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19932026
most citedThe Large Area Telescope on the Fermi Gamma-ray Space Telescope Mission

4.1k citations

Showing 2004Show all

26 papers · 1 filter

astro-ph2004★ 170 cited

On the polar caps of the 3 Musketeers

A. De Luca, P. A. Caraveo, S. Mereghetti +2

XMM-Newton observations of PSR B0656+14, PSR B1055-52 and Geminga have substantially increased the statistics available for these three isolated neutron stars, so apparently simila…

astro-ph2004★ 7 cited

XMM-Newton observation of 4U 1543-475: the X-ray spectrum of a stellar-mass black-hole at low luminosity

Nicola La Palombara, Sandro Mereghetti

We report the results of an observation of the galactic black-hole binary 4U 1543-475 performed by XMM-Newton on 2002 August 18, about two months after the start of an outburst det…

astro-ph2004★ 5 cited

GRB 040403: a faint X-ray rich Gamma-ray Burst discovered by INTEGRAL

S. Mereghetti, D. Gotz, M. I. Andersen +13

GRB 040403 is one of the faintest gamma-ray bursts for which a rapid and accurate localization has been obtained. Here we report on the gamma-ray properties of this burst, based on…

astro-ph2004★ 21 cited

The soft X-ray counterpart of the newly discovered INTEGRAL source IGRJ16195-4945

L. Sidoli, S. Vercellone, S. Mereghetti +1

The INTEGRAL satellite, during its regular scanning observations of the Galactic plane, has discovered several new X-ray sources emitting above 20 keV. The nature of the great majo…

astro-ph2004★ 12 cited

INTEGRAL and XMM-Newton Observations of GRB040106

L. Moran, S. Mereghetti, D. Gotz +10

On January 6th 2004, the IBAS burst alert system triggered the 8th gamma-ray burst (GRB) to be located by the INTEGRAL satellite. The position was determined and publicly distribut…

astro-ph2004★ 217 cited

The GALEX-VVDS Measurement of the Evolution of the 1500A Luminosity Function

S. Arnouts, D. Schiminovich, O. Ilbert +8

We present the first measurement of the galaxy luminosity function at 1500A between 0.2<z<1.2 based on GALEX-VVDS observations (1000 spectroscopic redshifts for galaxies with NUV<2…

astro-ph2004★ 85 cited

INTEGRAL discovery of persistent hard X-ray emission from the Soft Gamma Ray Repeater SGR 1806-20

S. Mereghetti, D. Gotz, I. F. Mirabel +1

We report the discovery of persistent hard X-ray emission extending up to 150 keV from the soft gamma-ray repeater SGR 1806-20 using data obtained with the INTEGRAL satellite in 20…

astro-ph2004★ 19 cited

Feasibility study of a Laue lens for hard X-rays for space astronomy

A. Pisa, F. Frontera, P. De Chiara +8

We report on the feasibility study of a Laue lens for hard X-rays (>60 keV)based on mosaic crystals, for astrophysical applications. In particular we discuss the scientific motivat…

astro-ph2004★ 23 cited

INTEGRAL observations of the PSR B1259-63 / SS2883 system after the 2004 periastron passage

S. E. Shaw, M. Chernyakova, J. Rodriguez +3

The millisecond pulsar PSR B1259-63 and the Be star SS2883 are situated in a highly eccentric binary system, with orbital period ~3.4 years. We report on hard X-ray observations ob…

astro-ph2004★ 22 cited

The broad-band X-ray spectrum of the dipping Low Mass X-ray Binary EXO0748--676

Lara Sidoli, Arvind N. Parmar, Tim Oosterbroek

We present results of a 0.1-100 keV BeppoSAX observation of the dipping LMXRB EXO 0748-676 performed in 2000 November. During the observation the source exhibited X-ray eclipses, t…

astro-ph2004★ 51 cited

Phase-resolved spectroscopy of Geminga shows rotating hot spot(s)

