THREE YEARS OF FERMI GBM EARTH OCCULTATION MONITORING: OBSERVATIONS OF HARD X-RAY/SOFT GAMMA-RAY SOURCES

The Gamma-ray Burst Monitor (GBM) on board Fermi has been providing continuous data to the astronomical community since 2008 August 12. In this paper, we present the results of the analysis of the first three years of these continuous data using the Earth occultation technique to monitor a catalog o...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:The Astrophysical journal. Supplement series 2012-08, Vol.201 (2), p.1-22
Hauptverfasser: Wilson-Hodge, Colleen A, Case, Gary L, Cherry, Michael L, Rodi, James, Camero-Arranz, Ascension, Jenke, Peter, CHAPLIN, VANDIVER, BEKLEN, ELIF, Finger, Mark, Bhat, Narayan
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 22
container_issue 2
container_start_page 1
container_title The Astrophysical journal. Supplement series
container_volume 201
creator Wilson-Hodge, Colleen A
Case, Gary L
Cherry, Michael L
Rodi, James
Camero-Arranz, Ascension
Jenke, Peter
CHAPLIN, VANDIVER
BEKLEN, ELIF
Finger, Mark
Bhat, Narayan
description The Gamma-ray Burst Monitor (GBM) on board Fermi has been providing continuous data to the astronomical community since 2008 August 12. In this paper, we present the results of the analysis of the first three years of these continuous data using the Earth occultation technique to monitor a catalog of 209 sources. From this catalog, we detect 99 sources, including 40 low-mass X-ray binary/neutron star systems, 31 high-mass X-ray binary/neutron star systems, 12 black hole binaries, 12 active galaxies, and 2 other sources, plus the Crab Nebula, and the Sun. Nine of these sources are detected in the 100-300 keV band, including seven black hole binaries, the active galaxy Cen A, and the Crab. The Crab and Cyg X-1 are also detected in the 300-500 keV band. GBM provides complementary data to other sky-monitors below 100 keV and is the only all-sky monitor above 100 keV. Up-to-date light curves for all of the catalog sources can be found online.
doi_str_mv 10.1088/0067-0049/201/2/33
format Article
fullrecord <record><control><sourceid>proquest_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_22047592</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1678014355</sourcerecordid><originalsourceid>FETCH-LOGICAL-c385t-b172a7b48759c2fc1fcbec5e1cbcbfa03a09e6c811053b37049c0d9d9a862fe33</originalsourceid><addsrcrecordid>eNqNkU1PwkAQhjdGExH9A5428eKldna32w9vpRZoQtmkLUZOm3bZBgxQ7JaD_94CxrOnybx55k0mD0KPBF4I-L4N4HoWgBPYFIhNbcau0IBw5lsOc_k1GvwBt-jOmE8A8DgLBmhdTLM4xss4zHIsxngcZ2mCJ6MU90kxxSKKFrMiLBIxx6mYJ4XIkvnkFYtRHmfv5_x8Nw2zN_xhZeHSzsW4wJMwTcPTinOxyKI4v0c3dbk1-uF3DtFiHBfR1JqJSRKFM0sxn3dWRTxaepXjezxQtFakVpVWXBNVqaougZUQaFf5hABnFfP6jxSsglVQ-i6tNWND9HTpbUy3kUZtOq3WqtnvteokpeD0xbSnni_UoW2-jtp0crcxSm-35V43RyOJ6_lAHMb5P1BCXOZAEPQovaCqbYxpdS0P7WZXtt-SgDx5kicN8qRB9p4klYyxH0_he3E</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1611634099</pqid></control><display><type>article</type><title>THREE YEARS OF FERMI GBM EARTH OCCULTATION MONITORING: OBSERVATIONS OF HARD X-RAY/SOFT GAMMA-RAY SOURCES</title><source>Institute of Physics Open Access Journal Titles</source><source>Institute of Physics IOPscience extra</source><source>EZB-FREE-00999 freely available EZB journals</source><source>Alma/SFX Local Collection</source><creator>Wilson-Hodge, Colleen A ; Case, Gary L ; Cherry, Michael L ; Rodi, James ; Camero-Arranz, Ascension ; Jenke, Peter ; CHAPLIN, VANDIVER ; BEKLEN, ELIF ; Finger, Mark ; Bhat, Narayan</creator><creatorcontrib>Wilson-Hodge, Colleen A ; Case, Gary L ; Cherry, Michael L ; Rodi, James ; Camero-Arranz, Ascension ; Jenke, Peter ; CHAPLIN, VANDIVER ; BEKLEN, ELIF ; Finger, Mark ; Bhat, Narayan</creatorcontrib><description>The Gamma-ray Burst Monitor (GBM) on board Fermi has been providing continuous data to the astronomical community since 2008 August 12. In this paper, we present the results of the analysis of the first three years of these continuous data using the Earth occultation technique to monitor a catalog of 209 sources. From this catalog, we detect 99 sources, including 40 low-mass X-ray binary/neutron star systems, 31 high-mass X-ray binary/neutron star systems, 12 black hole binaries, 12 active galaxies, and 2 other sources, plus the Crab Nebula, and the Sun. Nine of these sources are detected in the 100-300 keV band, including seven black hole binaries, the active galaxy Cen A, and the Crab. The Crab and Cyg X-1 are also detected in the 300-500 keV band. GBM provides complementary data to other sky-monitors below 100 keV and is the only all-sky monitor above 100 keV. Up-to-date light curves for all of the catalog sources can be found online.</description><identifier>ISSN: 0067-0049</identifier><identifier>EISSN: 1538-4365</identifier><identifier>DOI: 10.1088/0067-0049/201/2/33</identifier><language>eng</language><publisher>United States</publisher><subject>Active galaxies ; ASTROPHYSICS ; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; BINARY STARS ; Binary systems ; BLACK HOLES ; COSMIC GAMMA BURSTS ; COSMIC X-RAY SOURCES ; CRAB NEBULA ; Crabs ; DATA ANALYSIS ; Earth ; ECLIPSE ; GALAXIES ; GAMMA ASTRONOMY ; HARD X RADIATION ; KEV RANGE ; Monitors ; NEUTRON STARS ; Occultation ; X-rays</subject><ispartof>The Astrophysical journal. Supplement series, 2012-08, Vol.201 (2), p.1-22</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c385t-b172a7b48759c2fc1fcbec5e1cbcbfa03a09e6c811053b37049c0d9d9a862fe33</citedby><cites>FETCH-LOGICAL-c385t-b172a7b48759c2fc1fcbec5e1cbcbfa03a09e6c811053b37049c0d9d9a862fe33</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,780,784,885,27924,27925</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/22047592$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Wilson-Hodge, Colleen A</creatorcontrib><creatorcontrib>Case, Gary L</creatorcontrib><creatorcontrib>Cherry, Michael L</creatorcontrib><creatorcontrib>Rodi, James</creatorcontrib><creatorcontrib>Camero-Arranz, Ascension</creatorcontrib><creatorcontrib>Jenke, Peter</creatorcontrib><creatorcontrib>CHAPLIN, VANDIVER</creatorcontrib><creatorcontrib>BEKLEN, ELIF</creatorcontrib><creatorcontrib>Finger, Mark</creatorcontrib><creatorcontrib>Bhat, Narayan</creatorcontrib><title>THREE YEARS OF FERMI GBM EARTH OCCULTATION MONITORING: OBSERVATIONS OF HARD X-RAY/SOFT GAMMA-RAY SOURCES</title><title>The Astrophysical journal. Supplement series</title><description>The Gamma-ray Burst Monitor (GBM) on board Fermi has been providing continuous data to the astronomical community since 2008 August 12. In this paper, we present the results of the analysis of the first three years of these continuous data using the Earth occultation technique to monitor a catalog of 209 sources. From this catalog, we detect 99 sources, including 40 low-mass X-ray binary/neutron star systems, 31 high-mass X-ray binary/neutron star systems, 12 black hole binaries, 12 active galaxies, and 2 other sources, plus the Crab Nebula, and the Sun. Nine of these sources are detected in the 100-300 keV band, including seven black hole binaries, the active galaxy Cen A, and the Crab. The Crab and Cyg X-1 are also detected in the 300-500 keV band. GBM provides complementary data to other sky-monitors below 100 keV and is the only all-sky monitor above 100 keV. Up-to-date light curves for all of the catalog sources can be found online.