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20002023
most citedThe Man Behind the Curtain: X-rays Drive the UV through NIR Variability in the 2013 AGN Outburst in NGC 2617

1.9k citations · 15.3k across the 197 of their papers we have counts for

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Showing 2017Show all

11 papers · 1 filter

astro-ph.SR2017★ 17 cited

Metal-Rich RRc stars in the Carnegie RR Lyrae Survey

Christopher Sneden, George W. Preston, Juna A. Kollmeier +6

We describe and employ a stacking procedure to investigate abundances derived from the low S/N spectra obtained in the Carnegie RR Lyrae Survey (CARRS; Kollmeier et al. 2013). We f…

astro-ph.HE2017★ 839 cited

Light Curves of the Neutron Star Merger GW170817/SSS17a: Implications for R-Process Nucleosynthesis

M. R. Drout, A. L. Piro, B. J. Shappee +41

On 2017 August 17, gravitational waves were detected from a binary neutron star merger, GW170817, along with a coincident short gamma-ray burst, GRB170817A. An optical transient so…

astro-ph.HE2017★ 35 cited

The Unprecedented Properties of the First Electromagnetic Counterpart to a Gravitational Wave Source

Matthew R. Siebert, Ryan J. Foley, Maria R. Drout +15

We discovered Swope Supernova Survey 2017a (SSS17a) in the LIGO/Virgo Collaboration (LVC) localization volume of GW170817, the first detected binary neutron star (BNS) merger, only…

astro-ph.GA2017★ 67 cited

The Old Host-Galaxy Environment of SSS17a, the First Electromagnetic Counterpart to a Gravitational Wave Source

Y. -C. Pan, C. D. Kilpatrick, J. D. Simon +16

We present an analysis of the host-galaxy environment of Swope Supernova Survey 2017a (SSS17a), the discovery of an electromagnetic counterpart to a gravitational wave source, GW17…

astro-ph.HE2017★ 71 cited

Type II supernova spectral diversity II: Spectroscopic and photometric correlations

Claudia P. Gutiérrez, Joseph P. Anderson, Mario Hamuy +7

We present an analysis of observed trends and correlations between a large range of spectral and photometric parameters of more than 100 type II supernovae (SNe~II), during the pho…

astro-ph.HE2017★ 159 cited

Type II supernova spectral diversity I: Observations, sample characterization and spectral line evolution

Claudia P. Gutiérrez, Joseph P. Anderson, Mario Hamuy +23

We present 888 visual-wavelength spectra of 122 nearby type II supernovae (SNe II) obtained between 1986 and 2009, and ranging between 3 and 363 days post explosion. In this first…

astro-ph.IM2017★ 204 cited

The Carnegie Supernova Project I: Third Photometry Data Release of Low-Redshift Type Ia Supernovae and Other White Dwarf Explosions

Kevin Krisciunas, Carlos Contreras, Christopher R. Burns +27

We present final natural system optical (ugriBV) and near-infrared (YJH) photometry of 134 supernovae (SNe) with probable white dwarf progenitors that were observed in 2004-2009 as…

astro-ph.SR2017★ 96 cited

Light and color curve properties of type Ia supernovae: Theory vs. Observations

P. Hoeflich, E. Y. Hsiao, C. Ashall +10

We study optical light curve(LC) relations of type Ia supernovae(SNe~Ia) for their use in cosmology using high-quality photometry published by the Carnegie-Supernovae-Project (CSP-…

astro-ph.SR2017★ 39 cited

The Evolution and Physical Parameters of WN3/O3s: a New Type of Wolf-Rayet Star

Kathryn F. Neugent, Philip Massey, D. John Hillier +1

As part of a search for Wolf-Rayet (WR) stars in the Magellanic Clouds, we have discovered a new type of WR star in the Large Magellanic Cloud (LMC). These stars have both strong e…

astro-ph.SR2017★ 28 cited

A Modern Search for Wolf-Rayet Stars in the Magellanic Clouds. III. A Third Year of Discoveries

Philip Massey, Kathryn F. Neugent, Nidia Morrell

For the past three years we have been conducting a survey for WR stars in the Large and Small Magellanic Clouds (LMC, SMC). Our previous work has resulted in the discovery of a new…

astro-ph.HE2017★ 102 cited

SPIRITS: Uncovering Unusual Infrared Transients With Spitzer

Mansi M. Kasliwal, John Bally, Frank Masci +44

We present an ongoing, systematic search for extragalactic infrared transients, dubbed SPIRITS --- SPitzer InfraRed Intensive Transients Survey. In the first year, using Spitzer/IR…