15 years of galactic surveys and hard X-ray background measurements

dc.contributor.authorKrivonos Roman A.
dc.contributor.authorBird Anthony J.
dc.contributor.authorChurazov Eugene M.
dc.contributor.authorTomsick John A.
dc.contributor.authorBazzano Angela
dc.contributor.authorBeckmann Volker
dc.contributor.authorBélanger Guillaume
dc.contributor.authorBodaghee Arash
dc.contributor.authorChaty Sylvain
dc.contributor.authorKuulkers Erik
dc.contributor.authorLutovinov Alexander
dc.contributor.authorMalizia Angela
dc.contributor.authorMasetti Nicola
dc.contributor.authorMereminskiy Ilya A.
dc.contributor.authorSunyaev Rashid
dc.contributor.authorTsygankov Sergey S.
dc.contributor.authorUbertini Pietro
dc.contributor.authorWinkler Christoph
dc.contributor.organizationfi=Tuorlan observatorio|en=Tuorla Observatory|
dc.contributor.organization-code1.2.246.10.2458963.20.90670098848
dc.converis.publication-id53340388
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/53340388
dc.date.accessioned2022-10-28T14:09:01Z
dc.date.available2022-10-28T14:09:01Z
dc.description.abstract<p>The INTEGRAL hard X-ray surveys have proven to be of fundamental importance. INTEGRAL has mapped the Galactic plane with its large field of view and excellent sensitivity. Such hard X-ray snapshots of the whole Milky Way on a time scale of a year are beyond the capabilities of past and current narrow-FOV grazing incidence X-ray telescopes. By expanding the INTEGRAL X-ray survey into shorter timescales, a productive search for transient X-ray emitters was made possible. In more than fifteen years of operation, the INTEGRAL observatory has given us a sharper view of the hard X-ray sky, and provided the triggers for many follow-up campaigns from radio frequencies to gamma-rays. In addition to conducting a census of hard X-ray sources across the entire sky, INTEGRAL has carried out, through Earth occultation manoeuvres, unique observations of the large-scale cosmic X-ray background, which will without question be included in the annals of X-ray astronomy as one of the mission’s most salient contribution to our understanding of the hard X-ray sky.</p><div><br></div>
dc.identifier.eissn1872-9630
dc.identifier.jour-issn1387-6473
dc.identifier.olddbid186562
dc.identifier.oldhandle10024/169656
dc.identifier.urihttps://www.utupub.fi/handle/11111/38858
dc.identifier.urnURN:NBN:fi-fe2021042825323
dc.language.isoen
dc.okm.affiliatedauthorTsygankov, Sergey
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeA1 ScientificArticle
dc.publisherElsevier B.V.
dc.publisher.countryNetherlandsen_GB
dc.publisher.countryAlankomaatfi_FI
dc.publisher.country-codeNL
dc.relation.articlenumber101612
dc.relation.doi10.1016/j.newar.2021.101612
dc.relation.ispartofjournalNew Astronomy Reviews
dc.relation.volume92
dc.source.identifierhttps://www.utupub.fi/handle/10024/169656
dc.title15 years of galactic surveys and hard X-ray background measurements
dc.year.issued2021

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