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19992023
most citedThe Sloan Digital Sky Survey: Technical Summary

10.4k citations · 44.7k across the 82 of their papers we have counts for

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32 papers · 1 filter

astro-ph.CO2023★ 11 cited

Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing

Juliana Kwan, Shun Saito, Alexie Leauthaud +7

We construct accurate emulators for the projected and redshift space galaxy correlation functions and excess surface density as measured by galaxy-galaxy lensing, based on Halo Occ…

astro-ph.CO2023★ 1 cited

Modeling the Galaxy Distribution in Clusters using Halo Cores

Danila Korytov, Esteban Rangel, Lindsey Bleem +5

The galaxy distribution in dark matter-dominated halos is expected to approximately trace the details of the underlying dark matter substructure. In this paper we introduce halo `c…

astro-ph.CO2021★ 14 cited

Farpoint: A High-Resolution Cosmology Simulation at the Gigaparsec Scale

Nicholas Frontiere, Katrin Heitmann, Esteban Rangel +7

In this paper we introduce the Farpoint simulation, the latest member of the Hardware/Hybrid Accelerated Cosmology Code (HACC) gravity-only simulation family. The domain covers a v…

astro-ph.CO2021★ 8 cited

DESC DC2 Data Release Note

LSST Dark Energy Science Collaboration, Bela Abolfathi, Robert Armstrong +54

In preparation for cosmological analyses of the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST), the LSST Dark Energy Science Collaboration (LSST DESC) has created…

astro-ph.CO2020★ 22 cited

The Last Journey. I. An Extreme-Scale Simulation on the Mira Supercomputer

Katrin Heitmann, Nicholas Frontiere, Esteban Rangel +10

The Last Journey is a large-volume, gravity-only, cosmological N-body simulation evolving more than 1.24 trillion particles in a periodic box with a side-length of 5.025Gpc. It was…

astro-ph.CO2020

The Mira-Titan Universe. III. Emulation of the Halo Mass Function

Sebastian Bocquet, Katrin Heitmann, Salman Habib +5

We construct an emulator for the halo mass function over group and cluster mass scales for a range of cosmologies, including the effects of dynamical dark energy and massive neutri…

astro-ph.CO2019★ 123 cited

CosmoDC2: A Synthetic Sky Catalog for Dark Energy Science with LSST

Danila Korytov, Andrew Hearin, Eve Kovacs +27

This paper introduces cosmoDC2, a large synthetic galaxy catalog designed to support precision dark energy science with the Large Synoptic Survey Telescope (LSST). CosmoDC2 is the…

astro-ph.CO2019★ 104 cited

The Outer Rim Simulation: A Path to Many-Core Supercomputers

Katrin Heitmann, Hal Finkel, Adrian Pope +10

We describe the Outer Rim cosmological simulation, one of the largest high-resolution N-body simulations performed to date, aimed at promoting science to be carried out with large-…

astro-ph.CO2019★ 25 cited

HACC Cosmological Simulations: First Data Release

Katrin Heitmann, Thomas D. Uram, Hal Finkel +10

We describe the first major public data release from cosmological simulations carried out with Argonne's HACC code. This initial release covers a range of datasets from large gravi…

astro-ph.CO2019★ 5 cited

Effects of Massive Neutrinos and Dynamical Dark Energy on the Cluster Mass Function

Rahul Biswas, Katrin Heitmann, Salman Habib +3

The presence of massive neutrinos affects the growth of large-scale structure in the universe, leaving a potentially observable imprint on the abundance and properties of massive d…

astro-ph.CO2018★ 17 cited

The Borg Cube Simulation: Cosmological Hydrodynamics with CRK-SPH

J. D. Emberson, Nicholas Frontiere, Salman Habib +4

A challenging requirement posed by next-generation observations is a firm theoretical grasp of the impact of baryons on structure formation. Cosmological hydrodynamic simulations m…

astro-ph.CO2018★ 124 cited

Halo Profiles and the Concentration-Mass Relation for a ΛCDM Universe

Hillary L. Child, Salman Habib, Katrin Heitmann +4

Profiles of dark matter-dominated halos at the group and cluster scales play an important role in modern cosmology. Using results from two very large cosmological -body simulati…

