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20032006
most citedHypernova Signatures in the Late Rebrightening of GRB 050525A

97 citations · 127 across the 5 of their papers we have counts for

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9 papers

astro-ph200697 cited

Hypernova Signatures in the Late Rebrightening of GRB 050525A

M. Della Valle, D. Malesani, J. S. Bloom +22

We report observations of GRB 050525A, for which a Gemini North spectrum shows its redshift to be z = 0.606. This is the third closest long GRB discovered by Swift. We observed its…

astro-ph200630 cited

Archeops In-flight Performance, Data Processing and Map Making

J. F. Macias-Perez, G. Lagache, B. Maffei +69

Archeops is a balloon--borne experiment widely inspired by the Planck satellite and by its High Frequency Instrument (HFI). It is mainly dedicated to measure the Cosmic Microwave B…

astro-ph2006

The frontier of darkness: the cases of GRB 040223, GRB 040422, GRB 040624

P. D'Avanzo, P. Filliatre, P. Goldoni +23

Understanding the reasons for the faintness of the optical/near-infrared afterglows of the so-called dark bursts is essential to assess whether they form a subclass of GRBs, and he…

astro-ph2005

Out of the darkness: the infrared afterglow of the INTEGRAL burst GRB 040422 observed with the VLT

P. Filliatre, P. D'Avanzo, S. Covino +15

GRB 040422 was detected by the INTEGRAL satellite at an angle of only 3 degrees from the Galactic plane. Analysis of the prompt emission observed with the SPI and IBIS instruments…

astro-ph2004

The CMB temperature power spectrum from an improved analysis of the Archeops data

M. Tristram, G. Patanchon, J. F. Macias-Perez +47

We present improved results on the measurement of the angular power spectrum of the Cosmic Microwave Background (CMB) temperature anisotropies using the data from the last Archeops…

astro-ph2004

The optical/NIR counterpart of the INTEGRAL obscured source IGR J16318-4848 : a sgB[e] in a HMXB ?

P. Filliatre, S. Chaty

The X-ray source IGR J16318-4848 was the first source discovered by INTEGRAL. The high energy spectrum exhibits such a high column density that the source is undetectable in X-rays…