List of supernovae#Supernova statistics

! Supernova
designation
(year)

! Constellation

! Observations

! data-sort-type="number" | Apparent
magnitude

! Distance
(light years)

! Type

! width=160|Galaxy

! class=unsortable|Notes

| Centaurus

| 7 December 185

| align="center" | {{ntsh

| 9,100{{Cite journal|last1=Ksenofontov|first1=L. T.|last2=Berezhko|first2=E. G.|last3=Völk|first3=H. J.|date=2005-04-01|title=Magnetic field amplification in Tycho and other shell-type supernova remnants|journal=Astronomy & Astrophysics|language=en|volume=433|issue=1|pages=229–240|doi=10.1051/0004-6361:20042015|issn=0004-6361|bibcode=2005A&A...433..229V|arxiv=astro-ph/0409453|s2cid=16726273}}

| align="center" | {{ntsh|1}}Ia (?)

|Milky Way

| Surviving description sketchy; modern estimates of maximum apparent magnitude vary from +4 to −8. The remnant is probably RCW 86, some 8200 ly distant,[http://chandra.harvard.edu/photo/2006/rcw86/ "New evidence links stellar remains to oldest recorded supernova"] Chandra X-ray Observatory, released 2006-09-18, revised 2009-02-20, retrieved 2010-02-26. making it comparable to SN 1572. Some researchers have suggested it was a comet, not a supernova.{{Cite journal

|vauthors=Chin YN, Huang YL

|title=Identification of the Guest Star of AD 185 as a comet rather than a supernova

|journal=Nature

|volume=371

|issue=6496

|pages=398–399

|url=http://mail.tku.edu.tw/einmann/papers/SN185.ps

|url-status=dead

|archive-url=https://web.archive.org/web/20131105121538/http://mail.tku.edu.tw/einmann/papers/SN185.ps

|archive-date=2013-11-05

|bibcode=1994Natur.371..398C

|year=1994

|doi=10.1038/371398a0

|s2cid=4240119

|url-access=subscription

}}{{Cite journal|vauthors=Zhao FY, Strom RG, Jiang SY |title=The Guest Star of AD185 Must Have Been a Supernova |journal=Chinese Journal of Astronomy and Astrophysics |date=2006 |volume=6 |issue=5 |pages=635–40 |doi=10.1088/1009-9271/6/5/17 |bibcode = 2006ChJAA...6..635Z |doi-access=free }}

| Sagittarius

| April/May 386

| align="center" | {{ntsh|1.5}}+1.5

| 14,700

| align="center" | {{ntsh|2}}II

|Milky Way

| "suggested SN",{{Cite web|title=SNR Cat - U Manitoba|url=http://snrcat.physics.umanitoba.ca}} candidate remnant could be G11.2-0.3.

>{{Cite web

| author=SEDS

| title=Supernova 386

| url=http://spider.seds.org/spider/Misc/sn0386.html

}}{{Cite web

| author=National Radio Astronomy Observatory (NRAO)

| title=The Supernova of 386 AD

| url=http://images.nrao.edu/666

| access-date=2012-09-02

| archive-url=https://web.archive.org/web/20181006194848/http://images.nrao.edu/666

| archive-date=2018-10-06

| url-status=dead

}} There are three suggestions and doubtful if SN at all or classical nova or something else.{{Cite journal|last1=Hoffmann|first1=Susanne M|last2=Vogt|first2=Nikolaus|date=2020-09-11|title=A search for the modern counterparts of the Far Eastern guest stars 369 CE, 386 CE and 393 CE|url=https://academic.oup.com/mnras/article/497/2/1419/5879202|journal=Monthly Notices of the Royal Astronomical Society|language=en|volume=497|issue=2|pages=1419–1433|doi=10.1093/mnras/staa1970|doi-access=free |arxiv=2007.01013|bibcode=2020MNRAS.497.1419H |issn=0035-8711}}

| Scorpius

| 27 February − 28 March - 22 October − 19 November 393

| align="center" | {{ntsh|0}}–0

| 3,400

| align="center" | {{ntsh|2}} II/Ib

|Milky Way

| "possible SN", could also be classical nova or something else

| Lupus

| 17 April 1006 - 1 May 1006

| align="center" | {{ntsh

| Taurus

| {{OldStyleDate|{{circa|10 July}}|1054|{{circa|4 July}}}}
{{OldStyleDate|{{circa|12 April}}|1056|{{circa|6 April}}}}

| align="center" | {{ntsh

| 6,500

| align="center" | {{ntsh|2}}II

|Milky Way

| Remnant is the Crab Nebula with its pulsar (neutron star)

| Cassiopeia

| 4 August 1181 - 6 August 1181

| align="center" | {{ntsh|0}}0

| 7,100

| align="center" | {{ntsh|1}}sub-luminous Type Iax supernova

|Milky Way

| Remnant is Pa 31 with its hot stellar remnant{{Cite journal|last1=Ritter|first1=Andreas|last2=Parker|first2=Quentin A.|last3=Lykou|first3=Foteini|last4=Zijlstra|first4=Albert A.|last5=Guerrero|first5=Martín A.|last6=Le Dû|first6=Pascal|date=2021-09-01|title=The Remnant and Origin of the Historical Supernova 1181 AD|journal=The Astrophysical Journal Letters|volume=918|issue=2|pages=L33|doi=10.3847/2041-8213/ac2253 | arxiv=2105.12384|bibcode=2021ApJ...918L..33R |hdl=10261/255617 |s2cid=235195784 |issn=2041-8205 |doi-access=free }}

| Cassiopeia

| November 1572

| align="center" | {{ntsh

| 8,000

| align="center" | {{ntsh|1}}Ia

|Milky Way

| Tycho's Nova

| Ophiuchus

| 8–9 October 1604

| align="center" | {{ntsh

| 14,000

| align="center" | {{ntsh|1}}Ia

|Milky Way

| Kepler's Supernova; most recent readily visible supernova within the Milky Way

| Cassiopeia

| 1680

| align="center" | {{ntsh|5}}+5

| 9,000

| align="center" | {{ntsh|2}}IIb

|Milky Way

| Apparently never visually conspicuos, due to interstellar dust; but the remnant, Cas A, is the brightest extrasolar radio source in the sky

| Sagittarius

| 1868

| (visible light masked by dust)

| 25,000

| align="center" | {{ntsh|1}}Ia

| Milky Way

| Located near the Galactic Center; "Posthummusly" discovered in 1985; age determined in 2008

| Andromeda

| 20 August 1885

| align="center" | {{ntsh|5.85}}+5.85{{cite journal |title=S Andromedae 1885 - A centennial review |last1=de Vaucouleurs |first1= G. |last2=Corwin Jr. |first2=H. G. |journal=Astrophysical Journal |volume=295 |date=1985 |pages=287 |bibcode=1985ApJ...295..287D|doi = 10.1086/163374 |doi-access=free }}

| 2,500,000

| align="center" | {{ntsh|1}}Ipec

|Andromeda Galaxy

| First observation of an extragalactic supernova

| Centaurus

| 12 December 1895

| align="center" | {{ntsh|8}}+8.0{{cite web |title=List of Supernovae |url=http://www.cbat.eps.harvard.edu/lists/Supernovae.html |work=Central Bureau for Astronomical Telegrams |publisher=Harvard University |access-date=2021-07-09}}

