activity
20032009
most citedStellar and total baryon mass fractions in groups and clusters since redshift 1

328 citations · 943 across the 13 of their papers we have counts for

collaborators

16 papers

astro-ph.HE2009

Not only once: the amazing gamma-ray activity of the blazar PKS 1510-089

F. D'Ammando, C. M. Raiteri, M. Villata +6

PKS 1510-089 is a powerful Flat Spectrum Radio Quasar at z=0.361 with radiative output dominated by the gamma-ray emission. In the last two years PKS 1510-089 showed high variabili…

astro-ph.CO2009328 cited

Stellar and total baryon mass fractions in groups and clusters since redshift 1

S. Giodini, D. Pierini, A. Finoguenov +24

We investigate if the discrepancy between estimates of the total baryon mass fraction obtained from observations of the cosmic microwave background (CMB) and of galaxy groups/clust…

astro-ph.HE200940 cited

XMM-Newton and Suzaku analysis of the Fe K complex in the Seyfert 1 galaxy Mrk 509

G. Ponti, M. Cappi, C. Vignali +11

We report on partially overlapping XMM-Newton (~260 ks) and Suzaku (~100 ks) observations of the iron K band in the nearby, bright Seyfert 1 galaxy Mrk 509. The source shows a reso…

astro-ph200851 cited

Weighing the black holes in ultraluminous X-ray sources through timing

P. Casella, G. Ponti, A. Patruno +3

We describe a new method to estimate the mass of black holes in Ultraluminous X-ray Sources (ULXs). The method is based on the recently discovered ``variability plane'', populated…

astro-ph200769 cited

Stellar evolution through the ages: period variations in galactic RRab stars as derived from the GEOS database and TAROT telescopes

J. F. Le Borgne, A. Paschke, J. Vandenbroere +6

The theory of stellar evolution can be more closely tested if we have the opportunity to measure new quantities. Nowadays, observations of galactic RR Lyr stars are available on a…

astro-ph200745 cited

The HELLAS2XMM survey: XI. Unveiling the nature of X-ray Bright Optically Normal Galaxies

F. Civano, M. Mignoli, A. Comastri +8

X-ray Bright Optically Normal Galaxies (XBONGs) constitute a small but not negligible fraction of hard X-ray selected sources in recent Chandra and XMM-Newton surveys. Even though…