paper

The NuSTAR Extragalactic Survey of the James Webb Space Telescope North Ecliptic Pole Time-Domain Field

arXiv:2109.13839 · doi:10.1093/mnras/stab2885

Abstract

We present the extragalactic survey of the () North Ecliptic Pole (NEP) Time-Domain Field. The survey covers a 0.16 deg area with a total exposure of 681 ks acquired in a total of nine observations from three epochs. The survey sensitivities at 20% of the area are 2.39, 1.14, 2.76, 1.52, and 5.20 10 erg cm s in the 3-24, 3-8, 8-24, 8-16, and 16-24 keV bands, respectively. The NEP survey is one of the most sensitive extragalactic surveys with so far. A total of 33 sources were detected above 95% reliability in at least one of the five bands. We present the number counts, log-log, measured in the hard X-ray 8-24 and 8-16 keV bands, uniquely accessible by down to such faint fluxes. We performed source detection on the XMM- and observations of the same field to search for soft X-ray counterparts of each detection. The soft band positions were used to identify optical and infrared associations. We present the X-ray properties (hardness ratio and luminosity) and optical-to-X-ray properties of the detected sources. The measured fraction of candidate Compton-thick (N) active galactic nuclei, derived from the hardness ratio, is between 3% to 27%. As this survey was designed to have variability as its primary focus, we present preliminary results on multi-epoch flux variability in the 3-24 keV band.

22 pages, 17 figures

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