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Titolo: | VizieR Online Data Catalog: SN 2007on and SN 2011iv light curves (Gall+, 2018) | Autori: | Gall, C. Stritzinger, M. D. Ashall, C. Baron, E. Burns, C. R. Hoeflich, P. Hsiao, E. Y. Mazzali, P. A. Phillips, M. M. Filippenko, A. V. Anderson, J. P. Benetti, S. Brown, P. J. Campillay, A. Challis, P. Contreras, C. ELIAS DE LA ROSA, NANCY DEL CARMEN Folatelli, G. Foley, R. J. Fraser, M. Holmbo, S. Marion, G. H. Morrell, N. Pan, Y. -C. Pignata, G. Suntzeff, N. B. Taddia, F. Torres Robledo, S. Valenti, S. |
Data pubblicazione: | 2017 | Rivista: | VizieR Online Data Catalog | Da pagina:: | J/A+A/611/A58 | Abstract: | Detailed optical and NIR light curves of SN 2007on obtained by the first phase of the Carnegie Supernova Project (CSP-I, 2004-2009; Hamuy et al., 2006PASP..118....2H) were published by Stritzinger et al. (2011, Cat. J/AJ/142/156).UV uvw2-, uvm2-, and uvw1-band imaging of both SN 2007on and SN 2011iv were obtained with Swift (+ UVOT). Photome- try of SN 2007on and SN 2011iv was computed following the method described in detail by Brown et al. (2014Ap&SS.354...89B), who use the calibration published by Breeveld et al. (2011, AIPCS, 1358, 373). The Swift UVOT images and photometry are also available as part of the Swift Optical Ultraviolet Supernova Archive (SOUSA; Brown et al. 2014Ap&SS.354...89B). Optical ugriBV-band imaging of SN 2007on and SN 2011iv was obtained with the Henrietta Swope 1.0m telescope (+ SITe3 direct CCD camera) located at the Las Campanas Observatory (LCO). The NIR YJH-band imaging of SN 2007on was obtained with the Swope (+ RetroCam) and the Irenee du Pont 2.5m (+ WIRC: Wide Field Infrared Camera) telescopes (Stritzinger et al., Cat. J/AJ/142/156), while in the case of SN 2011iv all NIR YJH-band imaging was taken with RetroCam attached to the Irenee du Pont telescope. The optical local sequence is calibrated relative to Landolt (1992AJ....104..372L) (BV) and Smith et al. (2002AJ....123.2121S) (ugri) standard-star fields observed over multiple photometric nights. The NIR J-band and H-band local sequences were calibrated relative to the Persson et al. (1998AJ....116.2475P) standard stars, while the Y- band local sequence was calibrated relative to standard Y-band magnitudes computed using a combination of stellar atmosphere models (Castelli & Kurucz, 2003, IAUSymp, 210, A20) with the J-Ks colours of the Persson et al. standard-star catalogue (Hamuy et al., 2006PASP..118....2H). (5 data files). | URI: | http://hdl.handle.net/20.500.12386/27164 | URL: | http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/611/A58 | DOI: | 10.26093/cds/vizier.36110058 | Bibcode ADS: | 2017yCat..36110058G | Fulltext: | open |
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