Zhao, XiuruiCivano, FrancescaWillmer, Christopher N. A.Bonoli, SilviaChen, Chien-TingCreech, SamanthaDupke, RenatoFornasini, Francesca M.Jansen, Rolf A.Kikuta, SatoshiKoekemoer, Anton M.Laha, SibasishMarchesi, StefanoO'Brien, RosaliaSilver, RossWillner, S. P.Windhorst, Rogier A.Yan, HaojingAlcaniz, JailsonBenitez, NarcisoCarneiro, SauloCenarro, JavierCristóbal-Hornillos, DavidEderoclite, AlessandroHernán-Caballero, AntonioLópez-Sanjuan, CarlosMarín-Franch, Antoniode Oliveira, Claudia MendesMoles, MarianoSodré Jr., LaerteTaylor, KeithVarela, JesúsRamió, Héctor Vázquez2024-03-062024-03-062024-02-21https://doi.org/10.48550/arXiv.2402.13508http://hdl.handle.net/11603/31846We present the second NuSTAR and XMM-Newton extragalactic survey of the JWST North Ecliptic Pole (NEP) Time-Domain Field (TDF). The first NuSTAR NEP-TDF survey (Zhao et al. 2021) had 681 ks total exposure time executed in NuSTAR cycle 5, in 2019 and 2020. This second survey, acquired from 2020 to 2022 in cycle 6, adds 880 ks of NuSTAR exposure time. The overall NuSTAR NEP-TDF survey is the most sensitive NuSTAR extragalactic survey to date, and a total of 60 sources were detected above the 95% reliability threshold. We constrain the hard X-ray number counts, logN-log S, down to 1.7 x 10⁻¹⁴ erg cm⁻² s⁻¹ at 8-24 keV and detect an excess of hard X-ray sources at the faint end. About 47% of the NuSTAR-detected sources are heavily obscured (Nₕ > 10²³ cm⁻²), and 18⁺²⁰₋₈% of the NuSTAR-detected sources are Compton-thick (Nₕ>10²⁴ cm⁻²). These fractions are consistent with those measured in other NuSTAR surveys. Four sources presented >2σ variability in the 3-year survey. In addition to NuSTAR, a total of 62 ks of XMM-Newton observations were taken during NuSTAR cycle 6. The XMM-Newton observations provide soft X-ray (0.5-10 keV) coverage in the same field and enable more robust identification of the visible and infrared counterparts of the NuSTAR-detected sources. A total of 286 soft X-ray sources were detected, out of which 214 XMM-Newton sources have secure counterparts from multiwavelength catalogs.37 pagesen-USThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.Public Domain Mark 1.0https://creativecommons.org/publicdomain/mark/1.0/Astrophysics - Astrophysics of GalaxiesAstrophysics - High Energy Astrophysical PhenomenaText