![]() This object appears to be another case of the "discovery" of a known variable object around its maximum brightness masquerading as a possible extragalactic nova, e.g., see ATel # 4314, # 4315, # 4341, # 6359, and # 6388. 3.6-m Canada-France-Hawaii telescope, 2.2-m University of Hawaii reflector. 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. Science The Lambda-Cold Dark Matter hierarchical paradigm is robust to large scale observables, and it is on galactic scales that our understanding of the cosmological evolution of matter is most incomplete. ![]() 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. PI: Alan McConnachie, Herzberg Astronomy and Astrophysics Research Center, Victoria, Canada. 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. The headquarters are located in Waimea, which is about 90min from the top of the mountain. It is located near the summit of Maunakea, at an elevation of 4200m, on the Big Island of Hawaii. UBVRI Photometry of Stars in M31 and M33 by Massey et al. Canada-France-Hawaii Telescope Corporation, P.O. The object is also found in the Survey of Local Group Galaxies Currently Forming Stars: I. SITELLE is a Michelson-type interferometer able to reconstruct the spectrum of every light source within its 11 arcmin field of view in filter-selected bands of the visible (350900 nm). = +30o35'56".3 which is only 0.48" from the position of the PNV J01335049+3035559. We present an overview of SITELLE, an Imaging Fourier Transform Spectrometer (iFTS) available at the 3.6-m CanadaFranceHawaii Telescope. 2003) obtained for the CFHT Legacy Survey (CFHTLS) and analysed as the CFHT Lensing Survey (CFHTLenS): Fig. Catalogue of 36000 variable point sources, Hartman et al. In this paper, we describe how we have made weak lensing measurements using ground-based data from the CanadaFranceHawaii Telescope (CFHT) MegaCam camera (Boulade et al. 233761 in the Deep Canada-France-Hawaii Telescope photometric survey of the entire M33 galaxy - I. 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. Banner image: the Canada-France-Hawaii Telescope at Maunakea, Hawaii, operational since 1979. ![]()
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