X-ray spectral variability of blazars using principal component analysis

dc.creator	Gallant, D.
dc.creator	Gallo, Luigi C.
dc.creator	Parker, M.L.
dc.date.accessioned	2025-01-20T16:37:29Z
dc.date.available	2025-01-20T16:37:29Z
dc.date.issued	2018
dc.identifier.issn	0035-8711
dc.identifier.uri	10.1093/mnras/sty1987
dc.identifier.uri	https://library2.smu.ca/xmlui/handle/01/32086
dc.description	Publisher version	en_CA
dc.description.provenance	Submitted by Anna Labrador (anna.labrador@smu.ca) on 2025-01-20T16:37:29Z No. of bitstreams: 1 Gallo_Luigi_C_2018g.pdf: 4811453 bytes, checksum: d75a7c1d40b03b2991c6ff8ae17ea050 (MD5)	en
dc.description.provenance	Made available in DSpace on 2025-01-20T16:37:29Z (GMT). No. of bitstreams: 1 Gallo_Luigi_C_2018g.pdf: 4811453 bytes, checksum: d75a7c1d40b03b2991c6ff8ae17ea050 (MD5) Previous issue date: 2018	en
dc.language.iso	en	en_CA
dc.publisher	Oxford University Press	en_CA
dc.title	X-ray spectral variability of blazars using principal component analysis	en_CA
dc.type	Text	en_CA
dcterms.bibliographicCitation	Monthly Notices of the Royal Astronomical Society 480 (2), p.1999-2010, 2018	en_CA