---
_id: '2496'
abstract:
- lang: eng
  text: 'Glutamate is one candidate for the neurotransmitters and/or neuromodulators
    involved in taste signaling in taste buds. Group II metabotropic glutamate receptors
    (mGluRs: mGluR2 and mGluR3) are known to function as presynaptic receptors that
    regulate the release of glutamate and/or other neurotransmitters in the central
    nervous system. Group II mGluRs are negatively linked to adenylyl cyclase through
    Gαi subunits and thereby reduce the turnover of cAMP. In rat taste tissues, a
    subset of adenylyl-cyclase-8-expressing taste cells coexpress the Gαi subunits
    gustducin and Gαi2. However, the expression patterns of group II mGluRs in rat
    taste tissues have not yet been elucidated. We have therefore examined the expression
    patterns of mGluR2, mGluR3, and gustducin in rat gustatory tissues. Reverse transcription/polymerase
    chain reaction assays have revealed that mGluR2 and mGluR3 mRNAs are expressed
    in the circumvallate papillae. In situ hybridization analyses have detected positive
    signals for mGluR2 and mGluR3 mRNAs only in the circumvallate taste buds. Among
    the fungiform, foliate, and circumvallate papillae, an antibody against mGluR2/3
    labels a subset of taste bud cells and nerve fibers immediately beneath the taste
    lingual epithelium. Double-labeling experiments have demonstrated that mGluR2/3-positive
    cells coexpress gustducin. These results indicate that mGluR2 and mGluR3 are coupled
    to Gαi subunits and play roles in glutamate-mediated signaling in taste transductions.'
author:
- first_name: Takashi
  full_name: Toyono, Takashi
  last_name: Toyono
- first_name: Shinji
  full_name: Kataoka, Shinji
  last_name: Kataoka
- first_name: Yuji
  full_name: Seta, Yuji
  last_name: Seta
- first_name: Ryuichi
  full_name: Ryuichi Shigemoto
  id: 499F3ABC-F248-11E8-B48F-1D18A9856A87
  last_name: Shigemoto
  orcid: 0000-0001-8761-9444
- first_name: Kuniaki
  full_name: Toyoshima, Kuniaki
  last_name: Toyoshima
citation:
  ama: Toyono T, Kataoka S, Seta Y, Shigemoto R, Toyoshima K. Expression of group
    II metabotropic glutamate receptors in rat gustatory papillae. <i>Cell and Tissue
    Research</i>. 2007;328(1):57-63. doi:<a href="https://doi.org/10.1007/s00441-006-0351-9">10.1007/s00441-006-0351-9</a>
  apa: Toyono, T., Kataoka, S., Seta, Y., Shigemoto, R., &#38; Toyoshima, K. (2007).
    Expression of group II metabotropic glutamate receptors in rat gustatory papillae.
    <i>Cell and Tissue Research</i>. Springer. <a href="https://doi.org/10.1007/s00441-006-0351-9">https://doi.org/10.1007/s00441-006-0351-9</a>
  chicago: Toyono, Takashi, Shinji Kataoka, Yuji Seta, Ryuichi Shigemoto, and Kuniaki
    Toyoshima. “Expression of Group II Metabotropic Glutamate Receptors in Rat Gustatory
    Papillae.” <i>Cell and Tissue Research</i>. Springer, 2007. <a href="https://doi.org/10.1007/s00441-006-0351-9">https://doi.org/10.1007/s00441-006-0351-9</a>.
  ieee: T. Toyono, S. Kataoka, Y. Seta, R. Shigemoto, and K. Toyoshima, “Expression
    of group II metabotropic glutamate receptors in rat gustatory papillae,” <i>Cell
    and Tissue Research</i>, vol. 328, no. 1. Springer, pp. 57–63, 2007.
  ista: Toyono T, Kataoka S, Seta Y, Shigemoto R, Toyoshima K. 2007. Expression of
    group II metabotropic glutamate receptors in rat gustatory papillae. Cell and
    Tissue Research. 328(1), 57–63.
  mla: Toyono, Takashi, et al. “Expression of Group II Metabotropic Glutamate Receptors
    in Rat Gustatory Papillae.” <i>Cell and Tissue Research</i>, vol. 328, no. 1,
    Springer, 2007, pp. 57–63, doi:<a href="https://doi.org/10.1007/s00441-006-0351-9">10.1007/s00441-006-0351-9</a>.
  short: T. Toyono, S. Kataoka, Y. Seta, R. Shigemoto, K. Toyoshima, Cell and Tissue
    Research 328 (2007) 57–63.
date_created: 2018-12-11T11:58:00Z
date_published: 2007-04-01T00:00:00Z
date_updated: 2021-01-12T06:57:50Z
day: '01'
doi: 10.1007/s00441-006-0351-9
extern: 1
intvolume: '       328'
issue: '1'
month: '04'
page: 57 - 63
publication: Cell and Tissue Research
publication_status: published
publisher: Springer
publist_id: '4405'
quality_controlled: 0
status: public
title: Expression of group II metabotropic glutamate receptors in rat gustatory papillae
type: journal_article
volume: 328
year: '2007'
...
---
_id: '167'
abstract:
- lang: eng
  text: This book contains research articles on Diophantine Geometry, written by participants
    of a research program held at the Ennio De Giorgi Mathematical Research Center
    in Pisa, Italy, during the period April – July 2005. The authors are eminent experts
    in the field. Several subfields of the main topic are presented; the volume thus
    is particularly useful to get a broad overview of recent research developments.
alternative_title:
- CRM Series
article_processing_charge: No
arxiv: 1
author:
- first_name: Timothy D
  full_name: Browning, Timothy D
  id: 35827D50-F248-11E8-B48F-1D18A9856A87
  last_name: Browning
  orcid: 0000-0002-8314-0177
- first_name: Roger
  full_name: Heath Brown, Roger
  last_name: Heath Brown
citation:
  ama: 'Browning TD, Heath Brown R. Simultaneous equal sums of three powers. In: Zannier
    U, ed. <i>Diophantine Geometry</i>. Vol 4. Edizioni della Normale; 2007:93-100.'
  apa: Browning, T. D., &#38; Heath Brown, R. (2007). Simultaneous equal sums of three
    powers. In U. Zannier (Ed.), <i>Diophantine Geometry</i> (Vol. 4, pp. 93–100).
    Edizioni della Normale.
  chicago: Browning, Timothy D, and Roger Heath Brown. “Simultaneous Equal Sums of
    Three Powers.” In <i>Diophantine Geometry</i>, edited by Umberto Zannier, 4:93–100.
    Edizioni della Normale, 2007.
  ieee: T. D. Browning and R. Heath Brown, “Simultaneous equal sums of three powers,”
    in <i>Diophantine Geometry</i>, vol. 4, U. Zannier, Ed. Edizioni della Normale,
    2007, pp. 93–100.
  ista: 'Browning TD, Heath Brown R. 2007.Simultaneous equal sums of three powers.
    In: Diophantine Geometry. CRM Series, vol. 4, 93–100.'
  mla: Browning, Timothy D., and Roger Heath Brown. “Simultaneous Equal Sums of Three
    Powers.” <i>Diophantine Geometry</i>, edited by Umberto Zannier, vol. 4, Edizioni
    della Normale, 2007, pp. 93–100.
  short: T.D. Browning, R. Heath Brown, in:, U. Zannier (Ed.), Diophantine Geometry,
    Edizioni della Normale, 2007, pp. 93–100.
date_created: 2018-12-11T11:44:59Z
date_published: 2007-01-01T00:00:00Z
date_updated: 2021-01-12T06:52:24Z
day: '01'
editor:
- first_name: Umberto
  full_name: Zannier, Umberto
  last_name: Zannier
extern: '1'
external_id:
  arxiv:
  - '0509152'
intvolume: '         4'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://arxiv.org/abs/math/0509152
month: '01'
oa: 1
oa_version: Preprint
page: 93 - 100
publication: Diophantine Geometry
publication_status: published
publisher: Edizioni della Normale
publist_id: '7754'
quality_controlled: '1'
status: public
title: Simultaneous equal sums of three powers
type: book_chapter
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 4
year: '2007'
...
---
_id: '1750'
abstract:
- lang: eng
  text: The authors investigate the composition profile of SiGe islands after capping
    with Si to form quantum dots, using a two step etching procedure and atomic force
    microscopy. Initially, the Si capping layers are removed by etching selectively
    Si over Ge and then the composition of the disclosed islands is addressed by selectively
    etching Ge over Si. For samples grown at 580 °C the authors show that even when
    overgrowth leads to a flat Si surface and the islands undergo strong morphological
    changes, a Ge-rich core region is still preserved in the dot. At high growth and
    overgrowth temperatures (740 °C), the experiments show that the newly formed base
    of the buried islands is more Si rich than their top. Furthermore, the authors
    find that for the growth conditions used, no lateral motion takes place during
    capping.
author:
- 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: Armando
  full_name: Rastelli, Armando
  last_name: Rastelli
- first_name: Oliver
  full_name: Schmidt, Oliver G
  last_name: Schmidt
- first_name: Klaus
  full_name: Kern, Klaus
  last_name: Kern
- first_name: Jerry
  full_name: Tersoff, Jerry
  last_name: Tersoff
citation:
  ama: Katsaros G, Stoffel M, Rastelli A, Schmidt O, Kern K, Tersoff J. Three-dimensional
    isocompositional profiles of buried SiGeSi (001) islands. <i>Applied Physics Letters</i>.
    2007;91(1). doi:<a href="https://doi.org/10.1063/1.2752730">10.1063/1.2752730</a>
  apa: Katsaros, G., Stoffel, M., Rastelli, A., Schmidt, O., Kern, K., &#38; Tersoff,
    J. (2007). Three-dimensional isocompositional profiles of buried SiGeSi (001)
    islands. <i>Applied Physics Letters</i>. American Institute of Physics. <a href="https://doi.org/10.1063/1.2752730">https://doi.org/10.1063/1.2752730</a>
  chicago: Katsaros, Georgios, Mathieu Stoffel, Armando Rastelli, Oliver Schmidt,
    Klaus Kern, and Jerry Tersoff. “Three-Dimensional Isocompositional Profiles of
    Buried SiGeSi (001) Islands.” <i>Applied Physics Letters</i>. American Institute
    of Physics, 2007. <a href="https://doi.org/10.1063/1.2752730">https://doi.org/10.1063/1.2752730</a>.
  ieee: G. Katsaros, M. Stoffel, A. Rastelli, O. Schmidt, K. Kern, and J. Tersoff,
    “Three-dimensional isocompositional profiles of buried SiGeSi (001) islands,”
    <i>Applied Physics Letters</i>, vol. 91, no. 1. American Institute of Physics,
    2007.
  ista: Katsaros G, Stoffel M, Rastelli A, Schmidt O, Kern K, Tersoff J. 2007. Three-dimensional
    isocompositional profiles of buried SiGeSi (001) islands. Applied Physics Letters.
