Loading…

The potential of INTEGRAL for the detection of high redshift GRBs

We discuss INTEGRAL's ability to detect a high redshift population of Gamma-Ray Bursts (GRBs) in comparison to other high-energy missions. Emphasis is placed on the study of the relative capabilities of IBIS on board INTEGRAL with respect to SWIFT and HETE 2 in detecting a high redshift populat...

Full description

Saved in:
Bibliographic Details
Published in:Astronomy and astrophysics (Berlin) 2004-11, Vol.427 (1), p.87-93
Main Authors: Gorosabel, J., Lund, N., Brandt, S., Westergaard, N. J., Castro Cerón, J. M.
Format: Article
Language:English
Subjects:
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c419t-ac3a2ee83d4ec184d8327bcb13beb485578839fdd016f78c81866e3ec12793bc3
cites cdi_FETCH-LOGICAL-c419t-ac3a2ee83d4ec184d8327bcb13beb485578839fdd016f78c81866e3ec12793bc3
container_end_page 93
container_issue 1
container_start_page 87
container_title Astronomy and astrophysics (Berlin)
container_volume 427
creator Gorosabel, J.
Lund, N.
Brandt, S.
Westergaard, N. J.
Castro Cerón, J. M.
description We discuss INTEGRAL's ability to detect a high redshift population of Gamma-Ray Bursts (GRBs) in comparison to other high-energy missions. Emphasis is placed on the study of the relative capabilities of IBIS on board INTEGRAL with respect to SWIFT and HETE 2 in detecting a high redshift population of GRBs. We conclude that, if the GRB rate is proportional to the star formation rate, INTEGRAL's ability to study GRBs are complementary to the ones of missions like SWIFT and HETE 2, devoted to prompt localisations of GRBs. Whereas SWIFT and HETE 2 would detect a higher number of GRBs than INTEGRAL, IBIS might be able to detect high redshift ($z \ga 7$) GRBs, unreachable by SWIFT and HETE 2. We discuss the relevance of performing near-infrared (NIR) observations of the INTEGRAL GRBs and the strategy that large-class telescopes might follow.
doi_str_mv 10.1051/0004-6361:20034493
format article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_28419744</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>28419744</sourcerecordid><originalsourceid>FETCH-LOGICAL-c419t-ac3a2ee83d4ec184d8327bcb13beb485578839fdd016f78c81866e3ec12793bc3</originalsourceid><addsrcrecordid>eNqFkMtOwzAQRS0EEqXwA6yygV3Ar9gOu1KVtFJ5qCqCneU4DjGkSbFdCf6eRC1lyWo0uufOSAeAcwSvEEzQNYSQxowwdIMhJJSm5AAMECU4hpyyQzDYA8fgxPv3bsVIkAEYLSsTrdtgmmBVHbVlNHtYTrLFaB6VrYtClxYmGB1s2_RpZd-qyJnCV7YMUba49afgqFS1N2e7OQTPd5PleBrPH7PZeDSPNUVpiJUmChsjSEGNRoIWgmCe6xyR3ORUJAkXgqRlUUDESi60QIIxQzoW85TkmgzB5fbu2rWfG-ODXFmvTV2rxrQbL7Ho_nBK_wVRSiHlogfxFtSu9d6ZUq6dXSn3LRGUvVbZW5O9NfmrtStd7K4rr1VdOtVo6_-aDOMEdeAQxFvO-mC-9rlyH5JxwhMp4IucZk_kfswz-Up-AHAFg-A</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>19404784</pqid></control><display><type>article</type><title>The potential of INTEGRAL for the detection of high redshift GRBs</title><source>EZB Electronic Journals Library</source><creator>Gorosabel, J. ; Lund, N. ; Brandt, S. ; Westergaard, N. J. ; Castro Cerón, J. M.</creator><creatorcontrib>Gorosabel, J. ; Lund, N. ; Brandt, S. ; Westergaard, N. J. ; Castro Cerón, J. M.