</description><subject>Active galaxies</subject><subject>ASTROPHYSICS</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>BINARY STARS</subject><subject>Binary systems</subject><subject>BLACK HOLES</subject><subject>COSMIC GAMMA BURSTS</subject><subject>COSMIC X-RAY SOURCES</subject><subject>CRAB NEBULA</subject><subject>Crabs</subject><subject>DATA ANALYSIS</subject><subject>Earth</subject><subject>ECLIPSE</subject><subject>GALAXIES</subject><subject>GAMMA ASTRONOMY</subject><subject>HARD X RADIATION</subject><subject>KEV RANGE</subject><subject>Monitors</subject><subject>NEUTRON STARS</subject><subject>Occultation</subject><subject>X-rays</subject><issn>0067-0049</issn><issn>1538-4365</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2012</creationdate><recordtype>article</recordtype><recordid>eNqNkU1PwkAQhjdGExH9A5428eKldna32w9vpRZoQtmkLUZOm3bZBgxQ7JaD_94CxrOnybx55k0mD0KPBF4I-L4N4HoWgBPYFIhNbcau0IBw5lsOc_k1GvwBt-jOmE8A8DgLBmhdTLM4xss4zHIsxngcZ2mCJ6MU90kxxSKKFrMiLBIxx6mYJ4XIkvnkFYtRHmfv5_x8Nw2zN_xhZeHSzsW4wJMwTcPTinOxyKI4v0c3dbk1-uF3DtFiHBfR1JqJSRKFM0sxn3dWRTxaepXjezxQtFakVpVWXBNVqaougZUQaFf5hABnFfP6jxSsglVQ-i6tNWND9HTpbUy3kUZtOq3WqtnvteokpeD0xbSnni_UoW2-jtp0crcxSm-35V43RyOJ6_lAHMb5P1BCXOZAEPQovaCqbYxpdS0P7WZXtt-SgDx5kicN8qRB9p4klYyxH0_he3E</recordid><startdate>20120801</startdate><enddate>20120801</enddate><creator>Wilson-Hodge, Colleen A</creator><creator>Case, Gary L</creator><creator>Cherry, Michael L</creator><creator>Rodi, James</creator><creator>Camero-Arranz, Ascension</creator><creator>Jenke, Peter</creator><creator>CHAPLIN, VANDIVER</creator><creator>BEKLEN, ELIF</creator><creator>Finger, Mark</creator><creator>Bhat, Narayan</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>20120801</creationdate><title>THREE YEARS OF FERMI GBM EARTH OCCULTATION MONITORING: OBSERVATIONS OF HARD X-RAY/SOFT GAMMA-RAY SOURCES</title><author>Wilson-Hodge, Colleen A ; Case, Gary L ; Cherry, Michael L ; Rodi, James ; Camero-Arranz, Ascension ; Jenke, Peter ; CHAPLIN, VANDIVER ; BEKLEN, ELIF ; Finger, Mark ; Bhat, Narayan</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c385t-b172a7b48759c2fc1fcbec5e1cbcbfa03a09e6c811053b37049c0d9d9a862fe33</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2012</creationdate><topic>Active galaxies</topic><topic>ASTROPHYSICS</topic><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>BINARY STARS</topic><topic>Binary systems</topic><topic>BLACK HOLES</topic><topic>COSMIC GAMMA BURSTS</topic><topic>COSMIC X-RAY SOURCES</topic><topic>CRAB NEBULA</topic><topic>Crabs</topic><topic>DATA ANALYSIS</topic><topic>Earth</topic><topic>ECLIPSE</topic><topic>GALAXIES</topic><topic>GAMMA ASTRONOMY</topic><topic>HARD X RADIATION</topic><topic>KEV RANGE</topic><topic>Monitors</topic><topic>NEUTRON STARS</topic><topic>Occultation</topic><topic>X-rays</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Wilson-Hodge, Colleen A</creatorcontrib><creatorcontrib>Case, Gary L</creatorcontrib><creatorcontrib>Cherry, Michael