14 results on '"Andrew M M Reeves"'
Search Results
2. The GOGREEN survey: transition galaxies and the evolution of environmental quenching
- Author
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Karen McNab, Michael L Balogh, Remco F J van der Burg, Anya Forestell, Kristi Webb, Benedetta Vulcani, Gregory Rudnick, Adam Muzzin, M C Cooper, Sean McGee, Andrea Biviano, Pierluigi Cerulo, Jeffrey C C Chan, Gabriella De Lucia, Ricardo Demarco, Alexis Finoguenov, Ben Forrest, Caelan Golledge, Pascale Jablonka, Chris Lidman, Julie Nantais, Lyndsay Old, Irene Pintos-Castro, Bianca Poggianti, Andrew M M Reeves, Gillian Wilson, Howard K C Yee, and Dennis Zaritsky
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- 2021
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3. The GOGREEN survey: post-infall environmental quenching fails to predict the observed age difference between quiescent field and cluster galaxies at z > 1
- Author
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Kristi Webb, Michael L Balogh, Joel Leja, Remco F J van der Burg, Gregory Rudnick, Adam Muzzin, Kevin Boak, Pierluigi Cerulo, David Gilbank, Chris Lidman, Lyndsay J Old, Irene Pintos-Castro, Sean McGee, Heath Shipley, Andrea Biviano, Jeffrey C C Chan, Michael Cooper, Gabriella De Lucia, Ricardo Demarco, Ben Forrest, Pascale Jablonka, Egidijus Kukstas, Ian G McCarthy, Karen McNab, Julie Nantais, Allison Noble, Bianca Poggianti, Andrew M M Reeves, Benedetta Vulcani, Gillian Wilson, Howard K C Yee, and Dennis Zaritsky
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- 2020
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4. The GOGREEN survey: the environmental dependence of the star-forming galaxy main sequence at 1.0 < z < 1.5
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Lyndsay J Old, Michael L Balogh, Remco F J van der Burg, Andrea Biviano, Howard K C Yee, Irene Pintos-Castro, Kristi Webb, Adam Muzzin, Gregory Rudnick, Benedetta Vulcani, Bianca Poggianti, Michael Cooper, Dennis Zaritsky, Pierluigi Cerulo, Gillian Wilson, Jeffrey C C Chan, Chris Lidman, Sean McGee, Ricardo Demarco, Ben Forrest, Gabriella De Lucia, David Gilbank, Egidijus Kukstas, Ian G McCarthy, Pascale Jablonka, Julie Nantais, Allison Noble, Andrew M M Reeves, and Heath Shipley
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- 2020
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5. Constraining quenching time-scales in galaxy clusters by forward-modelling stellar ages and quiescent fractions in projected phase space
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Andrew M M Reeves, Michael J Hudson, and Kyle A Oman
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Space and Planetary Science ,Astrophysics of Galaxies (astro-ph.GA) ,FOS: Physical sciences ,Astronomy and Astrophysics ,Astrophysics - Astrophysics of Galaxies - Abstract
We forward-model mass-weighted stellar ages (MWAs) and quiescent fractions in projected phase space (PPS), using data from the Sloan Digital Sky Survey, to jointly constrain an infall quenching model for galaxies in $\log(M_{\mathrm{vir}}/\mathrm{M}_{\odot})>14$ galaxy clusters at $z\sim 0$. We find the average deviation in MWA from the MWA-$M_\star$ relation depends on position in PPS, with a maximum difference between the inner cluster and infalling interloper galaxies of $\sim 1$ Gyr. Our model employs infall information from N-body simulations and stochastic star-formation histories from the UniverseMachine model. We find total quenching times of $t_\mathrm{Q}=3.7\pm 0.4$ Gyr and $t_\mathrm{Q}=4.0\pm 0.2$ Gyr after first pericentre, for $9, 21 pages, 13 figures, submitted to MNRAS
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- 2023
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6. The GOGREEN survey: constraining the satellite quenching time-scale in massive clusters at z ≳ 1
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Devontae C Baxter, M C Cooper, Michael L Balogh, Timothy Carleton, Pierluigi Cerulo, Gabriella De Lucia, Ricardo Demarco, Sean McGee, Adam Muzzin, Julie Nantais, Irene Pintos-Castro, Andrew M M Reeves, Gregory H Rudnick, Florian Sarron, Remco F J van der Burg, Benedetta Vulcani, Gillian Wilson, Dennis Zaritsky, Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), and Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS)
