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Comparison between the NuSTAR E-CDF-S deblended fluxes (this work) and the total Chandra E-CDF-S (X16; left panel) and CDF-S (L17; right panel) fluxes in the 3–8 keV band (all fluxes are aperture-corrected). In each panel, the green 1∶1 line is centered at the shaded area indicating a factor of ≤3 ![]()
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Figures of the Article
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Stacked NuSTAR E-CDF-S science mosaic in the full band, with a total of 58 sources plotted as circles. The green (47/58) and red (4/58; being less significant detections) sources have the Chandra 250 ks E-CDF-S counterparts within rm=30″ . The magenta source (1/58) does not have any Chandra 250 ks E-CDF-S counterparts but can be matched to a Chandra 7 Ms CDF-S source. Among the unmatched sources (6/58), 3 yellow sources reside in the very edges of the mosaic and 3 cyan sources reside in the chip-gap areas. Numbers are source XIDs. The bottom color bar indicates the counts per pixel. -
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Comparison of net counts obtained by this work and M15 in the E-CDF-S. The diagonal dashed lines indicate the 1∶1 relations.
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Comparison between the NuSTAR E-CDF-S deblended fluxes (this work) and the total Chandra E-CDF-S (X16; left panel) and CDF-S (L17; right panel) fluxes in the 3–8 keV band (all fluxes are aperture-corrected). In each panel, the green 1∶1 line is centered at the shaded area indicating a factor of \le 3 difference from the 1∶1 line, and the horizontal dotted line indicates the detection limit. -
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Stacked NuSTAR CDF-N science mosaic in the 3–24 keV band (cf. Fig. 1), with a total of 42 sources plotted. The green (29/42) and red (4/42; being less significant detections) sources have the Chandra 2 Ms CDF-N counterparts within r_{\rm m}=30'' . Among the unmatched sources (9/42), 8 yellow sources reside in or near the edges of the mosaic, and 1 cyan source is only detected in the 8–24 keV band. -
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Same as Fig. 3, but for the comparison between the NuSTAR CDF-N deblended fluxes (this work) and the total Chandra CDF-N fluxes (X16) in the 3–8 keV band (all fluxes are aperture-corrected).
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Normalized distributions of deblended NuSTAR fluxes in the CDF-N and E-CDF-S.
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