Simultaneous NICER and NuSTAR Observations of the Neutron Star Low-mass X-Ray Binary Serpens X-1
We present the first contemporaneous NICER and NuSTAR analysis of the low-mass X-ray binary Serpens X-1 obtained in 2023 June, performing broadband X-ray spectral analysis modeling of the reprocessed emission with relxillNS from 0.4 to 30 keV. We test various continuum and background estimation mode...
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| Published in: | The Astrophysical journal Vol. 980; no. 2; pp. 234 - 244 |
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| Main Authors: | , , , , , , , |
| Format: | Journal Article |
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20.02.2025
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| ISSN: | 0004-637X, 1538-4357 |
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| Abstract | We present the first contemporaneous NICER and NuSTAR analysis of the low-mass X-ray binary Serpens X-1 obtained in 2023 June, performing broadband X-ray spectral analysis modeling of the reprocessed emission with relxillNS from 0.4 to 30 keV. We test various continuum and background estimation models to ensure that our results do not hinge on the choice of model used, and found that the detection of reflection features is independent of the choice of both continuum and background model. The position of the inner accretion disk is consistent with the last stable circular orbit ( R in ≤ 1.2 R ISCO ) and a low inclination of i ≤ 8.3°. Additionally, we investigate the presence of the low-energy (∼1 keV) Fe L complex in the data from NICER and the Reflection Grating Spectrometer on XMM-Newton that was previously reported in the literature. We find that the line is at most a 2% feature relative to the reprocessed continuum, and are unable to claim a definitive detection for the current data set. However, we discuss plausible conditions and systems that would increase the likelihood of detecting this feature in the future. |
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| AbstractList | We present the first contemporaneous NICER and NuSTAR analysis of the low-mass X-ray binary Serpens X-1 obtained in 2023 June, performing broadband X-ray spectral analysis modeling of the reprocessed emission with relxillNS from 0.4 to 30 keV. We test various continuum and background estimation models to ensure that our results do not hinge on the choice of model used, and found that the detection of reflection features is independent of the choice of both continuum and background model. The position of the inner accretion disk is consistent with the last stable circular orbit (Rin ≤ 1.2 RISCO) and a low inclination of i ≤ 8.3°. Additionally, we investigate the presence of the low-energy (∼1 keV) Fe L complex in the data from NICER and the Reflection Grating Spectrometer on XMM-Newton that was previously reported in the literature. We find that the line is at most a 2% feature relative to the reprocessed continuum, and are unable to claim a definitive detection for the current data set. However, we discuss plausible conditions and systems that would increase the likelihood of detecting this feature in the future. We present the first contemporaneous NICER and NuSTAR analysis of the low-mass X-ray binary Serpens X-1 obtained in 2023 June, performing broadband X-ray spectral analysis modeling of the reprocessed emission with relxillNS from 0.4 to 30 keV. We test various continuum and background estimation models to ensure that our results do not hinge on the choice of model used, and found that the detection of reflection features is independent of the choice of both continuum and background model. The position of the inner accretion disk is consistent with the last stable circular orbit ( R in ≤ 1.2 R ISCO ) and a low inclination of i ≤ 8.3°. Additionally, we investigate the presence of the low-energy (∼1 keV) Fe L complex in the data from NICER and the Reflection Grating Spectrometer on XMM-Newton that was previously reported in the literature. We find that the line is at most a 2% feature relative to the reprocessed continuum, and are unable to claim a definitive detection for the current data set. However, we discuss plausible conditions and systems that would increase the likelihood of detecting this feature in the future. |
| Author | Hall, H. García, J. A. Ludlam, R. M. Miller, J. M. Tomsick, J. A. Fabian, A. C. Coley, J. Coughenour, B. M. |
| Author_xml | – sequence: 1 givenname: H. orcidid: 0009-0000-4409-7914 surname: Hall fullname: Hall, H. organization: Wayne State University Department of Physics & Astronomy, 666 West Hancock St., Detroit, MI 48201, USA – sequence: 2 givenname: R. M. orcidid: 0000-0002-8961-939X surname: Ludlam fullname: Ludlam, R. M. organization: Wayne State University Department of Physics & Astronomy, 666 West Hancock St., Detroit, MI 48201, USA – sequence: 3 givenname: J. M. orcidid: 0000-0003-2869-7682 surname: Miller fullname: Miller, J. M. organization: University of Michigan Department of Astronomy, 1085 South University Ave., Ann Arbor, MI 48109-1107, USA – sequence: 4 givenname: A. C. orcidid: 0000-0002-9378-4072 surname: Fabian fullname: Fabian, A. C. organization: University of Cambridge Institute of Astronomy, Madingley Rd., Cambridge, CB3 0HA, UK – sequence: 5 givenname: J. A. orcidid: 0000-0001-5506-9855 surname: Tomsick fullname: Tomsick, J. A. organization: University of California, Berkeley Space Sciences Lab, 7 Gauss Way, Berkeley, CA 94720, USA – sequence: 6 givenname: J. orcidid: 0000-0001-7532-8359 surname: Coley fullname: Coley, J. organization: CRESST and NASA Goddard Space Flight Center , Astrophysics Science Division, 8800 Greenbelt Rd., Greenbelt, MD 20771, USA – sequence: 7 givenname: J. A. orcidid: 0000-0003-3828-2448 surname: García fullname: García, J. A. organization: NASA Goddard Space Flight Center X-ray Astrophysics Laboratory, Greenbelt, MD 20771, USA – sequence: 8 givenname: B. M. orcidid: 0000-0003-0870-6465 surname: Coughenour fullname: Coughenour, B. M. organization: Utah Valley University Department of Physics, 800 W. University Pkwy., MS 179, Orem, UT 84508, USA |
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| Snippet | We present the first contemporaneous NICER and NuSTAR analysis of the low-mass X-ray binary Serpens X-1 obtained in 2023 June, performing broadband X-ray... |
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| StartPage | 234 |
| SubjectTerms | Accretion Accretion disks Binary stars Broadband Circular orbits Low-mass x-ray binary stars Neutron stars Orbital stability Spectral analysis Spectrum analysis X ray binaries X ray spectra X ray stars X-rays XMM (spacecraft) |
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| Title | Simultaneous NICER and NuSTAR Observations of the Neutron Star Low-mass X-Ray Binary Serpens X-1 |
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