9 results on '"Andrew M. M. Reeves"'
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2. 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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3. 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
4. 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
5. 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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6. 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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7. 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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8. The GOGREEN and GCLASS surveys: first data release
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Jeffrey C. C. Chan, Melinda Townsend, Heath Shipley, Laura C. Parker, Allison Noble, Kevin C. Cooke, Pascale Jablonka, Caelan Golledge, Julie Nantais, Grayson C. Petter, Michael L. Balogh, Gabriella De Lucia, P. Cerulo, Kristi Webb, Dennis Zaritsky, Callum Bellhouse, C. Valotto, M. Victoria Alonso, Sean L. McGee, Alexis Finoguenov, Kevin Boak, Ricardo Demarco, Ben Forrest, Benedetta Vulcani, Lyndsay Old, Michael C. Cooper, Irene Pintos-Castro, Stephen Gwyn, Diego Lambas Garcia, Sean P. Fillingham, Gregory Rudnick, Bianca M. Poggianti, Nicole E. Drakos, David G. Gilbank, Gillian Wilson, Hernán Muriel, Tracy Webb, Howard K. C. Yee, Andrea Biviano, Karen McNab, Remco F. J. van der Burg, Chris Lidman, Jasleen Matharu, Adam Muzzin, Anna Davidson, Andrew M. M. Reeves, and Department of Physics
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galaxies: clusters ,Stellar mass ,galaxy redshift survey ,geec2 spectroscopic survey ,FOS: Physical sciences ,quiescent galaxies ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,01 natural sciences ,Spectral line ,similar-to 1 ,Photometry (optics) ,0103 physical sciences ,red-sequence ,Astrophysics::Solar and Stellar Astrophysics ,Spectroscopy ,010303 astronomy & astrophysics ,Astrophysics::Galaxy Astrophysics ,Physics ,010308 nuclear & particles physics ,Star formation ,formation history ,Astronomy and Astrophysics ,115 Astronomy, Space science ,Astrophysics - Astrophysics of Galaxies ,Galaxy ,Redshift ,velocity dispersions ,Space and Planetary Science ,star-formation rates ,Astrophysics of Galaxies (astro-ph.GA) ,distant cluster survey ,Halo ,stellar mass ,galaxies: evolution - Abstract
We present the first public data release of the GOGREEN and GCLASS surveys of galaxies in dense environments, spanning a redshift range $0.8, Comment: Accepted for publication in MNRAS Sept 28, 2020
9. 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, Lyndsay Old, Gillian Wilson, Ben Forrest, David G. Gilbank, Michael C. Cooper, Irene Pintos-Castro, Howard K. C. Yee, Ricardo Demarco, Bianca M. Poggianti, Michael L. Balogh, Gabriella De Lucia, Sean L. McGee, Benedetta Vulcani, Andrew M. M. Reeves, Julie Nantais, Chris Lidman, Heath Shipley, Adam Muzzin, Pascale Jablonka, Ian G. McCarthy, Andrea Biviano, Kristi Webb, Remco F. J. van der Burg, Egidijus Kukstas, P. Cerulo, Dennis Zaritsky, Jeffrey C. C. Chan, Gregory Rudnick, ITA, USA, and GBR
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redshift survey ,Stellar mass ,density environments ,Population ,quiescent galaxies ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,01 natural sciences ,similar-to 1 ,quenching time-scales ,0103 physical sciences ,Cluster (physics) ,spherical systems ,education ,010303 astronomy & astrophysics ,Galaxy cluster ,QC ,Astrophysics::Galaxy Astrophysics ,QB ,Physics ,education.field_of_study ,Field galaxy ,010308 nuclear & particles physics ,Star formation ,Astronomy and Astrophysics ,Astrophysics - Astrophysics of Galaxies ,formation histories ,Redshift ,Galaxy ,velocity dispersions ,Space and Planetary Science ,galaxies: clusters: general ,digital sky survey ,galaxies: evolution ,Astrophysics - Cosmology and Nongalactic Astrophysics ,spectroscopic confirmation - Abstract
We present results on the environmental dependence of the star-forming galaxy main sequence in 11 galaxy cluster fields at $1.0 < z < 1.5$ from the Gemini Observations of Galaxies in Rich Early Environments Survey (GOGREEN) survey. We use a homogeneously selected sample of field and cluster galaxies whose membership is derived from dynamical analysis. Using [OII]-derived star formation rates (SFRs), we find that cluster galaxies have suppressed SFRs at fixed stellar mass in comparison to their field counterparts by a factor of 1.4 $\pm$ 0.1 ($\sim3.3\sigma$) across the stellar mass range: $9.0 < \log(M_{*} /M_{\odot}) < 11.2$. We also find that this modest suppression in the cluster galaxy star-forming main sequence is mass and redshift dependent: the difference between cluster and field increases towards lower stellar masses and lower redshift. When comparing the distribution of cluster and field galaxy SFRs to the star-forming main sequence, we find an overall shift towards lower SFRs in the cluster population, and note the absence of a tail of high SFR galaxies as seen in the field. Given this observed suppression in the cluster galaxy star-forming main sequence, we explore the implications for several scenarios such as formation time differences between cluster and field galaxies, and environmentally-induced star formation quenching and associated timescales., Comment: Accepted for publication in MNRAS on February 25 2020, appended erratum accepted in MNRAS on September 17 2020
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