activity
20082016
most citedThe Thirteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-IV Survey MApping Nearby Galaxies at Apache Point Observatory

509 citations · 1k across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2016★ 509 cited

The Thirteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-IV Survey MApping Nearby Galaxies at Apache Point Observatory

SDSS Collaboration, Franco D. Albareti, Carlos Allende Prieto +335

The fourth generation of the Sloan Digital Sky Survey (SDSS-IV) began observations in July 2014. It pursues three core programs: APOGEE-2, MaNGA, and eBOSS. In addition, eBOSS cont…

astro-ph.CO2013★ 94 cited

HerMES: Clusters of Dusty Galaxies Uncovered by Herschel and Planck

D. L. Clements, F. G. Braglia, A. Hyde +21

The potential for Planck to detect clusters of dusty, star-forming galaxies at z greater than 1 is tested by examining the Herschel-SPIRE images of Planck Early Release Compact Sou…

astro-ph.CO2010★ 30 cited

HerMES: SPIRE/Sub-millimetre Emission from Radio Selected AGN

N. Seymour, M. Symeonidis, M. Page +1

We examine the rest-frame far-infrared emission from powerful radio sources with 1.4GHz luminosity densities of 25<=log(L_1.4/WHz^-1)<=26.5 in the extragalactic Spitzer First Look…

astro-ph.CO2010★ 33 cited

Herschel-SPIRE observations of the disturbed galaxy NGC4438

L. Cortese, G. J. Bendo, A. Boselli +56

We present Herschel-SPIRE observations of the perturbed galaxy NGC4438 in the Virgo cluster. These images reveal the presence of extra-planar dust up to ~4-5 kpc away from the gala…

astro-ph.CO2010★ 37 cited

Mapping the interstellar medium in galaxies with Herschel/SPIRE

S. A. Eales, M. W. L. Smith, C. D. Wilson +57

The standard method of mapping the interstellar medium in a galaxy, by observing the molecular gas in the CO 1-0 line and the atomic gas in the 21-cm line, is largely limited with…

astro-ph.CO2010★ 165 cited

The Herschel Space Observatory view of dust in M81

G. J. Bendo, C. D. Wilson, M. Pohlen +57

We use Herschel Space Observatory data to place observational constraints on the peak and Rayleigh-Jeans slope of dust emission observed at 70-500 microns in the nearby spiral gala…