X Zhao
The NuSTAR extragalactic survey of the James Webb Space Telescope North Ecliptic Pole time-domain field
Zhao, X; Civano, F; Fornasini, FM; Alexander, DM; Cappelluti, N; Chen, CT; Cohen, SH; Elvis, M; Gandhi, P; Grogin, NA; Hickox, RC; Jansen, RA; Koekemoer, A; Lanzuisi, G; Maksym, WP; Masini, A; Rosario, DJ; Ward, MJ; Willmer, CNA; Windhorst, RA
Authors
F Civano
FM Fornasini
Professor David Alexander d.m.alexander@durham.ac.uk
Professor
N Cappelluti
CT Chen
SH Cohen
M Elvis
P Gandhi
NA Grogin
RC Hickox
RA Jansen
A Koekemoer
G Lanzuisi
WP Maksym
A Masini
DJ Rosario
Professor Martin Ward martin.ward@durham.ac.uk
External Examiner (PGR)
CNA Willmer
RA Windhorst
Abstract
We present the NuSTAR extragalactic survey of the James Webb Space Telescope (JWST) North Ecliptic Pole (NEP) Time-Domain Field. The survey covers a ∼0.16 deg2 area with a total exposure of 681 ks acquired in a total of nine observations from three epochs. The survey sensitivities at 20 per cent of the area are 2.39, 1.14, 2.76, 1.52, and 5.20 × 10−14 erg cm−2 s−1 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 NuSTAR so far. A total of 33 sources were detected above 95 per cent reliability in at least one of the five bands. We present the number counts, logN-logS, measured in the hard X-ray 8–24 and 8–16 keV bands, uniquely accessible by NuSTAR down to such faint fluxes. We performed source detection on the XMM–Newton and Chandra observations of the same field to search for soft X-ray counterparts of each NuSTAR 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 (NH≥1024cm−2) active galactic nuclei, derived from the hardness ratio, is between 3 and 27 per cent. As this survey was designed to have variability as its primary focus, we present preliminary results on multiepoch flux variability in the 3–24 keV band.
Citation
Zhao, X., Civano, F., Fornasini, F., Alexander, D., Cappelluti, N., Chen, C., Cohen, S., Elvis, M., Gandhi, P., Grogin, N., Hickox, R., Jansen, R., Koekemoer, A., Lanzuisi, G., Maksym, W., Masini, A., Rosario, D., Ward, M., Willmer, C., & Windhorst, R. (2021). The NuSTAR extragalactic survey of the James Webb Space Telescope North Ecliptic Pole time-domain field. Monthly Notices of the Royal Astronomical Society, 508(4), 5176-5195. https://doi.org/10.1093/mnras/stab2885
Journal Article Type | Article |
---|---|
Acceptance Date | Sep 28, 2021 |
Online Publication Date | Oct 6, 2021 |
Publication Date | 2021-12 |
Deposit Date | Jan 28, 2022 |
Publicly Available Date | Jan 28, 2022 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 508 |
Issue | 4 |
Pages | 5176-5195 |
DOI | https://doi.org/10.1093/mnras/stab2885 |
Public URL | https://durham-repository.worktribe.com/output/1216579 |
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Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. © 2021 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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