astro-ph.CO2017★ 133 cited

The Mira-Titan Universe II: Matter Power Spectrum Emulation

Earl Lawrence, Katrin Heitmann, Juliana Kwan +7

We introduce a new cosmic emulator for the matter power spectrum covering eight cosmological parameters. Targeted at optical surveys, the emulator provides accurate predictions out…

astro-ph.CO2015★ 133 cited

The Mira-Titan Universe: Precision Predictions for Dark Energy Surveys

Katrin Heitmann, Derek Bingham, Earl Lawrence +8

Ground and space-based sky surveys enable powerful cosmological probes based on measurements of galaxy properties and the distribution of galaxies in the Universe. These probes inc…

astro-ph.CO2015★ 32 cited

Redshift-space distortions in massive neutrino and evolving dark energy cosmologies

Amol Upadhye, Juliana Kwan, Adrian Pope +4

Large-scale structure surveys in the coming years will measure the redshift-space power spectrum to unprecedented accuracy, allowing for powerful new tests of the LambdaCDM picture…

astro-ph.CO2014★ 41 cited

The Q Continuum Simulation: Harnessing the Power of GPU Accelerated Supercomputers

Katrin Heitmann, Nicholas Frontiere, Chris Sewell +6

Modeling large-scale sky survey observations is a key driver for the continuing development of high resolution, large-volume, cosmological simulations. We report the first results…

astro-ph.CO2013★ 103 cited

Cosmic Emulation: Fast Predictions for the Galaxy Power Spectrum

Juliana Kwan, Katrin Heitmann, Salman Habib +4

The halo occupation distribution (HOD) approach has proven to be an effective method for modeling galaxy clustering and bias. In this approach, galaxies of a given type are probabi…

astro-ph.CO2013★ 54 cited

Large-Scale Structure Formation with Massive Neutrinos and Dynamical Dark Energy

Amol Upadhye, Rahul Biswas, Adrian Pope +4

Over the next decade, cosmological measurements of the large-scale structure of the Universe will be sensitive to the combined effects of dynamical dark energy and massive neutrino…

astro-ph.CO2012★ 45 cited

Large Synoptic Survey Telescope: Dark Energy Science Collaboration

LSST Dark Energy Science Collaboration

This white paper describes the LSST Dark Energy Science Collaboration (DESC), whose goal is the study of dark energy and related topics in fundamental physics with data from the La…

astro-ph.CO2012★ 135 cited

GOODS-Herschel: radio-excess signature of hidden AGN activity in distant star-forming galaxies

A. Del Moro, D. M. Alexander, J. R. Mullaney +23

We present here a new spectral energy distribution (SED) fitting approach that we adopt to select radio-excess sources amongst distant star-forming galaxies in the GOODS-Herschel (…

astro-ph.CO2012★ 89 cited

The JCMT Nearby Galaxies Legacy Survey VIII. CO data and the L(CO3-2)-L(FIR) correlation in the SINGS sample

C. D. Wilson, B. E. Warren, F. P. Israel +57

The James Clerk Maxwell Telescope Nearby Galaxies Legacy Survey (NGLS) comprises an HI-selected sample of 155 galaxies spanning all morphological types with distances less than 25…

astro-ph.CO2011

Querying for heavily obscured AGN via high 9.7 micron optical depths: results from the 12 micron, GOODS, and FLS Spitzer spectroscopic samples

K. M. Dasyra, I. Georgantopoulos, A. Pope +1

To optimally identify candidates of the Compton-thick (CT) active galactic nuclei (AGN) that contribute to the unresolved X-ray background in infrared surveys, a tracer of column d…

astro-ph.CO2011★ 47 cited

GOODS-Herschel A population of 24micron dropout sources at z < 2

Georgios E. Magdis, D. Elbaz, M. Dickinson +25

Using extremely deep PACS 100- and 160um Herschel data from the GOODS-Herschel program, we identify 21 infrared bright galaxies previously missed in the deepest 24um surveys perfor…

astro-ph.CO2010★ 24 cited

Analyzing and Visualizing Cosmological Simulations with ParaView

Jonathan Woodring, Katrin Heitmann, James Ahrens +4

The advent of large cosmological sky surveys - ushering in the era of precision cosmology - has been accompanied by ever larger cosmological simulations. The analysis of these simu…