EDP Sciences logo
Subscriber Authentication Point
Search
Menu
Home All issues Volume 708 (April 2026) A&A, 708 (2026) A270 Full HTML
Open Access

Table D.6

Results from the X-ray analysis of Type Ibn SNe in the X-RAY sample.

Object Phasea tXbMathematical equation: $\[t_{X}^{b}\]$ LX M˙dMathematical equation: $\[\dot{M}^{d}\]$
(days) (days) (1041 erg/s) (M⊙/yr)
20191sm 7 − 43 17.0 < 1.4 < 1.0
2020able 0 − 24 16.2 < 0.3 < 0.4
2020nxt† 13 − 44 27.3 0.1 ± 0.1 0.4 ± 0.1
2021iyt 6 − 17 10.4 < 4.9 < 1.5
2021zfx 10 10.4 < 8.3 < 1.9
2022ablq 15 − 20 17.5 0.5 ± 0.2 0.6 ± 0.1
2022ablq 63 − 73 67.9 0.6 ± 0.2 1.3 ± 0.2
2022ablq 83 − 97 91.1 < 0.3 < 1.1
2022ablq 106 − 114 110.8 0.2 ± 0.1 1.0 ± 0.2
2022eux 2 − 35 15.8 < 0.6 < 0.6
2022ihx 6 − 22 11.9 < 0.3 < 0.4
2022pda 70 − 260 142.3 < 0.6 < 1.9
2022qhy† 2 − 8 4.6 0.04 ± 0.02 0.09 ± 0.02
2023emq 7 − 10 8.3 < 1.2 < 0.7
2023emq 11 11.1 1.9 ± 1.2 0.9 ± 0.3
2023emq 26 25.9 < 1.6 < 1.3
2023iuc 1 − 53 12.2 < 4.3 < 1.5
2023qre 6 − 82 26.0 < 2.8 < 1.7
2023rau 17 − 26 21.9 < 5.7 < 2.3
2023xgo 6 − 64 24.3 < 0.1 < 0.2

Notes. (a)Ranges of the dates of the XRT observations relative to the discovery date of each SN (Tab. D.3).

(b)Duration of the X-ray emission derived from the average date of the XRT observations with respect to the discovery date of each SN.

(c)X-ray luminosity obtained from the XRT observations at 1 keV.

(d)Mass-loss rates estimated through Eq. 1.

(†) X-ray emission from this source is likely from the host galaxy.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.