Scope of the Catalog: A comprehensive table of M33 novae going back to the first recorded nova in 1919 was created by W. Pietsch and posted on the Max Planck Institute for Extraterrestrial Physics (MPE) webpage (MPE M33 Catalog). The catalog was last updated on 2021 August 24. My purpose in the following table is to continue the M33 nova catalog, but in an abbreviated form. Eruptions of the recurrent nova M33N 2011-10a (= 2021-08a = 2025-10a), the first confirmed recurrent nova in M33, are shown in red. The four objects flagged in the MPE catalog as not novae (M33N 2014-08a, 2014-11a, 2014-11b and 2018-10a, all red long-period variables) are omitted.
At present, I give the nova name, the JD of the start of the eruption, the equatorial coordinates (J2000), the approximate magnitude near the start of the eruption, the spectroscopic class (where known), notes, and references. Note that the JD and magnitude do not necessarily correspond to maximum light, although in most cases they are close. Magnitudes are the brightest reported; filter codes are pg (photographic), Ha (Hα), w (unfiltered/white light), o (ATLAS orange), and standard band names; ? means no filter information is available. The Type column gives the spectroscopic class, based on the Fe II and He/N classes of Williams (1992), where one has been published, as given in the original references: Fe II; He/N; Fe IIb (broad-lined Fe II); Hybrid (Fe IIb systems displaying broad He and N lines); and Nova (spectroscopically confirmed as a nova, class not given). A question mark indicates an uncertain class, "X or Y" an ambiguous one, and a blank entry means that no class is available. For entries reported after the MPE catalog ends (from 2021-08b onward, except the recurrent-nova eruptions 2021-08a and 2025-10a), I have assigned designations following the MPE/CBAT convention (year-month and letter, in order of discovery within the month) and are not official; the AT name is given in the Notes. 2021-08b is lettered after 2021-08a, which MPE had already assigned to the recurrent nova, although it was found 5 days earlier. AT 2024pwl and AT 2025yal, which are long-period variables rather than novae, are listed under their AT names.
Author: A. W. Shafter (SDSU).
How to cite this catalog: If you use data from this catalog in a publication, please cite it as: Shafter, A. W., A Living Catalog of Novae in M33, https://ashafter.sdsu.edu/m33_nova_table.html (accessed [date]). Data for novae discovered through August 2021 are from the MPE catalog of W. Pietsch (https://www.mpe.mpg.de/~m31novae/opt/m33/M33_table.html), which should also be acknowledged. Where your work relies on the properties of individual novae, please also cite the original references given in the References column. This catalog is made available under a Creative Commons Attribution 4.0 International License (CC BY 4.0).
| Name | JD | R.A. (h, m, s) | Decl. (°, ',") | mag | Type | Notes | References |
|---|---|---|---|---|---|---|---|
