Caiazzo, IlariaIlariaCaiazzoHeyl, JeremyJeremyHeylIngram, Adam R.Adam R.IngramBELLONI, Tomaso Maria MelchiorreTomaso Maria MelchiorreBELLONICackett, EdwardEdwardCackettDE ROSA, ALESSANDRAALESSANDRADE ROSAFEROCI, MARCOMARCOFEROCISwetz, Daniel S.Daniel S.SwetzDamascelli, AndreaAndreaDamascelliDosanjh, PinderPinderDosanjhGallagher, SarahSarahGallagherGallo, LuigiLuigiGalloHaggard, DarylDarylHaggardHeinke, CraigCraigHeinkeHoffman, KelseyKelseyHoffmanKirmizibayrak, DemetDemetKirmizibayrakMorsink, SharonSharonMorsinkRau, WolfgangWolfgangRauRipoche, PaulPaulRipocheSafi-Harb, SamarSamarSafi-HarbSivakoff, Gregory R.Gregory R.SivakoffStairs, IngridIngridStairsSTELLA, LuigiLuigiSTELLAUllom, Joel N.Joel N.Ullom2020-12-142020-12-1420192330-9458http://hdl.handle.net/20.500.12386/28836The X-ray emission of neutron stars and black holes presents a rich phenomenology that can help us answer: Does general relativity apply in the strong gravity regime? Are black holes described by the Kerr metric? We consider how to investigate these questions with a combination of high- spectral and high-timing resolution using TES arrays.ELETTRONICOenArticlehttps://baas.aas.org/pub/2020n3i516/release/12019BAAS...51c.516CFIS/05 - ASTRONOMIA E ASTROFISICA