</creatorcontrib><description>We discuss INTEGRAL's ability to detect a high redshift population of Gamma-Ray Bursts (GRBs) in comparison to other high-energy missions. Emphasis is placed on the study of the relative capabilities of IBIS on board INTEGRAL with respect to SWIFT and HETE 2 in detecting a high redshift population of GRBs. We conclude that, if the GRB rate is proportional to the star formation rate, INTEGRAL's ability to study GRBs are complementary to the ones of missions like SWIFT and HETE 2, devoted to prompt localisations of GRBs. Whereas SWIFT and HETE 2 would detect a higher number of GRBs than INTEGRAL, IBIS might be able to detect high redshift ($z \ga 7$) GRBs, unreachable by SWIFT and HETE 2. We discuss the relevance of performing near-infrared (NIR) observations of the INTEGRAL GRBs and the strategy that large-class telescopes might follow.</description><identifier>ISSN: 0004-6361</identifier><identifier>EISSN: 1432-0746</identifier><identifier>DOI: 10.1051/0004-6361:20034493</identifier><identifier>CODEN: AAEJAF</identifier><language>eng</language><publisher>Les Ulis: EDP Sciences</publisher><subject>gamma rays: bursts</subject><ispartof>Astronomy and astrophysics (Berlin), 2004-11, Vol.427 (1), p.87-93</ispartof><rights>2004 INIST-CNRS</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c419t-ac3a2ee83d4ec184d8327bcb13beb485578839fdd016f78c81866e3ec12793bc3</citedby><cites>FETCH-LOGICAL-c419t-ac3a2ee83d4ec184d8327bcb13beb485578839fdd016f78c81866e3ec12793bc3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,778,782,27911,27912</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&amp;idt=16225149$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Gorosabel, J.</creatorcontrib><creatorcontrib>Lund, N.</creatorcontrib><creatorcontrib>Brandt, S.</creatorcontrib><creatorcontrib>Westergaard, N. J.</creatorcontrib><creatorcontrib>Castro Cerón, J. M.</creatorcontrib><title>The potential of INTEGRAL for the detection of high redshift GRBs</title><title>Astronomy and astrophysics (Berlin)</title><description>We discuss INTEGRAL's ability to detect a high redshift population of Gamma-Ray Bursts (GRBs) in comparison to other high-energy missions. Emphasis is placed on the study of the relative capabilities of IBIS on board INTEGRAL with respect to SWIFT and HETE 2 in detecting a high redshift population of GRBs. We conclude that, if the GRB rate is proportional to the star formation rate, INTEGRAL's ability to study GRBs are complementary to the ones of missions like SWIFT and HETE 2, devoted to prompt localisations of GRBs. Whereas SWIFT and HETE 2 would detect a higher number of GRBs than INTEGRAL, IBIS might be able to detect high redshift ($z \ga 7$) GRBs, unreachable by SWIFT and HETE 2. We discuss the relevance of performing near-infrared (NIR) observations of the INTEGRAL GRBs and the strategy that large-class telescopes might follow.</description><subject>gamma rays: bursts</subject><issn>0004-6361</issn><issn>1432-0746</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2004</creationdate><recordtype>article</recordtype><recordid>eNqFkMtOwzAQRS0EEqXwA6yygV3Ar9gOu1KVtFJ5qCqCneU4DjGkSbFdCf6eRC1lyWo0uufOSAeAcwSvEEzQNYSQxowwdIMhJJSm5AAMECU4hpyyQzDYA8fgxPv3bsVIkAEYLSsTrdtgmmBVHbVlNHtYTrLFaB6VrYtClxYmGB1s2_RpZd-qyJnCV7YMUba49afgqFS1N2e7OQTPd5PleBrPH7PZeDSPNUVpiJUmChsjSEGNRoIWgmCe6xyR3ORUJAkXgqRlUUDESi60QIIxQzoW85TkmgzB5fbu2rWfG-ODXFmvTV2rxrQbL7Ho_nBK_wVRSiHlogfxFtSu9d6ZUq6dXSn3LRGUvVbZW5O9NfmrtStd7K4rr1VdOtVo6_-aDOMEdeAQxFvO-mC-9rlyH5JxwhMp4IucZk_kfswz-Up-AHAFg-A</recordid><startdate>20041101</startdate><enddate>20041101</enddate><creator>Gorosabel, J.</creator><creator>Lund, N.</creator><creator>Brandt, S.</creator><creator>Westergaard, N. J.</creator><creator>Castro Cerón, J. M.