Search Results - "Wechsler, Risa H."
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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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Beyond assembly bias: exploring secondary halo biases for cluster-size haloes
Published in Monthly notices of the Royal Astronomical Society (01-03-2018)“…Abstract Secondary halo bias, commonly known as ‘assembly bias’, is the dependence of halo clustering on a halo property other than mass. This prediction of…”
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Weak lensing measurement of the mass–richness relation of SDSS redMaPPer clusters
Published in Monthly notices of the Royal Astronomical Society (21-04-2017)“…Abstract We perform a measurement of the mass–richness relation of the redMaPPer galaxy cluster catalogue using weak lensing data from the Sloan Digital Sky…”
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THE DEPENDENCE OF SUBHALO ABUNDANCE ON HALO CONCENTRATION
Published in The Astrophysical journal (01-09-2015)“…ABSTRACT Hierarchical structure formation implies that the number of subhalos within a dark matter halo depends not only on halo mass, but also on the…”
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Stringent σ8 constraints from small-scale galaxy clustering using a hybrid MCMC + emulator framework
Published in Monthly notices of the Royal Astronomical Society (01-07-2022)“…ABSTRACT We present a novel simulation-based hybrid emulator approach that maximally derives cosmological and Halo Occupation Distribution (HOD) information…”
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The Aemulus Project. I. Numerical Simulations for Precision Cosmology
Published in The Astrophysical journal (10-04-2019)“…The rapidly growing statistical precision of galaxy surveys has led to a need for ever more precise predictions of the observables used to constrain…”
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The Aemulus Project. II. Emulating the Halo Mass Function
Published in The Astrophysical journal (10-02-2019)“…Existing models for the dependence of the halo mass function on cosmological parameters will become a limiting source of systematic uncertainty for cluster…”
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The Aemulus Project. III. Emulation of the Galaxy Correlation Function
Published in The Astrophysical journal (20-03-2019)“…Using the N-body simulations of the Aemulus Project, we construct an emulator for the nonlinear clustering of galaxies in real and redshift space. We construct…”
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The SAGA Survey. I. Satellite Galaxy Populations around Eight Milky Way Analogs
Published in The Astrophysical journal (20-09-2017)“…We present the survey strategy and early results of the "Satellites Around Galactic Analogs" (SAGA) Survey. The SAGA Survey's goal is to measure 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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CONNECTING CO INTENSITY MAPPING TO MOLECULAR GAS AND STAR FORMATION IN THE EPOCH OF GALAXY ASSEMBLY
Published in The Astrophysical journal (01-02-2016)“…ABSTRACT Intensity mapping, which images a single spectral line from unresolved galaxies across cosmological volumes, is a promising technique for probing the…”
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Dark Matter Constraints from a Unified Analysis of Strong Gravitational Lenses and Milky Way Satellite Galaxies
Published in The Astrophysical journal (01-08-2021)“…Abstract Joint analyses of small-scale cosmological structure probes are relatively unexplored and promise to advance measurements of microphysical dark matter…”
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Signatures of Velocity-dependent Dark Matter Self-interactions in Milky Way-mass Halos
Published in The Astrophysical journal (01-06-2020)“…We explore the impact of elastic, anisotropic, velocity-dependent dark matter (DM) self-interactions on the host halo and subhalos of Milky Way (MW)-mass…”
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The impact of the fiducial cosmology assumption on BAO distance scale measurements
Published in Monthly notices of the Royal Astronomical Society (18-03-2020)“…ABSTRACT Standard analysis pipelines for measurements of Baryon Acoustic Oscillations (BAO) in galaxy surveys make use of a fiducial cosmological model to…”
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Galaxy cluster mass estimation from stacked spectroscopic analysis
Published in Monthly notices of the Royal Astronomical Society (21-08-2016)“…We use simulated galaxy surveys to study: (i) how galaxy membership in redMaPPer clusters maps to the underlying halo population, and (ii) the accuracy of a…”
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Forecasting [C ii] Line-intensity Mapping Measurements between the End of Reionization and the Epoch of Galaxy Assembly
Published in The Astrophysical journal (20-03-2020)“…We combine recent simulation work on the SFR-[C ii] correlation at high redshift with empirical modeling of the galaxy-halo connection (via UniverseMachine) to…”
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THE EATING HABITS OF MILKY WAY-MASS HALOS: DESTROYED DWARF SATELLITES AND THE METALLICITY DISTRIBUTION OF ACCRETED STARS
Published in The Astrophysical journal (10-04-2016)“…ABSTRACT We study the mass spectrum of destroyed dwarfs that contribute to the accreted stellar mass of Milky Way (MW)-mass (Mvir ∼ 1012.1 M ) halos using a…”
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UNIT project: Universe N-body simulations for the Investigation of Theoretical models from galaxy surveys
Published in Monthly notices of the Royal Astronomical Society (21-07-2019)“…Abstract We present the UNIT N-body cosmological simulations project, designed to provide precise predictions for non-linear statistics of the galaxy…”
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The Binary-Host Connection: Astrophysics of Gravitational-Wave Binaries from Host Galaxy Properties
Published in The Astrophysical journal (01-12-2020)“…Gravitational waves from the merger of binary neutron stars (BNSs) are accompanied by electromagnetic counterparts, making it possible to identify the…”
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From Images to Dark Matter: End-to-end Inference of Substructure from Hundreds of Strong Gravitational Lenses
Published in The Astrophysical journal (01-01-2023)“…Abstract Constraining the distribution of small-scale structure in our universe allows us to probe alternatives to the cold dark matter paradigm. Strong…”
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