Testing the Kerr Black Hole Hypothesis Using X-Ray Reflection Spectroscopy and a Thin Disk Model with Finite Thickness

dc.contributor.author	Nampalliwar, Sourabh
dc.date.accessioned	2020-12-09T09:26:22Z
dc.date.available	2020-12-09T09:26:22Z
dc.date.issued	2020
dc.identifier.issn	1538-4357
dc.identifier.uri	http://hdl.handle.net/10900/110458
dc.language.iso	en	de_DE
dc.publisher	Iop Publishing Ltd	de_DE
dc.relation.uri	http://dx.doi.org/10.3847/1538-4357/aba625	de_DE
dc.subject.ddc	520	de_DE
dc.subject.ddc	530	de_DE
dc.title	Testing the Kerr Black Hole Hypothesis Using X-Ray Reflection Spectroscopy and a Thin Disk Model with Finite Thickness	de_DE
dc.type	Article	de_DE
utue.quellen.id	20200929220116_00368
utue.personen.roh	Abdikamalov, Askar B.
utue.personen.roh	Ayzenberg, Dimitry
utue.personen.roh	Bambi, Cosimo
utue.personen.roh	Dauser, Thomas
utue.personen.roh	Garcia, Javier A.
utue.personen.roh	Nampalliwar, Sourabh
utue.personen.roh	Tripathi, Ashutosh
utue.personen.roh	Zhou, Menglei
dcterms.isPartOf.ZSTitelID	Astrophysical Journal	de_DE
dcterms.isPartOf.ZS-Issue	Article 80	de_DE
dcterms.isPartOf.ZS-Volume	899	de_DE
utue.fakultaet	07 Mathematisch-Naturwissenschaftliche Fakultät	de_DE