papers

Publications (12)

astro-ph.CO2026

Brightest Cluster Galaxy ellipticity as proxy for halo shape: Orientation bias, assembly bias, and potential selection effects in SZ-selected clusters

Radhakrishnan Srinivasan, Tae-hyeon Shin, Anja von der Linden +93

The orientation of triaxial galaxy clusters with respect to the line-of-sight is expected to be one of the prime sources of scatter and potential bias in optical observables (e.g.,…

astro-ph2008

An Improved Cluster Richness Estimator

Eduardo Rozo, Eli S. Rykoff, Benjamin P. Koester +11

Minimizing the scatter between cluster mass and accessible observables is an important goal for cluster cosmology. In this work, we introduce a new matched filter richness estimato…

astro-ph.CO2010

Precision Measurements of the Cluster Red Sequence using an Error Corrected Gaussian Mixture Model

Jiangang Hao, Benjamin P. Koester, Timothy A. Mckay +10

The red sequence is an important feature of galaxy clusters and plays a crucial role in optical cluster detection. Measurement of the slope and scatter of the red sequence are affe…

astro-ph.CO2025

Deep-Field Analytical Calibration

Andy Park, Xiangchong Li, Rachel Mandelbaum +1

The next generation of imaging surveys, including the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST), Euclid, and the Nancy Grace Roman Space Telescope, will plac…

astro-ph2008

Constraining the Scatter in the Mass-Richness Relation of maxBCG Clusters With Weak Lensing and X-ray Data

Eduardo Rozo, Eli S. Rykoff, August Evrard +10

We measure the logarithmic scatter in mass at fixed richness for clusters in the maxBCG cluster catalog, an optically selected cluster sample drawn from SDSS imaging data. Our meas…

cs.SE2026

Just-in-Time Catching Test Generation at Meta

Matthew Becker, Yifei Chen, Nicholas Cochran +12

We report on Just-in-Time catching test generation at Meta, designed to prevent bugs in large scale backend systems of hundreds of millions of line of code. Unlike traditional hard…

astro-ph.CO2014

Orientation Bias of Optically Selected Galaxy Clusters and Its Impact on Stacked Weak Lensing Analyses

Jörg P. Dietrich, Yuanyuan Zhang, Jeeseon Song +15

Weak-lensing measurements of the averaged shear profiles of galaxy clusters binned by some proxy for cluster mass are commonly converted to cluster mass estimates under the assumpt…

astro-ph.CO2016

Cosmology from large scale galaxy clustering and galaxy-galaxy lensing with Dark Energy Survey Science Verification data

Juliana Kwan, Carles Sanchez, Joseph Clampitt +80

We present cosmological constraints from the Dark Energy Survey (DES) using a combined analysis of angular clustering of red galaxies and their cross-correlation with weak gravitat…

astro-ph.CO2010

A GMBCG Galaxy Cluster Catalog of 55,424 Rich Clusters from SDSS DR7

Jiangang Hao, Timothy A. McKay, Benjamin P. Koester +11

We present a large catalog of optically selected galaxy clusters from the application of a new Gaussian Mixture Brightest Cluster Galaxy (GMBCG) algorithm to SDSS Data Release 7 da…

astro-ph.CO2021

Dark Energy Survey Year 1 Results: Constraining Baryonic Physics in the Universe

Hung-Jin Huang, Tim Eifler, Rachel Mandelbaum +74

Measurements of large-scale structure are interpreted using theoretical predictions for the matter distribution, including potential impacts of baryonic physics. We constrain the f…

cs.LG2026

Reducing Hallucination in Enterprise AI Workflows via Hybrid Utility Minimum Bayes Risk (HUMBR)

Chenhao Fang, Jordi Mola, Mark Harman +10

Although LLMs drive automation, it is critical to ensure immense consideration for high-stakes enterprise workflows such as those involving legal matters, risk management, and priv…

astro-ph.CO2014

redMaPPer IV: Photometric Membership Identification of Cluster Galaxies with 1% Precision

Eduardo Rozo, Eli S. Rykoff, Matthew Becker +2

In order to study the galaxy population of galaxy clusters with photometric data one must be able to accurately discriminate between cluster members and non-members. The redMaPPer…