output
20022024
most citedThe Transiting Exoplanet Survey Satellite

4.1k citations

Showing 2014Show all

97 papers · 1 filter

astro-ph.SR20143 cited

The Clusters AgeS Experiment (CASE). Variable stars in the field of the globular cluster NGC 6362

J. Kaluzny, I. B. Thompson, M. Rozyczka +2

The field of the globular cluster NGC 6362 was monitored between 1995 and 2009 in a search for variable stars. BV light curves were obtained for 69 periodic variables including 34…

astro-ph.SR201455 cited

AGB Sodium Abundances in the Globular Cluster 47 Tucanae (NGC 104)

Christian I. Johnson, Iain McDonald, Catherine A. Pilachowski +8

A recent analysis comparing the [Na/Fe] distributions of red giant branch (RGB) and asymptotic giant branch (AGB) stars in the Galactic globular cluster NGC 6752 found that the rat…

astro-ph.SR201471 cited

WISEP J004701.06+680352.1: An intermediate surface gravity, dusty brown dwarf in the AB Dor Moving Group

John E. Gizis, Katelyn N. Allers, Michael C. Liu +4

We present spectroscopy, astrometry, and photometry of the brown dwarf WISEP J004701.06+680352.1 (W0047+68), an unusually red field L dwarf at a distance of parsecs.…

astro-ph.GA20141.7k cited

Overview of the SDSS-IV MaNGA Survey: Mapping Nearby Galaxies at Apache Point Observatory

Kevin Bundy, Matthew A. Bershady, David R. Law +65

We present an overview of a new integral field spectroscopic survey called MaNGA (Mapping Nearby Galaxies at Apache Point Observatory), one of three core programs in the fourth-gen…

astro-ph.HE2014147 cited

Correlation between the photon index and X-ray luminosity of black hole X-ray binaries and active galactic nuclei: observations and interpretation

Qi-Xiang Yang, Fu-Guo Xie, Feng Yuan +4

We investigate the observed correlation between the 2--10 keV X-ray luminosity (in unit of the Eddington luminosity; ) and the photon index () of the X-r…

astro-ph.EP201438 cited

Exo-zodi modelling for the Large Binocular Telescope Interferometer

Grant M. Kennedy, Mark C. Wyatt, Vanessa Bailey +18

Habitable zone dust levels are a key unknown that must be understood to ensure the success of future space missions to image Earth analogues around nearby stars. Current detection…