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An Empirical Background Model for the NICER X-ray Timing Instrument

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arxiv 2105.09901 v1 pith:43K4UPED submitted 2021-05-20 astro-ph.IM astro-ph.HE

Ronald A. Remillard , Michael Loewenstein , James F. Steiner , Gregory Y. Prigozhin , Beverly LaMarr , Teruaki Enoto , Keith C. Gendreau , Zaven Arzoumanian
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Craig Markwardt Arkadip Basak Abigail L. Stevens Paul S. Ray Diego Altamirano Douglas J. K. Buisson
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keywords backgroundmodelgtispercentratefilteringempiricallimit
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NICER has a comparatively low background rate, but it is highly variable, and its spectrum must be predicted using measurements unaffected by the science target. We describe an empirical, three-parameter model based on observations of seven pointing directions that are void of detectable sources. An examination of 3556 good time intervals (GTIs), averaging 570 s, yields a median rate (0.4-12 keV; 50 detectors) of 0.87 c/s, but in 5 percent (1 percent) of cases, the rate exceeds 10 (300) c/s. Model residuals persist at 20-30 percent of the initial rate for the brightest GTIs, implying one or more missing model parameters. Filtering criteria are given to flag GTIs likely to have unsatisfactory background predictions. With such filtering, we estimate a detection limit, 1.20 c/s (3 sigma, single GTI) at 0.4-12 keV, equivalent to 3.6e-12 erg/cm^2/s for a Crab-like spectrum. The corresponding limit for soft X-ray sources is 0.51 c/s at 0.3-2.0 keV, or 4.3e-13 erg/cm^2/s for a 100 eV blackbody. Faint-source filtering selects 85 percent of the background GTIs, and higher rates are expected for targets scheduled more favorably. An application of the model to 1 s timescale makes it possible to distinguish source flares from possible surges in the background.

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Forward citations

Cited by 5 Pith papers

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