Spectral and timing properties of the accreting millisecond X-ray pulsar IGR J17498−2921 during its 2023 outburst

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Volume 691 (November 2024)

A&A, 691 (2024) A189

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Table 3.

List of estimated inner disk radii for AMXPs from modeling the reflection spectra.

Source	Telescope/Instrument	Model	R_in (R_g)	Ref.
SAX J1808.4−3658	XMM-Newton/EPIC-pn	`diskline`	$9_{- 3}^{+ 4}$ $9^{+4}_{-3}$	[1]
	XMM-Newton/EPIC-pn + Suzaku	`diskline`	13.2 ± 2.5	[2]
	NuSTAR	`relxillCp`	14.9 ± 2.5	[3]
	XMM-Newton/RGS, EPIC-pn	`diskline`	$10_{- 3}^{+ 8}$ $10^{+8}_{-3}$	[3]
IGR J17511−3057	XMM-Newton/RSG, EPIC-pn	`diskline`	$37_{- 9}^{+ 31}$ $37^{+31}_{-9}$	[4]
	XMM-Newton/RSG, EPIC-pn + RXTE/PCA, HEXTE	`diskline`	$22_{- 5}^{+ 9}$ $22^{+9}_{-5}$	[4]
	XMM-Newton/RSG, EPIC-pn + RXTE/PCA, HEXTE	`diskline`	$27_{- 9}^{+ 6}$ $27^{+6}_{-9}$	[4]
HETE J1900.1−2455	XMM-Newton/EPIC-pn	`rdblur*reflionx`	$23_{- 7}^{+ 10}$ $23^{+10}_{-7}$	[5]
	XMM-Newton/EPIC-pn + RXTE/PCA, HEXTE	`rdblur*reflionx`	$25_{- 11}^{+ 16}$ $25^{+16}_{-11}$	[5]
SAX J1748.9−2021	XMM-Newton/EPIC-pn + INTEGRAL/JEMX-1, JEMX-2, ISGRI	`diskline`	$29_{- 9}^{+ 12}$ $29^{+12}_{-9}$	[6]
IGR J00291+5934	XMM-Newton/RGS, EPIC-pn, MOS2 + NuSTAR	`diskline`	$43_{- 18}^{+ 910}$ $43^{+910}_{-18}$	[7]
MAXI J1816−195	NICER + NuSTAR	`relxillCp`	5.9±0.5	[8]

IGR J17498−2921	NICER + NuSTAR	`rdblur*rfxconv`	$21_{- 12}^{+ 17}$ $21^{+17}_{-12}$	This work

Notes. Uncertainties are reported at a level of statistical confidence of 90 percent.

[1] Papitto et al. (2009),

[2] Cackett et al. (2009),

[3] Di Salvo et al. (2019),

[4] Papitto et al. (2010),

[5] Papitto et al. (2013b),

[6] Pintore et al. (2016),

[7] Sanna et al. (2017b),

[8] Li et al. (2023).

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