L</creatorcontrib><creatorcontrib>Rodi, James</creatorcontrib><creatorcontrib>Camero-Arranz, Ascension</creatorcontrib><creatorcontrib>Jenke, Peter</creatorcontrib><creatorcontrib>CHAPLIN, VANDIVER</creatorcontrib><creatorcontrib>BEKLEN, ELIF</creatorcontrib><creatorcontrib>Finger, Mark</creatorcontrib><creatorcontrib>Bhat, Narayan</creatorcontrib><collection>CrossRef</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV</collection><jtitle>The Astrophysical journal. Supplement series</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Wilson-Hodge, Colleen A</au><au>Case, Gary L</au><au>Cherry, Michael L</au><au>Rodi, James</au><au>Camero-Arranz, Ascension</au><au>Jenke, Peter</au><au>CHAPLIN, VANDIVER</au><au>BEKLEN, ELIF</au><au>Finger, Mark</au><au>Bhat, Narayan</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>THREE YEARS OF FERMI GBM EARTH OCCULTATION MONITORING: OBSERVATIONS OF HARD X-RAY/SOFT GAMMA-RAY SOURCES</atitle><jtitle>The Astrophysical journal. Supplement series</jtitle><date>2012-08-01</date><risdate>2012</risdate><volume>201</volume><issue>2</issue><spage>1</spage><epage>22</epage><pages>1-22</pages><issn>0067-0049</issn><eissn>1538-4365</eissn><abstract>The Gamma-ray Burst Monitor (GBM) on board Fermi has been providing continuous data to the astronomical community since 2008 August 12. In this paper, we present the results of the analysis of the first three years of these continuous data using the Earth occultation technique to monitor a catalog of 209 sources. From this catalog, we detect 99 sources, including 40 low-mass X-ray binary/neutron star systems, 31 high-mass X-ray binary/neutron star systems, 12 black hole binaries, 12 active galaxies, and 2 other sources, plus the Crab Nebula, and the Sun. Nine of these sources are detected in the 100-300 keV band, including seven black hole binaries, the active galaxy Cen A, and the Crab. The Crab and Cyg X-1 are also detected in the 300-500 keV band. GBM provides complementary data to other sky-monitors below 100 keV and is the only all-sky monitor above 100 keV. Up-to-date light curves for all of the catalog sources can be found online.</abstract><cop>United States</cop><doi>10.1088/0067-0049/201/2/33</doi><tpages>22</tpages><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 0067-0049
ispartof The Astrophysical journal. Supplement series, 2012-08, Vol.201 (2), p.1-22
issn 0067-0049
1538-4365
language eng
recordid cdi_osti_scitechconnect_22047592
source Institute of Physics Open Access Journal Titles; Institute of Physics IOPscience extra; EZB-FREE-00999 freely available EZB journals; Alma/SFX Local Collection
subjects Active galaxies
ASTROPHYSICS
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
BINARY STARS
Binary systems
BLACK HOLES
COSMIC GAMMA BURSTS
COSMIC X-RAY SOURCES
CRAB NEBULA
Crabs
DATA ANALYSIS
Earth
ECLIPSE
GALAXIES
GAMMA ASTRONOMY
HARD X RADIATION
KEV RANGE
Monitors
NEUTRON STARS
Occultation
X-rays
title THREE YEARS OF FERMI GBM EARTH OCCULTATION MONITORING: OBSERVATIONS OF HARD X-RAY/SOFT GAMMA-RAY SOURCES
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-24T22%3A07%3A01IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=THREE%20YEARS%20OF%20FERMI%20GBM%20EARTH%20OCCULTATION%20MONITORING:%20OBSERVATIONS%20OF%20HARD%20X-RAY/SOFT%20GAMMA-RAY%20SOURCES&rft.jtitle=The%20Astrophysical%20journal.%20Supplement%20series&rft.au=Wilson-Hodge,%20Colleen%20A&rft.date=2012-08-01&rft.volume=201&rft.issue=2&rft.spage=1&rft.epage=22&rft.pages=1-22&rft.issn=0067-0049&rft.eissn=1538-4365&rft_id=info:doi/10.1088/0067-0049/201/2/33&rft_dat=%3Cproquest_osti_%3E1678014355%3C/proquest_osti_%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1611634099&rft_id=info:pmid/&rfr_iscdi=true