English

NuSTAR spectral analysis beyond 79 keV with stray light

High Energy Astrophysical Phenomena 2022-12-21 v1

Abstract

Due to the structure of the NuSTAR telescope, photons at large off-axis (> 1deg) can reach the detectors directly (stray light), without passing through the instrument optics. At these off-axis angles NuSTAR essentially turns into a collimated instrument and the spectrum can extend to energies above the Pt k-edge (79 keV) of the multi-layers, which limits the effective area bandpass of the optics. We present the first scientific spectral analysis beyond 79 keV using a Cygnus X-1 observation in StrayCats, the catalog of stray light observations. This serendipitous stray light observation occurred simultaneously with an INTEGRAL observation. When the spectra are modeled together in the 30-120 keV energy band, we find that the NuSTAR stray light flux is well calibrated and constrained to be consistent with the INTEGRAL flux at the 90% confidence level. Furthermore, we explain how to treat the background of the stray light spectral analysis, which is especially important at high energies.

Keywords

Cite

@article{arxiv.2209.14325,
  title  = {NuSTAR spectral analysis beyond 79 keV with stray light},
  author = {G. Mastroserio and B. W. Grefenstette and P. Thalhammer and D. J. K. Buisson and M. C. Brumback and R. M. Ludlam and R. M. T. Connors and J. A. Garcıa and V. Grinberg and K. K. Madsen and H. Miyasaka and J. A. Tomsick and J. Wilms},
  journal= {arXiv preprint arXiv:2209.14325},
  year   = {2022}
}

Comments

Accepted for publication in ApJ

R2 v1 2026-06-28T02:19:04.417Z