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20062009
most citedBright AGN Source List from the First Three Months of the Fermi Large Area Telescope All-Sky Survey

431 citations · 681 across the 7 of their papers we have counts for

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11 papers · 1 filter

astro-ph200832 cited

AGILE and Swift simultaneous observations of the blazar S50716+714 during the bright flare of October 2007

P. Giommi, S. Colafrancesco, S. Cutini +15

We present the results of a series of optical, UV, X-ray and gamma-ray observations of the BL Lac object S50716+714 carried out by the Swift and AGILE satellites in late 2007 when…

astro-ph20081 cited

A Null Test of the Metric Nature of the Cosmic Acceleration

A. Buzzi, C. Marinoni, S. Colafrancesco

We discuss the testable predictions of a phenomenological model in which the accelerated expansion of the universe is the result of the action of a non-gravitational force field, r…

astro-ph200827 cited

SZ effect from radio-galaxy lobes: astrophysical and cosmological relevance

S. Colafrancesco

We derive the SZ effect arising in radio-galaxy lobes that are filled with high-energy, non-thermal electrons. We provide here quantitative estimates for SZ effect expected from th…

astro-ph200828 cited

Warming rays in cluster cool cores

S. Colafrancesco, P. Marchegiani

We present a model of cosmic ray heating of clusters' cores that reproduces the observed temperature distribution in clusters by using an energy balance condition in which the emit…

astro-ph20071 cited

Blazar Duty-Cycle at gamma-ray Frequecies: Constraints from Extragalactic Background Radiation and Prospects for AGILE and GLAST

Carlotta Pittori, Elisabetta Cavazzuti, Sergio Colafrancesco +1

We take into account the constraints from the observed extragalactic gamma-ray background to estimate the maximum duty cycle allowed for a selected sample of WMAP Blazars, in order…

astro-ph200713 cited

Direct probes of Dark Matter in the cluster 1ES0657-556 through microwave observations

S. Colafrancesco, P. de Bernardis, S. Masi +2

The cluster 1ES0657-556 is an ideal astrophysical laboratory to study the distribution and the nature of Dark Matter because this last component is spatially separated from the int…