The existing counterpart showing large amplitude brightness changes and a red color suggests that the likely classification of the PNV J01335049+3035559 should be a Red LPV in M33, not a nova. A comparison of archival Massey's I-band and R-band images available through the link below clearly shows large amplitude variability of the object and its significantly red color. Observations can be queried by various criteria such as object name, position and RunID and retrieved.
#CANADA FRANCE HAWAII TELESCOPE ALAN ARCHIVE#
Since Massey's magnitudes are averages of different numbers of measurements obtained in different epochs in each band, they are influenced by the variability of the object. 233761 in the Deep Canada-France-Hawaii Telescope photometric survey of the entire M33. The CFHT Science Archive provides access to observations obtained with the Canada-France-Hawaii Telescope (CFHT) on Maunakea, Hawaii. USA) casts a new light on the formation process of the famous group of 5 colliding. UBVRI Photometry of Stars in M31 and M33 by Massey et al. The object is also found in the Survey of Local Group Galaxies Currently Forming Stars: I. = +30o35'56".3 which is only 0.48" from the position of the PNV J01335049+3035559. of Andromeda (M31) and the Triangulum Galaxy (M33) using the Canada-France-Hawaii Telescope (CFHT). Catalogue of 36000 variable point sources, Hartman et al. Canada-France-Hawaii Telescope Corporation, P.O. 233761 in the Deep Canada-France-Hawaii Telescope photometric survey of the entire M33 galaxy - I. 27 - 29 March 2013, Imiloa Astronomy Center of Hawaii, (University of Hawaii at Hilo), Hilo, Hawaii. Titan was observed with the Adaptive Optics Bonette at the CanadaFranceHawaii Telescope during October 27th 1998 (UTC), when the satellite was at greatest. FW13’s existence was confirmed by the Canada-France-Hawaii Telescope as well as two other observatories in Arizona according to Scientific American before being officially listed on April.
#CANADA FRANCE HAWAII TELESCOPE ALAN UPGRADE#
A search for known variable sources close to the position of the PNV J01335049+3035559 reveals a variable object (having amplitude of the brightness changes > 1.4 mag in Sloan i'-band) designated No. The Maunakea Spectroscopic Explorer (MSE) project is an enterprise to upgrade the existing Canada-France- Hawaii observatory into a spectroscopic facility.
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