Search Results - "Behroozi, Peter"
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A SIMPLE TECHNIQUE FOR PREDICTING HIGH-REDSHIFT GALAXY EVOLUTION
Published in The Astrophysical journal (20-01-2015)“…We show that the ratio of galaxies' specific star formation rates (SSFRs) to their host halos' specific mass accretion rates (SMARs) strongly constrains how…”
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THE AVERAGE STAR FORMATION HISTORIES OF GALAXIES IN DARK MATTER HALOS FROM z = 0-8
Published in The Astrophysical journal (10-06-2013)“…We present a robust-method to constrain average galaxy star formation rates (SFRs), star formation histories (SFHs), and the intracluster light (ICL) as a…”
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UniverseMachine: The correlation between galaxy growth and dark matter halo assembly from z = 0−10
Published in Monthly notices of the Royal Astronomical Society (21-09-2019)“…ABSTRACT We present a method to flexibly and self-consistently determine individual galaxies’ star formation rates (SFRs) from their host haloes’ potential…”
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Physical correlations of the scatter between galaxy mass, stellar content, and halo mass
Published in Monthly notices of the Royal Astronomical Society (01-03-2020)“…ABSTRACT We use the UniverseMachine to analyse the source of scatter between the central galaxy mass, the total stellar mass in the halo, and the dark matter…”
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THE CONNECTION BETWEEN GALAXIES AND DARK MATTER STRUCTURES IN THE LOCAL UNIVERSE
Published in The Astrophysical journal (01-07-2013)“…We provide new constraints on the connection between galaxies in the local universe, identified by the Sloan Digital Sky Survey, and dark matter halos and…”
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Evolution of the atomic and molecular gas content of galaxies in dark matter haloes
Published in Monthly notices of the Royal Astronomical Society (01-05-2015)“…We present a semi-empirical model to infer the atomic and molecular hydrogen content of galaxies as a function of halo mass and time. Our model combines the…”
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INTERPRETING SHORT GAMMA-RAY BURST PROGENITOR KICKS AND TIME DELAYS USING THE HOST GALAXY–DARK MATTER HALO CONNECTION
Published in The Astrophysical journal (10-09-2014)“…Nearly 20% of short gamma-ray bursts (sGRBs) have no observed host galaxies. Combining this finding with constraints on galaxies' dark matter halo potential…”
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On the physical origin of galactic conformity
Published in Monthly notices of the Royal Astronomical Society (11-09-2016)“…Correlations between the star formation rates (SFRs) of nearby galaxies (so-called galactic conformity) have been observed for projected separations up to…”
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GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with ∼4,000,000 Galaxies at z ∼ 2–7: Galaxy–AGN Transition, Star Formation Efficiency, and Implication for Evolution at z > 10
Published in The Astrophysical journal. Supplement series (01-03-2022)“…Abstract We present new measurements of rest-UV luminosity functions and angular correlation functions from 4,100,221 galaxies at z ∼ 2–7 identified in the…”
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The Universe at z > 10: predictions for JWST from the universemachine DR1
Published in Monthly notices of the Royal Astronomical Society (01-12-2020)“…ABSTRACT The James Webb Space Telescope (JWST) is expected to observe galaxies at z > 10 that are presently inaccessible. Here, we use a self-consistent…”
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CEERS Key Paper. I. An Early Look into the First 500 Myr of Galaxy Formation with JWST
Published in Astrophysical journal. Letters (01-03-2023)“…Abstract We present an investigation into the first 500 Myr of galaxy evolution from the Cosmic Evolution Early Release Science (CEERS) survey. CEERS, one of…”
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Disentangling satellite galaxy populations using orbit tracking in simulations
Published in Monthly notices of the Royal Astronomical Society (21-05-2013)“…Physical processes regulating star formation in satellite galaxies represent an area of ongoing research, but the projected nature of observed coordinates…”
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Semi-analytic forecasts for JWST – IV. Implications for cosmic reionization and LyC escape fraction
Published in Monthly notices of the Royal Astronomical Society (01-08-2020)“…ABSTRACT Galaxies forming in low-mass haloes are thought to be primarily responsible for reionizing the Universe during the first billion years after the big…”
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MERGERS AND MASS ACCRETION FOR INFALLING HALOS BOTH END WELL OUTSIDE CLUSTER VIRIAL RADII
Published in The Astrophysical journal (01-06-2014)“…We find that infalling dark matter halos (i.e., the progenitors of satellite halos) begin losing mass well outside the virial radius of their eventual host…”
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Haloes gone MAD: The Halo-Finder Comparison Project
Published in Monthly notices of the Royal Astronomical Society (11-08-2011)“…ABSTRACT We present a detailed comparison of fundamental dark matter halo properties retrieved by a substantial number of different halo finders. These codes…”
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A CEERS Discovery of an Accreting Supermassive Black Hole 570 Myr after the Big Bang: Identifying a Progenitor of Massive z > 6 Quasars
Published in Astrophysical journal. Letters (01-08-2023)“…Abstract We report the discovery of an accreting supermassive black hole at z = 8.679. This galaxy, denoted here as CEERS_1019, was previously discovered as a…”
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The relationship between galaxy and dark matter halo size from z ∼ 3 to the present
Published in Monthly notices of the Royal Astronomical Society (11-01-2018)Get full text
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Redshift-space clustering of SDSS galaxies – luminosity dependence, halo occupation distribution, and velocity bias
Published in Monthly notices of the Royal Astronomical Society (11-11-2015)“…We present the measurements and modelling of the small-to-intermediate scale (∼0.1–25 h −1 Mpc) projected and three-dimensional redshift-space two-point…”
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Lensing is low: cosmology, galaxy formation or new physics?
Published in Monthly notices of the Royal Astronomical Society (03-02-2017)“…Abstract We present high signal-to-noise galaxy–galaxy lensing measurements of the Baryon Oscillation Spectroscopic Survey constant mass (CMASS) sample using…”
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THE EVOLUTION OF THE GALAXY REST-FRAME ULTRAVIOLET LUMINOSITY FUNCTION OVER THE FIRST TWO BILLION YEARS
Published in The Astrophysical journal (01-09-2015)“…ABSTRACT We present a robust measurement and analysis of the rest-frame ultraviolet (UV) luminosity functions at z = 4-8. We use deep Hubble Space Telescope…”
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