| 10,900,000

| align="center" | {{ntsh|1}}Ia

|NGC 5253

|  

| Ursa Major

| January 1909

| align="center" | {{ntsh|12}}+12.1

| 21,000,000

| align="center" |

| Pinwheel Galaxy (M101)

| {{cite journal | bibcode=1909AN....180..245W | title=Var. 6.1909 Ursae majoris | last1=Wolf | first1=M. | journal=Astronomische Nachrichten | date=1909 | volume=180 | issue=14–15 | page=245 | doi=10.1002/asna.19091801405}}{{cite web | website=Transient Name Server | title=SN{{nbsp}}1909A | url=https://www.wis-tns.org/object/1909A | publisher = IAU | access-date=25 November 2024}}

| Canes Venatici

| 24 August 1937

| align="center" | {{ntsh|8.4}}+8.4

| 13,000,000

| align="center" | {{ntsh|1}}Ia

|IC 4182

|  

| Cepheus

| 17 July 1939

| align="center" | {{ntsh|13}}+13.0

| 25,200,000

| align="center" | {{ntsh|1}}I

|NGC 6946 (Fireworks Galaxy)

|  

| Coma Berenices

| 5 May 1940

| align="center" | {{ntsh|12.8}}+12.8

| 38,000,000

| align="center" | {{ntsh|2}}II-P

| NGC 4725

|  

| Ursa Major

| 1 September 1951

| align="center" | {{ntsh|17.5}}+17.5

| 21,000,000

| align="center" |

| Pinwheel Galaxy (M101)

| {{cite web

| url = https://www.rochesterastronomy.org/snimages/snother.html#1951H

| title = Other Supernovae images, entry for SN 1951H

| last = Bishop

| first = David

| website = Rochester Astronomy

| access-date = 25 November 2024

}}

| Perseus

| 11 July 1961

| align="center" | {{ntsh|12.5}}+12.5

| 30,000,000

| align="center" | {{ntsh|2}}II?

| NGC 1058

| Potential supernova impostor{{cite news|last=Voisey|first=Jon|title=What was SN 1961V?|url=http://www.universetoday.com/77535/what-was-sn-1961v/|access-date=1 August 2011|newspaper=Universe Today|date=5 November 2010}}

| Ursa Major

| 30 July 1970

| align="center" | {{ntsh|12}}+12.1

| 21,000,000

| align="center" | {{ntsh|2}}II

| Pinwheel Galaxy (M101)

| Stoyan, Ronald Atlas of the Messier Objects, Cambridge University Press 2008 page 329{{Cite journal | last1=Detre | first1=L | last2=Lovas | first2=Miklos | title=IAUC 2269 | journal=International Astronomical Union Circular | date=1970 | issue=2269 | pages=1 | url=http://www.cbat.eps.harvard.edu/iauc/02200/02269.html}}{{cite journal | bibcode=1971IBVS..505....1S | last1=Stienon | first1 = Francis | last2 = Wdowiak | first2 = Thomas | title=The Spectrum of the July 1970 Supernova in M101 | journal=Information Bulletin on Variable Stars | volume=505 | pages=1 | year=1971}}

| Centaurus

| 13 May 1972

| align="center" | {{ntsh|8.7}}+8.7{{cite journal

| last1=Ardeberg | first1=A.

| last2=de Groot | first2=M.

| title=The 1972 supernova in NGC 5253. Photometric results from the first observing season

| journal=Astronomy & Astrophysics

| date=1973 | volume=28 | pages=295–304 |bibcode = 1973A&A....28..295A }}

| 10,900,000

| align="center" | {{ntsh|1}}Ia

| NGC 5253

| Followed for more than a year; became the prototypical Type Ia supernova

| Hydra

| 3 July 1983

| align="center" | {{ntsh|11.8}}+11.8

| 15,000,000

| align="center" | {{ntsh|1}}Ib

| Messier 83

| First observation of a Type Ib supernova

| Andromeda

| 21 August 1986

| align="center" | {{ntsh|18.4}}+18.4

| 30,000,000

| align="center" | {{ntsh|2}}IIn

| NGC 891

| Bright in the radio frequency range

| Dorado

| 1987

| align="center" | {{ntsh|2.9}}+2.9

| 160,000

| align="center" | {{ntsh|2}}IIpec

| Large Magellanic Cloud

| Intense radiation reached Earth on February 23, 1987, 7:35:35 UT. Notable for archival photos of progenitor star and detection of supernova neutrinos. Most recent Local Group supernova

| Ursa Major

| 28 March 1993

| align="center" | {{ntsh|10.7}}+10.7{{cite journal

| author=J. C. Wheeler

| author2=E. Barker

| author3=R. Benjamin

| author4=J. Boisseau

| author5=A. Clocchiatti

| author6=G. de Vaucouleurs

| author7=N. Gaffney

| author8=R. P. Harkness

| author9=A. M. Khokhlov

| author10=D. F. Lester

| author11=B. J. Smith

| author12=V. V. Smith

| author13=J. Tomkin

| title=Early Observations of SN 1993J in M81 at McDonald Observatory

| journal=Astrophysical Journal

| date=1993

| volume=417

| pages=L71–L74

| bibcode=1993ApJ...417L..71W

| doi=10.1086/187097}}

| 11,000,000

| align="center" | {{ntsh|2}}IIb

| M81

| One of the brightest supernovae in the northern sky since 1954

| Virgo

| 7 March 1994

| align="center" | {{ntsh|15.2}}+15.2

| 50,000,000

| align="center" | {{ntsh|1}}Ia

| NGC 4526

|

| Telescopium

| 26 April 1998

| align="center" | ?

| 140,000,000

| align="center" | {{ntsh|1}}Ic

| ESO 184-G82

| Linked to GRB 980425, which was the first time a gamma-ray burst has been linked to a supernova.

| Lynx

| 12 October 1999

| align="center" | {{ntsh|18.3}}+18.3 +/- 0.3

| 84,000,000

| align="center" | {{ntsh|1}} I

| NGC 2770

| First supernovae in this galaxy, where 3 more were detected later.

| Lupus

| 2002

| align="center" | {{ntsh|14.7}}+14.7

| 160,000,000

| align="center" | {{ntsh|2}}IIn

| NGC 1821

| AM Canum Venaticorum-type outburst.{{cite news

|first=Robert

|last=Sanders

|title=Rapid supernova could be new class of exploding star

|publisher=University of California, Berkeley

|work=UC Newsroom

|url=http://www.universityofcalifornia.edu/news/article/22291

|access-date=2009-11-06

|url-status=dead

|archive-url=https://web.archive.org/web/20110613215023/http://www.universityofcalifornia.edu/news/article/22291

|archive-date=2011-06-13

}}

| Ursa Major

| 2002

| align="center" | {{ntsh|24.0}}+24.0

| 8,000,000,000

| align="center" | {{Ntsh|1}}Ia

| anonymous galaxy

| Furthest supernova observed through Hubble Deep Field.{{Cite web |last=information@eso.org |title=SN2002dd in the HDF North - 2002 |url=https://esahubble.org/images/opo0312c/ |access-date=2024-08-17 |website=www.esahubble.org |language=en}}