    91(1).
  mla: Katsaros, Georgios, et al. “Three-Dimensional Isocompositional Profiles of
    Buried SiGeSi (001) Islands.” <i>Applied Physics Letters</i>, vol. 91, no. 1,
    American Institute of Physics, 2007, doi:<a href="https://doi.org/10.1063/1.2752730">10.1063/1.2752730</a>.
  short: G. Katsaros, M. Stoffel, A. Rastelli, O. Schmidt, K. Kern, J. Tersoff, Applied
    Physics Letters 91 (2007).
date_created: 2018-12-11T11:53:48Z
date_published: 2007-01-01T00:00:00Z
date_updated: 2021-01-12T06:52:58Z
day: '01'
doi: 10.1063/1.2752730
extern: 1
intvolume: '        91'
issue: '1'
month: '01'
publication: Applied Physics Letters
publication_status: published
publisher: American Institute of Physics
publist_id: '5375'
quality_controlled: 0
status: public
title: Three-dimensional isocompositional profiles of buried SiGeSi (001) islands
type: journal_article
volume: 91
year: '2007'
...
---
_id: '1762'
abstract:
- lang: eng
  text: In quantum information science, the phase of a wave function plays an important
    role in encoding information. Although most experiments in this field rely on
    dynamic effects to manipulate this information, an alternative approach is to
    use geometric phase, which has been argued to have potential fault tolerance.
    We demonstrated the controlled accumulation of a geometric phase, Berry's phase,
    in a superconducting qubit; we manipulated the qubit geometrically by means of
    microwave radiation and observed the accumulated phase in an interference experiment.
    We found excellent agreement with Berry's predictions and also observed a geometry-dependent
    contribution to dephasing.
acknowledgement: Supported by the EC via an Intra-European Marie Curie Fellowship
  (P.J.L.), the Natural Sciences and Engineering Research Council of Canada, Canadian
  Institute for Advanced Research, and Fonds Québécois de la Recherche sur la Nature
  et les Technologies (A.B.), the National Security Agency under the Army Research
  Office, NSF, and Yale University (D.I.S., L.F., and R.J.S.), Consiglio Nazionale
  delle Ricerche–Istituto di Cibernetica, Pozzuoli, Italy (L.F.), the Ontario Research
  Development Challenge Fund and Mathematics of Information Technology and Complex
  Systems (J.M.G.), the Swiss National Science Foundation, and ETH Zürich
author:
- first_name: Peter
  full_name: Leek, Peter J
  last_name: Leek
- first_name: Johannes M
  full_name: Johannes Fink
  id: 4B591CBA-F248-11E8-B48F-1D18A9856A87
  last_name: Fink
  orcid: 0000-0001-8112-028X
- first_name: Alexandre
  full_name: Blais, Alexandre
  last_name: Blais
- first_name: R
  full_name: Bianchetti, R
  last_name: Bianchetti
- first_name: M
  full_name: Göppl, M
  last_name: Göppl
- first_name: Jay
  full_name: Gambetta, Jay M
  last_name: Gambetta
- first_name: David
  full_name: Schuster, David I
  last_name: Schuster
- first_name: Luigi
  full_name: Frunzio, Luigi
  last_name: Frunzio
- first_name: Robert
  full_name: Schoelkopf, Robert J
  last_name: Schoelkopf
- first_name: Andreas
  full_name: Wallraff, Andreas
  last_name: Wallraff
citation:
  ama: Leek P, Fink JM, Blais A, et al. Observation of Berry’s phase in a solid-state
    qubit. <i>Science</i>. 2007;318(5858):1889-1892. doi:<a href="https://doi.org/10.1126/science.1149858">10.1126/science.1149858</a>
  apa: Leek, P., Fink, J. M., Blais, A., Bianchetti, R., Göppl, M., Gambetta, J.,
    … Wallraff, A. (2007). Observation of Berry’s phase in a solid-state qubit. <i>Science</i>.
    American Association for the Advancement of Science. <a href="https://doi.org/10.1126/science.1149858">https://doi.org/10.1126/science.1149858</a>
  chicago: Leek, Peter, Johannes M Fink, Alexandre Blais, R Bianchetti, M Göppl, Jay
    Gambetta, David Schuster, Luigi Frunzio, Robert Schoelkopf, and Andreas Wallraff.
    “Observation of Berry’s Phase in a Solid-State Qubit.” <i>Science</i>. American
    Association for the Advancement of Science, 2007. <a href="https://doi.org/10.1126/science.1149858">https://doi.org/10.1126/science.1149858</a>.
  ieee: P. Leek <i>et al.</i>, “Observation of Berry’s phase in a solid-state qubit,”
    <i>Science</i>, vol. 318, no. 5858. American Association for the Advancement of
    Science, pp. 1889–1892, 2007.
  ista: Leek P, Fink JM, Blais A, Bianchetti R, Göppl M, Gambetta J, Schuster D, Frunzio
    L, Schoelkopf R, Wallraff A. 2007. Observation of Berry’s phase in a solid-state
    qubit. Science. 318(5858), 1889–1892.
  mla: Leek, Peter, et al. “Observation of Berry’s Phase in a Solid-State Qubit.”
    <i>Science</i>, vol. 318, no. 5858, American Association for the Advancement of
    Science, 2007, pp. 1889–92, doi:<a href="https://doi.org/10.1126/science.1149858">10.1126/science.1149858</a>.
  short: P. Leek, J.M. Fink, A. Blais, R. Bianchetti, M. Göppl, J. Gambetta, D. Schuster,
    L. Frunzio, R. Schoelkopf, A. Wallraff, Science 318 (2007) 1889–1892.
date_created: 2018-12-11T11:53:52Z
date_published: 2007-12-27T00:00:00Z
date_updated: 2021-01-12T06:53:02Z
day: '27'
doi: 10.1126/science.1149858
extern: 1
intvolume: '       318'
issue: '5858'
main_file_link:
- open_access: '1'
  url: http://arxiv.org/abs/0711.0218
month: '12'
oa: 1
page: 1889 - 1892
publication: Science
publication_status: published
publisher: American Association for the Advancement of Science
publist_id: '5360'
quality_controlled: 0
status: public
title: Observation of Berry's phase in a solid-state qubit
type: journal_article
volume: 318
year: '2007'
...
---
_id: '17714'
abstract:
- lang: eng
  text: We investigate the effect of planetary rotation on the transit spectrum of
    an extrasolar giant planet. During ingress and egress, absorption features arising
    from the planet's atmosphere are Doppler shifted by of order the planet's rotational
    velocity (~1-2 km/s) relative to where they would be if the planet were not rotating.
    We focus in particular on the case of HD209458b, which ought to be at least as
    good a target as any other known transiting planet. For HD209458b, this shift
    should give rise to a small net centroid shift of ~60 cm/s on the stellar absorption
    lines. Using a detailed model of the transmission spectrum due to a rotating star
    transited by a rotating planet with an isothermal atmosphere, we simulate the
    effect of the planet's rotation on the shape of the spectral lines, and in particular
    on the magnitude of their width and centroid shift. We then use this simulation
    to determine the expected signal-to-noise ratio for distinguishing a rotating
    from a non-rotating planet, and assess how this S/N scales with various parameters
    of HD209458b. We find that with a 6 m telescope, an equatorial rotational velocity
    of ~2 km/s could be detected with a S/N~5 by accumulating the signal over many
    transits over the course of several years. With a 30 m telescope, the time required
    to make such a detection reduces to less than 2 months.
article_processing_charge: No
article_type: original
author:
- first_name: David S.
  full_name: Spiegel, David S.
  last_name: Spiegel
- first_name: Zoltán
  full_name: Haiman, Zoltán
  id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
  last_name: Haiman
- first_name: B. Scott
  full_name: Gaudi, B. Scott
  last_name: Gaudi
citation:
  ama: Spiegel DS, Haiman Z, Gaudi BS. On constraining a transiting exoplanet’s rotation
    rate with its transit spectrum. <i>The Astrophysical Journal</i>. 2007;669(2):1324-1335.
    doi:<a href="https://doi.org/10.1086/521921">10.1086/521921</a>
  apa: Spiegel, D. S., Haiman, Z., &#38; Gaudi, B. S. (2007). On constraining a transiting
    exoplanet’s rotation rate with its transit spectrum. <i>The Astrophysical Journal</i>.
    American Astronomical Society. <a href="https://doi.org/10.1086/521921">https://doi.org/10.1086/521921</a>
  chicago: Spiegel, David S., Zoltán Haiman, and B. Scott Gaudi. “On Constraining
    a Transiting Exoplanet’s Rotation Rate with Its Transit Spectrum.” <i>The Astrophysical
    Journal</i>. American Astronomical Society, 2007. <a href="https://doi.org/10.1086/521921">https://doi.org/10.1086/521921</a>.
  ieee: D. S. Spiegel, Z. Haiman, and B. S. Gaudi, “On constraining a transiting exoplanet’s
    rotation rate with its transit spectrum,” <i>The Astrophysical Journal</i>, vol.
    669, no. 2. American Astronomical Society, pp. 1324–1335, 2007.
  ista: Spiegel DS, Haiman Z, Gaudi BS. 2007. On constraining a transiting exoplanet’s
    rotation rate with its transit spectrum. The Astrophysical Journal. 669(2), 1324–1335.
  mla: Spiegel, David S., et al. “On Constraining a Transiting Exoplanet’s Rotation
    Rate with Its Transit Spectrum.” <i>The Astrophysical Journal</i>, vol. 669, no.
    2, American Astronomical Society, 2007, pp. 1324–35, doi:<a href="https://doi.org/10.1086/521921">10.1086/521921</a>.
  short: D.S. Spiegel, Z. Haiman, B.S. Gaudi, The Astrophysical Journal 669 (2007)
    1324–1335.
date_created: 2024-09-06T08:58:16Z
date_published: 2007-11-10T00:00:00Z
date_updated: 2024-09-25T12:42:28Z
day: '10'
doi: 10.1086/521921
extern: '1'
intvolume: '       669'
issue: '2'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1086/521921
month: '11'
oa: 1
oa_version: Published Version
page: 1324-1335
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: On constraining a transiting exoplanet’s rotation rate with its transit spectrum
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 669
year: '2007'
...
