ASAS-SN bright supernova catalogue 2016 : J/MNRAS/471/4966

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Authors : Holoien T.W.-S. orcid , Brown J.S., Stanek K.Z. (hide) , Brown J.S., Stanek K.Z. et..al

VizieR DOI : 10.26093/cds/vizier.74714966
Bibcode : 2017MNRAS.471.4966H (ADS) (Simbad) (Objects)
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CDS Keywords : Surveys; Supernovae; Photometry, SDSS; Photometry, infrared; Redshifts
UAT : Surveys, Supernovae, Optical astronomy, Sloan photometry, Infrared photometry, Redshifted

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Inserted into VizieR : 22-Jul-2020
Last modification : 17-Aug-2024

The ASAS-SN bright supernova catalogue - III. 2016. (2017)

Keywords : catalogues - surveys - supernovae general

Abstract:This catalogue summarizes information for all supernovae discovered by the All-Sky Automated Survey for SuperNovae (ASAS-SN) and all other bright (m_peak_ <=17), spectroscopically confirmed supernovae discovered in 2016. We then gather the near-infrared through ultraviolet magnitudes of all host galaxies and the offsets of the supernovae from the centres of their hosts from public data bases. We illustrate the results using a sample that now totals 668 supernovae discovered since 2014 May 1, including the supernovae from our previous catalogues, with type distributions closely matching those of the ideal magnitude limited sample from Li et al. This is the third of a series of yearly papers on bright supernovae and their hosts from ...(more)
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Table 1 includes information for all SNe discovered by ASAS-SN between 2016 January 1 and 2016 December 31. As in Holoien et al. (2017, Cat.J/MNRAS/464/2672 and Cat. J/MNRAS/467/1098), all names, discovery dates and host names are taken from our discovery ATels, all of which are cited in Table 1. We also include the SN names designated by TNS, the official International Astronomical Union (IAU) mechanism for reporting new astronomical transients. In Table 2, we give information for all spectroscopically confirmed SNe with peak magnitudes of m_peak_<=17 that were discovered by other professional and amateur SN searches between 2016 January 1 and 2016 December 31. For the host galaxies of both SN samples, we collected Galactic extinction estimates for the direction to the host and host magnitudes spanning from the near-ultraviolet (NUV) to the infrared (IR) wavelengths. We present these data in Tables 3 and 4 for ASAS-SN hosts and non-ASAS-SN hosts, respectively. 


                


                

                    

                


                

                    

                


                

                    
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