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Space and Planetary Science ,galaxies: clusters: general ,[SDU]Sciences of the Universe [physics] ,galaxies: star formation ,galaxies: formation ,Astronomy and Astrophysics ,galaxies: evolution ,Astrophysics - Astrophysics of Galaxies - Abstract
International audience; We model satellite quenching at z ~ 1 by combining 14 massive (1013.8 < Mhalo/M⊙ < 1015) clusters at 0.8 < z < 1.3 from the GOGREEN and GCLASS surveys with accretion histories of 56 redshift-matched analogues from the IllustrisTNG simulation. Our fiducial model, which is parametrized by the satellite quenching time-scale (τquench), accounts for quenching in our simulated satellite population both at the time of infall by using the observed coeval field quenched fraction and after infall by tuning τquench to reproduce the observed satellite quenched fraction versus stellar mass trend. This model successfully reproduces the observed satellite quenched fraction as a function of stellar mass (by construction), projected cluster-centric radius, and redshift and is consistent with the observed field and cluster stellar mass functions at z ~ 1. We find that the satellite quenching time-scale is mass dependent, in conflict with some previous studies at low and intermediate redshift. Over the stellar mass range probed (M⋆ > 1010 M⊙), we find that the satellite quenching time-scale decreases with increasing satellite stellar mass from ~1.6 Gyr at 1010 M⊙ to ~0.6-1 Gyr at 1011 M⊙ and is roughly consistent with the total cold gas (HI + H2) depletion time-scales at intermediate z, suggesting that starvation may be the dominant driver of environmental quenching at z < 2. Finally, while environmental mechanisms are relatively efficient at quenching massive satellites, we find that the majority ($\sim 65{\!-\!}80{{\ \rm per\ cent}}$) of ultra-massive satellites (M⋆ > 1011 M⊙) are quenched prior to infall.
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- 2022
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7. Erratum: The GOGREEN survey: the environmental dependence of the star-forming galaxy main sequence at 1.0 < z < 1.5
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Allison Noble, Benedetta Vulcani, Gregory Rudnick, Sean L. McGee, Chris Lidman, Irene Pintos-Castro, Ricardo Demarco, Howard K. C. Yee, Ben Forrest, Gillian Wilson, Michael L. Balogh, Gabriella De Lucia, Michael C. Cooper, Remco F. J. van der Burg, Andrea Biviano, Bianca M. Poggianti, Heath Shipley, Ian G. McCarthy, Egidijus Kukstas, Pascale Jablonka, David G. Gilbank, Kristi Webb, Jeffrey C. C. Chan, P. Cerulo, Dennis Zaritsky, Andrew M. M. Reeves, Julie Nantais, Adam Muzzin, and Lyndsay Old
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Physics ,Space and Planetary Science ,Astronomy ,Astronomy and Astrophysics ,Star (graph theory) ,Galaxy ,Sequence (medicine) - Published
- 2020
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8. The GOGREEN survey: Transition Galaxies and The Evolution of Environmental Quenching
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Irene Pintos-Castro, Howard K. C. Yee, Lyndsay Old, Ben Forrest, Michael C. Cooper, Bianca M. Poggianti, P. Cerulo, Adam Muzzin, Michael L. Balogh, Dennis Zaritsky, Pascale Jablonka, Sean L. McGee, Remco F. J. van der Burg, Jeffrey C. C. Chan, Gabriella De Lucia, Benedetta Vulcani, Gillian Wilson, Kristi Webb, Ricardo Demarco, Andrew M. M. Reeves, Chris Lidman, Caelan Golledge, Julie Nantais, Anya Forestell, Gregory Rudnick, Alexis Finoguenov, Andrea Biviano, Karen McNab, Department of Physics, Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)
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Stellar mass ,Population ,FOS: Physical sciences ,STELLAR-MASS FUNCTION ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,STAR-FORMATION RATES ,SIMILAR-TO 1 ,SPECTROSCOPIC CONFIRMATION ,114 Physical sciences ,01 natural sciences ,0103 physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,RED-SEQUENCE ,education ,010303 astronomy & astrophysics ,Galaxy cluster ,Astrophysics::Galaxy Astrophysics ,Luminosity function (astronomy) ,[PHYS]Physics [physics] ,Physics ,education.field_of_study ,010308 nuclear & particles physics ,Star formation ,POST-STARBURST GALAXIES ,FORMATION HISTORIES ,Astronomy and Astrophysics ,DISTANT CLUSTERS ,Astrophysics - Astrophysics of Galaxies ,Accretion (astrophysics) ,Galaxy ,Redshift ,galaxies: clusters: general ,LUMINOSITY FUNCTION ,Space and Planetary Science ,Astrophysics of Galaxies (astro-ph.GA) ,galaxies: star formation ,QUIESCENT GALAXIES ,Astrophysics::Earth and Planetary Astrophysics ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,galaxies: evolution - Abstract