| Boötes

| 2003

| align="center" |

| 4,000,000,000

| align="center" | {{ntsh|1}}Ia

| anonymous galaxy

| Also known as the "Champagne supernova"

| Ursa Major

| March 2004

| align="center" |

| 11,500,000

| align="center" | {{ntsh|2}}II

| M82 (Cigar Galaxy)

| {{cite web |title=SN 2004am {{!}} Transient Name Server |url=https://wis-tns.weizmann.ac.il/object/2004am |website=wis-tns.weizmann.ac.il |access-date=14 July 2020}}

| Camelopardalis

| 31 July 2004
18:15

| align="center" |

| 8,000,000

| align="center" | {{ntsh|2}}II-P

| NGC 2403

| NGC 2403 is an outlying member of the M81 Group

| Aquarius

| November 2004-June 2005

| align="center" |

|

| align="center" | {{ntsh|2}}II

|

|{{Cite journal | last1 = Cooke | first1 = J. | last2 = Sullivan | first2 = M. | last3 = Gal-Yam | first3 = A. | last4 = Barton | first4 = E. J. | last5 = Carlberg | first5 = R. G. | last6 = Ryan-Weber | first6 = E. V.|author6-link=Emma Ryan-Weber | last7 = Horst | first7 = C. | last8 = Omori | first8 = Y. | last9 = Díaz | first9 = C. G. | doi = 10.1038/nature11521 | title = Superluminous supernovae at redshifts of 2.05 and 3.90 | journal = Nature | volume = 491 | issue = 7423 | pages = 228–231 | year = 2012 | pmid = 23123848| bibcode = 2012Natur.491..228C |arxiv = 1211.2003 | s2cid = 4397580 }}

| Coma Berenices

| 3 March 2005

| align="center" |

| 4,700,000,000

| align="center" | {{ntsh|2}}II

| ?

| Announced in 2007 to be the brightest supernova up to that point.

| Cetus

| 27 September 2005

| align="center" |

| 865,000,000

| align="center" | {{ntsh|1}}Ia/II-n

| ?

| Notable for having characteristics of both Type Ia and Type IIn.

| Pisces

| 5 October 2005

| align="center" | {{ntsh|16.5}}+16.5

| 200,000,000

| align="center" | {{ntsh|2}}II-n

| NGC 266

| Star could be found on old pictures.{{Cite journal

| author=David Bishop

| title=Supernova 2005gl in NGC 266

| journal=Central Bureau Electronic Telegrams

| issue=250

| pages=1

| publisher=Rochester Academy of Science

| url=http://www.rochesterastronomy.org/sn2005/sn2005gl.html

| access-date=26 August 2012

| bibcode=2005CBET..250....1P

| year=2005

}}

| Perseus

| 18 September 2006

| align="center" | {{ntsh|15}}+15

| 240,000,000

| align="center" | {{ntsh|2}}IIn ^(*)

| NGC 1260

| Observed by NASA,
^*with a peak of over 70 days, possibly a new type.

| Lynx

| 9 October 2006

| align="center" |

| 77,000,000

| align="center" | {{ntsh|1}}Ibn

| UGC 4904

|

| Virgo

| Early 2007

| align="center" | {{ntsh|18.3}}+18.3

|

| align="center" | {{ntsh|1}}Ia

| anonymous dwarf galaxy

| Extremely bright and long-lasting, the first good observational match for the pair-instability supernova model postulated for stars of initial mass greater than 140 solar masses (even better than SN 2006gy). The precursor is estimated at 200 solar masses, similar to the first stars of the early universe.Science Daily, [https://www.sciencedaily.com/releases/2009/12/091202153939.htm "Superbright Supernova Is First of Its Kind"], 5 December 2009 (accessed 2009-12-15)

| Lynx

| 31 December 2007

| align="center" | {{ntsh|16.8}}+16.8

| 84,000,000

| align="center" | {{ntsh|1}}Ibc

| NGC 2770

| Got overshadowed by SN 2008D.

| Lynx

| 9 January 2008

| align="center" |

| 88,000,000

| align="center" | {{ntsh|1}}Ibc

| NGC 2770

| First supernova to be observed while it exploded.

| Aries

|

| align="center" | {{ntsh|28.7}}+28.7

| 1,000,000,000
(z=0.0613)

| align=center | {{ntsh|1}}Ia

| anonymous red globular cluster associated with anonymous red elliptical galaxy in cluster Abell 399

| Observed in 2009. Supernova associated with a globular cluster{{cite journal |title= Confirmation of Hostless Type Ia Supernovae Using Hubble Space Telescope Imaging |author1=Melissa L. Graham |author2=David J. Sand |author3=Dennis Zaritsky |author4=Chris J. Pritchet |date= 13 May 2015 |arxiv= 1505.03407 |bibcode= 2015ApJ...807...83G |doi=10.1088/0004-637X/807/1/83 |volume=807 |issue=1 |journal=The Astrophysical Journal |pages=83|s2cid=118555601 }}{{cite news |url= https://newscenter.berkeley.edu/2015/06/04/exiled-stars-explode-far-from-home/ |title= Exiled stars explode far from home |date= 4 June 2015 |author= Robert Sanders |publisher= UC Berkeley News Center |archive-date= 12 June 2015 |access-date= 6 June 2015 |archive-url= https://web.archive.org/web/20150612021338/http://newscenter.berkeley.edu/2015/06/04/exiled-stars-explode-far-from-home/ |url-status= dead }}

| Piscis Austrinus

| 2009

| align="center" |

| 66,000,000

| align="center" | {{ntsh|2}}IIn

| NGC 7259

| In 2009 classified as supernova. Redesignated as Luminous blue variable (LBV) Supernova impostor.{{cite web|title=Supernova impostor explodes for real|url=https://www.newscientist.com/article/dn22345-astrophile-supernova-impostor-explodes-for-real/|website=www.newscientist.com|access-date=November 29, 2017}} In September 2012 classified as a young type IIn supernova.{{cite journal|title=Supernova 2009ip in NGC 7259|url=http://www.rochesterastronomy.org/sn2009/sn2009ip.html|journal=Central Bureau Electronic Telegrams|issue=1928|pages=1|access-date=November 29, 2017|bibcode=2009CBET.1928....1M|last1=Maza|first1=J.|last2=Hamuy|first2=M.|last3=Antezana|first3=R.|last4=Gonzalez|first4=L.|last5=Lopez|first5=P.|last6=Silva|first6=S.|last7=Folatelli|first7=G.|last8=Iturra|first8=D.|last9=Cartier|first9=R.|last10=Forster|first10=F.|last11=Marchi|first11=S.|last12=Rojas|first12=A.|last13=Pignata|first13=G.|last14=Conuel|first14=B.|last15=Reichart|first15=D.|last16=Ivarsen|first16=K.|last17=Haislip|first17=J.|last18=Crain|first18=A.|last19=Foster|first19=D.|last20=Nysewander|first20=M.|last21=Lacluyze|first21=A.|year=2009|archive-url=https://web.archive.org/web/20160911044925/http://www.rochesterastronomy.org/sn2009/sn2009ip.html|archive-date=September 11, 2016|url-status=dead}}

| Camelopardalis

| 2 January 2011

| align="center" | {{ntsh|17}}+17.0

| 240,000,000

| align="center" | {{ntsh|1}}Ia (sub-luminous)

| UGC 3378

| Discovered by 10-year-old girl, the youngest person to discover a supernova.

