Open Access

Table A.2.

Datasets used to obtain the final models for each of the 35 analysed events. The description of the columns is at the end of the table. A full version of this table is available at the CDS.

GaiaDR3- Survey, Num. k GaiaDR3- Survey, Num. k
ULENS- filter of points ULENS- filter of points
018 Gaia, G 24 1.00
Gaia, GBP 22 1.00
Gaia, G 27 1.00 Gaia, GRP 22 3.13
003 Gaia, GBP 27 1.00 OGLE, I 2780 1.02
Gaia, GRP 27 1.00 KMTNet SAAO, I 563 4.47
ASASSN, V 84 1.79 KMTNet CTIO, I 840 1.97
KMTNet SSO, I 750 2.11

... ... ... ... ... ... ...

Gaia, G 21 1.00 363 Gaia, G 23 1.00
Gaia, GBP 17 Gaia, GBP 19
Gaia, GRP 19 1.00 Gaia, GRP 22
359 OGLE, I 553 1.00 OGLE, I 824 1.00
KMTNet SAAO, I 260 2.79 KMTNet SAAO, I 780 1.68
KMTNet CTIO, I 994 1.58 KMTNet CTIO, I 386 1.39
KMTNet SSO, I 895 1.88 KMTNet SSO, I 364 1.45

Notes: The table contains the event name, the name of the survey and the filter, the number of points used to obtain the best models, and the scale factor k used to re-scale the photometric uncertainties. Light curves not used in the modelling process are marked with a strike-through. Light curves that were cleaned using the procedure outlined in Sect. 4 are marked in bold.

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