X-ray spectropolarimetry of the bright atoll Serpens X-1

dc.contributor.authorUrsini, F.
dc.contributor.authorGnarini, A.
dc.contributor.authorBianchi, S.
dc.contributor.authorBobrikova, A.
dc.contributor.authorCapitanio, F.
dc.contributor.authorCocchi, M.
dc.contributor.authorFabiani, S.
dc.contributor.authorFarinelli, R.
dc.contributor.authorKaaret, P.
dc.contributor.authorMatt, G.
dc.contributor.authorNg, M.
dc.contributor.authorPoutanen, J.
dc.contributor.authorRavi, S.
dc.contributor.authorTarana, A.
dc.contributor.organizationfi=Tuorlan observatorio|en=Tuorla Observatory|
dc.contributor.organization-code1.2.246.10.2458963.20.90670098848
dc.converis.publication-id458966958
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/458966958
dc.date.accessioned2025-08-27T22:54:50Z
dc.date.available2025-08-27T22:54:50Z
dc.description.abstractWe present simultaneous X-ray polarimetric and spectral observations of the bright atoll source Ser X-1 carried out with the Imaging X-ray Polarimetry Explorer (IXPE), NICER, and NuSTAR. We obtain an upper limit of 2% (99% confidence level) on the polarization degree in the 2 8 keV energy band. We detect four type-I X-ray bursts, two of which during the IXPE observation. This is the first time that has IXPE observed type-I X-ray bursts, and it allows us to place an upper limit on their polarization degree; however, due to the limited total number of counts in each burst, we obtain a relatively high upper limit (80%). We confirm the presence of reflection features in the X-ray spectrum, notably a broad iron line. Fitting the data with a relativistic reflection model, we derive a disk inclination of 25. The spectral and polarization properties are comparable with other atolls observed by IXPE, suggesting a similar accretion geometry, and the relatively low polarization is consistent with the low inclination.
dc.identifier.eissn1432-0746
dc.identifier.jour-issn0004-6361
dc.identifier.olddbid203037
dc.identifier.oldhandle10024/186064
dc.identifier.urihttps://www.utupub.fi/handle/11111/49025
dc.identifier.urlhttps://doi.org/10.1051/0004-6361/202451584
dc.identifier.urnURN:NBN:fi-fe2025082789973
dc.language.isoen
dc.okm.affiliatedauthorBobrikova, Anna
dc.okm.affiliatedauthorPoutanen, Juri
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.publisherEDP Sciences
dc.publisher.countryFranceen_GB
dc.publisher.countryRanskafi_FI
dc.publisher.country-codeFR
dc.relation.articlenumberA200
dc.relation.doi10.1051/0004-6361/202451584
dc.relation.ispartofjournalAstronomy and Astrophysics
dc.relation.volume690
dc.source.identifierhttps://www.utupub.fi/handle/10024/186064
dc.titleX-ray spectropolarimetry of the bright atoll Serpens X-1
dc.year.issued2024

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