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http://hdl.handle.net/20.500.12386/24437
Title: | Calibration of the NuSTAR High-energy Focusing X-ray Telescope | Authors: | Madsen, Kristin K. Harrison, Fiona A. Markwardt, Craig B. An, Hongjun Grefenstette, Brian W. BACHETTI, Matteo Miyasaka, Hiromasa Kitaguchi, Takao Bhalerao, Varun Boggs, Steve Christensen, Finn E. Craig, William W. Forster, Karl Fuerst, Felix Hailey, Charles J. PERRI, Matteo Puccetti, Simonetta Rana, Vikram Stern, Daniel Walton, Dominic J. Jørgen Westergaard, Niels Zhang, William W. |
Issue Date: | 2015 | Journal: | THE ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | Number: | 220 | Issue: | 1 | First Page: | 8 | Abstract: | We present the calibration of the Nuclear Spectroscopic Telescope Array (NuSTAR) X-ray satellite. We used the Crab as the primary effective area calibrator and constructed a piece-wise linear spline function to modify the vignetting response. The achieved residuals for all off-axis angles and energies, compared to the assumed spectrum, are typically better than ±2% up to 40 keV and 5%-10% above due to limited counting statistics. An empirical adjustment to the theoretical two-dimensional point-spread function (PSF) was found using several strong point sources, and no increase of the PSF half-power diameter has been observed since the beginning of the mission. We report on the detector gain calibration, good to 60 eV for all grades, and discuss the timing capabilities of the observatory, which has an absolute timing of ±3 ms. Finally, we present cross-calibration results from two campaigns between all the major concurrent X-ray observatories (Chandra, Swift, Suzaku, and XMM-Newton), conducted in 2012 and 2013 on the sources 3C 273 and PKS 2155-304, and show that the differences in measured flux is within ̃10% for all instruments with respect to NuSTAR. | Acknowledgments: | We would like to thank the referee for helpful comments and suggestions which helped improve the paper. This work was supported under NASA Contract No. NNG08FD60C, and made use of data from the NuSTAR mission, a project led by the California Institute of Technology, managed by the Jet Propulsion Laboratory, and funded by the National Aeronautics and Space Administration. We thank the NuSTAR Operations, Software and Calibration teams for support with the execution and analysis of these observations. This research has made use of the NuSTAR Data Analysis Software (NuSTARDAS) jointly developed by the ASI Science Data Center (ASDC, Italy) and the California Institute of Technology (USA). Facilities: CXO , NuSTAR , Swift , Suzaku , and XMM . | URI: | http://hdl.handle.net/20.500.12386/24437 | URL: | https://iopscience.iop.org/article/10.1088/0067-0049/220/1/8/meta | ISSN: | 0067-0049 | DOI: | 10.1088/0067-0049/220/1/8 | Bibcode ADS: | 2015ApJS..220....8M | Fulltext: | open |
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Madsen_2015_ApJS_220_8.pdf | PDF editoriale | 2.8 MB | Adobe PDF | View/Open |
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