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19952009
most citedThe ACS Nearby Galaxy Survey Treasury

564 citations · 1.6k across the 16 of their papers we have counts for

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26 papers · 1 filter

astro-ph200874 cited

The ACS Nearby Galaxy Survey Treasury I. The Star Formation History of the M81 Outer Disk

Benjamin F. Williams, Julianne J. Dalcanton, Anil C. Seth +16

The ACS Nearby Galaxy Survey Treasury (ANGST) is a large Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS) treasury program to obtain resolved stellar photometry for a…

astro-ph2008101 cited

The Luminosity and Mass Functions of Low-Mass Stars in the Galactic Disk: I. The Calibration Region

Kevin R. Covey, Suzanne L. Hawley, John J. Bochanski +6

We present measurements of the luminosity and mass functions of low-mass stars constructed from a catalog of matched Sloan Digital Sky Survey (SDSS) and 2 Micron All Sky Survey (2M…

astro-ph200816 cited

GALEX, Optical and IR Light Curves of MQ Dra: UV Excesses at Low Accretion Rates

Paula Szkody, Albert P. Linnell, Ryan K. Campbell +5

Ultraviolet light curves constructed from NUV and FUV detectors on GALEX reveal large amplitude variations during the orbital period of the Low Accretion Rate Polar MQ Dra (SDSSJ15…

astro-ph200863 cited

First-Year Spectroscopy for the SDSS-II Supernova Survey

Chen Zheng, Roger W. Romani, Masao Sako +77

This paper presents spectroscopy of supernovae discovered in the first season of the Sloan Digital Sky Survey-II Supernova Survey. This program searches for and measures multi-band…

astro-ph200831 cited

Two More Candidate AM Canum Venaticorum (AM CVn) Binaries from the Sloan Digital Sky Survey

S. F. Anderson, A. C. Becker, D. Haggard +18

AM CVn systems are a select group of ultracompact binaries with the shortest orbital periods of any known binary subclass; mass-transfer is likely from a low-mass (partially-)degen…

astro-ph200740 cited

Argon Abundances in the Solar Neighborhood: Non-LTE Analysis of Orion Association B-type Stars

Thierry Lanz, Katia Cunha, Jon Holtzman +1

Argon abundances have been derived for a sample of B main-sequence stars in the Orion association. The abundance calculations are based on NLTE metal line-blanketed model atmospher…