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gamma-ray observations
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INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) is a currently operational space telescope for observing gamma rays.
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GRB 970228 was the first gamma-ray burst (GRB) for which an afterglow was observed.
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With the advent of the space age, astronomers are now able to observe the entire electromagnetic spectrum, from radio waves to gamma rays.
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Since 1993, physicists had predicted GRBs to be followed by a lower-energy afterglow (in wavelengths such as radio waves, x-rays, and even visible light), but until this event, GRBs had only been observed in highly luminous bursts of high-energy gamma rays (the most energetic form of electromagnetic radiation); this resulted in large positional uncertainties which left their nature very unclear.
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VLT Observations of Gamma-ray Burst Reveal Surprising Ingredients of Early Galaxies | ESO Australia
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VLT Observations of Gamma-ray Burst Reveal Surprising Ingredients of Early Galaxies | ESO Shqipëria
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VLT Observations of Gamma-ray Burst Reveal Surprising Ingredients of Early Galaxies
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VLT Observations of Gamma-ray Burst Reveal Surprising Ingredients of Early Galaxies | ESO
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It now performs follow-up observations of gamma-ray bursts, some of the most energetic events in the Universe.
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The MPG/ESO 2.2-metre telescope observed using the Gamma-Ray burst Optical/Near-infrared Detector (GROND) instrument.
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In the new study, astronomers combined Swift data with new observations made using GROND [2] — a dedicated gamma-ray burst follow-up observation instrument, which is attached to the 2.2-metre MPG/ESO telescope at La Silla in Chile.
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Gamma-ray bursts (GRBs) are intense bursts of extremely high energy observed in distant galaxies — the brightest explosive phenomenon in the Universe.
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This will allow the world's most ambitious gamma-ray observatory to access not only Chile’s pristine observing conditions, but also ESO’s state-of-the-art infrastructure, expertise, and facilities.
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However, the Earth’s atmosphere prevents gamma rays from reaching its surface, so rather than hunting for these rays directly the CTA will observe something known as Cherenkov radiation — ghostly blue flashes of light produced when gamma rays interact with particles in our atmosphere.
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Early this year, astronomers used the Subaru Telescope to observe a single gamma-ray burst, from which they hypothesised that dark gamma-ray bursts may indeed be a separate sub-class that form through a different mechanism, such as the merger of binary stars.
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The VLT observations show that the brilliant light from the gamma-ray burst had passed through its own host galaxy and another galaxy nearby.
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On 27 October 2015, at 22:40 GMT, the NASA/ASI/UKSA Swift satellite discovered its 1000th gamma-ray burst (GRB). This landmark event was subsequently observed and characterised by ESO telescopes at the La Silla Paranal Observatory in northern Chile, which revealed that this GRB was an especially interesting object.
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In any case, these ALMA observations support the hypothesis that it is dust that absorbs the afterglow radiation, causing the dark gamma-ray bursts.
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The almost simultaneous detections of both gravitational waves and gamma rays from GW170817 raised hopes that this object was indeed a long-sought kilonova and observations with ESO facilities have revealed properties remarkably close to theoretical predictions.
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The VLT has stimulated a new age of discoveries, with several notable scientific firsts, including the first image of an extrasolar planet (eso0428), tracking individual stars moving around the supermassive black hole at the centre of the Milky Way (eso0846), and observing the afterglow of the furthest known Gamma-Ray Burst. More about Science with the VLT
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08 Korrik 2015: Observations from ESO’s La Silla and Paranal Observatories in Chile have for the first time demonstrated a link between a very long-lasting burst of gamma rays and an unusually bright supernova explosion.
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08/07/2015: Observations from ESO’s La Silla and Paranal Observatories in Chile have for the first time demonstrated a link between a very long-lasting burst of gamma rays and an unusually bright supernova explosion.
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8 July 2015: Observations from ESO’s La Silla and Paranal Observatories in Chile have for the first time demonstrated a link between a very long-lasting burst of gamma rays and an unusually bright supernova explosion.
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The new observations of the rapid changes in the gamma radiation give strong support to the models that place the source close to the black holes and help us to understand the mechanisms of gamma ray production, says Poutanen.
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