| Ursa Major

| 24 August 2011

| align="center" | {{ntsh|10}}+10.0

| 21,000,000

| align="center" | {{ntsh|1}}Ia

| M101

| One of the very few extragalactic supernovae visible in 50mm binoculars.

| Cetus

| April 2013

| align="center" |

| 166,000,000,000

| align="center" |

|

| Also Known as SN Wilson.{{Cite news |last=Major |first=Jason |date=5 April 2013 |title=Hubble Spots the Most Distant Supernova Ever |url=http://news.discovery.com/space/galaxies/hubble-spots-the-most-distant-supernova-ever-130405.htm |url-status=dead |archive-url=https://web.archive.org/web/20160326225736/http://news.discovery.com/space/galaxies/hubble-spots-the-most-distant-supernova-ever-130405.htm |archive-date=26 March 2016 |access-date=28 June 2015 |publisher=Discovery Channel}}

{{cite news|last=Yglesias |first=Matthew |url=http://www.slate.com/blogs/bad_astronomy/2013/04/04/exploding_stars_supernova_found_is_most_distant_of_its_kind_yet.html |title=Exploding stars: Supernova found is most distant of its kind yet |publisher=Slate.com |date=2013-04-04 |access-date=2013-04-08}}

{{Cite web |date=2013-04-04 |title=Hubble breaks record for furthest supernova |url=https://esahubble.org/news/heic1306/ |access-date=2024-08-31 |website=esahubble.org |language=en}}

{{Cite journal |last1=Jones |first1=David O. |last2=Rodney |first2=Steven A. |last3=Riess |first3=Adam G. |last4=Mobasher |first4=Bahram |last5=Dahlen |first5=Tomas |last6=McCully |first6=Curtis |last7=Frederiksen |first7=Teddy F. |last8=Casertano |first8=Stefano |last9=Hjorth |first9=Jens |last10=Keeton |first10=Charles R. |last11=Koekemoer |first11=Anton |last12=Strolger |first12=Louis-Gregory |last13=Wiklind |first13=Tommy G. |last14=Challis |first14=Peter |last15=Graur |first15=Or |date=25 April 2013 |title=The Discovery of the Most Distant Known Type Ia Supernova at Redshift 1.914 |url=https://iopscience.iop.org/article/10.1088/0004-637X/768/2/166 |journal=The Astrophysical Journal |volume=768 |issue=2 |pages=166 |arxiv=1304.0768 |bibcode=2013ApJ...768..166J |doi=10.1088/0004-637X/768/2/166 |issn=0004-637X}}

| Ursa Major

| Mid January 2014

| align="center" | {{ntsh|10.1}}+10.1

| 11,500,000

| align="center" | {{ntsh|1}}Ia

| M82

| Closest supernova since SN 2004dj in NGC 2403.

| Leo

| 7 March 2014

| align="center" |

| 310,000,000

| align="center" | {{ntsh|1}}Ia

| NGC 3861

| {{Cite web|url=http://rochesterastronomy.org/sn2014/index.html#2014aa|title=Bright Supernovae - 2014.|last=|website=rochesterastronomy.org|access-date=2018-07-28}}{{Cite web|url=https://wis-tns.weizmann.ac.il/object/2014aa|title=SN 2014aa {{!}} Transient Name Server|website=wis-tns.weizmann.ac.il|language=en|access-date=2018-07-28}}{{Cite web|url=https://sne.space/sne/2014aa/|title=2014aa - The Open Supernova Catalog|website=sne.space|language=en-US|access-date=2018-07-28|archive-date=2018-07-28|archive-url=https://web.archive.org/web/20180728221727/https://sne.space/sne/2014aa/|url-status=dead}}

| Leo

| 11 November 2014

| align="center" |

| 14,400,000,000

| align="center" |

| SP 1149

| It is the first detected multiply-lensed supernova, visible within the field of the galaxy cluster MACS J1149+2223.{{Cite journal | doi = 10.1126/science.aaa3350| title = Multiple images of a highly magnified supernova formed by an early-type cluster galaxy lens| journal = Science| volume = 347| issue = 6226| pages = 1123–1126| year = 2015| last1 = Kelly | first1 = P. L.| last2 = Rodney | first2 = S. A.| last3 = Treu | first3 = T.| last4 = Foley | first4 = R. J.| last5 = Brammer | first5 = G.| last6 = Schmidt | first6 = K. B.| last7 = Zitrin | first7 = A.| last8 = Sonnenfeld | first8 = A.| last9 = Strolger | first9 = L. -G. | last10 = Graur | first10 = O.| last11 = Filippenko | first11 = A. V.| last12 = Jha | first12 = S. W.| last13 = Riess | first13 = A. G.| last14 = Bradac | first14 = M.| last15 = Weiner | first15 = B. J.| last16 = Scolnic | first16 = D.| last17 = Malkan | first17 = M. A.| last18 = von Der Linden | first18 = A.| last19 = Trenti | first19 = M.| last20 = Hjorth | first20 = J.| last21 = Gavazzi | first21 = R.| last22 = Fontana | first22 = A.| last23 = Merten | first23 = J. C.| last24 = McCully | first24 = C.| last25 = Jones | first25 = T.| last26 = Postman | first26 = M.| last27 = Dressler | first27 = A.| last28 = Patel | first28 = B.| last29 = Cenko | first29 = S. B.| last30 = Graham | first30 = M. L.| display-authors = 29|arxiv =1411.6009|bibcode = 2015Sci...347.1123K | pmid=25745167| s2cid = 206633888}}{{cite news |last=Overbye |first=Dennis |authorlink=Dennis Overbye |title=Astronomers Observe Supernova and Find They're Watching Reruns |url=https://www.nytimes.com/2015/03/06/science/astronomers-observe-supernova-and-find-theyre-watching-reruns.html |date=March 5, 2015 |work=New York Times |accessdate=March 5, 2015 }}{{cite web|url=http://www.latimes.com/science/sciencenow/la-sci-sn-supernova-four-way-einstein-cross-gravitational-lens-galaxy-cluster-20150305-story.html|title=Don't believe the light: Supernova in 'Einstein Cross' is a cosmic trick|work=Los Angeles Times|date=5 March 2015|author=Amina Khan}}{{Cite journal | doi = 10.1088/2041-8205/800/2/L26| title = Revised Lens Model for the Multiply Imaged Lensed Supernova, "Sn Refsdal" in Macs J1149+2223| journal = The Astrophysical Journal| volume = 800| issue = 2| pages = L26| year = 2015| last1 = Sharon | first1 = K. | last2 = Johnson | first2 = T. L. |arxiv = 1411.6933 |bibcode = 2015ApJ...800L..26S | s2cid = 118735742}}

| Virgo

| 1 April 2015

| align="center" |

| 1,000,000,000

| align="center" | {{ntsh|1}}Ia

| NGC 4866

| {{cite news|author1=Piascik, A. S.|author2=Steele, I. A.|date=2015-01-01|title=ATel #7333: Spectral Classification of ASASSN-15ga in NGC4866|work=The Astronomer's Telegram|url=http://www.astronomerstelegram.org/?read=7333|accessdate=2021-02-02}}

| Indus

| 14 June 2015

| align="center" | {{ntsh|16.9}}+16.9

| 3,800,000,000

| align="center" | {{ntsh|1}}Ic

| APMUKS(BJ) B215839.70−615403.9

| Most luminous hypernova ever observed.

