CORRELATION BETWEEN HARDNESS RATIO AND DURATION OF FERMI GAMMA-RAY BURSTS
Using the latest gamma-ray bursts (GRB) observed by Fermi-GBM, we perform a statistical analysis of the relation between hardness ratio (HR) and duration (ΔT) of GRBs, and find that HR and ΔT are still anti-correlated. we also find that this correlation strongly depends upon the spectral shape of GR...
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Veröffentlicht in: | International journal of modern physics. Conference series 2013, Vol.23, p.298-300 |
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description | Using the latest gamma-ray bursts (GRB) observed by Fermi-GBM, we perform a statistical analysis of the relation between hardness ratio (HR) and duration (ΔT) of GRBs, and find that HR and ΔT are still anti-correlated. we also find that this correlation strongly depends upon the spectral shape of GRBs and energy bands, and the bursts with the curved spectra in the typical BATSE energy bands show a tighter anti-correlation than those with the power-law spectra in the typical BAT energy bands. This might explain why the HR – ΔT correlation is not evident for Swift-BAT GRB sample as well as other GRB sample detected by instruments with a narrower/softer energy bandpass such as HETE-2. |
doi_str_mv | 10.1142/S2010194513011501 |
format | Article |
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Conference series</title><description>Using the latest gamma-ray bursts (GRB) observed by Fermi-GBM, we perform a statistical analysis of the relation between hardness ratio (HR) and duration (ΔT) of GRBs, and find that HR and ΔT are still anti-correlated. we also find that this correlation strongly depends upon the spectral shape of GRBs and energy bands, and the bursts with the curved spectra in the typical BATSE energy bands show a tighter anti-correlation than those with the power-law spectra in the typical BAT energy bands. This might explain why the HR – ΔT correlation is not evident for Swift-BAT GRB sample as well as other GRB sample detected by instruments with a narrower/softer energy bandpass such as HETE-2.</description><subject>Bandpass</subject><subject>Correlation</subject><subject>Energy bands</subject><subject>Gamma ray bursts</subject><subject>Gamma rays</subject><subject>Statistical analysis</subject><issn>2010-1945</issn><issn>2010-1945</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><recordid>eNplkEFrg0AQhZfSQkObH9DbQs-2O7rD6tEkm0RIFFZD6UncVcGQxnRNKP33VSylkNMbHu-bYR4hT8BeALj7mroMGAQcwWMAyOCGTAbLGbzbf_M9mXbdnjEGvvAD5BMSzROl5CbMoiSmM5m9SRnTdagWsUxTqgafhvGCLnZqzCRLupRqG9FVuN2Gjgrf6Wyn0ix9JHd1ceiq6a8-kN1SZvO1s0lW0TzcOAaQgwN1wLA0RruiKH2hhQtG6MIX6Je1qQpda3Q5x8p4TPQqkAmhdVmKABCRew_kedx7su3nperO-b692GN_Mnf731EAetinYEwZ23adrer8ZJuPwn7nwPKhtPyqtJ5hI_PV2kPZmaY6npu6MX_oNfIDtqJlsw</recordid><startdate>2013</startdate><enddate>2013</enddate><creator>ZHANG, FU-WEN</creator><general>World Scientific Publishing Company</general><general>World Scientific Publishing Co. Pte., Ltd</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>2013</creationdate><title>CORRELATION BETWEEN HARDNESS RATIO AND DURATION OF FERMI GAMMA-RAY BURSTS</title><author>ZHANG, FU-WEN</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c1541-1f905dccb27ad87b721c7ba8758dfceabfb52445ec30744575077bbdd79155543</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Bandpass</topic><topic>Correlation</topic><topic>Energy bands</topic><topic>Gamma ray bursts</topic><topic>Gamma rays</topic><topic>Statistical analysis</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>ZHANG, FU-WEN</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>International journal of modern physics. 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Conference series</jtitle><date>2013</date><risdate>2013</risdate><volume>23</volume><spage>298</spage><epage>300</epage><pages>298-300</pages><issn>2010-1945</issn><eissn>2010-1945</eissn><abstract>Using the latest gamma-ray bursts (GRB) observed by Fermi-GBM, we perform a statistical analysis of the relation between hardness ratio (HR) and duration (ΔT) of GRBs, and find that HR and ΔT are still anti-correlated. we also find that this correlation strongly depends upon the spectral shape of GRBs and energy bands, and the bursts with the curved spectra in the typical BATSE energy bands show a tighter anti-correlation than those with the power-law spectra in the typical BAT energy bands. 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subjects | Bandpass Correlation Energy bands Gamma ray bursts Gamma rays Statistical analysis |
title | CORRELATION BETWEEN HARDNESS RATIO AND DURATION OF FERMI GAMMA-RAY BURSTS |
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