: Letters'
publication_identifier:
issn:
- 1745-3933
- 1745-3925
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: Focusing on warm dark matter with lensed high-redshift galaxies
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 435
year: '2013'
...
---
_id: '17638'
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.
article_number: '224012'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Takamitsu L
full_name: Tanaka, Takamitsu L
last_name: Tanaka
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
citation:
ama: Tanaka TL, Haiman Z. Electromagnetic signatures of supermassive black hole
binaries resolved by PTAs. Classical and Quantum Gravity. 2013;30(22).
doi:10.1088/0264-9381/30/22/224012
apa: Tanaka, T. L., & Haiman, Z. (2013). Electromagnetic signatures of supermassive
black hole binaries resolved by PTAs. Classical and Quantum Gravity. IOP
Publishing. https://doi.org/10.1088/0264-9381/30/22/224012
chicago: Tanaka, Takamitsu L, and Zoltán Haiman. “Electromagnetic Signatures of
Supermassive Black Hole Binaries Resolved by PTAs.” Classical and Quantum Gravity.
IOP Publishing, 2013. https://doi.org/10.1088/0264-9381/30/22/224012.
ieee: T. L. Tanaka and Z. Haiman, “Electromagnetic signatures of supermassive black
hole binaries resolved by PTAs,” Classical and Quantum Gravity, vol. 30,
no. 22. IOP Publishing, 2013.
ista: Tanaka TL, Haiman Z. 2013. Electromagnetic signatures of supermassive black
hole binaries resolved by PTAs. Classical and Quantum Gravity. 30(22), 224012.
mla: Tanaka, Takamitsu L., and Zoltán Haiman. “Electromagnetic Signatures of Supermassive
Black Hole Binaries Resolved by PTAs.” Classical and Quantum Gravity, vol.
30, no. 22, 224012, IOP Publishing, 2013, doi:10.1088/0264-9381/30/22/224012.
short: T.L. Tanaka, Z. Haiman, Classical and Quantum Gravity 30 (2013).
date_created: 2024-09-06T07:16:12Z
date_published: 2013-11-04T00:00:00Z
date_updated: 2024-09-24T11:39:17Z
day: '04'
doi: 10.1088/0264-9381/30/22/224012
extern: '1'
external_id:
arxiv:
- '1309.2302'
intvolume: ' 30'
issue: '22'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: ' https://doi.org/10.48550/arXiv.1309.2302'
month: '11'
oa: 1
oa_version: Preprint
publication: Classical and Quantum Gravity
publication_identifier:
issn:
- 0264-9381
- 1361-6382
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: Electromagnetic signatures of supermassive black hole binaries resolved by
PTAs
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 30
year: '2013'
...
---
_id: '17646'
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.
article_processing_charge: No
article_type: original
author:
- first_name: R. S.
full_name: de Souza, R. S.
last_name: de Souza
- first_name: A.
full_name: Mesinger, A.
last_name: Mesinger
- first_name: A.
full_name: Ferrara, A.
last_name: Ferrara
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
- first_name: R.
full_name: Perna, R.
last_name: Perna
- first_name: N.
full_name: Yoshida, N.
last_name: Yoshida
citation:
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. Monthly
Notices of the Royal Astronomical Society. 2013;432(4):3218-3227. doi:10.1093/mnras/stt674
apa: de Souza, R. S., 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. Oxford University
Press. https://doi.org/10.1093/mnras/stt674
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.” Monthly Notices of the Royal Astronomical Society. Oxford University
Press, 2013. https://doi.org/10.1093/mnras/stt674.
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,”
Monthly Notices of the Royal Astronomical Society, vol. 432, no. 4. Oxford
University Press, pp. 3218–3227, 2013.
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.
mla: de Souza, R. S., et al. “Constraints on Warm Dark Matter Models from High-Redshift
Long Gamma-Ray Bursts.” Monthly Notices of the Royal Astronomical Society,
vol. 432, no. 4, Oxford University Press, 2013, pp. 3218–27, doi:10.1093/mnras/stt674.
