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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