Zobrazeno 1 - 10
of 99
pro vyhledávání: '"Andrew R Zentner"'
Autor:
Alan N. Pearl, Andrew R. Zentner, Jeffrey A. Newman, Rachel Bezanson, Kuan Wang, John Moustakas, Jessica N. Aguilar, Steven Ahlen, David Brooks, Todd Claybaugh, Shaun Cole, Kyle Dawson, Axel de la Macorra, Peter Doel, Jamie E. Forero-Romero, Satya Gontcho A Gontcho, Klaus Honscheid, Martin Landriau, Marc Manera, Paul Martini, Aaron Meisner, Ramon Miquel, Jundan Nie, Will Percival, Francisco Prada, Mehdi Rezaie, Graziano Rossi, Eusebio Sanchez, Michael Schubnell, Gregory Tarlé, Benjamin A. Weaver, Zhimin Zhou
Publikováno v:
The Astrophysical Journal, Vol 963, Iss 2, p 116 (2024)
We explore the galaxy-halo connection information that is available in low-redshift samples from the early data release of the Dark Energy Spectroscopic Instrument (DESI). We model the halo occupation distribution (HOD) from z = 0.1 to 0.3 using Surv
Externí odkaz:
https://doaj.org/article/7149a6ab1f2c4a6d80b9cbca866b6165
Autor:
Kuan Wang, Yao-Yuan Mao, Andrew R Zentner, Hong Guo, Johannes U Lange, Frank C van den Bosch, Lorena Mezini
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 516:4003-4024
We present observational constraints on the galaxy-halo connection, focusing particularly on galaxy assembly bias, from a novel combination of counts-in-cylinders statistics, $P(N_{\rm{CIC}})$, with the standard measurements of the projected two-poin
Autor:
Andrew R. Zentner, Héctor Martínez-Rodríguez, Rachel Tao, Troy J Raen, Carles Badenes, Travis J. Hurst
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 503:5611-5623
Most of the dark matter (DM) search over the last few decades has focused on WIMPs, but the viable parameter space is quickly shrinking. Asymmetric Dark Matter (ADM) is a WIMP-like DM candidate with slightly smaller masses and no present day annihila
Autor:
Travis J. Hurst, Andrew R. Zentner
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 494:4687-4694
We investigate analytically whether in a close encounter with a star, a dark matter (DM) particle can be accelerated above the escape speed of a globular cluster and be ejected. We find that this mechanism is not sufficient to eject a massive, extend
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 488:4984-5013
We present a Bayesian hierarchical inference formalism (Basilisk) to constrain the galaxy-halo connection using satellite kinematics. Unlike traditional methods, Basilisk does not resort to stacking the kinematics of satellite galaxies in bins of cen
Autor:
Andrew R. Zentner, Johannes U. Lange, Antonio Villarreal, Kuan Wang, Frank C. van den Bosch, Duncan Campbell, Andrew Hearin, Yao-Yuan Mao, Chad M. Schafer
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 488:3541-3567
Most models for the connection between galaxies and their haloes ignore the possibility that galaxy properties may be correlated with halo properties other than mass, a phenomenon known as galaxy assembly bias. Yet, it is known that such correlations
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 487:3112-3129
We present new results on the relationship between central galaxies and dark matter haloes inferred from observations of satellite kinematics in the Sloan Digital Sky Survey (SDSS) DR7. We employ an updated analysis framework that includes detailed m
Autor:
Antonio Villarreal, Andrew P. Hearin, Andrew R. Zentner, Frank C. van den Bosch, Johannes U. Lange
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 485:1196-1209
We constrain the newly-introduced decorated Halo Occupation Distribution (HOD) model using SDSS DR7 measurements of projected galaxy clustering or r-band luminosity threshold samples. The decorated HOD is a model for the galaxy-halo connection that a
Autor:
Alan N. Pearl, Rachel Bezanson, Andrew R. Zentner, Jeffrey A. Newman, Andy D. Goulding, Katherine E. Whitaker, Sean D. Johnson, Jenny E. Greene
In the coming decade, a new generation of massively multiplexed spectroscopic surveys, such as the Prime Focus Spectrograph Galaxy Evolution Survey (PFS), Wide Area Vista Extragalactic Survey-Deep (WAVES), and Multi-Object Optical and Near-infrared S
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8ac92f2d4b6f4180a623c793c5648ba8
Autor:
Aaron M. Meisner, Michael Levi, Francisco Prada, Abhishek Prakash, Yutong Duan, David J. Brooks, Rongpu Zhou, Yao-Yuan Mao, Martin Landriau, Andrew R. Zentner, Gregory Tarlé, Jeffrey A. Newman, John Moustakas, Adam D. Myers
Publikováno v:
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
Monthly Notices of the Royal Astronomical Society, vol 501, iss 3
Digital.CSIC. Repositorio Institucional del CSIC
instname
Consejo Superior de Investigaciones Científicas (CSIC)
Monthly Notices of the Royal Astronomical Society, vol 501, iss 3
Digital.CSIC. Repositorio Institucional del CSIC
instname
We present measurements of the redshift-dependent clustering of a DESI-like luminous red galaxy (LRG) sample selected from the Legacy Survey imaging data set, and use the halo occupation distribution (HOD) framework to fit the clustering signal. The
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::087ef2e1e0c6f699a413a62c3cb761c3