---
_id: '17716'
abstract:
- lang: eng
  text: Recent observations imply that the observed number counts of Lyα emitters
    (LAEs) evolved significantly between z= 5.7 and 6.5. It has been suggested that
    this was due to a rapid evolution in the ionization state, and hence transmission
    of the intergalactic medium (IGM) which caused Lyα flux from z= 6.5 galaxies to
    be more strongly suppressed. In this paper, we consider the joint evolution of
    the Lyα and the ultraviolet luminosity functions (LFs) and show that the IGM transmission
    evolved between z= 6.5 and 5.7 by a factor 1.1 < R < 1.8 (95 per cent confidence
    level). This result is insensitive to the underlying model of the Lyα LF (as well
    as cosmic variance). Using a model for IGM transmission, we find that the evolution
    of the mean IGM density through cosmic expansion alone may result in a value for
    the ratio of transmissions as high as R= 1.3. Thus, the existing LFs do not provide
    evidence for overlap. Furthermore, the constraint R < 1.8 suggests that the Universe
    at z= 6.5 was more than half-ionized by volume, that is, xi,V > 0.5.
article_processing_charge: No
article_type: original
author:
- first_name: M.
  full_name: Dijkstra, M.
  last_name: Dijkstra
- first_name: J. S. B.
  full_name: Wyithe, J. S. B.
  last_name: Wyithe
- first_name: Zoltán
  full_name: Haiman, Zoltán
  id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
  last_name: Haiman
citation:
  ama: Dijkstra M, Wyithe JSB, Haiman Z. Luminosity functions of Lyα emitting galaxies
    and cosmic reionization of hydrogen. <i>Monthly Notices of the Royal Astronomical
    Society</i>. 2007;379(1):253-259. doi:<a href="https://doi.org/10.1111/j.1365-2966.2007.11936.x">10.1111/j.1365-2966.2007.11936.x</a>
  apa: Dijkstra, M., Wyithe, J. S. B., &#38; Haiman, Z. (2007). Luminosity functions
    of Lyα emitting galaxies and cosmic reionization of hydrogen. <i>Monthly Notices
    of the Royal Astronomical Society</i>. Oxford University Press. <a href="https://doi.org/10.1111/j.1365-2966.2007.11936.x">https://doi.org/10.1111/j.1365-2966.2007.11936.x</a>
  chicago: Dijkstra, M., J. S. B. Wyithe, and Zoltán Haiman. “Luminosity Functions
    of Lyα Emitting Galaxies and Cosmic Reionization of Hydrogen.” <i>Monthly Notices
    of the Royal Astronomical Society</i>. Oxford University Press, 2007. <a href="https://doi.org/10.1111/j.1365-2966.2007.11936.x">https://doi.org/10.1111/j.1365-2966.2007.11936.x</a>.
  ieee: M. Dijkstra, J. S. B. Wyithe, and Z. Haiman, “Luminosity functions of Lyα
    emitting galaxies and cosmic reionization of hydrogen,” <i>Monthly Notices of
    the Royal Astronomical Society</i>, vol. 379, no. 1. Oxford University Press,
    pp. 253–259, 2007.
  ista: Dijkstra M, Wyithe JSB, Haiman Z. 2007. Luminosity functions of Lyα emitting
    galaxies and cosmic reionization of hydrogen. Monthly Notices of the Royal Astronomical
    Society. 379(1), 253–259.
  mla: Dijkstra, M., et al. “Luminosity Functions of Lyα Emitting Galaxies and Cosmic
    Reionization of Hydrogen.” <i>Monthly Notices of the Royal Astronomical Society</i>,
    vol. 379, no. 1, Oxford University Press, 2007, pp. 253–59, doi:<a href="https://doi.org/10.1111/j.1365-2966.2007.11936.x">10.1111/j.1365-2966.2007.11936.x</a>.
  short: M. Dijkstra, J.S.B. Wyithe, Z. Haiman, Monthly Notices of the Royal Astronomical
    Society 379 (2007) 253–259.
date_created: 2024-09-06T09:01:21Z
date_published: 2007-06-21T00:00:00Z
date_updated: 2024-09-25T13:02:42Z
day: '21'
doi: 10.1111/j.1365-2966.2007.11936.x
extern: '1'
intvolume: '       379'
issue: '1'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1111/j.1365-2966.2007.11936.x
month: '06'
oa: 1
oa_version: Published Version
page: 253-259
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: Luminosity functions of Lyα emitting galaxies and cosmic reionization of hydrogen
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 379
year: '2007'
...
---
_id: '17724'
abstract:
- lang: eng
  text: The continuous improvement in localization errors (sky position and distance)
    in real time as LISA observes the gradual inspiral of a supermassive black hole
    (SMBH) binary can be of great help in identifying any prompt electromagnetic counterpart
    associated with the merger. We develop a new method, based on a Fourier decomposition
    of the time-dependent, LISA-modulated gravitational-wave signal, to study this
    intricate problem. The method is faster than standard Monte Carlo simulations
    by orders of magnitude. By surveying the parameter space of potential LISA sources,
    we find that counterparts to SMBH binary mergers with total mass M~10^5-10^7 M_Sun
    and redshifts z<~3 can be localized to within the field of view of astronomical
    instruments (~deg^2) typically hours to weeks prior to coalescence. This will
    allow targeted searches for variable electromagnetic counterparts as the merger
    proceeds, as well as monitoring of the most energetic coalescence phase. A rich
    set of astrophysical and cosmological applications would emerge from the identification
    of electromagnetic counterparts to these gravitational-wave standard sirens.
article_number: '022003'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Bence
  full_name: Kocsis, Bence
  last_name: Kocsis
- first_name: Zoltán
  full_name: Haiman, Zoltán
  id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
  last_name: Haiman
- first_name: Kristen
  full_name: Menou, Kristen
  last_name: Menou
- first_name: Zsolt
  full_name: Frei, Zsolt
  last_name: Frei
citation:
  ama: 'Kocsis B, Haiman Z, Menou K, Frei Z. Premerger localization of gravitational-wave
    standard sirens with LISA: Harmonic mode decomposition. <i>Physical Review D</i>.
    2007;76(2). doi:<a href="https://doi.org/10.1103/physrevd.76.022003">10.1103/physrevd.76.022003</a>'
  apa: 'Kocsis, B., Haiman, Z., Menou, K., &#38; Frei, Z. (2007). Premerger localization
    of gravitational-wave standard sirens with LISA: Harmonic mode decomposition.
    <i>Physical Review D</i>. American Physical Society. <a href="https://doi.org/10.1103/physrevd.76.022003">https://doi.org/10.1103/physrevd.76.022003</a>'
  chicago: 'Kocsis, Bence, Zoltán Haiman, Kristen Menou, and Zsolt Frei. “Premerger
    Localization of Gravitational-Wave Standard Sirens with LISA: Harmonic Mode Decomposition.”
    <i>Physical Review D</i>. American Physical Society, 2007. <a href="https://doi.org/10.1103/physrevd.76.022003">https://doi.org/10.1103/physrevd.76.022003</a>.'
  ieee: 'B. Kocsis, Z. Haiman, K. Menou, and Z. Frei, “Premerger localization of gravitational-wave
    standard sirens with LISA: Harmonic mode decomposition,” <i>Physical Review D</i>,
    vol. 76, no. 2. American Physical Society, 2007.'
  ista: 'Kocsis B, Haiman Z, Menou K, Frei Z. 2007. Premerger localization of gravitational-wave
    standard sirens with LISA: Harmonic mode decomposition. Physical Review D. 76(2),
    022003.'
  mla: 'Kocsis, Bence, et al. “Premerger Localization of Gravitational-Wave Standard
    Sirens with LISA: Harmonic Mode Decomposition.” <i>Physical Review D</i>, vol.
    76, no. 2, 022003, American Physical Society, 2007, doi:<a href="https://doi.org/10.1103/physrevd.76.022003">10.1103/physrevd.76.022003</a>.'
  short: B. Kocsis, Z. Haiman, K. Menou, Z. Frei, Physical Review D 76 (2007).
date_created: 2024-09-06T09:11:38Z
date_published: 2007-07-12T00:00:00Z
date_updated: 2024-09-25T14:08:55Z
day: '12'
doi: 10.1103/physrevd.76.022003
extern: '1'
external_id:
  arxiv:
  - '0701629'
intvolume: '        76'
issue: '2'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: ' https://doi.org/10.48550/arXiv.astro-ph/0701629'
month: '07'
oa: 1
oa_version: Preprint
publication: Physical Review D
publication_identifier:
  issn:
  - 1550-7998
  - 1550-2368
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'Premerger localization of gravitational-wave standard sirens with LISA: Harmonic
  mode decomposition'
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 76
year: '2007'
...
---
_id: '17729'
abstract:
- lang: eng
  text: 'We make use of hydrodynamical simulations of the intergalactic medium (IGM)
    to create model quasar absorption spectra. We compare these model spectra with
    the observed Keck spectra of three z>6.2 quasars with full Gunn-Peterson troughs:
    SDSS J1148+5251 (z=6.42), SDSS J1030+0524 (z=6.28), and SDSS J1623+3112 (z=6.22).
    We fit the probability density distributions (PDFs) of the observed Ly alpha optical
    depths with those generated from the simulation, by exploring a range of values
    for the size of the quasar''s surrounding HII region, R_S, the volume-weighted
    mean neutral hydrogen fraction in the ambient IGM, x_H, and the quasar''s ionizing
    photon emissivity, N_Q. In order to avoid averaging over possibly large sightline-to-sightline
    fluctuations in IGM properties, we analyze each observed quasar independently.
    We find the following results for J1148+5251, J1030+0524, and J1623+3112: The
    best-fit sizes R_S are 40, 41, and 29 (comoving) Mpc, respectively. These constraints
    are tight, with only ~ 10% uncertainties, comparable to those caused by redshift--determination
    errors. The best-fit values of N_Q are 2.1, 1.3, and 0.9 x 10^{57} s^{-1}, respectively,
    with a factor of ~ 2 uncertainty in each case. Finally, the best--fit values of
    x_H are 0.16, 1.0, and 1.0, respectively. The uncertainty in the case of J1148+5251
    is large, and x_H is not well constrained. However, for both J1030+0524 and J1623+3112,
    we find a significant lower limit of x_H >~ 0.033. Our method is different from
    previous analyses of the GP absorption spectra of these quasars, and our results
    strengthen the evidence that the rapid end--stage of reionization is occurring
    near z ~ 6.'
article_processing_charge: No
article_type: original
author:
- 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: Mesinger A, Haiman Z. Constraints on reionization and Source Properties from
    the Absorption Spectra of z &#62; 6.2 quasars. <i>The Astrophysical Journal</i>.