|Ursa Major

| September 2014

| align="center" | {{ntsh|17.7}}+17.7

|509,000,000

| align="center" | unknown

|SDSS J092034.44+504148.7 (possible dwarf galaxy)

|Unusual supernova

| Draco

| 22 February 2016

| align="center" | {{ntsh|17.8}}+18.11

| 3,600,000,000

| align="center" | {{ntsh|2}}SLSB-II

| ?

| Most luminous supernova-like event to date.

| Dorado

| 14 August 2017

| align="center" |

| 517,000,000

| align="center" | {{ntsh|1}} I

| NGC 1672

|

| Puppis

| 15 January 2018

| align="center" |

| 70,000,000

| align="center" | {{ntsh|1}}Ia

| NGC 2525

| {{cite web | website=Transient Name Server | title=SN{{nbsp}}2018gv | url=https://www.wis-tns.org/object/2018gv | publisher = IAU | access-date=9 December 2024}}{{cite journal | bibcode=2018ATel11175....1S| title=Spectroscopic Classification of SN 2018gv with Keck I/LRIS| last1=Siebert| first1=M. R.| last2=Dimitriadis| first2=G.| last3=Foley| first3=R. J.| journal=The Astronomer's Telegram| date=2018| volume=11175| page=1 | url=http://www.astronomerstelegram.org/?read=11175}}{{cite journal | bibcode=2018ATel11177....1B| title=EPESSTO spectroscopic classification of optical transients: SN2018gv a very young SN Ia| last1=Bufano| first1=F.| last2=Berton| first2=M.| last3=Vogl| first3=C.| last4=Floers| first4=A.| last5=Taubenberger| first5=S.| last6=Anderson| first6=J.| last7=Galbany| first7=L.| last8=Schulze| first8=S.| last9=Yaron| first9=O.| last10=Manulis| first10=I.| last11=Inserra| first11=C.| last12=Kankare| first12=E.| last13=Maguire| first13=K.| last14=Smartt| first14=S. J.| last15=Young| first15=D.| last16=Smith| first16=K. W.| last17=McBrien| first17=O.| last18=Tonry| first18=J.| last19=Denneau| first19=L.| last20=Heinze| first20=A.| last21=Weiland| first21=H.| last22=Stalder| first22=B.| last23=Rest| first23=A.| journal=The Astronomer's Telegram| date=2018| volume=11177| page=1 | url=https://www.astronomerstelegram.org/?read=11177}}{{Citation|title=Time-Lapse of Supernova in NGC 2525|url=https://www.spacetelescope.org/videos/heic2018a/|language=en|access-date=2021-11-05|website=European Space Agency}}{{Cite web |title=Check out this exploding supernova captured by the Hubble telescope |author=NASA, ESA, J. DePasquale (STScI), M. Kornmesser and M. Zamani (ESA/Hubble), A. Riess (STScI/JHU) and the SH0ES team, and the Digitized Sky Survey|website=CBBC Newsround |date=6 October 2020 |url= https://www.bbc.co.uk/newsround/54416190 |quote=Supernova SN 2018gv}}

| Camelopardalis

| 2 March 2018

| align="center" | {{ntsh|17.8}}+17.8

| 70,000,000

| align="center" | {{ntsh|1}}Ia-csm

| NGC 2146

| First electron capture supernova ever detected

| Hercules

| 16 June 2018, 10:35:02

| align="center" |

| 200,000,000

| align="center" | {{ntsh|1}}Ib

| CGCG 137-068

| {{cite news |last=Morris |first=Amanda |title=Astrophysicists capture new class of transient objects |url=https://phys.org/news/2020-05-astrophysicists-capture-class-transient.html |date=26 May 2020 |work=Phys.org |access-date=26 May 2020 }}

| Leo Minor

| 9 January 2019

| align="center" | {{ntsh|13.0}}+13.0

| 75,000,000

| align="center" | {{ntsh|1}} Ia

| NGC 3254

|{{cite web | website=Transient Name Server | title=SN{{nbsp}}2019np | url=https://www.wis-tns.org/object/2019np | publisher = IAU | access-date=27 November 2024}}{{cite web

| url = https://www.rochesterastronomy.org/sn2019/index.html

| title = Bright Supernovae - 2019

| last = Bishop

| first = David

| website = Rochester Astronomy

| access-date = 9 December 2024

}}

| Boötes

|

| align="center" | {{ntsh|20.16}}+20.16

| 920,000,000

| align="center" | {{ntsh|1}}Icn

|

| First detected supernova of a Wolf-Rayet star{{Cite journal|last1=Gal-Yam|first1=A.|last2=Bruch|first2=R.|last3=Schulze|first3=S.|last4=Yang|first4=Y.|last5=Perley|first5=D. A.|last6=Irani|first6=I.|last7=Sollerman|first7=J.|last8=Kool|first8=E. C.|last9=Soumagnac|first9=M. T.|last10=Yaron|first10=O.|last11=Strotjohann|first11=N. L.|date=12 January 2022|title=A WC/WO star exploding within an expanding carbon–oxygen–neon nebula|url=https://www.nature.com/articles/s41586-021-04155-1|journal=Nature|language=en|volume=601|issue=7892|pages=201–204|arxiv=2111.12435|doi=10.1038/s41586-021-04155-1|pmid=35022591 |bibcode=2022Natur.601..201G |s2cid=244527654 |issn=1476-4687}}{{Cite web|title=Astronomers discover first supernova explosion of a Wolf-Rayet star|url=https://www.iac.es/en/outreach/news/astronomers-discover-first-supernova-explosion-wolf-rayet-star|access-date=2022-02-08|website=Instituto de Astrofísica de Canarias • IAC|date=12 January 2022 |language=en}}

| Coma Berenices

| 7 January 2020

| align="center" | {{ntsh|17.28}}+17.28

| 46,000,000

| align="center" | {{ntsh|1}}Ic

| Messier 100

|{{citation needed|date=April 2025}}

| Virgo

| 31 March 2020

| align="center" | {{ntsh|19}}+19.0

| 59,400,000

| align="center" | {{ntsh|2}}IIb

| NGC 4568

| Earliest known observation of an explosion, 26 hours after{{Cite web|last=Jenner|first=Lynn|date=2021-10-19|title=Hubble Gives Unprecedented, Early View of a Doomed Star's Destruction|url=http://www.nasa.gov/feature/goddard/2021/hubble-gives-unprecedented-early-view-of-a-doomed-stars-destruction|access-date=2021-11-05|website=NASA}}{{Cite web|last=Gough|first=Evan|date=2021-10-29|title=Quick Action Let Hubble Watch the Earliest Stages of an Unfolding Supernova Detonation|url=https://www.universetoday.com/153114/quick-action-let-hubble-watch-the-earliest-stages-of-an-unfolding-supernova-detonation/|access-date=2021-11-05|website=Universe Today|language=en-US}}{{Cite journal|last1=Tinyanont|first1=Samaporn|last2=Ridden-Harper|first2=R|last3=Foley|first3=R J|last4=Morozova|first4=V|last5=Kilpatrick|first5=C D|last6=Dimitriadis|first6=G|last7=DeMarchi|first7=L|last8=Gagliano|first8=A|last9=Jacobson-Galán|first9=W V|last10=Messick|first10=A|last11=Pierel|first11=J D R|date=2021-10-26|title=Progenitor and close-in Circumstellar Medium of Type II Supernova 2020fqv from high-cadence photometry and ultra-rapid UV spectroscopy|journal=Monthly Notices of the Royal Astronomical Society|volume=512 |issue=stab2887|pages=2777–2797 |arxiv=2110.10742|doi=10.1093/mnras/stab2887|doi-access=free |issn=0035-8711}}

