PLATO 2.0 Survey

The expected PLATO fields are shown in Fig. 11. Its northern long-pointing field is centered near a galactic latitude of +30° and a longitude of 65° (i.e. RA 17h40m, DEC+39°40’) and includes the Kepler field. It is not finalized yet. We are expecting ≈2300 square degrees for the full PLATO FOV (48.5° × 48.5° with “round” field edges), which would formally require ≈44 individual pointings by the BMK10k. The Tenerife Teide Observatory geographic coordinates are 28°18′00′′N 16°30′35′′W.

Our operations goal is to cover the full PLATO long-pointing field once per night. This is only feasible in a single-filter operation. If we assume a (field) overlapping factor of near 30%, a total of 60 pointings is required by BMK10k to cover the full 2300 square degrees of PLATO. Due to CCD image dynamics and full-well capacity, we envision three exposures per pointing (200s, 60s, and 10s). Detailed exposure times are still tbd.

The first pointing would start at low declination at the west-most observable field depending on the telescope mount and dome limits. Consecutive fields would be observed at increasing declination. The overlap of the pointings is still to be considered. Each pointing has a long exposure with 200s (tbc), a middle exposure with 60s, and a short exposure of 10s (tbc). The single long exposure would cover the magnitude range fainter than 10th mag, the middle exposure will cover stars up to 9th mag, and the short exposure would favor the targets brighter than 8 th mag (being 3 mags brighter the exposure has to be shortened by a factor of 7.5 to ensure the proper magnitude range). The exposure times are restricted by background contamination in the Milky Way as well as atmospheric influences as moon-light or sky-glow and also by the tracking precision. Fainter stars than 16 th mag are reached with stacking the consecutive images.

From the two constraints – PLATO field sky location and BMK10k geographic location – follows the visibility of the initial northern field with a minimum of 1300 observing hours per observing season (see Fig. 12a). Note that the initial northern field is a summer field and thus well suited for the Canary island weather pattern (great in summer, poor in winter).

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