We measure the rate of environmentally-driven star formation quenching in galaxies at $z\sim 1$, using eleven massive ($M\approx 2\times10^{14}\,\mathrm{M}_\odot$) galaxy clusters spanning a redshift range $1.010.5$) we do not find any significant excess of transition galaxies in clusters, relative to a comparison field sample at the same redshift. It is likely that such galaxies were quenched prior to their accretion in the cluster, in group, filament or protocluster environments. For lower stellar mass galaxies ($9.5, Comment: Accepted for publication in MNRAS Sept 6, 2021
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- 2021
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9. The GOGREEN survey: dependence of galaxy properties on halo mass at z > 1 and implications for environmental quenching
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Ricardo Demarco, Andrea Biviano, Michael L. Balogh, Jeffrey C. C. Chan, Sean L. McGee, Alexis Finoguenov, Benedetta Vulcani, Gregory Rudnick, Gillian Wilson, Pascale Jablonka, M. C. Cooper, Egidijus Kukstas, Ian G. McCarthy, Remco F. J. van der Burg, Adam Muzzin, Kristi Webb, P. Cerulo, Dennis Zaritsky, Gabriella De Lucia, Howard K. C. Yee, Andrew M. M. Reeves, Department of Physics, and Doctoral Programme in Particle Physics and Universe Sciences
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010504 meteorology & atmospheric sciences ,Stellar mass ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,01 natural sciences ,Measure (mathematics) ,galaxies: groups: general ,galaxies: high-redshift ,0103 physical sciences ,LARGE-SCALE STRUCTURE ,X-RAY GROUPS ,Astrophysics::Solar and Stellar Astrophysics ,RED-SEQUENCE ,STAR-FORMATION ACTIVITY ,010303 astronomy & astrophysics ,QC ,Astrophysics::Galaxy Astrophysics ,0105 earth and related environmental sciences ,QB ,Quenching ,Physics ,Background subtraction ,TIME-SCALES ,CLUSTER GALAXIES ,Astronomy and Astrophysics ,115 Astronomy, Space science ,Astrophysics - Astrophysics of Galaxies ,Galaxy ,Redshift ,FORMATION RATES ,galaxies: haloes ,Space and Planetary Science ,galaxies: clusters: general ,STELLAR POPULATION SYNTHESIS ,galaxies: star formation ,DIGITAL SKY SURVEY ,Halo ,GEEC2 SPECTROSCOPIC SURVEY ,galaxies: evolution - Abstract
We use photometric redshifts and statistical background subtraction to measure stellar mass functions in galaxy group-mass ($4.5-8\times10^{13}~\mathrm{M}_\odot$) haloes at $11$., Comment: Accepted July 6, 2021, MNRAS
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- 2021
10. The GOGREEN survey: post-infall environmental quenching fails to predict the observed age difference between quiescent field and cluster galaxies at z > 1
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Egidijus Kukstas, Remco F. J. van der Burg, Ricardo Demarco, Howard K. C. Yee, Michael C. Cooper, Bianca M. Poggianti, Allison Noble, Irene Pintos-Castro, Benedetta Vulcani, Heath Shipley, Chris Lidman, Pascale Jablonka, David G. Gilbank, Kevin Boak, Michael L. Balogh, Gabriella De Lucia, Julie Nantais, Ben Forrest, Andrew M. M. Reeves, Sean L. McGee, Adam Muzzin, Gregory Rudnick, Ian G. McCarthy, Lyndsay Old, P. Cerulo, Dennis Zaritsky, Jeffrey C. C. Chan, Joel Leja, Kristi Webb, Gillian Wilson, Andrea Biviano, and Karen McNab
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Field (physics) ,FOS: Physical sciences ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,fundamental-plane ,01 natural sciences ,star-formation histories ,red-sequence ,0103 physical sciences ,Cluster (physics) ,band luminosity function ,010303 astronomy & astrophysics ,QC ,Astrophysics::Galaxy Astrophysics ,Galaxy cluster ,QB ,Physics ,Quenching ,massive galaxies ,Age differences ,010308 nuclear & particles physics ,Star formation ,Astronomy and Astrophysics ,elliptic galaxies ,Astrophysics - Astrophysics of Galaxies ,Galaxy ,intermediate redshift ,galaxies: clusters: general ,Space and Planetary Science ,Astrophysics of Galaxies (astro-ph.GA) ,digital sky survey ,galaxies: evolution ,stellar population synthesis ,spectroscopic survey - Abstract
