Table 2.
Gaia DR2 source identifier, right ascension and declination and their standard deviation (in milliarcseconds) at epoch and magnitude of the stars of the catalogue Gaia DR2 involved in occultations presented in this paper.
Date | Gaia source identifier | Right ascension | Declination | σα | σδ | Gmag |
---|---|---|---|---|---|---|
1988-06-09 | 3652000074629749376 | 14h52m09.962000s | +00°45′03.30297″ | 2.14 | 2.06 | 12.1 |
2002-07-20 | 4333071455580364160 | 17h00m18.029957s | −12°41′42.01220″ | 1.12 | 0.73 | 12.6 |
2002-08-21 | 4333042833914281856 | 16h58m49.431538s | −12°51′31.85910″ | 1.87 | 1.12 | 15.4 |
2006-06-12 | 4124931567980280832 | 17h41m12.074271s | −15°41′34.47421″ | 0.63 | 0.49 | 14.7 |
2007-03-18 | 4144912550502784384 | 17h55m05.699098s | −16°28′34.36682″ | 0.74 | 0.60 | 14.8 |
2007-06-14 | 4147858103406546048 | 17h50m20.744804s | −16°22′42.22719″ | 0.83 | 0.73 | 15.3 |
2008-06-22 | 4144621347334603520 | 17h58m33.013236s | −17°02′38.39643″ | 0.67 | 0.54 | 12.3 |
2008-06-24 | 4144621244254585728 | 17h58m22.390423s | −17°02′49.36558″ | 0.93 | 0.78 | 15.6 |
2010-02-14 | 4096385295578625536 | 18h19m14.378482s | −18°16′42.35590″ | 0.50 | 0.42 | 10.3 |
2010-06-04 | 4096389556186605568 | 18h18m47.930034s | −18°12′51.82967″ | 0.37 | 0.31 | 14.8 |
2011-06-04 | 4093175335706340480 | 18h27m53.819996s | −18°45′30.78871″ | 0.62 | 0.50 | 16.4 |
2011-06-23 | 4093163211131448704 | 18h25m55.479351s | −18°48′07.09094″ | 0.35 | 0.31 | 14.0 |
2012-07-18 | 4092849712861519360 | 18h32m14.673688s | −19°24′19.34329″ | 0.19 | 0.17 | 14.4 |
2013-05-04 | 4086200313156846336 | 18h47m52.531982s | −19°41′24.39714″ | 0.10 | 0.09 | 14.2 |
2014-07-23 | 4085914882468876672 | 18h49m31.736687s | −20°22′23.82473″ | 0.21 | 0.19 | 17.2 |
2014-07-24 | 4085914745029913216 | 18h49m26.511650s | −20°22′36.98627″ | 0.39 | 0.35 | 18.1 |
2015-06-29 | 4084956039611370112 | 19h00m49.474124s | −20°41′40.81016″ | 0.04 | 0.04 | 12.0 |
2016-07-19 | 4082062610353732096 | 19h07m22.117772s | −21°10′28.43508″ | 0.05 | 0.05 | 13.9 |
Notes. The coordinates and their precision are provided for the epoch of the occultation taking into account the proper motions and parallax, and their precision.
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