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Table 1.

Dates of the observations made with different instruments.

Date Facility Type Filters λmean Fλ Reference
[Å] [×10−16 erg s−1 cm−2 Å−1]
1999-11-22 DENIS p I 7930 1.43 ± 0.16 (1)
2003-06-11 HST STIS s FUV 1545 29.89 ± 0.20
2005-09-21 CRTS start p Clear 6178 4.89 ± 0.68 (2)
2012-12-18 CRTS end p Clear 6178 4.42 ± 0.52 (2)
2006-10-24 GALEX p FUV 1545 28.9 ± 1.4 (3)
2006-10-24 GALEX p NUV 2345 16.48 ± 0.51 (3)
2011-10-30 GALEX p NUV 2345 13.32 ± 0.62 (3)
2010-04-13 HST COS s FUV 1545 25.151 ± 0.033
2013-10-01 DES p g 4862 4.102 ± 0.035 (4)
2013-10-01 DES p r 6460 2.566 ± 0.019 (4)
2013-10-01 DES i V 5524 3.290 ± 0.040
2014-09-24 MUSE s V 5524 3.4125 ± 0.0062
2014-12-21 MUSE s V 5524 3.2494 ± 0.0055
2014-11-09 SkyMapper p g 5099 3.80 ± 0.24 (5)
2014-11-09 SkyMapper p r 6157 3.152 ± 0.053 (5)
2014-11-09 SkyMapper i V 5524 3.52 ± 0.25
2017-01-03 SAAO p V 5524 3.88 ± 0.32 (6)
2017-01-03 SAAO p I 8859 2.263 ± 0.047 (6)

Notes. ‘Type’ column denotes if data product is photometry (p), was computed from spectroscopy (s), or was interpolated from neighboring filters (i). The subsequent columns present filter name, observed mean wavelength of the filter, and observed flux. In the last column, we give references to the original photometric measurements, catalogs, or surveys used to obtain the flux values.

References. (1) Baudrand et al. (2007); (2) Drake et al. (2009); (3) Martin et al. (2005); (4) Abbott et al. (2018); (5) Wolf et al. (2018); (6) Bankowicz et al. (2020).

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