| M33N 1919-12a | 2422306.50 | 1 33 59.05 | 30 39 51.5 | 17.2 pg | Hubble N1 | Hubble 1926; Samus et al. 2004 (GCVS) | |
| M33N 1922-08a | 2423292.00 | 1 33 29.26 | 30 49 16.3 | 17.5 pg | Suspected nova | Duncan 1922; Samus et al. 2004 (GCVS) | |
| M33N 1925-07a | 2424348.50 | 1 34 14.38 | 30 49 03.0 | 17.9 pg | Hubble N2 | Hubble 1926; Samus et al. 2004 (GCVS) | |
| M33N 1925-12a | 2424493.30 | 1 34 12.22 | 30 34 21.1 | 18.1 pg | Hubble N3 | Hubble 1929; Samus et al. 2004 (GCVS) | |
| M33N 1927-07a | 2425091.60 | 1 33 24.23 | 30 46 52.4 | 17.7 pg | Hubble N4 | Hubble 1929; Samus et al. 2004 (GCVS) | |
| M33N 1927-09a | 2425124.50 | 1 33 53.21 | 30 37 39.6 | ... | Year only | Stratton 1936; Samus et al. 2004 (GCVS) | |
| M33N 1928-10a | 2425534.50 | 1 33 43.12 | 30 31 09.9 | 16.0 pg | Carpenter 1929; Samus et al. 2004 (GCVS) | ||
| M33N 1949-08a | 2433157.50 | 1 32 15.86 | 30 28 48.4 | 16.6 pg | Suspected nova | Rosino & Bianchini 1973; Samus et al. 2004 (GCVS) | |
| M33N 1955-07a | 2435289.50 | 1 33 34.43 | 30 34 26.2 | 17.2 V | Year only | Humphreys & Sandage 1980; Samus et al. 2004 (GCVS); Sharov 1997 (IBVS 4415) | |
| M33N 1960-11a | 2437253.51 | 1 34 06.97 | 30 40 27.2 | 16.4 pg | Rosino & Bianchini 1973; Samus et al. 2004 (GCVS) | ||
| M33N 1961-03a | 2437365.32 | 1 35 02.37 | 30 35 49.6 | 18.5 pg | Rosino & Bianchini 1973; Samus et al. 2004 (GCVS) | ||
| M33N 1961-11a | 2437632.29 | 1 34 05.20 | 30 33 33.3 | 18.0 pg | Rosino & Bianchini 1973; Samus et al. 2004 (GCVS) | ||
| M33N 1962-09a | 2437917.56 | 1 33 03.75 | 30 44 25.0 | 18.0 pg | Rosino & Bianchini 1973; Samus et al. 2004 (GCVS) | ||
| M33N 1962-09b | 2437929.53 | 1 33 55.25 | 30 41 33.6 | 17.3 pg | Rosino & Bianchini 1973; Samus et al. 2004 (GCVS) | ||
| M33N 1969-11a | 2440529.78 | 1 34 23.38 | 30 46 56.8 | 18.0 V | Suspected nova | Kowal 1969 (IAUC 2195); Samus et al. 2004 (GCVS) | |
| M33N 1970-09a | 2440836.00 | 1 34 25.49 | 30 57 08.7 | 18.0 pg | Suspected nova | Samus et al. 2004 (GCVS); Sharov 1988 (MoIzN) | |
| M33N 1974-12a | 2442386.50 | 1 34 43.3 | 30 32 48 | 16.3 pg | Position from finding chart | Della Valle 1994 | |
| M33N 1975-10a | 2442691.50 | 1 33 36.0 | 30 36 36 | 18.8 pg | Position from finding chart | Della Valle 1994 | |
| M33N 1977-12a | 2443506.50 | 1 33 10.6 | 30 25 36 | 17.9 pg | Position from finding chart | Della Valle 1994 | |
| M33N 1982-09a | 2445229.41 | 1 34 05.46 | 30 46 04.6 | 17.9 B | Sharov 1997 (IBVS 4415); Della Valle 1994 | ||
| M33N 1986-10a | 2446703.36 | 1 33 35.70 | 30 35 03.3 | 18.5 B | Sharov 1997 (IBVS 4415); Della Valle 1994 | ||
| M33N 1995-08a | 2449955.50 | 1 33 47.1 | 30 40 26 | 16.0 Ha | Williams & Shafter 2004 | ||
| M33N 1995-08b | 2449957.50 | 1 33 17.2 | 30 33 11 | 16.6 Ha | Williams & Shafter 2004 | ||
| M33N 1995-09a | 2450012.50 | 1 34 06.9 | 30 37 18 | 16.2 Ha | Williams & Shafter 2004 | ||
| M33N 1996-12a | 2450426.50 | 1 34 20.7 | 30 34 39 | 19.1 Ha | Williams & Shafter 2004 | ||
| M33N 1997-09a | 2450692.50 | 1 34 24.4 | 30 42 43 | 19.3 Ha | Williams & Shafter 2004 | ||