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.
date_created: 2024-09-06T07:25:13Z
date_published: 2013-05-09T00:00:00Z
date_updated: 2024-09-24T12:40:52Z
day: '09'
doi: 10.1093/mnras/stt674
extern: '1'
intvolume: ' 432'
issue: '4'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1093/mnras/stt674
month: '05'
oa: 1
oa_version: Published Version
page: 3218-3227
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
issn:
- 0035-8711
- 1365-2966
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: Constraints on warm dark matter models from high-redshift long gamma-ray bursts
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 432
year: '2013'
...
---
_id: '17653'
abstract:
- lang: eng
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.
article_processing_charge: No
article_type: original
author:
- first_name: Takamitsu L.
full_name: Tanaka, Takamitsu L.
last_name: Tanaka
- first_name: Miao
full_name: Li, Miao
last_name: Li
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
citation:
ama: Tanaka TL, Li M, Haiman Z. The effect of baryonic streaming motions on the
formation of the first supermassive black holes. Monthly Notices of the Royal
Astronomical Society. 2013;435(4):3559-3567. doi:10.1093/mnras/stt1553
apa: Tanaka, T. L., 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. Oxford University Press. https://doi.org/10.1093/mnras/stt1553
chicago: Tanaka, Takamitsu L., Miao Li, and Zoltán Haiman. “The Effect of Baryonic
Streaming Motions on the Formation of the First Supermassive Black Holes.” Monthly
Notices of the Royal Astronomical Society. Oxford University Press, 2013.
https://doi.org/10.1093/mnras/stt1553.
ieee: T. L. Tanaka, M. Li, and Z. Haiman, “The effect of baryonic streaming motions
on the formation of the first supermassive black holes,” Monthly Notices of
the Royal Astronomical Society, vol. 435, no. 4. Oxford University Press,
pp. 3559–3567, 2013.
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.
mla: Tanaka, Takamitsu L., et al. “The Effect of Baryonic Streaming Motions on the
Formation of the First Supermassive Black Holes.” Monthly Notices of the Royal
Astronomical Society, vol. 435, no. 4, Oxford University Press, 2013, pp.
3559–67, doi:10.1093/mnras/stt1553.
short: T.L. Tanaka, M. Li, Z. Haiman, Monthly Notices of the Royal Astronomical
Society 435 (2013) 3559–3567.
date_created: 2024-09-06T07:31:32Z
date_published: 2013-09-10T00:00:00Z
date_updated: 2024-09-24T13:26:36Z
day: '10'
doi: 10.1093/mnras/stt1553
extern: '1'
intvolume: ' 435'
issue: '4'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1093/mnras/stt1553
month: '09'
oa: 1
oa_version: Published Version
page: 3559-3567
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
issn:
- 1365-2966
- 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: The effect of baryonic streaming motions on the formation of the first supermassive
black holes
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 435
year: '2013'
...
---
_id: '17657'
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.
article_number: '32'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: James E.
full_name: Rhoads, James E.
last_name: Rhoads
- first_name: Sangeeta
full_name: Malhotra, Sangeeta
last_name: Malhotra
- first_name: Daniel
full_name: Stern, Daniel
last_name: Stern
- first_name: Mark
full_name: Dickinson, Mark
last_name: Dickinson
- first_name: Norbert
full_name: Pirzkal, Norbert
last_name: Pirzkal
- first_name: Hyron
full_name: Spinrad, Hyron
last_name: Spinrad
- first_name: Naveen
full_name: Reddy, Naveen
last_name: Reddy
- first_name: Nimish
full_name: Hathi, Nimish
last_name: Hathi
- first_name: Norman
full_name: Grogin, Norman
last_name: Grogin
- first_name: Anton
full_name: Koekemoer, Anton
last_name: Koekemoer
- first_name: Michael A.
full_name: Peth, Michael A.
last_name: Peth
- first_name: Seth
full_name: Cohen, Seth
last_name: Cohen
- first_name: Zhenya
full_name: Zheng, Zhenya
last_name: Zheng
- first_name: Tamas
full_name: Budavari, Tamas
last_name: Budavari
- first_name: Ignacio
full_name: Ferreras, Ignacio
last_name: Ferreras
- first_name: Jonathan P.
full_name: Gardner, Jonathan P.
