output
19922026
most citedThe clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample

3.1k citations

Showing 2007 · astro-phShow all

18 papers · 2 filters

astro-ph2007★ 354 cited

The Afterglows of Swift-era Gamma-Ray Bursts. I. Comparing pre-Swift and Swift era Long/Soft (Type II) GRB Optical Afterglows

D. A. Kann, S. Klose, B. Zhang +73

We have gathered optical photometry data from the literature on a large sample of Swift-era gamma-ray burst (GRB) afterglows including GRBs up to September 2009, for a total of 76…

astro-ph2007★ 27 cited

Redshift Limits of BL Lacertae Objects from Optical Spectroscopy

J. D. Finke, J. C. Shields, M. Boettcher +1

Context: BL Lacertae objects have been the targets for numerous recent multiwavelength campaigns, continuum spectral variability studies, and theoretical spectral and variability m…

astro-ph2007

X-ray Observables of Magnetically Dominated Cavities in Clusters

Steven Diehl, Masanori Nakamura, Hui Li +1

We present results from magneto-hydrodynamic jet simulations in the magnetically dominated regime and find that they inflate cavities into the intracluster medium. Mock Chandra X-r…

astro-ph2007★ 39 cited

The Hot Interstellar Medium in Normal Elliptical Galaxies. II. Morphological Evidence for AGN Feedback

Steven Diehl, Thomas S. Statler

We report on the discovery of a new quantitative relationship between X-ray gas morphology and radio and X-ray AGN luminosities in normal elliptical galaxies. This is the second pa…

astro-ph2007★ 21 cited

Spatially resolved spectroscopy of Coma cluster early-type galaxies IV. Completing the dataset

E. M. Corsini, G. Wegner, R. P. Saglia +3

The long-slit spectra obtained along the minor axis, offset major axis and diagonal axis are presented for 12 E and S0 galaxies of the Coma cluster drawn from a magnitude-limited s…

astro-ph2007★ 1.3k cited

Heating Hot Atmospheres with Active Galactic Nuclei

B. R. McNamara, P. E. J. Nulsen

High resolution X-ray spectroscopy of the hot gas in galaxy clusters has shown that the gas is not cooling to low temperatures at the predicted rates of hundreds to thousands of so…