| cting transiting planetary candidates from photometric surveys. It complements official candidate lists such as the Kepler Objects of Interest and TESS Objects of Interest. The methodology is described by Caceres, Feigelson et al. (2019AJ....158...58C) and Melton, Feigelson et al. (2024AJ....167..202M). The ARPS methodology produces catalogs that are both sensitive to smaller planets and relatively free of contaminating False Positive and False Alarm. The procedure has been applied to the 4-year Kepler survey (Caceres, Feigelson et al. 2019AJ....158...58C) with the IAU-approved KARPS acronym, and has now been applied to the TESS Year 1 survey of the southern sky (DTARPS-S, Melton, Feigelson et al. 2024AJ....167..203M). The DTARPS-S objects are the host stars of candidate transiting planets; they generally have bright magnitudes with V<12 and are thus already in historical stellar catalogs (BD, TYC, Gaia, etc). The DTARPS-S catalog is provided in the Machine Readable Table from the Astronomical Journal (Melton, Feigelson et al. 2024AJ....167..203M). | |
| Notes: | We are currently preparing a similar catalog based on the TESS Year 2 survey of the northern hemisphere, and expect to request IAU approval for the DTARPS-N catalog. In the future, we hope to produce other catalogs such as DTARPS-E from TESS survey of the ecliptic pole regions. |
| Ref: | =2024AJ....167..203M |
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