Open Access

Table 2.

Observational data.

Target UV Optical


Source ID Reference Resolution Source ID Reference Resolution
(Å) (Å)
R136 HST/STIS 12465 (1) 1.2 ESO/MUSE 0104.D-0084 (2) 2.3
NGC 3125-A1 HST/COS 15828 (3) 0.08 ESO/FORS 074.B-0108 (4) 15
NGC 5253-5 HST/STIS 8232 (5) 1.8 ESO/UVES 073.B-0283 (5) 0.2
Tol 89-A HST/STIS 7513 (6) 3.1 ESO/UVES 073.B-0238 (6) 0.2
NGC 5447S HST/COS 15126 0.6 GTC/OSIRIS GTC14-16A (7) 6.52
NGC 5455 HST/COS 15126 0.6 GTC/OSIRIS GTC14-16A (7) 6.52 (B) and 2.46 (V)
NGC 5462S HST/COS 15126 0.6 GTC/OSIRIS GTC14-16A (7) 6.52 (B) and 2.46 (V)
SIP2007-1 HST/COS 15126 0.6 SDSS (8) 2.5
HGGK 1054 HST/COS 15126 0.6 SDSS (8) 2.5
HGGK 1216 HST/COS 15126 0.6 GTC/OSIRIS GTC14-16A (7) 6.52 (B) and 2.46 (V)
NGC 4214 HST/STIS 9036 (9, 10) 1.2 HST/STIS 15846 0.56
NGC 4670 HST/COS 15193 (11) 0.08 HST/STIS 15846 0.56
Mrk 33 HST/STIS 9036 (9, 10) 1.2 SDSS (8) 2.5
J0036−3333 HST/COS 13017 (12, 13, 14) 0.073 SDSS (8) 2.5
J0115−0051/SB49 HST/COS 15185 (15) 0.073 SDSS (8) 2.5
J0823+2806 HST/COS 13017 (11,12,13) 0.073 SDSS (8) 2.5
J0942+0928/SB80 HST/COS 14168 (16) 0.073 SDSS (8) 2.5
J1105+4444 HST/COS 15840 (13) 0.073 SDSS (8) 2.5
J1129+2034/SB179 HST/COS 15840 (12,13) 0.2 SDSS (8) 2.5
J1132+1411/SB125 HST/COS 15840 (12, 13) 0.073 SDSS (8) 2.5
J1157+3220 HST/COS 15840 (12, 13) 0.073 SDSS (8) 2.5
J1200+1343 HST/COS 15840 (12, 13) 0.073 SDSS (8) 2.5
J1215+2038/SB191 HST/COS 14168 (16) 0.073 SDSS (8) 2.5
J1304−0333/SB9 HST/COS 15185 (15) 0.073 ESO/MUSE 0104.D-0199 2.3
J1314+3452/SB153 HST/COS 15840 (12, 13) 0.073 SDSS (8) 2.5
J1428+1653 HST/COS 13017 (12, 13, 14) 0.2 SDSS (8) 2.5
J1525+0757 HST/COS 13017 (12, 13, 14) 0.2 SDSS (8) 2.5

Notes. Columns are the source ID, the source of UV data, the program ID and reference, the UV spectral resolution, the source of the optical data, the program ID and reference, and the optical spectral resolution. For OSIRIS data, the optical spectra are separated into B and V band and have a different resolution.

References. (1) Crowther et al. (2016); (2) Castro et al. (2018a); (3) Wofford et al. (2023); (4) Hadfield & Crowther (2006); (5) Smith et al. (2016); (6) Sidoli et al. (2006); (7) Esteban et al. (2020); (8) Eisenstein et al. (2011); (9) Chandar et al. (2003); (10) Chandar et al. (2004), (11) Hernandez et al. (2020) (12) Berg et al. (2022); (13) James et al. (2022); (14) Heckman et al. (2015); (15) Senchyna et al. (2021); (16) Senchyna et al. (2017).

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