    2007;660(2):923-932. doi:<a href="https://doi.org/10.1086/513688">10.1086/513688</a>
  apa: Mesinger, A., &#38; Haiman, Z. (2007). Constraints on reionization and Source
    Properties from the Absorption Spectra of z &#62; 6.2 quasars. <i>The Astrophysical
    Journal</i>. American Astronomical Society. <a href="https://doi.org/10.1086/513688">https://doi.org/10.1086/513688</a>
  chicago: Mesinger, Andrei, and Zoltán Haiman. “Constraints on Reionization and Source
    Properties from the Absorption Spectra of z &#62; 6.2 Quasars.” <i>The Astrophysical
    Journal</i>. American Astronomical Society, 2007. <a href="https://doi.org/10.1086/513688">https://doi.org/10.1086/513688</a>.
  ieee: A. Mesinger and Z. Haiman, “Constraints on reionization and Source Properties
    from the Absorption Spectra of z &#62; 6.2 quasars,” <i>The Astrophysical Journal</i>,
    vol. 660, no. 2. American Astronomical Society, pp. 923–932, 2007.
  ista: Mesinger A, Haiman Z. 2007. Constraints on reionization and Source Properties
    from the Absorption Spectra of z &#62; 6.2 quasars. The Astrophysical Journal.
    660(2), 923–932.
  mla: Mesinger, Andrei, and Zoltán Haiman. “Constraints on Reionization and Source
    Properties from the Absorption Spectra of z &#62; 6.2 Quasars.” <i>The Astrophysical
    Journal</i>, vol. 660, no. 2, American Astronomical Society, 2007, pp. 923–32,
    doi:<a href="https://doi.org/10.1086/513688">10.1086/513688</a>.
  short: A. Mesinger, Z. Haiman, The Astrophysical Journal 660 (2007) 923–932.
date_created: 2024-09-06T09:15:25Z
date_published: 2007-05-10T00:00:00Z
date_updated: 2024-09-26T07:30:51Z
day: '10'
doi: 10.1086/513688
extern: '1'
intvolume: '       660'
issue: '2'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1086/513688
month: '05'
oa: 1
oa_version: Published Version
page: 923-932
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: Constraints on reionization and Source Properties from the Absorption Spectra
  of z > 6.2 quasars
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 660
year: '2007'
...
---
_id: '17732'
abstract:
- lang: eng
  text: Energetic feedback processes during the formation of galaxy clusters may have
    heated and ionized a large fraction of the intergalactic gas in proto-cluster
    regions. When such a highly ionized hot ``super-bubble'' falls along the sightline
    to a background quasar, it would be seen as a large void, with little or no absorption,
    in the Lyman alpha forest. We examine the spectra of 137 quasars in the Sloan
    Digital Sky Survey, to search for such voids, and find no clear evidence of their
    existence. The size distribution of voids in the range 5-70 Angstrom (corresponding
    to physical sizes of approximately 3-35 comoving Mpc/h) is consistent with the
    standard model for the Lyman alpha forest without additional hot bubbles. We adapt
    a physical model for HII bubble growth during cosmological reionization (Furlanetto,
    Zaldarriaga and Hernquist 2004), to describe the expected size-distribution of
    hot super-bubbles at redshift around z = 3. This model incorporates the conjoining
    of bubbles around individual neighboring galaxies. Using the non-detection of
    voids, we find that models in which the volume filling factor of hot bubbles exceeds
    approximately 20 percent at z=3 can be ruled out, primarily because they overproduce
    the number of large (40-50 Angstrom) voids. We conclude that any pre-heating mechanism
    that explains galaxy cluster observations must avoid heating the low-density gas
    in the proto-cluster regions, either by operating relatively recently (z<3) or
    by depositing entropy in the high-density regions.
article_processing_charge: No
article_type: original
author:
- first_name: Cien
  full_name: Shang, Cien
  last_name: Shang
- first_name: Arlin
  full_name: Crotts, Arlin
  last_name: Crotts
- first_name: Zoltán
  full_name: Haiman, Zoltán
  id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
  last_name: Haiman
citation:
  ama: Shang C, Crotts A, Haiman Z. Constraints on the abundance of highly ionized
    protocluster regions from the absence of large voids in the Lyα forest. <i>The
    Astrophysical Journal</i>. 2007;671(1):136-145. doi:<a href="https://doi.org/10.1086/522331">10.1086/522331</a>
  apa: Shang, C., Crotts, A., &#38; Haiman, Z. (2007). Constraints on the abundance
    of highly ionized protocluster regions from the absence of large voids in the
    Lyα forest. <i>The Astrophysical Journal</i>. American Astronomical Society. <a
    href="https://doi.org/10.1086/522331">https://doi.org/10.1086/522331</a>
  chicago: Shang, Cien, Arlin Crotts, and Zoltán Haiman. “Constraints on the Abundance
    of Highly Ionized Protocluster Regions from the Absence of Large Voids in the
    Lyα Forest.” <i>The Astrophysical Journal</i>. American Astronomical Society,
    2007. <a href="https://doi.org/10.1086/522331">https://doi.org/10.1086/522331</a>.
  ieee: C. Shang, A. Crotts, and Z. Haiman, “Constraints on the abundance of highly
    ionized protocluster regions from the absence of large voids in the Lyα forest,”
    <i>The Astrophysical Journal</i>, vol. 671, no. 1. American Astronomical Society,
    pp. 136–145, 2007.
  ista: Shang C, Crotts A, Haiman Z. 2007. Constraints on the abundance of highly
    ionized protocluster regions from the absence of large voids in the Lyα forest.
    The Astrophysical Journal. 671(1), 136–145.
  mla: Shang, Cien, et al. “Constraints on the Abundance of Highly Ionized Protocluster
    Regions from the Absence of Large Voids in the Lyα Forest.” <i>The Astrophysical
    Journal</i>, vol. 671, no. 1, American Astronomical Society, 2007, pp. 136–45,
    doi:<a href="https://doi.org/10.1086/522331">10.1086/522331</a>.
  short: C. Shang, A. Crotts, Z. Haiman, The Astrophysical Journal 671 (2007) 136–145.
date_created: 2024-09-06T09:17:23Z
date_published: 2007-12-10T00:00:00Z
date_updated: 2024-09-26T07:42:13Z
day: '10'
doi: 10.1086/522331
extern: '1'
intvolume: '       671'
issue: '1'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1086/522331
month: '12'
oa: 1
oa_version: Published Version
page: 136-145
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: Constraints on the abundance of highly ionized protocluster regions from the
  absence of large voids in the Lyα forest
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 671
year: '2007'
...
---
_id: '17738'
abstract:
- lang: eng
  text: Recent observations reveal that a majority of galaxies contain a central massive
    object (CMO), either a supermassive black hole (SMBH) or a compact stellar nucleus,
    regardless of the galaxy mass or morphological type. The masses of these CMOs
    correlate tightly with those of the host galaxies, MCMO ≈ 0.002Mgal. Several recent
    studies argue that feedback from black holes can successfully explain the MBH-σ
    correlation in massive elliptical galaxies that contain SMBHs. However, puzzles
    remain in spirals or dwarf spheroids that do not appear to have black holes but
    instead harbor a compact central stellar cluster. Here we use three-dimensional,
    smoothed particle hydrodynamics simulations of both isolated and merging galaxies
    to study the formation and evolution of CMOs in bulgeless disk galaxies, and the
    transition of the CMO-host relations from late-type bulgeless spirals to early-type
    ellipticals. Our simulations show that the mass of the CMO correlates with that
    of the host galaxy in both isolated bulgeless spirals and in ellipticals formed
    through mergers, and that MCMO correlates with the global star formation efficiency
    in the galaxy. We find that the final mass of the CMO is dominated by the accreted
    mass, rather than the initial fragment mass, and that both the final accreted
    CMO mass and the recently formed stellar mass increase monotonically with the
    total mass of the galaxy. Our results suggest that the observed correlations may
    be established primarily by the depletion of gas in the central region by accretion
    and star formation, and may hold for all galaxy types. A systematic search for
    CMOs in the nuclei of bulgeless disk galaxies would offer a test of this conclusion.
article_processing_charge: No
article_type: original
author:
- first_name: Yuexing
  full_name: Li, Yuexing
  last_name: Li
- first_name: Zoltán
  full_name: Haiman, Zoltán
  id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
  last_name: Haiman
- first_name: Mordecai‐Mark
  full_name: Mac Low, Mordecai‐Mark
  last_name: Mac Low
citation:
  ama: 'Li Y, Haiman Z, Mac Low M. Correlations between central massive objects and
    their host galaxies: From bulgeless spirals to ellipticals. <i>The Astrophysical
    Journal</i>. 2007;663(1):61-70. doi:<a href="https://doi.org/10.1086/518398">10.1086/518398</a>'
  apa: 'Li, Y., Haiman, Z., &#38; Mac Low, M. (2007). Correlations between central
    massive objects and their host galaxies: From bulgeless spirals to ellipticals.
    <i>The Astrophysical Journal</i>. American Astronomical Society. <a href="https://doi.org/10.1086/518398">https://doi.org/10.1086/518398</a>'
  chicago: 'Li, Yuexing, Zoltán Haiman, and Mordecai‐Mark Mac Low. “Correlations between
    Central Massive Objects and Their Host Galaxies: From Bulgeless Spirals to Ellipticals.”
    <i>The Astrophysical Journal</i>. American Astronomical Society, 2007. <a href="https://doi.org/10.1086/518398">https://doi.org/10.1086/518398</a>.'
  ieee: 'Y. Li, Z. Haiman, and M. Mac Low, “Correlations between central massive objects
    and their host galaxies: From bulgeless spirals to ellipticals,” <i>The Astrophysical
    Journal</i>, vol. 663, no. 1. American Astronomical Society, pp. 61–70, 2007.'
  ista: 'Li Y, Haiman Z, Mac Low M. 2007. Correlations between central massive objects
    and their host galaxies: From bulgeless spirals to ellipticals. The Astrophysical
    Journal. 663(1), 61–70.'
  mla: 'Li, Yuexing, et al. “Correlations between Central Massive Objects and Their
    Host Galaxies: From Bulgeless Spirals to Ellipticals.” <i>The Astrophysical Journal</i>,
    vol. 663, no. 1, American Astronomical Society, 2007, pp. 61–70, doi:<a href="https://doi.org/10.1086/518398">10.1086/518398</a>.'
  short: Y. Li, Z. Haiman, M. Mac Low, The Astrophysical Journal 663 (2007) 61–70.
date_created: 2024-09-06T09:21:21Z
date_published: 2007-07-01T00:00:00Z
date_updated: 2024-09-26T14:06:48Z
day: '01'
doi: 10.1086/518398
extern: '1'
intvolume: '       663'
issue: '1'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1086/518398
month: '07'
oa: 1
oa_version: Published Version
page: 61-70
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: 'Correlations between central massive objects and their host galaxies: From
  bulgeless spirals to ellipticals'
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 663
year: '2007'
...
