J/AJ/157/226ivo://CDS.VizieR/J/AJ/157/226doi:10.26093/cds/vizier.51570226CDSFeliz D.L.Blank D.L.Collins K.A.White G.L.Stassun K.G.Curtis I.A.,Hart R.Kielkopf J.F.Nelson P.Relles H.Stockdale C.Jayawardene B.,Shankland P.Reichart D.E.Haislip J.B.Kouprianov V.V.2020-04-06T14:42:59Z2019-08-19T14:13:28ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frphotometryUsing a global network of small telescopes, we have obtained light curves of Proxima Centauri at 329 observation epochs from 2006 to 2017. The planet Proxima b discovered by Anglada-Escude et al. (2016Natur.536..437A) with an orbital period of 11.186 days has an a priori transit probability of ~1.5%; if it transits, the predicted transit depth is about 5 mmag. In Blank et al. (2018AJ....155..228B), we analyzed 96 of our light curves that overlapped with predicted transit ephemerides from previously published tentative transit detections and found no evidence in our data that would corroborate claims of transits with a period of 11.186 days. Here we broaden our analysis, using 262 high-quality light curves from our data set to search for any periodic transit-like events over a range of periods from 1 to 30 days. We also inject a series of simulated planet transits and find that our data are sufficiently sensitive to have detected transits of 5 mmag depth, with recoverability ranging from ~100% for an orbital period of 1 day to ~20% for an orbital period of 20 days for the parameter spaces tested. Specifically, at the 11.186-day period and 5 mmag transit depth, we rule out transits in our data with high confidence. We are able to rule out virtually all transits of other planets at periods shorter than 5 days and depths greater than 3 mmag; however, we cannot confidently rule out transits at the period of Proxima b due to incomplete orbital phase coverage and a lack of sensitivity to transits shallower than 4 mmag.2019AJ....157..226Fhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/157/226CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/AJ/153/93 : MOST photometry of Proxima (Kipping+, 2017)J/AJ/155/12 : Photometry of Proxima Centauri observed by BSST (Liu+, 2018)J/AJ/156/234 : KELT transit false positive catalog for TESS (Collins+, 2018)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/157/226https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/157/226http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/157/226https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/157/226https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/157/226http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/157/226GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/AJ/157/226/table3Photometry of Proxima CentaurirecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintBJDBarycentric Julian Date in the Barycentric Dynamical Time of observation (TDB)dtime.epochdoubleFlux[0.92078/1.08324] Undetrended normalized relative flux (1)phot.flux;arith.ratiodoublee_Flux[0.00069/0.22068] Uncertainty in Fluxstat.error;phot.fluxdoubleJ/AJ/157/226/table4Detrended photometry of Proxima CentaurirecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintBJDBarycentric Julian Date in the Barycentric Dynamical Time of observation (TDB)dtime.epochdoubleFlux[0.958507/1.081338] Detrended normalized relative flux (1)phot.flux;arith.ratiodoublee_Flux[0.000734/0.11062] Uncertainty in Fluxstat.error;phot.fluxdouble