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DTSTART:20150329T010000
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DTSTART:20151025T010000
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DTSTART:20160327T010000
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DTSTART:20161030T010000
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DTSTART:20170326T010000
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DTSTART:20171029T010000
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DTSTART;TZID=Europe/Rome:20161011T114500
DTEND;TZID=Europe/Rome:20161011T124500
DTSTAMP:20260429T071717
CREATED:20160725T151446Z
LAST-MODIFIED:20160725T151446Z
UID:1336-1476186300-1476189900@www.oa-roma.inaf.it
SUMMARY:Gamma-ray busrts as probes of high redshift galaxies and their environments
DESCRIPTION:The launch of the Swift mission has revolutionised the study\nof the Gamma-Ray Bursts\, enabling the optical follow-up of the early afterglow.\nThanks to the fast broadcast of the GRB coordinates\nand to the rapid response mode systems built up in 8-meter class\ntelescopes\, these afterglows have be observed from hours down to a few\nminutes after the GRB explosion. The high signal-to noise achievable\nallows us to acquire medium-to-high resolution spectra\, which carry a lot of\ninformation both on the GRB environment and the Inter-Stellar Medium\nof high redshift galaxies. I will give a short review of what we have\nlearned through the medium-to-high resolution spectroscopy of GRB afterglows\,\nmainly with UVES and X-shooter at the VLT.
URL:https://www.oa-roma.inaf.it/event/gamma-ray-busrts-as-probes-of-high-redshift-galaxies-and-their-environments/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20161011T114500
DTEND;TZID=Europe/Rome:20161011T124500
DTSTAMP:20260429T071717
CREATED:20160725T151446Z
LAST-MODIFIED:20160725T151446Z
UID:4674-1476186300-1476189900@www.oa-roma.inaf.it
SUMMARY:Gamma-ray busrts as probes of high redshift galaxies and their environments
DESCRIPTION:The launch of the Swift mission has revolutionised the study\nof the Gamma-Ray Bursts\, enabling the optical follow-up of the early afterglow.\nThanks to the fast broadcast of the GRB coordinates\nand to the rapid response mode systems built up in 8-meter class\ntelescopes\, these afterglows have be observed from hours down to a few\nminutes after the GRB explosion. The high signal-to noise achievable\nallows us to acquire medium-to-high resolution spectra\, which carry a lot of\ninformation both on the GRB environment and the Inter-Stellar Medium\nof high redshift galaxies. I will give a short review of what we have\nlearned through the medium-to-high resolution spectroscopy of GRB afterglows\,\nmainly with UVES and X-shooter at the VLT.
URL:https://www.oa-roma.inaf.it/event/gamma-ray-busrts-as-probes-of-high-redshift-galaxies-and-their-environments-2/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
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