---
_id: '17753'
abstract:
- lang: eng
  text: 'We use the spectra of 22,000 nearby early-type galaxies from the Sloan Digital
    Sky Survey (SDSS) to determine the age distribution of these galaxies as a function
    of their velocity dispersion sigma_v in the range 100 km/s < sigma_v < 280 km/s.
    We then combine the inferred age-distributions with the local abundance of spheroids,
    including early-type galaxies and late-type bulges, to predict the evolution of
    the quasar luminosity function (LF) in the redshift range 0<z<6. We make the following
    simple assumptions: (i) the formation of stars in each galaxy, at the epoch identified
    with the mean mass-weighted stellar age, is accompanied by the prompt assembly
    of the nuclear supermassive black hole (SMBH); (ii) the mass of the SMBH obeys
    the M_bh-sigma_v correlation observed in nearby galaxies; (iii) the SMBH radiates
    at a fraction f_Edd of the Eddington limit for a fixed duration t_Q, and is identified
    as a luminous quasar during this epoch, (iv) the intrinsic dispersions in the
    Eddington ratio and the M_bh-sigma_v relation produce a combined scatter of Delta(log
    L_Q) around the mean logarithmic quasar luminosity <log L_Q> at fixed sigma_v.
    These assumptions require that the SMBH remnants of quasars with bolometric luminosity
    below L_bol=10^{12.5} f_Edd L_sun reside predominantly in bulges of late type
    galaxies. We find that evolution of the observed quasar LF can be fit over the
    entire redshift range in this simple model, 0<z<6 with the choices of Delta(log
    L_Q)=0.6-0.9, t_Q= (6-8)x10^7 yr, and <f_Edd>=0.3-0.5. We find no evidence that
    any of the model parameters evolves with redshift, supporting the strong connection
    between the formation of stars and nuclear SMBHs in spheroids.'
article_processing_charge: No
article_type: original
author:
- first_name: Zoltán
  full_name: Haiman, Zoltán
  id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
  last_name: Haiman
- first_name: Raul
  full_name: Jimenez, Raul
  last_name: Jimenez
- first_name: Mariangela
  full_name: Bernardi, Mariangela
  last_name: Bernardi
citation:
  ama: Haiman Z, Jimenez R, Bernardi M. Reconstructing the cosmic evolution of quasars
    from the age distribution of local early‐type galaxies. <i>The Astrophysical Journal</i>.
    2007;658(2):721-730. doi:<a href="https://doi.org/10.1086/510840">10.1086/510840</a>
  apa: Haiman, Z., Jimenez, R., &#38; Bernardi, M. (2007). Reconstructing the cosmic
    evolution of quasars from the age distribution of local early‐type galaxies. <i>The
    Astrophysical Journal</i>. American Astronomical Society. <a href="https://doi.org/10.1086/510840">https://doi.org/10.1086/510840</a>
  chicago: Haiman, Zoltán, Raul Jimenez, and Mariangela Bernardi. “Reconstructing
    the Cosmic Evolution of Quasars from the Age Distribution of Local Early‐type
    Galaxies.” <i>The Astrophysical Journal</i>. American Astronomical Society, 2007.
    <a href="https://doi.org/10.1086/510840">https://doi.org/10.1086/510840</a>.
  ieee: Z. Haiman, R. Jimenez, and M. Bernardi, “Reconstructing the cosmic evolution
    of quasars from the age distribution of local early‐type galaxies,” <i>The Astrophysical
    Journal</i>, vol. 658, no. 2. American Astronomical Society, pp. 721–730, 2007.
  ista: Haiman Z, Jimenez R, Bernardi M. 2007. Reconstructing the cosmic evolution
    of quasars from the age distribution of local early‐type galaxies. The Astrophysical
    Journal. 658(2), 721–730.
  mla: Haiman, Zoltán, et al. “Reconstructing the Cosmic Evolution of Quasars from
    the Age Distribution of Local Early‐type Galaxies.” <i>The Astrophysical Journal</i>,
    vol. 658, no. 2, American Astronomical Society, 2007, pp. 721–30, doi:<a href="https://doi.org/10.1086/510840">10.1086/510840</a>.
  short: Z. Haiman, R. Jimenez, M. Bernardi, The Astrophysical Journal 658 (2007)
    721–730.
date_created: 2024-09-06T09:40:51Z
date_published: 2007-04-01T00:00:00Z
date_updated: 2024-09-30T07:55:40Z
day: '01'
doi: 10.1086/510840
extern: '1'
intvolume: '       658'
issue: '2'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1086/510840
month: '04'
oa: 1
oa_version: Published Version
page: 721-730
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: Reconstructing the cosmic evolution of quasars from the age distribution of
  local early‐type galaxies
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 658
year: '2007'
...
---
_id: '17755'
article_processing_charge: No
author:
- first_name: B.
  full_name: Kocsis, B.
  last_name: Kocsis
- first_name: Zoltán
  full_name: Haiman, Zoltán
  id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
  last_name: Haiman
- first_name: Z.
  full_name: Frei, Z.
  last_name: Frei
citation:
  ama: 'Kocsis B, Haiman Z, Frei Z. Detecting virialization shocks around galaxy clusters
    through the SZ effect. In: <i>ESO Astrophysics Symposia</i>. ESO Astrophysics
    Symposia. Berlin, Heidelberg: Springer Berlin Heidelberg; 2007:334-336. doi:<a
    href="https://doi.org/10.1007/978-3-540-74713-0_77">10.1007/978-3-540-74713-0_77</a>'
  apa: 'Kocsis, B., Haiman, Z., &#38; Frei, Z. (2007). Detecting virialization shocks
    around galaxy clusters through the SZ effect. In <i>ESO Astrophysics Symposia</i>
    (pp. 334–336). Berlin, Heidelberg: Springer Berlin Heidelberg. <a href="https://doi.org/10.1007/978-3-540-74713-0_77">https://doi.org/10.1007/978-3-540-74713-0_77</a>'
  chicago: 'Kocsis, B., Zoltán Haiman, and Z. Frei. “Detecting Virialization Shocks
    around Galaxy Clusters through the SZ Effect.” In <i>ESO Astrophysics Symposia</i>,
    334–36. ESO Astrophysics Symposia. Berlin, Heidelberg: Springer Berlin Heidelberg,
    2007. <a href="https://doi.org/10.1007/978-3-540-74713-0_77">https://doi.org/10.1007/978-3-540-74713-0_77</a>.'
  ieee: B. Kocsis, Z. Haiman, and Z. Frei, “Detecting virialization shocks around
    galaxy clusters through the SZ effect,” in <i>ESO Astrophysics Symposia</i>, Munich,
    Germany, 2007, pp. 334–336.
  ista: Kocsis B, Haiman Z, Frei Z. 2007. Detecting virialization shocks around galaxy
    clusters through the SZ effect. ESO Astrophysics Symposia. Proceedings of the
    MPE/USM/MPA/ESO Joint Astronomy ConferenceESO Astrophysics Symposia, 334–336.
  mla: Kocsis, B., et al. “Detecting Virialization Shocks around Galaxy Clusters through
    the SZ Effect.” <i>ESO Astrophysics Symposia</i>, Springer Berlin Heidelberg,
    2007, pp. 334–36, doi:<a href="https://doi.org/10.1007/978-3-540-74713-0_77">10.1007/978-3-540-74713-0_77</a>.
  short: B. Kocsis, Z. Haiman, Z. Frei, in:, ESO Astrophysics Symposia, Springer Berlin
    Heidelberg, Berlin, Heidelberg, 2007, pp. 334–336.
conference:
  end_date: 2005-11-11
  location: Munich, Germany
  name: Proceedings of the MPE/USM/MPA/ESO Joint Astronomy Conference
  start_date: 2005-11-07
date_created: 2024-09-06T09:43:32Z
date_published: 2007-10-20T00:00:00Z
date_updated: 2024-09-30T08:33:49Z
day: '20'
doi: 10.1007/978-3-540-74713-0_77
extern: '1'
language:
- iso: eng
main_file_link:
- url: https://doi.org/10.1007/978-3-540-74713-0_77
month: '10'
oa_version: None
page: 334-336
place: Berlin, Heidelberg
publication: ESO Astrophysics Symposia
publication_identifier:
  isbn:
  - '9783540747123'
publication_status: published
publisher: Springer Berlin Heidelberg
quality_controlled: '1'
scopus_import: '1'
series_title: ESO Astrophysics Symposia
status: public
title: Detecting virialization shocks around galaxy clusters through the SZ effect
type: conference
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
year: '2007'
...
---
_id: '17768'
abstract:
- lang: eng
  text: 'We develop an analytic approach to study inhomogeneous reionization on large
    scales by solving the equations of ionization balance and radiative transfer to
    first order in perturbations. Given the spatial distribution and spectrum of the
    ionizing sources, our formalism can be used to predict the large-scale power spectra
    of fluctuations in the abundances of H ii, H i and radiation. Our approach avoids
    common approximations/assumptions in existing analytic methods – for instance,
    we do not assume a specific ionization topology from the outset; nor do we make
    a step-function bubble-like approximation to the H ii distribution. Applying our
    formalism to sources biased according to the Press–Schechter prescription, we
    find: (1) reionization always proceeds ‘inside–out’, with dense regions more highly
    ionized, at least on large scales; (2) on sufficiently large scales, H ii, H i
    and radiation exhibit a scale-independent bias relative to dark matter; (3) the
    bias is suppressed on scales comparable to or smaller than the mean free path
    of the ionizing photons; (4) if the ionizing source spectrum is sufficiently soft,
    the H ii bias closely tracks the source bias for most of the reionization process
    but drops precipitously after percolation; and (5) if the ionizing source spectrum
    is sufficiently hard, the H ii bias drops in a more steady fashion throughout
    the reionization process. The tools developed here will be useful for interpreting
    future 21-cm, cosmic microwave background and Lyman α forest observations, both
    to learn about the reionization astrophysics (such as the hardness of the source
    spectrum and therefore the nature of the ionizing sources) and to possibly extract
    interesting cosmological information.'
article_processing_charge: No
article_type: original
author:
- first_name: J.
  full_name: Zhang, J.
  last_name: Zhang
- first_name: L.
  full_name: Hui, L.
  last_name: Hui
- first_name: Zoltán
  full_name: Haiman, Zoltán
  id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
  last_name: Haiman
citation:
  ama: Zhang J, Hui L, Haiman Z. A linear perturbation theory of inhomogeneous reionization.
    <i>Monthly Notices of the Royal Astronomical Society</i>. 2007;375(1):324-336.
    doi:<a href="https://doi.org/10.1111/j.1365-2966.2006.11311.x">10.1111/j.1365-2966.2006.11311.x</a>
  apa: Zhang, J., Hui, L., &#38; Haiman, Z. (2007). A linear perturbation theory of
    inhomogeneous reionization. <i>Monthly Notices of the Royal Astronomical Society</i>.
