A new era of sub-millimeter GRB afterglow follow-ups with the Greenland Telescope

A planned rapid submillimeter (submm) Gamma Ray Burst (GRBs) follow-up observations conducted using the Greenland Telescope (GLT) is presented. The GLT is a 12-m submm telescope to be located at the top of the Greenland ice sheet, where the high-altitude and dry weather porvides excellent conditions...

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Main Authors: Urata, Yuji, Huang, Kuiyun, Asada, Keiichi, Hirashita, Hiroyuki, Inoue, Makoto, Ho, Paul T. P.
Format: Text
Language:unknown
Published: arXiv 2015
Subjects:
High Energy Astrophysical Phenomena astro-ph.HE
FOS Physical sciences
Greenland
Greenland Telescope
Ice Sheet
Online Access:https://dx.doi.org/10.48550/arxiv.1503.07594
https://arxiv.org/abs/1503.07594
id ftdatacite:10.48550/arxiv.1503.07594
record_format openpolar
spelling ftdatacite:10.48550/arxiv.1503.07594 2023-05-15T16:26:53+02:00 A new era of sub-millimeter GRB afterglow follow-ups with the Greenland Telescope Urata, Yuji Huang, Kuiyun Asada, Keiichi Hirashita, Hiroyuki Inoue, Makoto Ho, Paul T. P. 2015 https://dx.doi.org/10.48550/arxiv.1503.07594 https://arxiv.org/abs/1503.07594 unknown arXiv https://dx.doi.org/10.1155/2015/165030 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences article-journal Article ScholarlyArticle Text 2015 ftdatacite https://doi.org/10.48550/arxiv.1503.07594 https://doi.org/10.1155/2015/165030 2022-04-01T12:19:25Z A planned rapid submillimeter (submm) Gamma Ray Burst (GRBs) follow-up observations conducted using the Greenland Telescope (GLT) is presented. The GLT is a 12-m submm telescope to be located at the top of the Greenland ice sheet, where the high-altitude and dry weather porvides excellent conditions for observations at submm wavelengths. With its combination of wavelength window and rapid responding system, the GLT will explore new insights on GRBs. Summarizing the current achievements of submm GRB follow-ups, we identify the following three scientific goals regarding GRBs: (1) systematic detection of bright submm emissions originating from reverse shock (RS) in the early afterglow phase, (2) characterization of forward shock and RS emissions by capturing their peak flux and frequencies and performing continuous monitoring, and (3) detections of GRBs as a result of the explosion of first-generation stars result of GRBs at a high redshift through systematic rapid follow ups. The light curves and spectra calculated by available theoretical models clearly show that the GLT could play a crucial role in these studies. : 10 pages, 9 figures (emulateapj), accepted for publication in Advances in Astronomy GRB special issue Text Greenland Greenland Telescope Ice Sheet DataCite Metadata Store (German National Library of Science and Technology) Greenland
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic High Energy Astrophysical Phenomena astro-ph.HE
FOS Physical sciences
spellingShingle High Energy Astrophysical Phenomena astro-ph.HE
FOS Physical sciences
Urata, Yuji
Huang, Kuiyun
Asada, Keiichi
Hirashita, Hiroyuki
Inoue, Makoto
Ho, Paul T. P.
A new era of sub-millimeter GRB afterglow follow-ups with the Greenland Telescope
topic_facet High Energy Astrophysical Phenomena astro-ph.HE
FOS Physical sciences
description A planned rapid submillimeter (submm) Gamma Ray Burst (GRBs) follow-up observations conducted using the Greenland Telescope (GLT) is presented. The GLT is a 12-m submm telescope to be located at the top of the Greenland ice sheet, where the high-altitude and dry weather porvides excellent conditions for observations at submm wavelengths. With its combination of wavelength window and rapid responding system, the GLT will explore new insights on GRBs. Summarizing the current achievements of submm GRB follow-ups, we identify the following three scientific goals regarding GRBs: (1) systematic detection of bright submm emissions originating from reverse shock (RS) in the early afterglow phase, (2) characterization of forward shock and RS emissions by capturing their peak flux and frequencies and performing continuous monitoring, and (3) detections of GRBs as a result of the explosion of first-generation stars result of GRBs at a high redshift through systematic rapid follow ups. The light curves and spectra calculated by available theoretical models clearly show that the GLT could play a crucial role in these studies. : 10 pages, 9 figures (emulateapj), accepted for publication in Advances in Astronomy GRB special issue
format Text
author Urata, Yuji
Huang, Kuiyun
Asada, Keiichi
Hirashita, Hiroyuki
Inoue, Makoto
Ho, Paul T. P.
author_facet Urata, Yuji
Huang, Kuiyun
Asada, Keiichi
Hirashita, Hiroyuki
Inoue, Makoto
Ho, Paul T. P.
author_sort Urata, Yuji
title A new era of sub-millimeter GRB afterglow follow-ups with the Greenland Telescope
title_short A new era of sub-millimeter GRB afterglow follow-ups with the Greenland Telescope
title_full A new era of sub-millimeter GRB afterglow follow-ups with the Greenland Telescope
title_fullStr A new era of sub-millimeter GRB afterglow follow-ups with the Greenland Telescope
title_full_unstemmed A new era of sub-millimeter GRB afterglow follow-ups with the Greenland Telescope
title_sort new era of sub-millimeter grb afterglow follow-ups with the greenland telescope
publisher arXiv
publishDate 2015
url https://dx.doi.org/10.48550/arxiv.1503.07594
https://arxiv.org/abs/1503.07594
geographic Greenland
geographic_facet Greenland
genre Greenland
Greenland Telescope
Ice Sheet
genre_facet Greenland
Greenland Telescope
Ice Sheet
op_relation https://dx.doi.org/10.1155/2015/165030
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.1503.07594
https://doi.org/10.1155/2015/165030
_version_ 1766015878818693120

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