We study the star formation histories (SFHs) and mass-weighted ages of 331 UVJ-selected quiescent galaxies in 11 galaxy clusters and in the field at 11 has been driven by different physical processes than those at play at z=0., Comment: accepted Sept 7 2020, MNRAS
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- 2020
11. The GOGREEN Survey: A deep stellar mass function of cluster galaxies at 1.0 < z < 1.4 and the complex nature of satellite quenching
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Pascale Jablonka, Michael L. Balogh, Gabriella De Lucia, Michael C. Cooper, Ben Forrest, Mauro Stefanon, Bianca M. Poggianti, Benedetta Vulcani, Stephen D. J. Gwyn, Chris Lidman, Sean L. McGee, David Gilbank, Remco F. J. van der Burg, Julie Nantais, Irene Pintos-Castro, Danilo Marchesini, Howard Yee, Gregory Rudnick, Ricardo Demarco, Heath Shipley, Andrea Biviano, Kristi Webb, Andrew M. M. Reeves, Egidijus Kukstas, Adam Muzzin, Lyndsay Old, Gillian Wilson, Allison Noble, Jeffrey C. C. Chan, P. Cerulo, Dennis Zaritsky, Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)
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assembly bias ,Field (physics) ,Stellar mass ,media_common.quotation_subject ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,01 natural sciences ,star-formation histories ,population synthesis ,0103 physical sciences ,red-sequence ,evolution ,Cluster (physics) ,formation rates ,Astrophysics::Solar and Stellar Astrophysics ,010303 astronomy & astrophysics ,Galaxy cluster ,Astrophysics::Galaxy Astrophysics ,media_common ,Physics ,Quenching ,[PHYS]Physics [physics] ,010308 nuclear & particles physics ,Astronomy and Astrophysics ,Astrophysics - Astrophysics of Galaxies ,Galaxy ,Universe ,Redshift ,galaxies: luminosity function ,galaxies: photometry ,Space and Planetary Science ,mass function ,galaxies: clusters: general ,galaxies: stellar content ,Astrophysics::Earth and Planetary Astrophysics ,galaxies: evolution ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,density relation ,environment ,bimodality ,spectroscopic confirmation - Abstract
We study the stellar mass functions (SMFs) of star-forming and quiescent galaxies in 11 galaxy clusters at 1.0, Comment: 19 pages, 9 figures (excluding appendices). Accepted for publication in A&A
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- 2020
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12. The GOGREEN Survey: Evidence of an Excess of Quiescent Disks in Clusters at 1.0 < z < 1.4
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Andrea Biviano, Julie Nantais, Andrew M. M. Reeves, Gillian Wilson, Sean L. McGee, Irene Pintos-Castro, P. Cerulo, Michael C. Cooper, Bianca M. Poggianti, Lyndsay Old, Dennis Zaritsky, Adam Muzzin, Pascale Jablonka, Michael L. Balogh, Benedetta Vulcani, Kristi Webb, Jeffrey C. C. Chan, Remco F. J. van der Burg, Chris Lidman, Howard K. C. Yee, Ricardo Demarco, Gabriella De Lucia, Ben Forrest, and Gregory Rudnick
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Physics ,Angular momentum ,Stellar mass ,Space and Planetary Science ,Galaxy formation and evolution ,Astronomy and Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,Astrophysics - Astrophysics of Galaxies ,Astrophysics::Galaxy Astrophysics ,Galaxy cluster - Abstract
We present results on the measured shapes of 832 galaxies in 11 galaxy clusters at 1.0 < z, Comment: Accepted for publication in ApJ. 25 pages, 15 figures
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- 2021
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13. The Rest-frame H-band Luminosity Function of Red-sequence Galaxies in Clusters at 1.0 < z < 1.3
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Michael L. Balogh, Sean L. McGee, Andrea Biviano, J. Nantais, Remco F. J. van der Burg, Danilo Marchesini, Irene Pintos-Castro, Chris Lidman, Mauro Stefanon, Adam Muzzin, Allison Noble, Michael C. Cooper, Lyndsay Old, Andrew M. M. Reeves, Gillian Wilson, Gabriella De Lucia, Ricardo Demarco, Gregory Rudnick, Kristi Webb, Ben Forrest, Howard Yee, Mohamed H. Abdullah, Jeffrey C. C. Chan, P. Cerulo, and Dennis Zaritsky