| Virgo

| 6 May 2020

| align="center" |

| 45,610,000

| align="center" | {{ntsh|2}}II

| M61

|{{cite journal |last1=Sollerman |first1=J. |arxiv=2107.14503 |title=The Type II supernova SN 2020jfo in M 61, implications for progenitor system, and explosion dynamics |journal=Astronomy & Astrophysics |date=2021-07-30|volume=655 |pages=A105 |doi=10.1051/0004-6361/202141374 |bibcode=2021A&A...655A.105S |s2cid=239388865 }}{{cite journal |last1=Vallely |first1=P.J. |last2=Kocanek |first2=CS |last3=Stanek |first3=KZ |last4=Fausnaugh |first4=M |last5=Shappee |first5=BJ |title=High-cadence, early-time observations of core-collapse supernovae from the TESS prime mission |journal=Monthly Notices of the Royal Astronomical Society |volume=500 |issue=4 |date=February 2021 |pages=5639–5656 |doi=10.1093/mnras/staa3675|doi-access=free |arxiv=2010.06596 }}{{cite journal |last1=Jones |first1=DO |title=The Young Supernova Experiment: Survey Goals, Overview, and Operations |journal=The Astrophysical Journal |year=2021 |volume=908 |issue=143 |page=143 |doi=10.3847/1538-4357/abd7f5|arxiv=2010.09724 |bibcode=2021ApJ...908..143J |s2cid=224803297 |doi-access=free }}

| Boötes

| 2020

| align="center" | {{ntsh|15.89}}+15.89

| 120,000,000

| align="center" | {{ntsh|2}}IIn

| NGC 5731

| First red supergiant observed before, during and after explosion; earliest known observation, at 130 days before explosion{{cite journal|last1=Jacobson-Galán|first1=W. V.|last2=Dessart |first2=L.|last3=Jones |first3=D. O.|last4=Margutti|first4=R.|last5=Coppejans|first5=D.L.|last6=Dimitriadis|first6=G.|last7=Foley|first7=R. J.|last8=Kilpatrick|first8=C. D.|last9=Matthews|first9=D. J.|last10=Rest|first10=S.|last11=Terreran|first11=G.|last12=Aleo|first12=P. D.|last13=Auchettl |first13=K.|last14=Blanchard |first14=P. K.|last15=Coulter |first15=D. A.|last16=Davis|first16=K. W.|last17=de Boer|first17=T. J. L.|last18=DeMarchi|first18=L.|last19=Drout|first19=M. R.|last20=Earl|first20=N.|last21=Gagliano|first21=A.|last22=Gall|first22=C.|last23=Hjorth|first23=J.|last24=Huber|first24= M. E.|last25=Ibik |first25=A. L.|last26=Milisavljevic|first26= D.|last27=Pan |first27=Y.-C.|last28=Rest |first28=A.|last29=Ridden-Harper|first29=R.|last30=Rojas-Bravo|first30=C.|last31=Siebert |first31=M. R.|last32=Smith |first32=K. W.|last33=Taggart |first33=K.|last34=Tinyanont|first34=S.|last35=Wang|first35=Q.|last36=Zenati|first36=Y.|title=Final Moments. I. Precursor Emission, Envelope Inflation, and Enhanced Mass Loss Preceding the Luminous Type II Supernova 2020tlf |journal=The Astrophysical Journal|volume=924|date=6 January 2022|issue=1 |pages=15|doi=10.3847/1538-4357/ac3f3a |publisher=American Astronomical Society|s2cid=237940678 |doi-access=free|arxiv=2109.12136|bibcode=2022ApJ...924...15J }}{{Cite web|last=Anderson|first=Paul Scott|title=Dying star's explosive end seen by astronomers|url=https://earthsky.org/space/dying-stars-explosive-end-supernova-sn-2020tlf/|date=14 January 2022|website=EarthSky|access-date=16 January 2022|publisher=Deborah Byrd}}

| Ursa Major

| 20 March 2021

| align="center" | {{ntsh|11.2}}+11.2

| 34,800,00

| align="center" | {{ntsh|2}}II-P

| NGC 3310

|{{cite web

| title=SN 2021gmj

| website=Transient Name Server

| url=https://www.wis-tns.org/object/2021gmj

| access-date=2021-12-20 }}

| Draco

| April 2, 2021

| align="center" |

| 129,000,000 ± 29

| align="center" | {{ntsh|1}}Ia

| NGC 3147

|{{cite web

| title=Supernovae 2021jad in NGC 1964

| first=David | last=Bishop | date=May 13, 2021

| website=Rochester Astronomy

| publisher=Rochester Academy of Science

| url=https://www.rochesterastronomy.org/sn2021/sn2021jad.html

| access-date=2021-12-19 }}

| Lepus

| April 2021

| align="center" |

| 65,000,000

| align="center" | {{ntsh|1}}Ia

| NGC 1964

|{{cite web

| title=Supernovae 2021jad in NGC 1964

| first=David | last=Bishop | date=May 13, 2021

| website=Rochester Astronomy

| publisher=Rochester Academy of Science

| url=https://www.rochesterastronomy.org/sn2021/sn2021jad.html

| access-date=2021-12-19 }}

| Eridanus

| 8 September 2021

| align="center" |

| 750,000,000

| align="center" | {{ntsh|2}}II

| NGC 1325{{cite journal

| title=ATLAS21bidw (AT2021yja): discovery of a candidate SN in NGC 1325 (22 Mpc)

| last1=Smith | first1=K. W. | last2=Srivastav | first2=S.

| last3=Smartt | first3=S. J. | last4=Gillanders | first4=J.

| last5=Fulton | first5=M. | last6=Young | first6=D. R.

| last7=Shingles | first7=L. | last8=McCollum | first8=M.

| last9=Richman | first9=C. | last10=Chen | first10=T. W.

| last11=Anderson | first11=J. | last12=Denneau | first12=L.

| last13=Heinze | first13=A. | last14=Tonry | first14=J.

| last15=Weiland | first15=H. | last16=Stalder | first16=B.

| last17=Rest | first17=A. | last18=Wright | first18=D. E.

| display-authors=1 | journal=Transient Name Server AstroNote 2021-235

| date=September 2021 | volume=235 | page=1 | bibcode=2021TNSAN.235....1S }}{{cite journal

| title=Radio observations of SN 2021yja

| last1=Ryder | first1=S. D. | last2=Marnoch | first2=L.

| last3=Kundu | first3=E. | last4=Filipovic | first4=M. D.

| last5=Alsaberi | first5=R. | last6=Anderson | first6=G.

