Table 1.

Differential photometry of SGR 0501+4516 relative to 2MASS stars within the field of view of NIRI, UFTI, and LIRIS, plus HST NIR magnitudes for SGR 0501+4516 in 2010, 2012, and 2020 (given in the last four rows).

Start time Exposure time Filter Magnitude Telescope + instrument
Year-month-date-UT (seconds) (Vega)
2008 08 25 03:11:12 6525 KS 19.12 ± 0.05 WHT + LIRIS
2008 08 31 02:31:01 2085 KS 19.22 ± 0.11 WHT + LIRIS
2008 09 01 03:44:35 2250 KS 19.27 ± 0.10 WHT + LIRIS
2008 09 06 04:35:00 1188 KS 19.05 ± 0.16 WHT + LIRIS
2008 09 20 03:43:15 3735 KS 19.24 ± 0.15 WHT + LIRIS
2008 08 23 14:27:03 1020 J 21.02 ± 0.05 Gemini + NIRI
2008 09 01 14:28:09 960 J 21.07 ± 0.07 Gemini + NIRI
2008 08 23 14:15:25 480 H 19.95 ± 0.04 Gemini + NIRI
2008 08 23 14:03:44 510 K 18.76 ± 0.07 Gemini + NIRI
2008 08 26 15:04:16 480 K 18.85 ± 0.07 Gemini + NIRI
2008 09 01 14:53:07 900 K 19.06 ± 0.08 Gemini + NIRI
2009 01 28 07:42:57 170 K 19.51 ± 0.28 Gemini + NIRI
2009 04 03 06:16:53 270 K 20.02 ± 0.34 Gemini + NIRI
2009 11 02 10:57:00 3120 K 20.41 ± 0.10 Gemini + NIRI
2008 08 22 14:31:39 270 H 19.67 ± 0.14 UKIRT + UFTI
2008 08 22 14:27:52 405 J 21.28 ± 0.34 UKIRT + UFTI
2008 08 22 14:34:43 270 K 18.61 ± 0.11 UKIRT + UFTI
2010 10 19 02:37:24 2797 F160W 22.45 ± 0.02 HST + WFC3/IR
2012 10 08 19:23:37 2797 F160W 22.48 ± 0.02 HST + WFC3/IR
2020 08 04 11:42:00 ( † ) 598 F125W 23.33 ± 0.07 HST + WFC3/IR
2020 08 04 11:55:03 ( † ) 598 F160W 22.56 ± 0.07 HST + WFC3/IR

Notes. An additional error of about 0.07 magnitudes has been added in quadrature to the K-band magnitude errors: this is the scatter in the transformation of 2MASS reference star magnitudes from Ks to K, using Ks = K + 0.002 + 0.026(J − K). Magnitudes are not corrected for Galactic extinction (see Fig. 4). ( † ) Photometry from Chrimes et al. (2022b).

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