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20042014
most citedFermi Large Area Telescope Bright Gamma-ray Source List

513 citations · 7.5k across the 53 of their papers we have counts for

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astro-ph2008

The Fermi Gamma Ray Space Telescope discovers the Pulsar in the Young Galactic Supernova-Remnant CTA 1

Fermi LAT Collaboration

Energetic young pulsars and expanding blast waves (supernova remnants, SNRs) are the most visible remains after massive stars, ending their lives, explode in core-collapse supernov…

astro-ph2008★ 15 cited

GRB 070707: the first short gamma-ray burst observed by INTEGRAL

S. McGlynn, S. Foley, S. McBreen +4

INTEGRAL has observed 47 long-duration GRBs (T_90 > 2s) and 1 short-duration GRB (T_90 < 2s) in five years of observation since October 2002. This work presents the properties of t…

astro-ph2008★ 54 cited

The Spectral Lag of GRB060505: A Likely Member of the Long Duration Class

S. McBreen, S. Foley, D. Watson +7

Two long gamma-ray bursts, GRB 060505 and GRB 060614, occurred in nearby galaxies at redshifts of 0.089 and 0.125 respectively. Due to their proximity and durations, deep follow-up…

astro-ph2008★ 44 cited

Global characteristics of GRBs observed with INTEGRAL and the inferred large population of low-luminosity GRBs

S. Foley, S. McGlynn, L. Hanlon +2

INTEGRAL has two sensitive gamma-ray instruments that have detected 46 gamma-ray bursts (GRBs) up to July 2007. We present the spectral, spatial, and temporal properties of the bur…

astro-ph2007★ 151 cited

Polarisation studies of the prompt gamma-ray emission from GRB 041219a using the Spectrometer aboard INTEGRAL

S. McGlynn, D. J. Clark, A. J. Dean +6

The spectrometer aboard INTEGRAL, SPI, has the capability to detect the signature of polarised emission from a bright gamma-ray source. GRB 041219a is the most intense burst locali…

astro-ph2006★ 38 cited

Observations of the intense and ultra-long burst GRB041219a with the Germanium Spectrometer on INTEGRAL

S. McBreen, L. Hanlon, S. McGlynn +5

GRB041219a is the brightest burst localised by INTEGRAL. The intense burst occurred about ~250s after the precursor and the long delay enabled optical and near infrared telescopes…