activity
20022017
most citedEarly Spectra of the Gravitational Wave Source GW170817: Evolution of a Neutron Star Merger

342 citations · 659 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2017★ 342 cited

Early Spectra of the Gravitational Wave Source GW170817: Evolution of a Neutron Star Merger

B. J. Shappee, J. D. Simon, M. R. Drout +33

On 2017 August 17, Swope Supernova Survey 2017a (SSS17a) was discovered as the optical counterpart of the binary neutron star gravitational wave event GW170817. We report time-seri…

astro-ph.GA2016★ 28 cited

Welcome to the Twilight Zone: The Mid-Infrared Properties of Poststarburst Galaxies

K. Alatalo, T. Bitsakis, L. Lanz +17

We investigate the optical and Wide-field Survey Explorer (WISE) colors of "E+A" identified post-starburst galaxies, including a deep analysis on 190 post-starbursts detected in th…

astro-ph.CO2015

CLASH-VLT: Substructure in the galaxy cluster MACS J1206.2-0847 from kinematics of galaxy populations

M. Girardi, A. Mercurio, I. Balestra +35

In the effort to understand the link between the structure of galaxy clusters and their galaxy populations, we focus on MACSJ1206.2-0847 at z~0.44 and probe its substructure in the…

astro-ph.CO2011★ 42 cited

Kinematics of Gas in Lyman Alpha Nebulae

Yujin Yang, Ann Zabludoff, Knud Jahnke +4

Exploring the origin of Ly-alpha nebulae (blobs) requires measurements of their gas kinematics that are impossible with only the resonant, optically-thick LyA line. To define gas m…

astro-ph.CO2009★ 123 cited

The Carnegie Supernova Project: First Near-Infrared Hubble Diagram to z~0.7

Wendy L. Freedman, Christopher R. Burns, M. M. Phillips +37

The Carnegie Supernova Project (CSP) is designed to measure the luminosity distance for Type Ia supernovae (SNe Ia) as a function of redshift, and to set observational constraints…

astro-ph2002★ 124 cited

Determination of the Dark Matter Profile of Abell 2199 from Integrated Starlight

Daniel D. Kelson, Ann I. Zabludoff, K. A. Williams +3

We have obtained deep, long-slit spectroscopy along the major axis of NGC 6166, the cD galaxy in the cluster Abell 2199, in order to measure the kinematics of intracluster starligh…