output
19952026
most citedThe Apache Point Observatory Galactic Evolution Experiment (APOGEE)

1.8k citations

Showing 2016 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2016★ 3 cited

The time evolution of HH~2 from four epochs of HST images

A. C. Raga, B. Reipurth, P. F. Velázquez +2

We have analyzed four epochs of H and [S~II] HST images of the HH~1/2 outflow (covering a time interval from 1994 to 2014) to determine proper motions and emission line fluxes o…

astro-ph.GA2016★ 28 cited

Constraining the ISM properties of the Cloverleaf quasar host galaxy with Herschel spectroscopy

Bade D. Uzgil, C. Matt Bradford, Steve Hailey-Dunsheath +2

We present Herschel observations of far-infrared (FIR) fine-structure (FS) lines [CII]158m, [OI]63m, [OIII]52m, and [SiII]35m in the z=2.56 Cloverleaf quasar, and combi…

astro-ph.GA2016★ 20 cited

The Role of Host Galaxy for the Environmental Dependence of Active Nuclei in Local Galaxies

R. I. Davies, E. K. S. Hicks, P. Erwin +22

We discuss the environment of local hard X-ray selected active galaxies, with reference to two independent group catalogues. We find that the fraction of these AGN in S0 host galax…

astro-ph.GA2016★ 101 cited

An Ultra-Faint Galaxy Candidate Discovered in Early Data from the Magellanic Satellites Survey

A. Drlica-Wagner, K. Bechtol, S. Allam +21

We report a new ultra-faint stellar system found in Dark Energy Camera data from the first observing run of the Magellanic Satellites Survey (MagLiteS). MagLiteS J0644-5953 (Pictor…

astro-ph.GA2016★ 58 cited

Constraints on the Broad Line Region Properties and Extinction in Local Seyferts

Allan Schnorr-Müller, R. I. Davies, K. T. Korista +22

We use high spectral resolution (R > 8000) data covering 3800-13000Å to study the physical conditions of the broad line region (BLR) of nine nearby Seyfert 1 galaxies. Up to six br…

astro-ph.GA2016★ 67 cited

Toward gas exhaustion in the W51 high-mass protoclusters

Adam Ginsburg, W. M. Goss, Ciriaco Goddi +10

We present new JVLA observations of the high-mass cluster-forming region W51A from 2 to 16 GHz with resolution 0.3 - 0.5". The data reveal a wealth of observatio…