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==Naming convention== [[Image:Keplers supernova.jpg|thumb|Multi-wavelength [[X-ray]], [[infrared]], and [[optical]] compilation image of [[Johannes Kepler|Kepler's]] [[supernova remnant]], [[SN 1604]]]]Supernova discoveries are reported to the [[International Astronomical Union]]'s [[Central Bureau for Astronomical Telegrams]], which sends out a circular with the name it assigns to that supernova.<ref>{{Cite web |title=What Kinds of Discovered Objects to Report for IAUC Publication |url=http://www.cbat.eps.harvard.edu/WhatToReport.html |access-date=2023-03-08 |website=cbat.eps.harvard.edu}}</ref> The name is formed from the prefix ''SN'', followed by the year of discovery, suffixed with a one or two-letter designation. The first 26 supernovae of the year are designated with a capital letter from ''A'' to ''Z''. Next, pairs of lower-case letters are used: ''aa'', ''ab'', and so on. Hence, for example, ''SN 2003C'' designates the third supernova reported in the year 2003.<ref>{{cite journal |last1=Kirshner |first1=R. P. |year=1980 |title=Type I supernovae: An observer's view |journal=[[AIP Conference Proceedings]] |volume=63 |pages=33β37 |bibcode=1980AIPC...63...33K |doi=10.1063/1.32212 |hdl=2027.42/87614 |url=https://deepblue.lib.umich.edu/bitstream/handle/2027.42/87614/33_1.pdf |hdl-access=free |access-date=20 March 2020 |archive-date=7 August 2020 |archive-url=https://web.archive.org/web/20200807191945/https://deepblue.lib.umich.edu/bitstream/handle/2027.42/87614/33_1.pdf |url-status=live }}</ref> The last supernova of 2005, SN 2005nc, was the 367th (14 Γ 26 + 3 = 367). Since 2000, professional and amateur astronomers have been finding several hundred supernovae each year (572 in 2007, 261 in 2008, 390 in 2009; 231 in 2013).<ref> {{cite web |title=List of Supernovae |url=http://cbat.eps.harvard.edu/lists/Supernovae.html |publisher=[[International Astronomical Union|IAU Central Bureau for Astronomical Telegrams]] |access-date=25 October 2010 |url-status=live |archive-url=https://web.archive.org/web/20101112022554/http://www.cbat.eps.harvard.edu/lists/Supernovae.html |archive-date=12 November 2010 }}</ref><ref> {{cite web |title=The Padova-Asiago supernova catalogue |url=http://graspa.oapd.inaf.it/cgi-bin/sncat.php |publisher=[[Asiago Astrophysical Observatory|Osservatorio Astronomico di Padova]] |access-date=10 January 2014 |url-status=live |archive-url=https://web.archive.org/web/20140110184455/http://graspa.oapd.inaf.it/cgi-bin/sncat.php |archive-date=10 January 2014 }}</ref> Historical supernovae are known simply by the year they occurred: SN 185, SN 1006, SN 1054, SN 1572 (called ''Tycho's Nova'') and SN 1604 (''Kepler's Star'').<ref>{{Cite book |last1=Stephenson |first1=F. Richard |url=https://www.worldcat.org/oclc/50403827 |title=Historical Supernovae and Their Remnants |date=2002 |publisher=Clarendon Press |first2=David A. |last2=Green |isbn=0-19-850766-6 |location=Oxford |oclc=50403827 |pages=1–5, 60, 82}}</ref> Since 1885 the additional letter notation has been used, even if there was only one supernova discovered that year (for example, SN 1885A, SN 1907A, etc.); this last happened with SN 1947A. ''SN'', for SuperNova, is a standard prefix. Until 1987, two-letter designations were rarely needed; since 1988, they have been needed every year. Since 2016, the increasing number of discoveries has regularly led to the additional use of three-letter designations.<ref>{{cite web| url = https://sne.space/| title = Open Supernova Catalog| access-date = 5 February 2020| archive-date = 3 March 2016| archive-url = https://web.archive.org/web/20160303230459/https://sne.space/| url-status = live}}</ref> After zz comes aaa, then aab, aac, and so on. For example, the last supernova retained in the Asiago Supernova Catalogue  when it was terminated on 31 December 2017 bears the designation SN 2017jzp.<!-- SN 2017jmk was the last addition to the catalogue, but jzp is the highest-lettered designation --><ref>Padova-Asiago Supernova Group, [http://graspa.oapd.inaf.it/asnc.html Asiago Supernova Catalogue], accessed 2023-12-27</ref>
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