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19982009
most citedBright AGN Source List from the First Three Months of the Fermi Large Area Telescope All-Sky Survey

431 citations · 972 across the 14 of their papers we have counts for

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Showing 2003Show all

6 papers · 1 filter

astro-ph2003

Log-parabolic spectra and particle acceleration in the BL Lac object Mkn 421: spectral analysis of the complete BeppoSAX wide band X-ray data set

E. Massaro, M. Perri, P. Giommi +1

We report the results of a new analysis of 13 wide band BeppoSAX observations of the BL Lac object Mkn 421. The data from LECS, MECS and PDS, covering an energy interval from 0.1 t…

astro-ph2003

The phase of the radio and X-ray pulses of PSR B1937+21

G. Cusumano, W. Hermsen, M. Kramer +6

We present timing and spectral results of PSR B1937+21, the fastest known millisecond pulsar (P about 1.56 ms), observed with RXTE. The pulse profile, detected up to 20 keV, shows…

astro-ph2003

Wide band X-ray and optical observations of the BL Lac object 1ES 1959+650 in high state

G. Tagliaferri, M. Ravasio, G. Ghisellini +5

The blazar 1ES 1959+650 was observed twice by BeppoSAX in September 2001 simultaneously with optical observations. We report here the X-ray data together with the optical, R_C magn…

astro-ph2003

The X-ray emission of the Crab-like pulsar PSR J0537-6910

T. Mineo, G. Cusumano, E. Massaro

In this paper we present some preliminary result on the spectral and timing analysis of the X-ray pulsed emission from the 16 ms pulsar PSR J0537-6910 in the energy range 0.1--30 k…

astro-ph2003

BeppoSAX Observations of Centaurus A: the Hard Continuum and the Iron Line Feature

P. Grandi, M. Fiocchi, C. G. Perola +7

The radio galaxy Centaurus A was observed by the BeppoSAX satellite five times from 1997 to 2000. From July 6 1999 to August 17 1999, the source was also simultaneously pointed by…

astro-ph2003

Timing, glitches and braking index of PSR B0540-69

G. Cusumano, E. Massaro, T. Mineo

We report a pulse-time history of PSR B054069 based on the analysis of an extended Data set including ASCA, BeppoSAX and RXTE observations spanning a time interval of about 8 ye…