last_name: Gardner
- first_name: Caryl
full_name: Gronwall, Caryl
last_name: Gronwall
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
- first_name: Martin
full_name: Kümmel, Martin
last_name: Kümmel
- first_name: Gerhardt
full_name: Meurer, Gerhardt
last_name: Meurer
- first_name: Leonidas
full_name: Moustakas, Leonidas
last_name: Moustakas
- first_name: Nino
full_name: Panagia, Nino
last_name: Panagia
- first_name: Anna
full_name: Pasquali, Anna
last_name: Pasquali
- first_name: Kailash
full_name: Sahu, Kailash
last_name: Sahu
- first_name: Sperello
full_name: di Serego Alighieri, Sperello
last_name: di Serego Alighieri
- first_name: Rachel
full_name: Somerville, Rachel
last_name: Somerville
- first_name: Amber
full_name: Straughn, Amber
last_name: Straughn
- first_name: Jeremy
full_name: Walsh, Jeremy
last_name: Walsh
- first_name: Rogier
full_name: Windhorst, Rogier
last_name: Windhorst
- first_name: Chun
full_name: Xu, Chun
last_name: Xu
- first_name: Haojing
full_name: Yan, Haojing
last_name: Yan
citation:
ama: Rhoads JE, Malhotra S, Stern D, et al. A Lyman break galaxy in the epoch of
reionization from hubble space telescope grism spectroscopy. The Astrophysical
Journal. 2013;773(1). doi:10.1088/0004-637x/773/1/32
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. The Astrophysical Journal. American
Astronomical Society. https://doi.org/10.1088/0004-637x/773/1/32
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.” The Astrophysical
Journal. American Astronomical Society, 2013. https://doi.org/10.1088/0004-637x/773/1/32.
ieee: J. E. Rhoads et al., “A Lyman break galaxy in the epoch of reionization
from hubble space telescope grism spectroscopy,” The Astrophysical Journal,
vol. 773, no. 1. American Astronomical Society, 2013.
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.
mla: Rhoads, James E., et al. “A Lyman Break Galaxy in the Epoch of Reionization
from Hubble Space Telescope Grism Spectroscopy.” The Astrophysical Journal,
vol. 773, no. 1, 32, American Astronomical Society, 2013, doi:10.1088/0004-637x/773/1/32.
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).
date_created: 2024-09-06T07:35:50Z
date_published: 2013-07-22T00:00:00Z
date_updated: 2024-09-25T07:11:08Z
day: '22'
doi: 10.1088/0004-637x/773/1/32
extern: '1'
external_id:
arxiv:
- '1302.7005'
intvolume: ' 773'
issue: '1'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: ' https://doi.org/10.48550/arXiv.1302.7005'
month: '07'
oa: 1
oa_version: Preprint
publication: The Astrophysical Journal
publication_identifier:
issn:
- 0004-637X
- 1538-4357
publication_status: published
publisher: American Astronomical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: A Lyman break galaxy in the epoch of reionization from hubble space telescope
grism spectroscopy
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 773
year: '2013'
...
---
_id: '17670'
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.
article_number: '49'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: D.
full_name: Bard, D.
last_name: Bard
- first_name: J. M.
full_name: Kratochvil, J. M.
last_name: Kratochvil
- first_name: C.
full_name: Chang, C.
last_name: Chang
- first_name: M.
full_name: May, M.
last_name: May
- first_name: S. M.
full_name: Kahn, S. M.
last_name: Kahn
- first_name: Y.
full_name: AlSayyad, Y.
last_name: AlSayyad
- first_name: Z.
full_name: Ahmad, Z.
last_name: Ahmad
- first_name: J.
full_name: Bankert, J.
last_name: Bankert
- first_name: A.
full_name: Connolly, A.
last_name: Connolly
- first_name: R. R.
full_name: Gibson, R. R.
last_name: Gibson
- first_name: K.
full_name: Gilmore, K.
last_name: Gilmore
- first_name: E.
full_name: Grace, E.
last_name: Grace
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
- first_name: M.
full_name: Hannel, M.
last_name: Hannel
- first_name: K. M.
full_name: Huffenberger, K. M.
last_name: Huffenberger
- first_name: J. G.
full_name: Jernigan, J. G.
last_name: Jernigan
- first_name: L.
full_name: Jones, L.
last_name: Jones
- first_name: S.
full_name: Krughoff, S.
last_name: Krughoff
- first_name: S.
full_name: Lorenz, S.
last_name: Lorenz
- first_name: S.
