M67 Kepler/K2 variable stars

DOI

In the third paper of this series we continue the exploitation of Kepler/K2 data in dense stellar fields using our PSF-based method. This work is focused on a ~720-arcmin^2^ region centred on the Solar-metallicity and Solar-age open cluster M 67. We extracted light curves for all detectable sources in the Kepler channels 13 and 14, adopting our technique based on the usage of a high-angular-resolution input catalogue and target-neighbour subtraction. We detrended light curves for systematic errors, and searched for variables and exoplanets using several tools. We found 451 variables, of which 299 are new detection. Three planetary candidates were detected by our pipeline in this field. Raw and detrended light curves, catalogues, and K2 stacked images used in this work will be released to the community.

Cone search capability for table J/MNRAS/463/1831/m67-ch13 (Input catalog for Ch13)

Cone search capability for table J/MNRAS/463/1831/m67-ch14 (Input catalog for Ch14)

Cone search capability for table J/MNRAS/463/1831/var-ch13 (Variable stars in K2/C5/M67 field (Ch13))

Cone search capability for table J/MNRAS/463/1831/var-ch14 (Variable stars in K2/C5/M67 field (Ch14))

Identifier
DOI http://doi.org/10.26093/cds/vizier.74631831
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/463/1831
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/463/1831
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/463/1831
Provenance
Creator Nardiello D.; Libralato M.; Bedin L.R.; Piotto G.; Borsato L.; Granata V.,Malavolta L.; Nascimbeni V.
Publisher CDS
Publication Year 2018
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy