activity
20092026
most citedFirst Cosmology Results using Type Ia Supernovae from the Dark Energy Survey: Constraints on Cosmological Parameters

276 citations · 1.2k across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.CO2026★ 1 cited

Union3.1: Reducing Systematics in Supernova Cosmology with Self-consistent Measurements of Host Galaxy Properties for 2000 Type Ia Supernovae

Taylor J. Hoyt, David Rubin, Greg Aldering +3

Photometrically derived distances of Type Ia supernovae (SNe Ia) rely on a empirical correction based on host galaxy properties, e.g., global stellar mass. Unbiased cosmo…

astro-ph.CO2021★ 16 cited

The HST See Change Program: I. Survey Design, Pipeline, and Supernova Discoveries

Brian Hayden, David Rubin, Kyle Boone +53

The See Change survey was designed to make cosmological measurements by efficiently discovering high-redshift Type Ia supernovae (SNe Ia) and improving cluster mass measureme…

astro-ph.CO2018★ 52 cited

First Cosmology Results Using Type Ia Supernovae From the Dark Energy Survey: Survey Overview and Supernova Spectroscopy

C. B. D'Andrea, M. Smith, M. Sullivan +108

We present spectroscopy from the first three seasons of the Dark Energy Survey Supernova Program (DES-SN). We describe the supernova spectroscopic program in full: strategy, observ…

astro-ph.CO2018★ 276 cited

First Cosmology Results using Type Ia Supernovae from the Dark Energy Survey: Constraints on Cosmological Parameters

T. M. C. Abbott, S. Allam, P. Andersen +141

We present the first cosmological parameter constraints using measurements of type Ia supernovae (SNe Ia) from the Dark Energy Survey Supernova Program (DES-SN). The analysis uses…

physics.ed-ph2018★ 8 cited

New Science, New Media: An Assessment of the Online Education and Public Outreach Initiatives of The Dark Energy Survey

R. C. Wolf, A. K. Romer, B. Nord +25

As large-scale international collaborations become the standard for astronomy research, a wealth of opportunities have emerged to create innovative education and public outreach (E…

astro-ph.GA2017★ 30 cited

The Discovery of a Gravitationally Lensed Supernova Ia at Redshift 2.22

David Rubin, Brian Hayden, Xiaosheng Huang +32

We present the discovery and measurements of a gravitationally lensed supernova (SN) behind the galaxy cluster MOO J1014+0038. Based on multi-band Hubble Space Telescope and Very L…

astro-ph.CO2016★ 105 cited

Host Galaxy Identification for Supernova Surveys

Ravi R. Gupta, Steve Kuhlmann, Eve Kovacs +57

Host galaxy identification is a crucial step for modern supernova (SN) surveys such as the Dark Energy Survey (DES) and the Large Synoptic Survey Telescope (LSST), which will disco…

astro-ph.CO2016★ 26 cited

SDSS-II Supernova Survey: An Analysis of the Largest Sample of Type Ia Supernovae and Correlations with Host-Galaxy Spectral Properties

Rachel C. Wolf, Chris B. D'Andrea, Ravi R. Gupta +13

Using the largest single-survey sample of Type Ia supernovae (SNe Ia) to date, we study the relationship between properties of SNe Ia and those of their host galaxies, focusing pri…

astro-ph.SR2014★ 87 cited

The Core Collapse Supernova Rate from the SDSS-II Supernova Survey

Matt Taylor, David Cinabro, Ben Dilday +8

We use the Sloan Digital Sky Survey II Supernova Survey (SDSS-II SNS) data to measure the volumetric core collapse supernova (CCSN) rate in the redshift range (0.03<z<0.09). Using…

astro-ph.CO2014★ 213 cited

The Data Release of the Sloan Digital Sky Survey-II Supernova Survey

Masao Sako, Bruce Bassett, Andrew C. Becker +46

This paper describes the data release of the Sloan Digital Sky Survey-II (SDSS-II) Supernova Survey conducted between 2005 and 2007. Light curves, spectra, classifications, and anc…

astro-ph.CO2013★ 20 cited

Host Galaxy Spectra and Consequences for SN Typing From The SDSS SN Survey

Matthew D. Olmstead, Peter J. Brown, Masao Sako +28

We present the spectroscopy from 5254 galaxies that hosted supernovae (SNe) or other transient events in the Sloan Digital Sky Survey II (SDSS-II). Obtained during SDSS-I, SDSS-II,…

astro-ph.CO2013★ 13 cited

Properties of type Ia supernovae inside rich galaxy clusters

Henrique S. Xavier, Ravi R. Gupta, Masao Sako +9

We used the GMBCG galaxy cluster catalogue and SDSS-II supernovae data with redshifts measured by the BOSS project to identify 48 SNe Ia residing in rich galaxy clusters and compar…

astro-ph.CO2012★ 64 cited

The Fundamental Metallicity Relation Reduces Type Ia SN Hubble Residuals More Than Host Mass Alone

Brian T. Hayden, Ravi R. Gupta, Peter M. Garnavich +3

Type Ia Supernova Hubble residuals have been shown to correlate with host galaxy mass, imposing a major obstacle for their use in measuring dark energy properties. Here, we calibra…

astro-ph.CO2012★ 85 cited

SNe Ia host galaxy properties from Sloan Digital Sky Survey-II spectroscopy

Jonas Johansson, Daniel Thomas, Janine Pforr +7

We study the stellar populations of SNe Ia host galaxies using SDSS-II spectroscopy. We focus on the relationships of SNe Ia properties with stellar velocity dispersion and the ste…

astro-ph.CO2011★ 93 cited

Spectroscopic Properties of Star-Forming Host Galaxies and Type Ia Supernova Hubble Residuals in a Nearly Unbiased Sample

Chris B. D'Andrea, Ravi R. Gupta, Masao Sako +13

We examine the correlation between supernova host galaxy properties and their residuals on the Hubble diagram. We use supernovae discovered during the Sloan Digital Sky Survey II -…

astro-ph.CO2011★ 123 cited

Improved Constraints on Type Ia Supernova Host Galaxy Properties using Multi-Wavelength Photometry and their Correlations with Supernova Properties

Ravi R. Gupta, Chris B. D'Andrea, Masao Sako +11

We improve estimates of stellar mass and mass-weighted average age of Type Ia supernova (SN Ia) host galaxies by combining UV and near-IR photometry with optical photometry in our…

astro-ph.CO2009★ 5 cited

Evidence for Non-Linear Growth of Structure from an X-ray Selected Cluster Survey using a Novel Joint Analysis of the Chandra and XMM-Newton Archives

J. R. Peterson, J. G. Jernigan, R. R. Gupta +2

We present a large X-ray selected serendipitous cluster survey based on a novel joint analysis of archival Chandra and XMM-Newton data. The survey provides enough depth to reach cl…