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Galactic survey of Ti-44 sources with the IBIS telescope onboard INTEGRAL
Tekijät: Tsygankov SS, Krivonos RA, Lutovinov AA, Revnivtsev MG, Churazov EM, Sunyaev RA, Grebenev SA
Kustantaja: OXFORD UNIV PRESS
Julkaisuvuosi: 2016
Journal: Monthly Notices of the Royal Astronomical Society
Tietokannassa oleva lehden nimi: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Lehden akronyymi: MON NOT R ASTRON SOC
Vuosikerta: 458
Numero: 4
Aloitussivu: 3411
Lopetussivu: 3419
Sivujen määrä: 9
ISSN: 0035-8711
eISSN: 1365-2966
DOI: https://doi.org/10.1093/mnras/stw549
Tiivistelmä
We report the results of the deepest Galactic plane (vertical bar b vertical bar< 17.degrees 5) survey in the 67.9 and 78.4 keV nuclear de-excitation lines of titanium-44 (Ti-44) performed using the data acquired with the IBIS/ISGRI instrument onboard the INTEGRAL satellite during 12 yr of operation. The peak sensitivity of our survey reached an unprecedented level of 4.8 x 10(-6) ph cm(-2) s(-1) (3s) that improves the sensitivity of the survey done by Compton Gamma-Ray Observatory/COMPTEL by a factor of similar to 5. As a result, constraining upper limits for all sources from the catalogue of Galactic supernova remnants (SNRs; Green 2014) are derived. These upper limits can be used to estimate the exposure needed to detect Ti-44 emission from any known SNR using existing and prospective X-and gamma-ray telescopes. Among the youngest Galactic SNRs, only Cas A shows significant Ti-44 emission flux in good agreement with the NuSTAR measurements. We did not detect any other sources of titanium emission in the Galactic plane at significance level higher than 5s confirming previous claims of the rarity of such Ti-44-producing SNRs.
We report the results of the deepest Galactic plane (vertical bar b vertical bar< 17.degrees 5) survey in the 67.9 and 78.4 keV nuclear de-excitation lines of titanium-44 (Ti-44) performed using the data acquired with the IBIS/ISGRI instrument onboard the INTEGRAL satellite during 12 yr of operation. The peak sensitivity of our survey reached an unprecedented level of 4.8 x 10(-6) ph cm(-2) s(-1) (3s) that improves the sensitivity of the survey done by Compton Gamma-Ray Observatory/COMPTEL by a factor of similar to 5. As a result, constraining upper limits for all sources from the catalogue of Galactic supernova remnants (SNRs; Green 2014) are derived. These upper limits can be used to estimate the exposure needed to detect Ti-44 emission from any known SNR using existing and prospective X-and gamma-ray telescopes. Among the youngest Galactic SNRs, only Cas A shows significant Ti-44 emission flux in good agreement with the NuSTAR measurements. We did not detect any other sources of titanium emission in the Galactic plane at significance level higher than 5s confirming previous claims of the rarity of such Ti-44-producing SNRs.
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