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Table 1.
Sample of SXTs used in this work.
X-ray transient | Type | Spectra | Observing period | Resolution | Spectral | Telescope/ | References |
---|---|---|---|---|---|---|---|
(km s−1) | band | instrument | |||||
Nova Mus 1991 | BH | 17 × 1200 s | 13/04/13–10/05/13 | 70 | J, H, K | VLT/X-shooter | 1 |
A0620-00 | BH | 12 × 240 s | 17/02/05 | 150 | K | Keck II/NIRSPEC | 2 |
XTE J1118+480 | BH | 48 × 310 s | 02/04/11 and 12/04/11 | 176 | J, H, K | Gemini/GNIRS | 3 |
GX 339-4 | BH | 16 × 275 s | 22/05/16–07/09/16 | 55 | J, H | VLT/X-shooter | 4 |
GRS 1915+105 | BH | 27 × 2400 s | 09/06/10–03/09/11 | 37 | J, H, K | VLT/X-shooter | 5 |
Aql X-1 | NS | 24 × 900 s | 20/05/10–29/09/11 | 75 | K | VLT/SINFONI | 6 |
References. (1) González Hernández et al. (2017); (2) Harrison et al. (2007); (3) Khargharia et al. (2013); (4) Heida et al. (2017); (5) Steeghs et al. (2013); (6) Mata Sánchez et al. (2017).
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