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Table 3.

Stars brighter than V = 3 located within the IGAPS footprint.

Star RA Dec b V IDs of affected fields
Capella 05 16 41.36 +45 59 52.77 162.589 +4.566 0.08 2298, 2298o
Deneb 20 41 25.92 +45 16 49.22 84.285 +1.998 1.25 6116, 6116o, 6083o,6093
Elnath 05 26 17.51 +28 36 26.83 177.994 −3.745 1.65 2416,2416o,2452,2452o
Alhena 06 37 42.71 +16 23 57.41 196.774 +4.453 1.92 3720,3720o,3690,3690o
γ Cyg 20 22 13.70 +40 15 24.04 78.149 1.867 2.23 5868,5868o,5831,5831o,5855,5855o
β Cas 00 09 10.69 +59 08 59.21 117.528 −3.278 2.27 0043,0043o,0052,0052o,0066
γ Cas 00 56 42.53 +60 43 00.27 123.577 −2.148 2.39 0324,0302,0302o,0296,0296o
δ Cas 01 25 48.95 +60 14 07.02 127.190 −2.352 2.68 0459o,0475o,0477,0477o
μ Gem 06 22 57.63 +22 30 48.90 189.727 4.169 2.87 3413,3413o,3428
γ Per 03 04 47.79 +53 30 23.17 142.067 −4.337 2.93 1051o,1055,1055o
ζ Aql 19 05 24.61 +13 51 48.52 46.854 +3.245 2.99 4483,4483o
ϵ Aur 05 01 58.13 +43 49 23.87 162.788 +1.179 2.99 2084,2084o,2106,2106o,2119

Notes. It is recommended that catalogue users seeking photometry in the vicinity of these objects should check images (Greimel et al., in prep.) to better understand the likely impact these bright stars have on the photometry. For convenience both celestial and Galactic coordinates are given.

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