full_name: Marshall, S.
last_name: Marshall
- first_name: A.
full_name: Meert, 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
- first_name: A. P.
full_name: Rasmussen, A. P.
last_name: Rasmussen
- first_name: M.
full_name: Shmakova, M.
last_name: Shmakova
- first_name: N.
full_name: Sylvestre, N.
last_name: Sylvestre
- first_name: N.
full_name: Todd, N.
last_name: Todd
- first_name: M.
full_name: Young, M.
last_name: Young
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. The Astrophysical Journal. 2013;774(1). doi:10.1088/0004-637x/774/1/49
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. The Astrophysical
Journal. American Astronomical Society. https://doi.org/10.1088/0004-637x/774/1/49
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.” The Astrophysical
Journal. American Astronomical Society, 2013. https://doi.org/10.1088/0004-637x/774/1/49.
ieee: D. Bard et al., “Effect of measurement errors on predicted cosmological
constraints from shear peak statistics with large synoptic survey telescope,”
The Astrophysical Journal, vol. 774, no. 1. American Astronomical Society,
2013.
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.
mla: Bard, D., et al. “Effect of Measurement Errors on Predicted Cosmological Constraints
from Shear Peak Statistics with Large Synoptic Survey Telescope.” The Astrophysical
Journal, vol. 774, no. 1, 49, American Astronomical Society, 2013, doi:10.1088/0004-637x/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).
date_created: 2024-09-06T07:47:50Z
date_published: 2013-08-16T00:00:00Z
date_updated: 2024-09-25T08:04:49Z
day: '16'
doi: 10.1088/0004-637x/774/1/49
extern: '1'
external_id:
arxiv:
- '1301.0830'
intvolume: ' 774'
issue: '1'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: ' https://doi.org/10.48550/arXiv.1301.0830'
month: '08'
oa: 1
oa_version: Preprint
publication: The Astrophysical Journal
publication_identifier:
issn:
- 0004-637X
- 1538-4357
publication_status: published
publisher: American Astronomical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Effect of measurement errors on predicted cosmological constraints from shear
peak statistics with large synoptic survey telescope
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 774
year: '2013'
...
---
_id: '17671'
abstract:
- lang: eng
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.
article_number: '221102'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Imre
full_name: Bartos, Imre
last_name: Bartos
- first_name: Zoltán
full_name: Haiman, 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
citation:
ama: Bartos I, Haiman Z, Kocsis B, Márka S. Gas cloud G2 can illuminate the black
hole population near the galactic center. Physical Review Letters. 2013;110(22).
doi:10.1103/physrevlett.110.221102
apa: 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. American Physical Society. https://doi.org/10.1103/physrevlett.110.221102
chicago: Bartos, Imre, Zoltán Haiman, Bence Kocsis, and Szabolcs Márka. “Gas Cloud
G2 Can Illuminate the Black Hole Population near the Galactic Center.” Physical
Review Letters. American Physical Society, 2013. https://doi.org/10.1103/physrevlett.110.221102.
ieee: I. Bartos, Z. Haiman, B. Kocsis, and S. Márka, “Gas cloud G2 can illuminate
the black hole population near the galactic center,” Physical Review Letters,
vol. 110, no. 22. American Physical Society, 2013.
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.
mla: Bartos, Imre, et al. “Gas Cloud G2 Can Illuminate the Black Hole Population
near the Galactic Center.” Physical Review Letters, vol. 110, no. 22, 221102,
American Physical Society, 2013, doi:10.1103/physrevlett.110.221102.
short: I. Bartos, Z. Haiman, B. Kocsis, S. Márka, Physical Review Letters 110 (2013).
date_created: 2024-09-06T07:48:38Z
date_published: 2013-05-30T00:00:00Z
date_updated: 2024-09-25T08:25:00Z
day: '30'
doi: 10.1103/physrevlett.110.221102
extern: '1'
external_id:
arxiv:
- '1302.3220'
intvolume: ' 110'
issue: '22'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: ' https://doi.org/10.48550/arXiv.1302.3220'
month: '05'
oa: 1
oa_version: Preprint
publication: Physical Review Letters
publication_identifier:
issn:
- 0031-9007
- 1079-7114
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Gas cloud G2 can illuminate the black hole population near the galactic center
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 110
year: '2013'
...