output
20022026
most citedThe Transiting Exoplanet Survey Satellite

4.1k citations

Showing 2017 · astro-ph.GAShow all

9 papers · 2 filters

astro-ph.GA2017258 cited

Galaxy And Mass Assembly (GAMA): the G02 field, Herschel-ATLAS target selection and Data Release 3

I. K. Baldry, J. Liske, M. J. I. Brown +39

We describe data release 3 (DR3) of the Galaxy And Mass Assembly (GAMA) survey. The GAMA survey is a spectroscopic redshift and multi-wavelength photometric survey in three equator…

astro-ph.GA201730 cited

Galaxy And Mass Assembly: Automatic Morphological Classification of Galaxies Using Statistical Learning

Sreevarsha Sreejith, Sergiy Pereverzyev, Lee S. Kelvin +15

We apply four statistical learning methods to a sample of galaxies () from the Galaxy and Mass Assembly (GAMA) survey to test the feasibility of using automated algo…

astro-ph.GA201716 cited

The Baryonic Collapse Efficiency of Galaxy Groups in the RESOLVE and ECO Surveys

Kathleen D. Eckert, Sheila J. Kannappan, Claudia del P. Lagos +6

We examine the z = 0 group-integrated stellar and cold baryonic (stars + cold atomic gas) mass functions (group SMF and CBMF) and the baryonic collapse efficiency (group cold baryo…

astro-ph.GA2017293 cited

Target Selection for the SDSS-IV APOGEE-2 Survey

G. Zasowski, R. E. Cohen, S. D. Chojnowski +34

APOGEE-2 is a high-resolution, near-infrared spectroscopic survey observing roughly 300,000 stars across the entire sky. It is the successor to APOGEE and is part of the Sloan Digi…

astro-ph.GA2017102 cited

The SAMI Galaxy Survey: Global stellar populations on the size-mass plane

Nicholas Scott, S. Brough, Scott M. Croom +20

We present an analysis of the global stellar populations of galaxies in the SAMI Galaxy Survey. Our sample consists of 1319 galaxies spanning four orders of magnitude in stellar ma…

astro-ph.GA201729 cited

The Time-Domain Spectroscopic Survey: Target Selection for Repeat Spectroscopy

Chelsea L. MacLeod, Paul J. Green, Scott F. Anderson +35

As astronomers increasingly exploit the information available in the time domain, spectroscopic variability in particular opens broad new channels of investigation. Here we describ…