dc.contributor.author | Corsi, A. | |
dc.contributor.author | DE PASQUALE, Massımılıano | |
dc.contributor.author | Piro, L. | |
dc.contributor.author | Gendre, B. | |
dc.date.accessioned | 2022-02-18T11:17:17Z | |
dc.date.available | 2022-02-18T11:17:17Z | |
dc.date.issued | 2006 | |
dc.identifier.citation | Gendre 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.issn | 2037-4895 | |
dc.identifier.other | av_e6a52059-aea3-43b7-b267-8512dcb002bf | |
dc.identifier.other | vv_1032021 | |
dc.identifier.uri | http://hdl.handle.net/20.500.12627/180850 | |
dc.identifier.uri | https://doi.org/10.1393/neb/i2007-10288-7 | |
dc.description.abstract | We 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.iso | eng | |
dc.subject | Temel Bilimler (SCI) | |
dc.subject | Temel Bilimler | |
dc.subject | FİZİK, MULTİDİSİPLİNER | |
dc.subject | Fizik | |
dc.subject | Disiplinlerarası Fizik ve İlgili Bilim ve Teknoloji Alanları | |
dc.title | The BeppoSAX, XMM-Newton and Chandra X-ray afterglow catalog | |
dc.type | Makale | |
dc.relation.journal | NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-BASIC TOPICS IN PHYSICS | |
dc.contributor.department | , , | |
dc.identifier.volume | 121 | |
dc.identifier.issue | 12 | |
dc.identifier.startpage | 1485 | |
dc.identifier.endpage | 1486 | |
dc.contributor.firstauthorID | 3374333 | |