Table A.2.
Spectral properties from X-ray observations of SN 2024iss.
| Instrument | Phasea | Nintb | kT | Normc | Fluxd | Unabsorbed Fluxd |
|---|---|---|---|---|---|---|
| (days) | (1022 cm−2) | (keV) | 10−4 cm−5 | (erg/cm2/s) | (erg/cm2/s) | |
| Swift-XRT | 2.0 ± 1.1 | < 0.008 | 32.6 | ![]() |
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| EP-FXT | 2.3 ± 0.2 | < 0.008 | 32.6 | ![]() |
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| Swift-XRT | 4.9 ± 1.5 | < 0.008 | 32.6 | ![]() |
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| NuSTAR | 5.2 ± 0.4 | < 0.008 | ![]() |
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| Swift-XRT | 10.6 ± 2.3 | < 0.008 | 32.6 | ![]() |
![]() |
![]() |
| EP-FXT | 10.6 ± 0.1 | < 0.008 | 32.6 | ![]() |
![]() |
![]() |
| NuSTAR | 20.7 ± 0.6 | < 0.008 | 32.6 | ![]() |
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| Swift-XRT | 33.9 ± 7.4 | < 0.008 | 32.6 | < 0.2 | < 4.8 × 10−14 | < 4.8 × 10−14 |
| Swift-XRT | 206.3 ± 21.5 | < 0.008 | 32.6 | < 10.9 | < 2.0 × 10−12 | < 2.0 × 10−12 |
| Swift-XRT | 276.8 ± 6.8 | < 0.008 | 32.6 | < 0.3 | < 5.4 × 10−14 | < 5.3 × 10−14 |
Notes.
Time with respect to MJD = 60,442.21.
Intrinsic neutral hydrogen column density, with the neutral density contribution from the Milky Way excluded (0.009 × 1022 cm−2).
The normalization of the apec spectrum, defined as
EM, where DL is the luminosity distance to the source (cm), EM is the emission measure defined as
; ne and nH denote the electron and hydrogen densities, respectively.
The absorbed flux and unabsorbed flux are in the ranges 0.5–10 keV for FXT, 0.3–10 keV for XRT, and 3–79 keV for NuSTAR. We adopt a fixed plasma temperature, as estimated from the fourth observation in the column, for all other observations. Because of the limited photon counts and the restricted energy coverage of FXT (0.5–10 keV), the plasma temperature (kT) of SN 2024iss at each epoch cannot be reliably constrained independently (see Sect. 2.4).
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