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Physics ,010504 meteorology & atmospheric sciences ,Center (category theory) ,Astronomy and Astrophysics ,Astrophysics ,H band ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Rest frame ,01 natural sciences ,Astrophysics - Astrophysics of Galaxies ,Galaxy ,Spitzer Space Telescope ,Space and Planetary Science ,0103 physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,010303 astronomy & astrophysics ,Astrophysics::Galaxy Astrophysics ,0105 earth and related environmental sciences ,Luminosity function (astronomy) - Abstract
We present results on the rest-frame $H$-band luminosity functions (LF) of red sequence galaxies in seven clusters at 1.0 < z < 1.3 from the Gemini Observations of Galaxies in Rich Early Environments Survey (GOGREEN). Using deep GMOS-z' and IRAC $3.6 \mu$m imaging, we identify red sequence galaxies and measure their LFs down to $M_{H} \sim M_{H}^{*} + (2.0 - 3.0)$. By stacking the entire sample, we derive a shallow faint end slope of $ \alpha \sim -0.35^{+0.15}_{-0.15} $ and $ M_{H}^{*} \sim -23.52^{+0.15}_{-0.17} $, suggesting that there is a deficit of faint red sequence galaxies in clusters at high redshift. By comparing the stacked red sequence LF of our sample with a sample of clusters at z~0.6, we find an evolution in the faint end of the red sequence over the ~2.6 Gyr between the two samples, with the mean faint end red sequence luminosity growing by more than a factor of two. The faint-to-luminous ratio of our sample ($0.78^{+0.19}_{-0.15}$) is consistent with the trend of decreasing ratio with increasing redshift as proposed in previous studies. A comparison with the field shows that the faint-to-luminous ratios in clusters are consistent with the field at z~1.15 and exhibit a stronger redshift dependence. Our results support the picture that the build up of the faint red sequence galaxies occurs gradually over time and suggest that faint cluster galaxies, similar to bright cluster galaxies, experience the quenching effect induced by environment already at z~1.15., Comment: Accepted for publication in ApJ. 24 pages, 13 figures
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- 2019
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14. The Rest-frame H-band Luminosity Function of Red-sequence Galaxies in Clusters at 1.0 < z < 1.3.
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Jeffrey C. C. Chan, Gillian Wilson, Gregory Rudnick, Adam Muzzin, Michael Balogh, Julie Nantais, Remco F. J. van der Burg, Pierluigi Cerulo, Andrea Biviano, Michael C. Cooper, Ricardo Demarco, Ben Forrest, Chris Lidman, Allison Noble, Lyndsay Old, Irene Pintos-Castro, Andrew M. M. Reeves, Kristi A. Webb, Howard K. C. Yee, and Mohamed H. Abdullah
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LUMINOSITY ,REDSHIFT ,GALAXIES ,PROTHROMBIN ,GALAXY clusters - Abstract
We present results on the rest-frame H-band luminosity functions (LFs) of red-sequence galaxies in seven clusters at 1.0 < z < 1.3 from the Gemini Observations of Galaxies in Rich Early Environments Survey. Using deep GMOS and IRAC 3.6 μm imaging, we identify red-sequence galaxies and measure their LFs down to . By stacking the entire sample, we derive a shallow faint-end slope of and , suggesting that there is a deficit of faint red-sequence galaxies in clusters at high redshift. By comparing the stacked red-sequence LF of our sample with a sample of clusters at z ∼ 0.6, we find an evolution of the faint end of the red sequence over the ∼2.6 Gyr between the two samples, with the mean faint-end red-sequence luminosity growing by more than a factor of 2. The faint-to-luminous ratio of our sample () is consistent with the trend of decreasing ratio with increasing redshift proposed in previous studies. A comparison with the field shows that the faint-to-luminous ratios in clusters are consistent with those in the field at z ∼ 1.15 and exhibit a stronger redshift dependence. Our results support the picture that the buildup of faint red-sequence galaxies occurs gradually over time and suggest that faint cluster galaxies, similar to bright cluster galaxies, already experience the quenching effect induced by the environment at z ∼ 1.15. [ABSTRACT FROM AUTHOR]
- Published
- 2019
- Full Text
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