Astrophysical: Gamma-ray bursts

  • Publication
    The cooling tail of a long X-ray burst from XTE J1701-407
    Swift XRT observed the recently discovered source XTE J1701-407 (Markwardt et al., ATel #1569, Degenaar et al., ATel #1572) on July 17th, 2008 at UT 13:31:45...
  • Publication
    The Einstein Probe Transient EP240414a: Linking Fast X-Ray Transients, Gamma-Ray Bursts, and Luminous Fast Blue Optical Transients
    Detections of fast X-ray transients (FXTs) have accrued over the last few decades. However, their origin has remained mysterious. Rapid progress is now being...
  • Publication
    The Epeakrest E correlation in GRBs in the BATSE catalog
    The energy emission involved in a Gamma-Ray Burst evidently can be estimated only provided that we know the distance to the source. The same is true for the...
  • Publication
    The GRB 030227 Detected by INTEGRAL: Another Sign of Compton Scattering in X-rays
    Multiwavelengthp observations of a GRB detected by INTEGRAL (GRB 030227) revealed a dim optical afterglow (OA) that would not have been detected by many...
  • News
    The IAC hosts an international meeting to advance the design and construction of the New Robotic Telescope
    On 27 and 28 November, the Instituto de Astrofísica de Canarias (IAC) hosted a meeting between representatives of the partner institutions of the New Robotic...
  • Publication
    The Kangaroo's First Hop: The Early Fast Cooling Phase of EP250108a/SN 2025kg
    Fast X-ray transients are a rare and poorly understood population of events. Previously difficult to detect in real time, the launch of the Einstein Probe with...
  • Publication
    The latest two GRB detected by Hete-2: GRB 051022 and GRB 051028
    We present multiwavelength observations of the latest two GRB detected by Hete-2 in 2005. For GRB 051022, no optical/nIR afterglow has been detected, in spite...
  • Publication
    The Search for the Afterglow of the Dark GRB 001109
    We present optical and near IR follow up observations of the dark GRB 001109, 1-300 days after the event. No transient emission has been found for these...
  • Publication
    The Swift Gamma-Ray Burst Mission
    Swift is a first-of-its-kind multiwavelength transient observatory for GRB astronomy. It has the optimum capabilities for the next breakthroughs in determining...