VizieR Online Data Catalog: Multiwavelength obs. of gamma-ray NOVA Sco 2012 (Finzell+, 2018)
Abstract
V1324 Sco falls within one of the fields that the Microlensing Observations in Astrophysics collaboration (MOA; Wagner+ 2012ATel.4157....1W) continually observes with the MOAII 1.8m telescope at Mt. Johns Observatory in New Zealand. V1324 Sco was initially detected in 2012 April by their high-cadence I-band photometry. We take 2012 June 1 to be day 0, or the start of the nova outburst. Apart from the standard I broadband filter, the MicroFUN group (http://www.astronomy.ohio-state.edu/~microfun/) follow-up observations also used V and I Bessel filters. Other observations were made in B, V, and I filters using the Small & Moderate Aperture Research Telescope System (SMARTS) 1.3m telescope and Auckland Observatories. Along with the MOA and MicroFUN data, we also present multicolor photometry from Fred Walter's ongoing Stony Brook/SMARTS Atlas of (mostly) Southern Novae (see Walter+ 2012PASP..124.1057W for further information on this data set), as well as data from the American Association of Variable Star Observers (AAVSO). The SMARTS data use the ANDICAM instrument on the 1.3m telescope and provide both optical (B, V, R, I) and near-IR (J, H, K) filters going from day +35 to day +124, while the AAVSO data use optical (V, B, R) filters and go from day +7 to day +445. Finally, we incorporate the UV data taken contemporaneously with the X-ray observations. The UV data come from the Ultraviolet/Optical Telescope (UVOT) on board Swift. Each observation was taken using the UVM2 filter, which is centered on 2246Å. See Table 1 for the UV-Opt-IR data.
We obtained sensitive radio observations (spanning 2012 Jun to 2014 Dec) of V1324 Sco between 2012 June 26 and 2014 December 19 with the Karl G. Jansky Very Large Array (VLA) through programs S4322, 12A-483, 12B-375, 13A-461, 13B-057, and S61420 (coverage from 4 to 37GHz). See section 3. All spectroscopic observations (spanning 2012 Jun to 2013 Aug) taken with the VLT/UVES, Vixen/LISA, SMARTS 1.5m, MIKE, LBT/MODS1 or SOAR/Goodman, are listed in Table 3. See section 4. Multiple X-ray observations were made using the Swift X-ray Telescope (XRT), all of them yielding non-detections. See section 5. (3 data files).- Publication:
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VizieR Online Data Catalog
- Pub Date:
- September 2018
- DOI:
- 10.26093/cds/vizier.18520108
- Bibcode:
- 2018yCat..18520108F
- Keywords:
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- Novae;
- Photometry: UBVRI;
- Radio continuum;
- Spectra: optical