P. A. Caraveo, A. De Luca, S. Mereghetti +2

Isolated neutron stars are seen in x-rays through their nonthermal and/or surface thermal emissions. XMM-Newton observations of the Geminga pulsar show a 43 electron volt spectrum…

astro-ph2004★ 22 cited

A first XMM-Newton look at the relativistic double pulsar PSR J0737-3039

A. Pellizzoni, A. De Luca, S. Mereghetti +5

We present the results of a 50 ks long X-ray observation of the relativistic double pulsar system PSR J0737-3039 obtained with the XMM-Newton satellite in March 2004. The source ha…

astro-ph2004★ 29 cited

Prompt and afterglow X-ray emission from the X-Ray Flash of 2002 April 27

L. Amati, F. Frontera, J. J. M. in 't Zand +15

We report on the X-ray observations of the X-ray flash (XRF) which occurred on 2002 April 27, three days before BeppoSAX was switched off. The event was detected with the BeppoSAX…

astro-ph2004★ 20 cited

ATLAS and SYNTHE under Linux

L. Sbordone, P. Bonifacio, F. Castelli +1

We have successfully ported under GNU Linux ATLAS 9, the widely used stellar atmosphere modeling code, as well as both the SYNTHE suite of programs, its ``companion'' for spectral…

astro-ph2004

Data Reduction and Analysis Graphical Organizer

L. Paioro, B. M. Garilli, M. Scodeggio +1

Spectroscopic surveys are undergoing a rapid expansion in their data collecting capabilities, reaching the level of hundreds of spectra per pointing. An efficient use of such huge…

astro-ph2004★ 373 cited

SN 2003lw and GRB 031203: A Bright Supernova for a Faint Gamma-ray Burst

D. Malesani, G. Tagliaferri, G. Chincarini +23

Optical and near-infrared observations of the gamma-ray burst GRB 031203, at z = 0.1055, are reported. A very faint afterglow is detected superimposed to the host galaxy in our fir…

astro-ph2004★ 2 cited

Clusters outskirts at X-ray wavelengths: current status and future prospects

Silvano Molendi

A solid observational characterization of cluster regions around the virial radius would allow us to improve considerably our understanding of the physics of galaxy clusters as a w…

astro-ph2004★ 48 cited

Broad band X-ray spectra of short bursts from SGR 1900+14

M. Feroci, G. A. Caliandro, E. Massaro +2

We report on the X-ray spectral properties of 10 short bursts from SGR1900+14 observed with the Narrow Field Instruments onboard BeppoSAX in the hours following the intermediate fl…

astro-ph2004★ 2 cited

The Intra-Cluster Medium

Silvano Molendi

The Intra-Cluster Medium (ICM) is a rarefied, hot, highly ionized, metal rich, weakly magnetized plasma. In these proceeding, after having reviewed some basic ICM properties, I dis…

astro-ph2004★ 51 cited

Pronounced long term flux variability of the Anomalous X-ray Pulsar 1E1048.1-5937

S. Mereghetti, A. Tiengo, L. Stella +4

We present XMM-Newton and Chandra observations of 1E1048.1-5937, being the first to show evidence for a significant variation in the X-ray luminosity of this Anomalous X-ray Pulsar…

astro-ph2004★ 52 cited

Radiative cooling, heating and thermal conduction in M87

Simona Ghizzardi, Silvano Molendi, Fabio Pizzolato +1

The crisis of the standard cooling flow model brought about by Chandra and XMM-Newton observations of galaxy clusters, has led to the development of several models which explore di…

astro-ph2004★ 32 cited

Spectral Evolution of weak bursts from SGR 1806-20 observed with INTEGRAL

D. Gotz, S. Mereghetti, I. F. Mirabel +1

We report on bursts from the Soft Gamma-Ray Repeater SGR 1806--20 detected with INTEGRAL in October 2003, during a period of moderate activity of the source. The spectral and tempo…

astro-ph2004★ 54 cited

Bias in the Estimation of Global Luminosity Functions

O. Ilbert, L. Tresse, S. Arnouts +13

We discuss a bias present in the calculation of the global luminosity function (LF) which occurs when analysing faint galaxy samples. This effect exists because of the different sp…

astro-ph2004★ 24 cited

Detecting the Attenuation of Blazar Gamma-ray Emission by Extragalactic Background Light with GLAST

Andrew Chen, Luis C. Reyes, Steven Ritz

Gamma rays with energy above 10 GeV interact with optical-UV photons resulting in pair production. Therefore, a large sample of high redshift sources of these gamma rays can be use…