output
19922026
most citedPlanck 2015 results. XIII. Cosmological parameters

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astro-ph2006★ 1 cited

Were most Low Mass X ray Binaries born in Globular Clusters?

Francesca D'Antona, Anamaria Teodorescu, Paolo Ventura

We summarize the status of art of the secular evolution of low mass X-ray binaries (LMXBs) and take a close look at the orbital period distribution of LMXBs and of binary milliseco…

astro-ph2006★ 52 cited

The XMM-Newton wide-field survey in the COSMOS field: V. Angular Clustering of the X-ray Point Sources

Takamitsu Miyaji, Giovanni Zamorani, Nico Cappelluti +9

We present the first results of the measurements of angular auto-correlation functions (ACFs) of X-ray point sources detected in the XMM-Newton observations of the 2 deg2 COSMOS fi…

astro-ph2006★ 111 cited

The XMM-Newton wide-field survey in the COSMOS field. IV: X-ray spectral properties of Active Galactic Nuclei

V. Mainieri, G. Hasinger, N. Cappelluti +25

We present a detailed spectral analysis of point-like X-ray sources in the XMM-COSMOS field. Our sample of 135 sources only includes those that have more than 100 net counts in the…

astro-ph2006★ 175 cited

The XMM-Newton wide-field survey in the COSMOS field: III. optical identification and multiwavelength properties of a large sample of X-ray selected sources

M. Brusa, G. Zamorani, A. Comastri +31

[ABRIGED] We present the optical identification of a sample of 695 X-ray sources detected in the first 1.3 deg^2 of the XMM-COSMOS survey, down to a 0.5-2 keV (2-10 keV) limiting f…

astro-ph2006★ 353 cited

The XMM-Newton wide-field survey in the COSMOS field: I. Survey description

G. Hasinger, N. Cappelluti, H. Brunner +21

We present the first set of XMM-Newton EPIC observations in the 2 square degree COSMOS field. The strength of the COSMOS project is the unprecedented combination of a large solid a…

astro-ph2006★ 252 cited

On the Rates of Gamma Ray Bursts and Type Ib/c Supernovae

Dafne Guetta, Massimo Della Valle

We measure the local rates of ``low-luminosity'' (LL-GRBs, i.e. L<10^{48--49}erg/sec) and ``high-luminosity'' Gamma-ray Bursts (HL-GRBs). The values are in the range n0=100--1800 G…