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|Title:||VizieR Online Data Catalog: Follow-up photometry of M101 OT2015-1 (Blagorodnova+, 2017)||Authors:||Blagorodnova, N.
Kasliwal, M. M.
Cody, A. M.
Doran, G. B.
ELIAS DE LA ROSA, NANCY DEL CARMEN
Kudritzki, R. -P.
Kulkarni, S. R.
Masci, F. J.
Vreeswijk, P. M.
|Issue Date:||2017||Journal:||VizieR Online Data Catalog||First Page:||J/ApJ/834/107||Abstract:||The location of M101-OT2015-1 has been serendipitously imaged by numerous telescopes and instruments over the last 15 years (from 2000 to 2015). Our best quality pre-discovery image (seeing of 0.55") is an r-band exposure at -3625 days pre-peak from the Canada-France-Hawaii Telescope (CFHT). <P />The historical optical data for M101-OT was retrieved from the CFHT MegaPrime and CFHT12K/Mosaic, using single and combined exposures, Pan-STARRS-1/GPC1 (PS1), Isaac Newton Telescope/Wide Field Camera (INT/WFC), and Sloan Digital Sky Survey (SDSS) DR 10 (Ahn+ 2014, see V/147). Unfortunately, there are no HST images covering the location of the source. <P />Post-discovery optical magnitudes were obtained from the reported followup astronomer's telegrams (ATels), Liverpool Telescope (LT), the Nordic Optical Telescope (NOT), and the Palomar P48 and P60 telescopes. The infrared data were retrieved from CFHT/WIRCam, UKIRT/WFCAM, and the Spitzer Infrared Array Camera in 3.6 and 4.5um as part of the SPitzer InfraRed Intensive Transients Survey (SPIRITS) (Kasliwal+, 2017ApJ...839...88K). Details of pre-discovery photometry and post-discovery optical photometry may be found in the Appendices Tables 1 and 2, respectively. <P />We obtained spectra of M101-OT using a range of facilities in 2015 Feb-Jul. (3 data files).||URI:||http://hdl.handle.net/20.500.12386/27165||URL:||http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/ApJ/834/107||DOI:||10.26093/cds/vizier.18340107||Bibcode ADS:||2017yCat..18340107B||Fulltext:||open|
|Appears in Collections:||4.06 Banche Dati|
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