</creator><general>EDP Sciences</general><scope>BSCLL</scope><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20041101</creationdate><title>The potential of INTEGRAL for the detection of high redshift GRBs</title><author>Gorosabel, J. ; Lund, N. ; Brandt, S. ; Westergaard, N. J. ; Castro Cerón, J. M.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c419t-ac3a2ee83d4ec184d8327bcb13beb485578839fdd016f78c81866e3ec12793bc3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2004</creationdate><topic>gamma rays: bursts</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Gorosabel, J.</creatorcontrib><creatorcontrib>Lund, N.</creatorcontrib><creatorcontrib>Brandt, S.</creatorcontrib><creatorcontrib>Westergaard, N. J.</creatorcontrib><creatorcontrib>Castro Cerón, J. M.</creatorcontrib><collection>Istex</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Astronomy and astrophysics (Berlin)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Gorosabel, J.</au><au>Lund, N.</au><au>Brandt, S.</au><au>Westergaard, N. J.</au><au>Castro Cerón, J. M.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The potential of INTEGRAL for the detection of high redshift GRBs</atitle><jtitle>Astronomy and astrophysics (Berlin)</jtitle><date>2004-11-01</date><risdate>2004</risdate><volume>427</volume><issue>1</issue><spage>87</spage><epage>93</epage><pages>87-93</pages><issn>0004-6361</issn><eissn>1432-0746</eissn><coden>AAEJAF</coden><abstract>We discuss INTEGRAL's ability to detect a high redshift population of Gamma-Ray Bursts (GRBs) in comparison to other high-energy missions. Emphasis is placed on the study of the relative capabilities of IBIS on board INTEGRAL with respect to SWIFT and HETE 2 in detecting a high redshift population of GRBs. We conclude that, if the GRB rate is proportional to the star formation rate, INTEGRAL's ability to study GRBs are complementary to the ones of missions like SWIFT and HETE 2, devoted to prompt localisations of GRBs. Whereas SWIFT and HETE 2 would detect a higher number of GRBs than INTEGRAL, IBIS might be able to detect high redshift ($z \ga 7$) GRBs, unreachable by SWIFT and HETE 2. We discuss the relevance of performing near-infrared (NIR) observations of the INTEGRAL GRBs and the strategy that large-class telescopes might follow.</abstract><cop>Les Ulis</cop><pub>EDP Sciences</pub><doi>10.1051/0004-6361:20034493</doi><tpages>7</tpages><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 0004-6361
ispartof Astronomy and astrophysics (Berlin), 2004-11, Vol.427 (1), p.87-93
issn 0004-6361
1432-0746
language eng
recordid cdi_proquest_miscellaneous_28419744
source EZB Electronic Journals Library
subjects gamma rays: bursts
title The potential of INTEGRAL for the detection of high redshift GRBs
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-15T17%3A15%3A59IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=The%20potential%20of%20INTEGRAL%20for%20the%20detection%20of%20high%20redshift%20GRBs&rft.jtitle=Astronomy%20and%20astrophysics%20(Berlin)&rft.au=Gorosabel,%20J.&rft.date=2004-11-01&rft.volume=427&rft.issue=1&rft.spage=87&rft.epage=93&rft.pages=87-93&rft.issn=0004-6361&rft.eissn=1432-0746&rft.coden=AAEJAF&rft_id=info:doi/10.1051/0004-6361:20034493&rft_dat=%3Cproquest_cross%3E28419744%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c419t-ac3a2ee83d4ec184d8327bcb13beb485578839fdd016f78c81866e3ec12793bc3%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=19404784&rft_id=info:pmid/&rfr_iscdi=true