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20082026
most citedDetection of lensing substructure using ALMA observations of the dusty galaxy SDP.81

327 citations · 4.4k across the 74 of their papers we have counts for

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Showing 2017Show all

9 papers · 1 filter

astro-ph.GA2017★ 63 cited

Modeling the Impact of Baryons on Subhalo Populations with Machine Learning

Ethan O. Nadler, Yao-Yuan Mao, Risa H. Wechsler +2

We identify subhalos in dark matter-only (DMO) zoom-in simulations that are likely to be disrupted due to baryonic effects by using a random forest classifier trained on two hydrod…

astro-ph.IM2017★ 21 cited

DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs

Yao-Yuan Mao, Eve Kovacs, Katrin Heitmann +24

The use of high-quality simulated sky catalogs is essential for the success of cosmological surveys. The catalogs have diverse applications, such as investigating signatures of fun…

astro-ph.GA2017★ 66 cited

The Galaxy Clustering Crisis in Abundance Matching

Duncan Campbell, Frank C. van den Bosch, Nikhil Padmanabhan +5

Galaxy clustering on small scales is significantly under-predicted by sub-halo abundance matching (SHAM) models that populate (sub-)haloes with galaxies based on peak halo mass, $M…

astro-ph.GA2017★ 249 cited

The SAGA Survey: I. Satellite Galaxy Populations Around Eight Milky Way Analogs

Marla Geha, Risa H. Wechsler, Yao-Yuan Mao +8

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 distribution of satellite galax…

astro-ph.GA2017★ 31 cited

Brightest galaxies as halo centre tracers in SDSS DR7

Johannes U. Lange, Frank C. van den Bosch, Andrew Hearin +4

Determining the positions of halo centres in large-scale structure surveys is crucial for many cosmological studies. A common assumption is that halo centres correspond to the loca…

astro-ph.CO2017★ 44 cited

The Immitigable Nature of Assembly Bias: The Impact of Halo Definition on Assembly Bias

Antonia S. Villarreal, Andrew R. Zentner, Yao-Yuan Mao +6

Dark matter halo clustering depends not only on halo mass, but also on other properties such as concentration and shape. This phenomenon is known broadly as assembly bias. We explo…