    Oxford University Press. <a href="https://doi.org/10.1111/j.1365-2966.2006.11311.x">https://doi.org/10.1111/j.1365-2966.2006.11311.x</a>
  chicago: Zhang, J., L. Hui, and Zoltán Haiman. “A Linear Perturbation Theory of
    Inhomogeneous Reionization.” <i>Monthly Notices of the Royal Astronomical Society</i>.
    Oxford University Press, 2007. <a href="https://doi.org/10.1111/j.1365-2966.2006.11311.x">https://doi.org/10.1111/j.1365-2966.2006.11311.x</a>.
  ieee: J. Zhang, L. Hui, and Z. Haiman, “A linear perturbation theory of inhomogeneous
    reionization,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol.
    375, no. 1. Oxford University Press, pp. 324–336, 2007.
  ista: Zhang J, Hui L, Haiman Z. 2007. A linear perturbation theory of inhomogeneous
    reionization. Monthly Notices of the Royal Astronomical Society. 375(1), 324–336.
  mla: Zhang, J., et al. “A Linear Perturbation Theory of Inhomogeneous Reionization.”
    <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 375, no. 1, Oxford
    University Press, 2007, pp. 324–36, doi:<a href="https://doi.org/10.1111/j.1365-2966.2006.11311.x">10.1111/j.1365-2966.2006.11311.x</a>.
  short: J. Zhang, L. Hui, Z. Haiman, Monthly Notices of the Royal Astronomical Society
    375 (2007) 324–336.
date_created: 2024-09-06T09:55:13Z
date_published: 2007-01-15T00:00:00Z
date_updated: 2024-09-30T09:36:26Z
day: '15'
doi: 10.1111/j.1365-2966.2006.11311.x
extern: '1'
intvolume: '       375'
issue: '1'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1111/j.1365-2966.2006.11311.x
month: '01'
oa: 1
oa_version: Published Version
page: 324-336
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: A linear perturbation theory of inhomogeneous reionization
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 375
year: '2007'
...
---
_id: '17783'
abstract:
- lang: eng
  text: 'We apply the technique of parameter-splitting to existing cosmological data
    sets, to check for a generic failure of dark energy models. Given a dark energy
    parameter, such as the energy density Omega_Lambda or equation of state w, we
    split it into two meta-parameters with one controlling geometrical distances,
    and the other controlling the growth of structure. Observational data spanning
    Type Ia Supernovae, the cosmic microwave background (CMB), galaxy clustering,
    and weak gravitational lensing statistics are fit without requiring the two meta-parameters
    to be equal. This technique checks for inconsistency between different data sets,
    as well as for internal inconsistency within any one data set (e.g., CMB or lensing
    statistics) that is sensitive to both geometry and growth. We find that the cosmological
    constant model is consistent with current data. Theories of modified gravity generally
    predict a relation between growth and geometry that is different from that of
    general relativity. Parameter-splitting can be viewed as a crude way to parametrize
    the space of such theories. Our analysis of current data already appears to put
    sharp limits on these theories: assuming a flat universe, current data constrain
    the difference Omega_Lambda(geom) - Omega_Lambda(grow) to be -0.0044 +/- 0.0058
    (68% C.L.); allowing the equation of state w to vary, the difference w(geom) -
    w(grow) is constrained to be 0.37 +/- 0.37 (68% C.L.). Interestingly, the region
    w(grow) > w(geom), which should be generically favored by theories that slow structure
    formation relative to general relativity, is quite restricted by data already.
    We find w(grow) < -0.80 at 2 sigma. As an example, the best-fit flat Dvali-Gabadadze-Porrati
    (DGP) model approximated by our parametrization lies beyond the 3 sigma contour
    for constraints from all the data sets.'
article_number: '063503'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Sheng
  full_name: Wang, Sheng
  last_name: Wang
- first_name: Lam
  full_name: Hui, Lam
  last_name: Hui
- first_name: Morgan
  full_name: May, Morgan
  last_name: May
- first_name: Zoltán
  full_name: Haiman, Zoltán
  id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
  last_name: Haiman
citation:
  ama: Wang S, Hui L, May M, Haiman Z. Is modified gravity required by observations?
    An empirical consistency test of dark energy models. <i>Physical Review D</i>.
    2007;76(6). doi:<a href="https://doi.org/10.1103/physrevd.76.063503">10.1103/physrevd.76.063503</a>
  apa: Wang, S., Hui, L., May, M., &#38; Haiman, Z. (2007). Is modified gravity required
    by observations? An empirical consistency test of dark energy models. <i>Physical
    Review D</i>. American Physical Society. <a href="https://doi.org/10.1103/physrevd.76.063503">https://doi.org/10.1103/physrevd.76.063503</a>
  chicago: Wang, Sheng, Lam Hui, Morgan May, and Zoltán Haiman. “Is Modified Gravity
    Required by Observations? An Empirical Consistency Test of Dark Energy Models.”
    <i>Physical Review D</i>. American Physical Society, 2007. <a href="https://doi.org/10.1103/physrevd.76.063503">https://doi.org/10.1103/physrevd.76.063503</a>.
  ieee: S. Wang, L. Hui, M. May, and Z. Haiman, “Is modified gravity required by observations?
    An empirical consistency test of dark energy models,” <i>Physical Review D</i>,
    vol. 76, no. 6. American Physical Society, 2007.
  ista: Wang S, Hui L, May M, Haiman Z. 2007. Is modified gravity required by observations?
    An empirical consistency test of dark energy models. Physical Review D. 76(6),
    063503.
  mla: Wang, Sheng, et al. “Is Modified Gravity Required by Observations? An Empirical
    Consistency Test of Dark Energy Models.” <i>Physical Review D</i>, vol. 76, no.
    6, 063503, American Physical Society, 2007, doi:<a href="https://doi.org/10.1103/physrevd.76.063503">10.1103/physrevd.76.063503</a>.
  short: S. Wang, L. Hui, M. May, Z. Haiman, Physical Review D 76 (2007).
date_created: 2024-09-06T10:16:50Z
date_published: 2007-09-12T00:00:00Z
date_updated: 2024-09-30T12:45:38Z
day: '12'
doi: 10.1103/physrevd.76.063503
extern: '1'
external_id:
  arxiv:
  - '0705.0165'
intvolume: '        76'
issue: '6'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.48550/arXiv.0705.0165
month: '09'
oa: 1
oa_version: Preprint
publication: Physical Review D
publication_identifier:
  issn:
  - 1550-7998
  - 1550-2368
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Is modified gravity required by observations? An empirical consistency test
  of dark energy models
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 76
year: '2007'
...
---
_id: '17784'
article_processing_charge: No
author:
- first_name: M.E.
  full_name: Gáspár, M.E.
  last_name: Gáspár
- first_name: Zoltán
  full_name: Haiman, Zoltán
  id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
  last_name: Haiman
- first_name: Z.
  full_name: Frei, Z.
  last_name: Frei
citation:
  ama: 'Gáspár ME, Haiman Z, Frei Z. Mass function of remnant black holes in nearby
    galaxies. In: <i>ESO Astrophysics Symposia</i>. Berlin, Heidelberg: Springer Berlin
    Heidelberg; 2007. doi:<a href="https://doi.org/10.1007/978-3-540-74713-0_31">10.1007/978-3-540-74713-0_31</a>'
  apa: 'Gáspár, M. E., Haiman, Z., &#38; Frei, Z. (2007). Mass function of remnant
    black holes in nearby galaxies. In <i>ESO Astrophysics Symposia</i>. Berlin, Heidelberg:
    Springer Berlin Heidelberg. <a href="https://doi.org/10.1007/978-3-540-74713-0_31">https://doi.org/10.1007/978-3-540-74713-0_31</a>'
  chicago: 'Gáspár, M.E., Zoltán Haiman, and Z. Frei. “Mass Function of Remnant Black
    Holes in Nearby Galaxies.” In <i>ESO Astrophysics Symposia</i>. Berlin, Heidelberg:
    Springer Berlin Heidelberg, 2007. <a href="https://doi.org/10.1007/978-3-540-74713-0_31">https://doi.org/10.1007/978-3-540-74713-0_31</a>.'
  ieee: M. E. Gáspár, Z. Haiman, and Z. Frei, “Mass function of remnant black holes
    in nearby galaxies,” in <i>ESO Astrophysics Symposia</i>, Munich, Germany, 2007.
  ista: Gáspár ME, Haiman Z, Frei Z. 2007. Mass function of remnant black holes in
    nearby galaxies. ESO Astrophysics Symposia. Proceedings of the MPE/USM/MPA/ESO
    Joint Astronomy Conference.
  mla: Gáspár, M. E., et al. “Mass Function of Remnant Black Holes in Nearby Galaxies.”
    <i>ESO Astrophysics Symposia</i>, Springer Berlin Heidelberg, 2007, doi:<a href="https://doi.org/10.1007/978-3-540-74713-0_31">10.1007/978-3-540-74713-0_31</a>.
  short: M.E. Gáspár, Z. Haiman, Z. Frei, in:, ESO Astrophysics Symposia, Springer
    Berlin Heidelberg, Berlin, Heidelberg, 2007.
conference:
  end_date: 2005-11-11
  location: Munich, Germany
  name: Proceedings of the MPE/USM/MPA/ESO Joint Astronomy Conference
  start_date: 2005-11-07
date_created: 2024-09-06T10:17:34Z
date_published: 2007-01-01T00:00:00Z
date_updated: 2024-09-30T12:52:00Z
doi: 10.1007/978-3-540-74713-0_31
extern: '1'
language:
- iso: eng
main_file_link:
- url: https://doi.org/10.1007/978-3-540-74713-0_31
month: '01'
oa_version: None
place: Berlin, Heidelberg
publication: ESO Astrophysics Symposia
publication_identifier:
  isbn:
  - '9783540747123'
publication_status: published
publisher: Springer Berlin Heidelberg
quality_controlled: '1'
scopus_import: '1'
status: public
title: Mass function of remnant black holes in nearby galaxies
type: conference
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
year: '2007'
...
