The Search for the Afterglow of the Dark GRB 001109

Bibcode
2003AIPC..662..424C
DOI
10.1063/1.1579393
Castro Cerón, J. M.; Gorosabel, J.; Castro-Tirado, A. J.; Sokolov, V. V.; Afanasiev, V. L.; Fatkhullin, T. A.; Dodonov, S. N.; Komarova, V. N.; Cherepashchuk, A. M.; Postnov, K. A.; Greiner, J.; Klose, S.; Hjorth, J.; Pedersen, H.; Rol, E.; Fliri, J.; Feldt, M.; Feulner, G.; Andersen, M. I.; Jensen, B. L.; Vrba, F. J.; Henden, A. A.; Israelian, G.
Referencia bibliográfica

GAMMA-RAY BURST AND AFTERGLOW ASTRONOMY 2001: A Workshop Celebrating the First Year of the HETE Mission. AIP Conference Proceedings, Volume 662, pp. 424-427 (2003).

Fecha de publicación:
4
2003
Número de autores
23
Número de autores del IAC
1
Número de citas
1
Número de citas referidas
1
Descripción
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 wavelengths within this GRB's (Gamma Ray Burst) BeppoSAX 1' radius error box. Strong limits are set with K' > 20. A highly reddened galaxy, with variable radio emission, was found at z = 0.398. It is undergoing star formation, but seems to be unrelated to the event. We discuss the implications of these observations in the context of the dark GRB class.
Tipo
Sin árbitro
Fuentes de rayos gamma
Estallidos de rayos gamma

Te puede interesar

  • Sin árbitro
    New Robotic Telescope system progress towards critical design review
    The 4m class New Robotic Telescope (NRT) is an optical facility designed to revolutionize the rapid follow-up and classification of variable and transient objects. The project is at the stage where key systems are progressing through their detailed design phases, which presents a major engineering challenge for all project partners to manage design
    Copley, David et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13094E..3WC
    Número de citas
    0
  • Sin árbitro
    Phase diversity application on the EST MCAO testbench
    Phase Diversity (PD) is a technique widely used to measure and compensate for Non-Common Path Aberrations (NCPA) in optical systems. Beyond its traditional applications, PD has found further uses in solar astrophysics, where it enhances image quality by processing multiple images to correct residual aberrations. In this work, we introduce a
    Rodriguez-Linares, Nicolas et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13097E..5OR
    Número de citas
    0
  • Sin árbitro
    First light of the upgraded Gregor Infrared Spectrograph
    For more than ten years, the Gregor Infrared Spectrograph (GRIS) has been the infrared spectropolarimeter on the Gregor telescope since its inauguration in 2012. The instrument mainly performs polarimetric observations of the wavelength regions at 1083 and 1565nm, which have high scientific potential. There, observers can find spectral lines that
    Quintero Noda, C. et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13094E..42Q
    Número de citas
    0