NGC 2264: VRIH{alpha} photometry

DOI

The young open cluster NGC 2264 was observed on 2002 January 67 with the CFH12K mosaic CCD on the 3.6m Canada-France-Hawaii Telescope to investigate the shape of the initial mass function (IMF). In order to select the pre-main-sequence (PMS) members more completely, Chandra X-Ray Observatory archival data were retrieved and used for the identification of X-ray-emitting weak-line T Tauri stars. In addition, the (R-I, V-I) diagram was used to exclude background late-type giants, and a statistical approach was applied to estimate the number of contaminating foreground main-sequence stars.

Cone search capability for table J/AJ/128/1684/table1 (Photometric data)

Cone search capability for table J/AJ/128/1684/table3 (X-Ray sources detected from pwdetect)

Identifier
DOI http://doi.org/10.26093/cds/vizier.51281684
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/AJ/128/1684
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/128/1684
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/128/1684
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/AJ/128/1684
Provenance
Creator Sung H.; Bessell M.S.; Chun M.-Y.
Publisher CDS
Publication Year 2005
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; Cosmology; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy