CSI2264 Spitzer Light Curve Table Virtual Observatory Resource

Authors
  1. CSI2264 team
  2. Published by
    NASA/IPAC Infrared Science Archive
Abstract
The CSI 2264 project performed photometric monitoring of young NGC 2264 cluster members using the Spitzer Infrared Array Camera (IRAC; Fazio et al. 2004) and the Convection, Rotation and Planetary Transits satellite (CoRoT; Baglin et al. 2006) simultaneously. Thirteen other telescopes monitored the region at different times concurrently with (or closely in time to) the primary Spitzer and CoRoT joint campaign. The CSI 2264 project is described in detail in Cody et al. (2014).

This table contains Spitzer light curves for objects that are very likely NGC 2264 members (using the criteria described in Cody et al. 2014), and that have at least 15 good data points in one of the IRAC bands. Only data from Warm Spitzer cycle 8 program 80040 (Dec. 2011- Jan. 2012) are provided. There are many rows for each object, because each object has many epochs of data. Columns 11, 12, and 13 (the IRAC excess flag and the light curve types) are duplications of information found in our first table, but are repeated here to make it easy for users to, e.g., pull out all of the light curves of a specific type.
Keywords
  1. star formation
See also HTML
https://irsa.ipac.caltech.edu/data/SPITZER/CSI2264/gator_docs/csi2264t3_colDescriptions.html
IVOA Identifier IVOID
ivo://irsa.ipac/Spitzer/Catalog/CSI2264/CSI2264_Spitzer_LC

Access

IVOA Cone Search SCS
For use with a cone search client (e.g., TOPCAT).
https://irsa.ipac.caltech.edu/SCS?table=csi2264t3&
IVOA Table Access TAP
https://irsa.ipac.caltech.edu/TAP
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).
Web browser access HTML
https://irsa.ipac.caltech.edu/cgi-bin/Gator/nph-dd?catalog=csi2264t3

History

2015-01-14T02:45:00Z
Resource record created
2014-11-20
update

Contact

Name
IRSA Support Team
Postal Address
E-Mail
irsasupport@ipac.caltech.edu
Telephone