---
_id: '17785'
abstract:
- lang: eng
  text: We study the potential of a large future weak-lensing survey to constrain
    dark energy properties by using both the number counts of detected galaxy clusters
    (sensitive primarily to density fluctuations on small scales) and tomographic
    shear-shear correlations (restricted to large scales). We use the Fisher matrix
    formalism, assume a flat universe and parameterize the equation of state of dark
    energy by w(a)=w_0+w_a(1-a), to forecast the expected statistical errors from
    either observable, and from their combination. We show that the covariance between
    these two observables is small, and argue that therefore they can be regarded
    as independent constraints. We find that when the number counts and the shear-shear
    correlations (on angular scales l < 1000) are combined, an LSST (Large Synoptic
    Survey Telescope)-like survey can yield statistical errors on (Omega_DE, w_0,
    w_a) as tight as (0.003, 0.03, 0.1). These values are a factor of 2-25 better
    than using either observable alone. The results are also about a factor of two
    better than those from combining number counts of galaxy clusters and their power
    spectrum.
article_number: '043010'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Wenjuan
  full_name: Fang, Wenjuan
  last_name: Fang
- first_name: Zoltán
  full_name: Haiman, Zoltán
  id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
  last_name: Haiman
citation:
  ama: Fang W, Haiman Z. Constraining dark energy by combining cluster counts and
    shear-shear correlations in a weak lensing survey. <i>Physical Review D</i>. 2007;75(4).
    doi:<a href="https://doi.org/10.1103/physrevd.75.043010">10.1103/physrevd.75.043010</a>
  apa: Fang, W., &#38; Haiman, Z. (2007). Constraining dark energy by combining cluster
    counts and shear-shear correlations in a weak lensing survey. <i>Physical Review
    D</i>. American Physical Society. <a href="https://doi.org/10.1103/physrevd.75.043010">https://doi.org/10.1103/physrevd.75.043010</a>
  chicago: Fang, Wenjuan, and Zoltán Haiman. “Constraining Dark Energy by Combining
    Cluster Counts and Shear-Shear Correlations in a Weak Lensing Survey.” <i>Physical
    Review D</i>. American Physical Society, 2007. <a href="https://doi.org/10.1103/physrevd.75.043010">https://doi.org/10.1103/physrevd.75.043010</a>.
  ieee: W. Fang and Z. Haiman, “Constraining dark energy by combining cluster counts
    and shear-shear correlations in a weak lensing survey,” <i>Physical Review D</i>,
    vol. 75, no. 4. American Physical Society, 2007.
  ista: Fang W, Haiman Z. 2007. Constraining dark energy by combining cluster counts
    and shear-shear correlations in a weak lensing survey. Physical Review D. 75(4),
    043010.
  mla: Fang, Wenjuan, and Zoltán Haiman. “Constraining Dark Energy by Combining Cluster
    Counts and Shear-Shear Correlations in a Weak Lensing Survey.” <i>Physical Review
    D</i>, vol. 75, no. 4, 043010, American Physical Society, 2007, doi:<a href="https://doi.org/10.1103/physrevd.75.043010">10.1103/physrevd.75.043010</a>.
  short: W. Fang, Z. Haiman, Physical Review D 75 (2007).
date_created: 2024-09-06T10:18:16Z
date_published: 2007-02-26T00:00:00Z
date_updated: 2024-09-30T12:55:54Z
day: '26'
doi: 10.1103/physrevd.75.043010
extern: '1'
external_id:
  arxiv:
  - '0612187'
intvolume: '        75'
issue: '4'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: ' https://doi.org/10.48550/arXiv.astro-ph/0612187'
month: '02'
oa: 1
oa_version: Preprint
publication: Physical Review D
publication_identifier:
  issn:
  - 1550-7998
  - 1550-2368
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Constraining dark energy by combining cluster counts and shear-shear correlations
  in a weak lensing survey
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 75
year: '2007'
...
---
_id: '17791'
abstract:
- lang: eng
  text: We consider the pumping of the 63.2 μm fine-structure line of neutral O I
    in the high-redshift intergalactic medium (IGM), in analogy with the Wouthuysen-Field
    effect for the 21 cm line of cosmic H I. We show that the soft UV background at
    ~1300 Å can affect the population levels, and if a significant fraction of the
    IGM volume is filled with "fossil H II regions" containing neutral O I, then this
    can produce a nonnegligible spectral distortion in the cosmic microwave background
    (CMB). O I from redshift z is seen in emission at (1 + z)63.2 μm, and in the range
    7 < z < 10 produces a mean spectral distortion of the CMB with y = (10^-9 to 3
    × 10^-8)(Z/10^-3 Z☉)(IUV), where Z is the mean metallicity of the IGM and IUV
    is the UV background at 1300 Å in units of 10^-20 ergs s-1 Hz^-1 cm-2 sr^-1. A
    measurement of this signature can trace the metallicity at the end of the dark
    ages, prior to the completion of cosmic reionization, and is complementary to
    cosmological 21 cm studies. While future CMB experiments such as Planck could
    constrain the metallicity to the 10^-2 Z☉ level, specifically designed experiments
    could potentially achieve a detection.
article_processing_charge: No
article_type: original
author:
- first_name: Carlos
  full_name: Hernández-Monteagudo, Carlos
  last_name: Hernández-Monteagudo
- first_name: Zoltán
  full_name: Haiman, Zoltán
  id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
  last_name: Haiman
- first_name: Raul
  full_name: Jimenez, Raul
  last_name: Jimenez
- first_name: Licia
  full_name: Verde, Licia
  last_name: Verde
citation:
  ama: 'Hernández-Monteagudo C, Haiman Z, Jimenez R, Verde L. Oxygen pumping: Probing
    intergalactic metals at the epoch of reionization. <i>The Astrophysical Journal</i>.
    2007;660(2):L85-L88. doi:<a href="https://doi.org/10.1086/518090">10.1086/518090</a>'
  apa: 'Hernández-Monteagudo, C., Haiman, Z., Jimenez, R., &#38; Verde, L. (2007).
    Oxygen pumping: Probing intergalactic metals at the epoch of reionization. <i>The
    Astrophysical Journal</i>. American Astronomical Society. <a href="https://doi.org/10.1086/518090">https://doi.org/10.1086/518090</a>'
  chicago: 'Hernández-Monteagudo, Carlos, Zoltán Haiman, Raul Jimenez, and Licia Verde.
    “Oxygen Pumping: Probing Intergalactic Metals at the Epoch of Reionization.” <i>The
    Astrophysical Journal</i>. American Astronomical Society, 2007. <a href="https://doi.org/10.1086/518090">https://doi.org/10.1086/518090</a>.'
  ieee: 'C. Hernández-Monteagudo, Z. Haiman, R. Jimenez, and L. Verde, “Oxygen pumping:
    Probing intergalactic metals at the epoch of reionization,” <i>The Astrophysical
    Journal</i>, vol. 660, no. 2. American Astronomical Society, pp. L85–L88, 2007.'
  ista: 'Hernández-Monteagudo C, Haiman Z, Jimenez R, Verde L. 2007. Oxygen pumping:
    Probing intergalactic metals at the epoch of reionization. The Astrophysical Journal.
    660(2), L85–L88.'
  mla: 'Hernández-Monteagudo, Carlos, et al. “Oxygen Pumping: Probing Intergalactic
    Metals at the Epoch of Reionization.” <i>The Astrophysical Journal</i>, vol. 660,
    no. 2, American Astronomical Society, 2007, pp. L85–88, doi:<a href="https://doi.org/10.1086/518090">10.1086/518090</a>.'
  short: C. Hernández-Monteagudo, Z. Haiman, R. Jimenez, L. Verde, The Astrophysical
    Journal 660 (2007) L85–L88.
date_created: 2024-09-06T10:23:23Z
date_published: 2007-04-11T00:00:00Z
date_updated: 2024-09-30T13:59:15Z
day: '11'
doi: 10.1086/518090
extern: '1'
intvolume: '       660'
issue: '2'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1086/518090
month: '04'
oa: 1
oa_version: Published Version
page: L85-L88
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: 'Oxygen pumping: Probing intergalactic metals at the epoch of reionization'
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 660
year: '2007'
...
---
_id: '17793'
abstract:
- lang: eng
  text: 'We use the spectra of ~22,000 early-type galaxies, selected from the Sloan
    Digital Sky Survey, to infer the ages, metallicities, and star formation histories
    of these galaxies. We find clear evidence of "downsizing," i.e., that galaxies
    with larger velocity dispersion have older stellar populations. In particular,
    we find that most early-type galaxies with velocity dispersion exceeding 200 km
    s-1 formed more than 90% of their current stellar mass at redshift z > 2.5. Therefore,
    star formation was suppressed around this redshift. We also show that chemical
    enrichment was rapid, lasting 1-2 Gyr, and find evidence that [Fe/H] is subsolar.
    We study the robustness of these results by comparing three different approaches:
    (1) using Lick absorption line indices, (2) fitting a single-burst stellar population
    model to the whole spectrum (lines and continuum), and (3) reconstructing the
    star formation and metallicity histories in multiple age bins, providing a method
    to measure mass-weighted ages and metallicities. We find good agreement between
    the luminosity-weighted ages and metallicities computed with these three methods.'
article_processing_charge: No
article_type: original
author:
- first_name: Raul
  full_name: Jimenez, Raul
  last_name: Jimenez
- first_name: Mariangela
  full_name: Bernardi, Mariangela
  last_name: Bernardi
- first_name: Zoltán
  full_name: Haiman, Zoltán
  id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
  last_name: Haiman
- first_name: Ben
  full_name: Panter, Ben
  last_name: Panter
- first_name: Alan F.
  full_name: Heavens, Alan F.
  last_name: Heavens
citation:
  ama: Jimenez R, Bernardi M, Haiman Z, Panter B, Heavens AF. The ages, metallicities,
    and star formation histories of early‐type galaxies in the SDSS. <i>The Astrophysical
    Journal</i>. 2007;669(2):947-951. doi:<a href="https://doi.org/10.1086/521323">10.1086/521323</a>
  apa: Jimenez, R., Bernardi, M., Haiman, Z., Panter, B., &#38; Heavens, A. F. (2007).
    The ages, metallicities, and star formation histories of early‐type galaxies in
    the SDSS. <i>The Astrophysical Journal</i>. American Astronomical Society. <a
    href="https://doi.org/10.1086/521323">https://doi.org/10.1086/521323</a>
  chicago: Jimenez, Raul, Mariangela Bernardi, Zoltán Haiman, Ben Panter, and Alan
    F. Heavens. “The Ages, Metallicities, and Star Formation Histories of Early‐type
    Galaxies in the SDSS.” <i>The Astrophysical Journal</i>. American Astronomical
    Society, 2007. <a href="https://doi.org/10.1086/521323">https://doi.org/10.1086/521323</a>.
  ieee: R. Jimenez, M. Bernardi, Z. Haiman, B. Panter, and A. F. Heavens, “The ages,
    metallicities, and star formation histories of early‐type galaxies in the SDSS,”
    <i>The Astrophysical Journal</i>, vol. 669, no. 2. American Astronomical Society,
    pp. 947–951, 2007.
  ista: Jimenez R, Bernardi M, Haiman Z, Panter B, Heavens AF. 2007. The ages, metallicities,
    and star formation histories of early‐type galaxies in the SDSS. The Astrophysical
    Journal. 669(2), 947–951.
  mla: Jimenez, Raul, et al. “The Ages, Metallicities, and Star Formation Histories
    of Early‐type Galaxies in the SDSS.” <i>The Astrophysical Journal</i>, vol. 669,
    no. 2, American Astronomical Society, 2007, pp. 947–51, doi:<a href="https://doi.org/10.1086/521323">10.1086/521323</a>.
  short: R. Jimenez, M. Bernardi, Z. Haiman, B. Panter, A.F. Heavens, The Astrophysical
    Journal 669 (2007) 947–951.
date_created: 2024-09-06T10:25:21Z
date_published: 2007-11-10T00:00:00Z
date_updated: 2024-09-30T14:09:15Z
day: '10'
doi: 10.1086/521323
extern: '1'
intvolume: '       669'
issue: '2'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1086/521323
month: '11'
oa: 1
oa_version: Published Version
page: 947-951
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: The ages, metallicities, and star formation histories of early‐type galaxies
  in the SDSS
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 669
year: '2007'
...
---
_id: '17795'
abstract:
- lang: eng
  text: The gravitational waves (GWs) emitted during the coalescence of supermassive
    black holes (SMBHs) will be detectable with the future Laser Interferometric Space
    Antenna (LISA). The direction and distance can be determined from the accumulated
    GW signal with a precision that increases rapidly in the final stages of the inspiral.
    We find that for M = (105 − 107)M⊙ near z = 1 the angular uncertainty decreases
    under 1ˆ at least several hours before the plunge, allowing a targeted electromagnetic
    (EM) observation of the final stages of the merger with a wide field instrument.
    We then calculate the size of the final, three dimensional error volume. Under
    the plausible assumption that SMBH-SMBH mergers are accompanied by gas accretion
    leading to Eddington-limited quasar activity, we find that many cases this error
    volume will contain at most a single quasar for M = (105 − 107) M⊙ near z = 1.
    This will allow a straightforward test of the hypothesis that GW events are accompanied
    by bright quasar activity. The identification and observation of counterparts
    would allow unprecedented tests of the physics of MBH accretion, such as precision–measurements
    of the Eddington ratio. They would clarify the role of gas as a catalyst in SMBH
    coalescences, and would also offer an alternative method to constrain cosmological
    parameters.
alternative_title:
- ESO Astrophysics Symposia
article_processing_charge: No
author:
- first_name: B.
  full_name: Kocsis, B.
  last_name: Kocsis
- first_name: Z.
  full_name: Frei, Z.
  last_name: Frei
- first_name: Zoltán
  full_name: Haiman, Zoltán
  id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
  last_name: Haiman
  orcid: 0000-0003-3633-5403
- first_name: K.
  full_name: Menou, K.
  last_name: Menou
citation:
  ama: 'Kocsis B, Frei Z, Haiman Z, Menou K. Finding the electromagnetic counterparts
    of standard sirens. In: <i>Proceedings of the 2005 MPE/USM/MPA/ESO Joint Astronomy
    Conference</i>. Berlin, Heidelberg: Springer Nature; 2007:82-86. doi:<a href="https://doi.org/10.1007/978-3-540-74713-0_18">10.1007/978-3-540-74713-0_18</a>'
  apa: 'Kocsis, B., Frei, Z., Haiman, Z., &#38; Menou, K. (2007). Finding the electromagnetic
    counterparts of standard sirens. In <i>Proceedings of the 2005 MPE/USM/MPA/ESO
    Joint Astronomy Conference</i> (pp. 82–86). Berlin, Heidelberg: Springer Nature.
    <a href="https://doi.org/10.1007/978-3-540-74713-0_18">https://doi.org/10.1007/978-3-540-74713-0_18</a>'
  chicago: 'Kocsis, B., Z. Frei, Zoltán Haiman, and K. Menou. “Finding the Electromagnetic
    Counterparts of Standard Sirens.” In <i>Proceedings of the 2005 MPE/USM/MPA/ESO
    Joint Astronomy Conference</i>, 82–86. Berlin, Heidelberg: Springer Nature, 2007.
    <a href="https://doi.org/10.1007/978-3-540-74713-0_18">https://doi.org/10.1007/978-3-540-74713-0_18</a>.'
  ieee: B. Kocsis, Z. Frei, Z. Haiman, and K. Menou, “Finding the electromagnetic
    counterparts of standard sirens,” in <i>Proceedings of the 2005 MPE/USM/MPA/ESO
    Joint Astronomy Conference</i>, Munich, Germany, 2007, pp. 82–86.
  ista: Kocsis B, Frei Z, Haiman Z, Menou K. 2007. Finding the electromagnetic counterparts
    of standard sirens. Proceedings of the 2005 MPE/USM/MPA/ESO Joint Astronomy Conference.
    , ESO Astrophysics Symposia, , 82–86.
  mla: Kocsis, B., et al. “Finding the Electromagnetic Counterparts of Standard Sirens.”
    <i>Proceedings of the 2005 MPE/USM/MPA/ESO Joint Astronomy Conference</i>, Springer
    Nature, 2007, pp. 82–86, doi:<a href="https://doi.org/10.1007/978-3-540-74713-0_18">10.1007/978-3-540-74713-0_18</a>.
  short: B. Kocsis, Z. Frei, Z. Haiman, K. Menou, in:, Proceedings of the 2005 MPE/USM/MPA/ESO
    Joint Astronomy Conference, Springer Nature, Berlin, Heidelberg, 2007, pp. 82–86.
conference:
  end_date: 2005-11-11
  location: Munich, Germany
  start_date: 2005-11-07
date_created: 2024-09-06T10:27:32Z
date_published: 2007-10-19T00:00:00Z
date_updated: 2024-10-02T06:35:30Z
day: '19'
doi: 10.1007/978-3-540-74713-0_18
extern: '1'
language:
- iso: eng
month: '10'
oa_version: None
page: 82-86
place: Berlin, Heidelberg
publication: Proceedings of the 2005 MPE/USM/MPA/ESO Joint Astronomy Conference
publication_identifier:
  isbn:
  - '9783540747123'
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
status: public
title: Finding the electromagnetic counterparts of standard sirens
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2007'
...
---
_id: '7704'
abstract:
- lang: eng
  text: Gradients of axon guidance molecules instruct the formation of continuous
    neural maps, such as the retinotopic map in the vertebrate visual system. Here
    we show that molecular gradients can also instruct the formation of a discrete
    neural map. In the fly olfactory system, axons of 50 classes of olfactory receptor
    neurons (ORNs) and dendrites of 50 classes of projection neurons (PNs) form one-to-one
    connections at discrete units called glomeruli. We provide expression, loss- and
    gain-of-function data to demonstrate that the levels of transmembrane Semaphorin-1a
    (Sema-1a), acting cell-autonomously as a receptor or part of a receptor complex,
    direct the dendritic targeting of PNs along the dorsolateral to ventromedial axis
    of the antennal lobe. Sema-1a also regulates PN axon targeting in higher olfactory
    centers. Thus, graded expression of Sema-1a contributes to connection specificity
    from ORNs to PNs and then to higher brain centers, ensuring proper representation
    of olfactory information in the brain.
article_processing_charge: No
article_type: original
author:
- first_name: Takaki
  full_name: Komiyama, Takaki
  last_name: Komiyama
- first_name: Lora Beatrice Jaeger
  full_name: Sweeney, Lora Beatrice Jaeger
  id: 56BE8254-C4F0-11E9-8E45-0B23E6697425
  last_name: Sweeney
  orcid: 0000-0001-9242-5601
- first_name: Oren
  full_name: Schuldiner, Oren
  last_name: Schuldiner
- first_name: K. Christopher
  full_name: Garcia, K. Christopher
  last_name: Garcia
- first_name: Liqun
  full_name: Luo, Liqun
  last_name: Luo
citation:
  ama: Komiyama T, Sweeney LB, Schuldiner O, Garcia KC, Luo L. Graded expression of
    semaphorin-1a cell-autonomously directs dendritic targeting of olfactory projection
    neurons. <i>Cell</i>. 2007;128(2):399-410. doi:<a href="https://doi.org/10.1016/j.cell.2006.12.028">10.1016/j.cell.2006.12.028</a>
  apa: Komiyama, T., Sweeney, L. B., Schuldiner, O., Garcia, K. C., &#38; Luo, L.
    (2007). Graded expression of semaphorin-1a cell-autonomously directs dendritic
    targeting of olfactory projection neurons. <i>Cell</i>. Elsevier. <a href="https://doi.org/10.1016/j.cell.2006.12.028">https://doi.org/10.1016/j.cell.2006.12.028</a>
  chicago: Komiyama, Takaki, Lora B. Sweeney, Oren Schuldiner, K. Christopher Garcia,
    and Liqun Luo. “Graded Expression of Semaphorin-1a Cell-Autonomously Directs Dendritic
    Targeting of Olfactory Projection Neurons.” <i>Cell</i>. Elsevier, 2007. <a href="https://doi.org/10.1016/j.cell.2006.12.028">https://doi.org/10.1016/j.cell.2006.12.028</a>.
  ieee: T. Komiyama, L. B. Sweeney, O. Schuldiner, K. C. Garcia, and L. Luo, “Graded
    expression of semaphorin-1a cell-autonomously directs dendritic targeting of olfactory
    projection neurons,” <i>Cell</i>, vol. 128, no. 2. Elsevier, pp. 399–410, 2007.
  ista: Komiyama T, Sweeney LB, Schuldiner O, Garcia KC, Luo L. 2007. Graded expression
    of semaphorin-1a cell-autonomously directs dendritic targeting of olfactory projection
    neurons. Cell. 128(2), 399–410.
  mla: Komiyama, Takaki, et al. “Graded Expression of Semaphorin-1a Cell-Autonomously
    Directs Dendritic Targeting of Olfactory Projection Neurons.” <i>Cell</i>, vol.
    128, no. 2, Elsevier, 2007, pp. 399–410, doi:<a href="https://doi.org/10.1016/j.cell.2006.12.028">10.1016/j.cell.2006.12.028</a>.
  short: T. Komiyama, L.B. Sweeney, O. Schuldiner, K.C. Garcia, L. Luo, Cell 128 (2007)
    399–410.
date_created: 2020-04-30T10:37:08Z
date_published: 2007-01-26T00:00:00Z
date_updated: 2024-01-31T10:14:48Z
day: '26'
doi: 10.1016/j.cell.2006.12.028
extern: '1'
intvolume: '       128'
issue: '2'
language:
- iso: eng
month: '01'
oa_version: None
page: 399-410
publication: Cell
publication_identifier:
  issn:
  - 0092-8674
publication_status: published
publisher: Elsevier
quality_controlled: '1'
status: public
title: Graded expression of semaphorin-1a cell-autonomously directs dendritic targeting
  of olfactory projection neurons
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 128
year: '2007'
...