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).

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
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>
Format text/xml+votable
Version 20-Nov-2020
Discipline Observational Astronomy;Stellar Astronomy