Opt & NIR SMARTS/ANDICAM photometry for DQ Tau (Muzerolle+, 2019)

We observed DQ Tau, during 2012 Nov 15-2013 Jan 30 and 2013 Sep 9 - 2014 Feb 3, with the ANDICAM instrument on the CTIO 1.3m telescope, operated by the SMARTS Consortium. The optical channel has a field of view of ~6'x6' and detector pixel scale of ~0.3", while the NIR channel has a field of view of ~2.4'x2.4' and detector pixel scale of ~0.2". We used BVI filters (standard KPNO Johnson-Cousins) with the optical channel and JHK filters (CIT/CTIO) with the infrared channel. We observed DQ Tau with the SpeX spectrograph at Infrared Telescope Facility (IRTF) on 2012 Dec 13, 22, and 30 and 2013 Jan 5 and 8; with a combined wavelength coverage of 0.8 to 5um for a spectral resolution of ~1000 (see Figure 1).

Identifier
Source http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/ApJ/877/29
Related Identifier https://ui.adsabs.harvard.edu/abs/2019ApJ...877...29M
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_datacite&identifier=ivo://CDS.VizieR/J/ApJ/877/29
Provenance
Creator Muzerolle J., Flaherty K., Balog Z., Beck T., Gutermuth R.
Publisher CDS
Contributor International Virtual Observatory Alliance (IVOA)
Publication Year 2021
Rights public
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Format text/xml+votable
Version 20-Nov-2020
Discipline Observational Astronomy;Stellar Astronomy