output
19912026
most citedObservation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC

10.9k citations

Showing 2016 · astro-ph.GAShow all

24 papers · 2 filters

astro-ph.GA2016★ 534 cited

The Chandra Deep Field-South Survey: 7 Ms Source Catalogs

B. Luo, W. N. Brandt, Y. Q. Xue +23

We present X-ray source catalogs for the Ms exposure of the Chandra Deep Field-South (CDF-S), which covers a total area of 484.2 arcmin. Utilizing WAVDETECT for init…

astro-ph.GA2016

The XMM Deep Survey in the CDFS

A. Comastri, K. Iwasawa, C. Vignali +3

The Chandra Deep Field South (CDF-S) was observed by XMM-Newton for a total of about 3 Ms in many periods over the past decade (2001-2002 and 2008-2009). The main goal of the surve…

astro-ph.GA2016★ 34 cited

Abundances of disk and bulge giants from hi-res optical spectra: II. O, Mg, Ca, and Ti in the bulge sample

H. Jönsson, N. Ryde, M. Schultheis +1

Determining elemental abundances of bulge stars can, via chemical evolution modeling, help to understand the formation and evolution of the bulge. Recently there have been claims b…

astro-ph.GA2016★ 12 cited

Abundances of disk and bulge giants from hi-res optical spectra: I. O, Mg, Ca, and Ti in the Solar neighborhood and Kepler field samples

H. Jönsson, N. Ryde, T. Nordlander +4

The galactic bulge is a significant part of our galaxy, but it is hard to observe, being both distant and covered by dust in the disk. Therefore there do not exist many hi-res opti…

astro-ph.GA2016★ 119 cited

The origin of the Milky Way globular clusters

Florent Renaud, Oscar Agertz, Mark Gieles

We present a cosmological zoom-in simulation of a Milky Way-like galaxy used to explore the formation and evolution of star clusters. We investigate in particular the origin of the…

astro-ph.GA2016★ 36 cited

The selection function of the RAVE survey

Jennifer Wojno, Georges Kordopatis, Tilmann Piffl +23

We characterize the selection function of RAVE using 2MASS as our underlying population, which we assume represents all stars which could have potentially been observed. We evaluat…