| last7=Stockdale | first7=C. | last8=Maeda | first8=K.

| last9=Renaud | first9=M. | last10=Kotak | first10=R.

| display-authors=1 | journal=The Astronomer's Telegram

| volume=14915 | date=September 2021

| page=1 | bibcode=2021ATel14915....1R }}

|

| Dorado

| 11 November 2021

| align="center" | {{ntsh|17.2}}+17.2

| 69,000,000

| align="center" | {{ntsh|1}}Ia

| NGC 1566

|{{cite web |title=Bright Supernovae - 2021. |url=https://www.rochesterastronomy.org/sn2021/index.html#2021aefx |website=www.rochesterastronomy.org |access-date=21 January 2024}}

| Sculptor

| 23 November 2021

| align="center" | {{ntsh|18.8}}+18.8

| 500,000,000

| align="center" | {{ntsh|2}}II

| Cartwheel Galaxy

| {{cite web | url=https://www.rochesterastronomy.org/supernova.html#2021afdx | title=2021afdx | author=David Bishop | website=rochesterastronomy.org | date=23 November 2021 | access-date=28 November 2021}}{{cite web | url=https://www.wis-tns.org/object/2021afdx | title=SN 2021afdx | work=Transient Name Server | publisher=IAU Supernova Working Group | date=23 November 2021 | access-date=28 November 2021}}

| Cetus

| 5 May 2022

| align="center" | {{ntsh|14}}+14

| 75,000,000

| type I-c

| NGC 157

| Type Ic, shows periodicity{{cite journal |last1=Moore |first1=T. |last2=Smartt |first2=S. J. |last3=Nicholl |first3=M. |last4=Srivastav |first4=S. |last5=Stevance |first5=H. F. |last6=Jess |first6=D. B. |last7=Grant |first7=S. D. T. |last8=Fulton |first8=M. D. |last9=Rhodes |first9=L. |last10=Sim |first10=S. A. |last11=Hirai |first11=R. |last12=Podsiadlowski |first12=P. |last13=Anderson |first13=J. P. |last14=Ashall |first14=C. |last15=Bate |first15=W. |last16=Fender |first16=R. |last17=Gutiérrez |first17=C. P. |last18=Howell |first18=D. A. |last19=Huber |first19=M. E. |last20=Inserra |first20=C. |last21=Leloudas |first21=G. |last22=Monard |first22=L. A. G. |last23=Müller-Bravo |first23=T. E. |last24=Shappee |first24=B. J. |last25=Smith |first25=K. W. |last26=Terreran |first26=G. |last27=Tonry |first27=J. |last28=Tucker |first28=M. A. |last29=Young |first29=D. R. |last30=Aamer |first30=A. |last31=Chen |first31=T.-W. |last32=Ragosta |first32=F. |last33=Galbany |first33=L. |last34=Gromadzki |first34=M. |last35=Harvey |first35=L. |last36=Hoeflich |first36=P. |last37=McCully |first37=C. |last38=Newsome |first38=M. |last39=Gonzalez |first39=E. P. |last40=Pellegrino |first40=C. |last41=Ramsden |first41=P. |last42=Pérez-Torres |first42=M. |last43=Ridley |first43=E. J. |last44=Sheng |first44=X. |last45=Weston |first45=J. |title=SN 2022jli: A Type Ic Supernova with Periodic Modulation of Its Light Curve and an Unusually Long Rise |journal=The Astrophysical Journal Letters |date=October 2023 |volume=956 |issue=1 |pages=L31 |doi=10.3847/2041-8213/acfc25 |doi-access=free |bibcode=2023ApJ...956L..31M |language=en |issn=2041-8205 |display-authors=1|arxiv=2309.12750 }}{{cite journal |last1=Chen |first1=Ping |last2=Gal-Yam |first2=Avishay |last3=Sollerman |first3=Jesper |last4=Schulze |first4=Steve |last5=Post |first5=Richard S. |last6=Liu |first6=Chang |last7=Ofek |first7=Eran O. |last8=Das |first8=Kaustav K. |last9=Fremling |first9=Christoffer |last10=Horesh |first10=Assaf |last11=Katz |first11=Boaz |last12=Kushnir |first12=Doron |last13=Kasliwal |first13=Mansi M. |last14=Kulkarni |first14=Shri R. |last15=Liu |first15=Dezi |last16=Liu |first16=Xiangkun |last17=Miller |first17=Adam A. |last18=Rose |first18=Kovi |last19=Waxman |first19=Eli |last20=Yang |first20=Sheng |last21=Yao |first21=Yuhan |last22=Zackay |first22=Barak |last23=Bellm |first23=Eric C. |last24=Dekany |first24=Richard |last25=Drake |first25=Andrew J. |last26=Fang |first26=Yuan |last27=Fynbo |first27=Johan P. U. |last28=Groom |first28=Steven L. |last29=Helou |first29=George |last30=Irani |first30=Ido |last31=Jegou du Laz |first31=Theophile |last32=Liu |first32=Xiaowei |last33=Mazzali |first33=Paolo A. |last34=Neill |first34=James D. |last35=Qin |first35=Yu-Jing |last36=Riddle |first36=Reed L. |last37=Sharon |first37=Amir |last38=Strotjohann |first38=Nora L. |last39=Wold |first39=Avery |last40=Yan |first40=Lin |title=A 12.4-day periodicity in a close binary system after a supernova |journal=Nature |date=January 2024 |volume=625 |issue=7994 |pages=253–258 |doi=10.1038/s41586-023-06787-x |pmid=38200292 |arxiv=2310.07784 |bibcode=2024Natur.625..253C |s2cid=263909264 |url=https://www.nature.com/articles/s41586-023-06787-x |access-date=12 January 2024 |language=en |issn=1476-4687 |display-authors=1}}{{cite web |title=Missing link found: supernovae give rise to black holes or neutron stars |url=https://www.eso.org/public/news/eso2401/ |website=www.eso.org |access-date=12 January 2024 |language=en}}{{cite web |title=Supernova 2022jli in NGC 157 |url=https://www.rochesterastronomy.org/sn2022/sn2022jli.html |website=www.rochesterastronomy.org |access-date=12 January 2024}}

| Gemini

| November 2022

| align="center" |

| 600,000,000

| align="center" | {{ntsh|1}}Ia

|

|{{cite web |url=https://esahubble.org/images/potw2504a/ |title=SN 2022aajn |work=ESA |access-date=18 October 2024}}

| Ursa Major

| 19 May 2023
17:27

| align="center" | {{ntsh|10.8}}+10.8

| 21,000,000

| type II-L

| Pinwheel Galaxy (M101){{Cite journal |last=O'Callaghan |first=Jonathan |date=October 2023 |title=Out with a Bang |journal=Scientific American |volume=329 |issue=3 |pages=8–11|doi=10.1038/scientificamerican1023-8 |pmid=39017247 }}

| Closest and brightest supernova since SN 2014J

| Fornax

| 8 September 2023

| align="center" | {{ntsh|13.9}}+13.9

| 450,000,000

| align="center" | {{ntsh|2}}II

| NGC 1097{{cite web|url=https://www.wis-tns.org/object/2023rve|title=AT 2023rve|work=IAU Supernova Working Group|date=8 September 2023|access-date=10 September 2023|first=Mohammad|last=Odeh}}{{cite web|url=https://www.wis-tns.org/astronotes/astronote/2023-246|title=SN 2023rve: follow-up photometry with LCOGT DeltaRho 350 + QHY600

