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First Look at the High-resolution X-Ray Spectra in the Highly Absorbed High-mass X-Ray Binary IGR J16318−4848 with Chandra

  • Authors: Pragati Pradhan, David P. Huenemoerder, Biswajit Paul, Roberta Amato, Ralf Ballhausen, Claude Canizares, Joel B. Coley, Camille M. Diez, Felix Fürst, Poshak Gandhi, Victoria Grinberg, Sean Gunderson, Richard Ignace, Peter Kretschmar, Maximilian Lorenz, Christian Malacaria, Antonios Manousakis, Silvia Martínez-Núñez, Katja Pottschmidt, Jérôme Rodriguez, Richard E. Rothschild, José M. Torrejón, Bert Vander Meulen, Jörn Wilms

Pragati Pradhan et al 2026 The Astrophysical Journal 1004 .

  • Provider: AAS Journals

Caption: Figure 1.

Orbital intensity profile of IGR J16318−4848 obtained by folding the Swift/BAT daily light curves with a period of 80.09 days (±0.012) and a reference epoch of MJD 53477.577, adopted from N. Iyer & B. Paul (2017). The reference epoch is chosen such that the peak BAT flux occurs at an orbital phase of ϕorb = 0.5. The orbital phases of the Chandra ObsIDs closest to the BAT data points (within a phase difference <0.007) are listed on the right.

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