Show simple item record

The BeppoSAX, XMM-Newton and Chandra X-ray afterglow catalog

dc.contributor.authorCorsi, A.
dc.contributor.authorDE PASQUALE, Massımılıano
dc.contributor.authorPiro, L.
dc.contributor.authorGendre, B.
dc.date.accessioned2022-02-18T11:17:17Z
dc.date.available2022-02-18T11:17:17Z
dc.date.issued2006
dc.identifier.citationGendre B., Corsi A., Piro L., DE PASQUALE M., "The BeppoSAX, XMM-Newton and Chandra X-ray afterglow catalog", NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-BASIC TOPICS IN PHYSICS, cilt.121, sa.12, ss.1485-1486, 2006
dc.identifier.issn2037-4895
dc.identifier.otherav_e6a52059-aea3-43b7-b267-8512dcb002bf
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/180850
dc.identifier.urihttps://doi.org/10.1393/neb/i2007-10288-7
dc.description.abstractWe present a catalog of X-ray afterglows observed by BeppoSAX, XMM-Newton and Chandra. We observe a temporal evolution of the afterglow properties, that we link with a jet effect. We then investigate on the Sako and Rutledge method to detect X-ray lines within the afterglow spectra, and find that this rnethod can be improved.
dc.language.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectTemel Bilimler
dc.subjectFİZİK, MULTİDİSİPLİNER
dc.subjectFizik
dc.subjectDisiplinlerarası Fizik ve İlgili Bilim ve Teknoloji Alanları
dc.titleThe BeppoSAX, XMM-Newton and Chandra X-ray afterglow catalog
dc.typeMakale
dc.relation.journalNUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-BASIC TOPICS IN PHYSICS
dc.contributor.department, ,
dc.identifier.volume121
dc.identifier.issue12
dc.identifier.startpage1485
dc.identifier.endpage1486
dc.contributor.firstauthorID3374333


Files in this item

FilesSizeFormatView

There are no files associated with this item.

This item appears in the following Collection(s)

Show simple item record