|work=IAU Supernova Working Group|date=12 September 2023|access-date=14 September 2023|first=P.|last=Arrizabalaga}}{{cite web|url=https://www.rochesterastronomy.org/sn2023/sn2023rve.html|title=Supernovae 2023rve in NGC 1097|work=Bright Supernovae|date=12 September 2023|access-date=14 September 2023|first=David|last=Bishop}}{{cite web|url=https://www.aavso.org/vsx/index.php?view=detail.top&oid=2388107|title=The International Variable Star Index: SN 2023rve|work=AAVSO|date=12 September 2023|access-date=14 September 2023|first=Sebastian|last=Otero}}{{cite web|url=https://www.astronomycenter.net/articles/2023/09/10/sn2023rve?l=en|title=New Supernova is Discovered From the UAE

|work=IAC|date=8 September 2023|access-date=14 September 2023|first=Osama|last=Ghannam}}

| Brightest Supernova Since SN 2023ixf.

| Pegasus

| 28 October 2023

| align="center" |

| 783,000,000

| align="center" | {{ntsh|1}}Ia

| NGC 7625

| {{citation | postscript=.

| title=Supernovae 2023vyl in NGC 7625 | date=January 26, 2024

| publisher=Astronomy Section, Rochester Academy of Science

| url=https://www.rochesterastronomy.org/sn2023/sn2023vyl.html

| access-date=2024-01-28 }}{{cite web | website=Transient Name Server | title=SN 2023vyl | url=https://www.wis-tns.org/object/2023vyl |publisher = IAU | access-date=14 August 2024}}

| Grus

| 12 December 2023

| align="center" |

| 816,000,000

| align="center" | {{ntsh|2}}II

| NGC 7421

| {{citation | postscript=.

| title=SN 2023abdg

| work=Transient Name Server

| url=https://www.wis-tns.org/object/2023abdg

| access-date=2024-02-04 }}

|

|

| align="center" | {{ntsh|15.55}}+15.55

|

| align=center|{{ntsh|2}} II

|

|The most metal-poor supernova found to date.{{Cite journal |last1=Tucker |first1=Michael A. |last2=Hinkle |first2=Jason |last3=Angus |first3=Charlotte R. |last4=Auchettl |first4=Katie |last5=Hoogendam |first5=Willem B. |last6=Shappee |first6=Benjamin |last7=Kochanek |first7=Christopher S. |last8=Ashall |first8=Chris |last9=Boer |first9=Thomas de |last10=Chambers |first10=Kenneth C. |last11=Desai |first11=Dhvanil D. |last12=Do |first12=Aaron |last13=Fulton |first13=Michael D. |last14=Gao |first14=Hua |last15=Herman |first15=Joanna |date=2024 |title=The Extremely Metal-poor SN 2023ufx: A Local Analog to High-redshift Type II Supernovae |journal=The Astrophysical Journal |language=en |volume=976 |issue=2 |pages=178 |doi=10.3847/1538-4357/ad8448 |doi-access=free |arxiv=2405.00113 |bibcode=2024ApJ...976..178T |issn=0004-637X}}

| Ursa Major

| 2023

| align="center" |

|

| align="center" | {{ntsh|1}}Ia

| PLCK G165.7+67.0 Arc 1

|{{cite journal |arxiv= 2306.12385 |doi= 10.1051/0004-6361/202346964 |title= Spectroscopy of the supernova H0pe host galaxy at redshift 1.78 |date= July 2023 | last1=Polletta | first1=M. | last2=Nonino | first2=M. | last3=Frye | first3=B. | last4=Gargiulo | first4=A. | last5=Bisogni | first5=S. | last6=Garuda | first6=N. | last7=Thompson | first7=D. | last8=Lehnert | first8=M. | last9=Pascale | first9=M. | last10=Willner | first10=S. P. | last11=Kamieneski | first11=P. | last12=Leimbach | first12=R. | last13=Cheng | first13=C. | last14=Coe | first14=D. | last15=Cohen | first15=S. H. | last16=Conselice | first16=C. J. | last17=Dai | first17=L. | last18=Diego | first18=J. | last19=Dole | first19=H. | last20=Driver | first20=S. P. | last21=d'Silva | first21=J. C. J. | last22=Fontana | first22=A. | last23=Foo | first23=N. | last24=Furtak | first24=L. J. | last25=Grogin | first25=N. A. | last26=Harrington | first26=K. | last27=Hathi | first27=N. P. | last28=Jansen | first28=R. A. | last29=Kelly | first29=P. | last30=Koekemoer | first30=A. M. |journal= Astronomy & Astrophysics |volume= 675 |pages= L4 |bibcode= 2023A&A...675L...4P |s2cid= 259212330 |display-authors= 3 }}

| Virgo

| 4 January 2024

| align="center" | {{ntsh|12.8}}+12.8

| 55,000,000

| align="center" | {{ntsh|1}} Ia

| NGC 4216

| {{cite web | website=Transient Name Server | title=SN{{nbsp}}2024gy | url=https://www.wis-tns.org/object/2024gy | publisher = IAU | access-date=17 December 2024}}

| Hydra

| 11 April 2024

| align="center" | {{ntsh|11.9}}+11.9

| 21,700,000

| align="center" | {{ntsh|2}} II

| NGC 3621

| {{cite web | website=Transient Name Server | title=SN{{nbsp}}2024ggi | url=https://www.wis-tns.org/object/2024ggi | publisher = IAU | access-date=4 December 2024}}

| Leo

| 10 May 2024

| align="center" | {{ntsh|12.1}}+12.1

| 82,200,000

| align="center" | {{ntsh|1}} Ia

| NGC 3524

| {{cite web | website=Transient Name Server | title=SN{{nbsp}}2024inv | url=https://www.wis-tns.org/object/2024inv | publisher = IAU | access-date=16 December 2024}}

| Virgo

| 26 June 2024

| align="center" | {{ntsh|12.7}}+12.7

| 65,000,000

| align="center" | {{ntsh|1}} Ia

| NGC 4699

| {{cite web | website=Transient Name Server | title=SN{{nbsp}}2024muv | url=https://www.wis-tns.org/object/2024muv | publisher = IAU | access-date=27 November 2024}}

| Camelopardalis

| 15 November 2024

| align="center" |

| 41,000,000

| align="center" | {{ntsh|2}} II

| NGC 2146

| {{cite web | website=Transient Name Server | title=SN{{nbsp}}2024abfl | url=https://www.wis-tns.org/object/2024abfl | publisher = IAU | access-date=15 November 2024}}

| Serpens

| 26 March 2025

| align="center" | {{ntsh|13.8}}+13.8

| 100,000,000

| align="center" | {{ntsh|1}} Ia

| NGC 5957

| {{cite web |title=2025fvw {{!}} Transient Name Server |url=https://www.wis-tns.org/object/2025fvw |website=www.wis-tns.org |access-date=31 March 2025}}

|+Yearly extragalactic supernovae reported

! Year

! Total

! Type I

! Type II

! LBV
(imposters)

! Brighter than
apmag 13

! Apmag of brightest
Supernova of that year

|2000–2023