| M33N 2001-11a | 2452229.26 | 1 33 42.8 | 30 40 52 | 16.5 w | Trondal et al. 2001 (IAUC 7756); Williams & Shafter 2004 | ||
| M33N 2003-09a | 2452883.90 | 1 33 51.16 | 30 39 50.2 | 16.9 w | Fe IIb? | Ganeshalingam & Li 2003 (IAUC 8195); Shporer et al. 2003 (IAUC 8199); Schwarz et al. 2003 (IAUC 8234); Shafter et al. 2012 | |
| M33N 2006-09a | 2454006.70 | 1 33 18.66 | 30 49 49.2 | 16.6 w | Fe II | Quimby et al. 2006 (CBET 655); Shafter et al. 2012; Shafter et al. 2006 (ATel 923) | |
| M33N 2007-09a | 2454362.13 | 1 33 58.65 | 30 57 34.4 | 16.2 R | He/N | Nakano et al. 2007 (CBET 1074); Wagner et al. 2007 (CBET 1080); Shafter et al. 2012; Shafter et al. 2007 (ATel 1225) | |
| M33N 2008-02a | 2454523.97 | 1 34 16.42 | 30 39 28.6 | 16.5 w | Fe II | Nakano et al. 2008 (CBET 1272); Shafter et al. 2012 | |
| M33N 2009-01a | 2454839.04 | 1 33 40.42 | 30 25 42.1 | 17.0 w | He/N | Nakano 2009 (CBET 1659); Shafter et al. 2012; Shafter et al. 2009 (ATel 1900) | |
| M33N 2010-07a | 2455376.50 | 1 33 36.86 | 30 46 22.2 | 17.1 w | PTF10ncv | Nishiyama et al. 2010 (CBET 2375); Shafter et al. 2012 | |
| M33N 2010-10a | 2455495.65 | 1 33 57.10 | 30 45 53.4 | 17.7 w | Fe IIb (hybrid) | Nishiyama et al. 2010 (CBET 2533); Shafter et al. 2012; Shafter et al. 2010 (ATel 2982); Shafter et al. 2010 (CBET 2533) | |
| M33N 2010-11a | 2455528.03 | 1 33 27.55 | 30 17 28.4 | 16.1 w | Fe IIb | Ruan & Gao 2010 (CBET 2559); Yusa 2010 (CBET 2559); Nishiyama & Kabashima 2010 (CBET 2559); Shafter et al. 2010 (ATel 3063); Shafter et al. 2012 | |
| M33N 2010-12a | 2455547.92 | 1 34 17.98 | 30 43 58.3 | 16.4 w | He/N | Yusa et al. 2010 (CBET 2595); Shafter et al. 2010 (ATel 3086); Shafter et al. 2012 | |
| M33N 2011-10a | 2455842.67 | 1 35 01.94 | 30 43 19.8 | ... | RN; 1st known eruption (recovered in archival PTF images) | Shafter et al. 2025 (ATel 17435) | |
| M33N 2012-02a | 2455976.95 | 1 33 11.24 | 30 40 10.4 | 16.4 w | CBAT TOCP | ||
| M33N 2012-10a | 2456203.67 | 1 32 57.23 | 30 24 26.0 | 15.8 w | Fe II | Zheng et al. 2012 (CBET 3250); Nishiyama et al. 2012 (CBET 3250); Caldwell et al. 2012 (CBET 3250); Shafter et al. 2012 (ATel 4464) | |
| M33N 2013-01a | 2456296.97 | 1 34 04.39 | 30 39 04.3 | 17.0 w | Fe II | CBAT TOCP; Shafter et al. 2013 (ATel 4720) | |
| M33N 2013-12a | 2456650.71 | 1 33 10.92 | 30 37 51.1 | 17.9 w | Fe II? | CBAT TOCP; Fabrika et al. 2014 (ATel 5746) | |
| M33N 2014-02a | 2456714.33 | 1 33 00.51 | 30 33 47.9 | 17.4 w | CBAT TOCP | ||
| M33N 2014-07a | 2456858.57 | 1 34 02.88 | 30 35 11.1 | 18.5 R | Confirmed in Hα | Hornoch 2014 (ATel 6331); Hornoch et al. 2014 (ATel 6350); Hornoch et al. 2014 (ATel 6356) | |
| M33N 2014-07b | 2456867.71 | 1 34 07.56 | 30 50 41.3 | 20.8 R | Confirmed in Hα | Hornoch et al. 2014 (ATel 6373); CBAT TOCP | |
| M33N 2014-11c | 2456978.67 | 1 34 38.34 | 31 05 07.2 | 16.6 w | CBAT TOCP | ||
| M33N 2015-12a | 2457358.29 | 1 33 47.26 | 30 26 51.3 | 15.7 w | Fe II | ASASSN-15th | CBAT TOCP; CBAT TOCP; CBAT TOCP; Popova et al. 2015 (ATel 8407); Gress et al. 2015 (ATel 8416); Wagner et al. 2015 (ATel 8352); Darnley & Williams 2015 (ATel 8396) |
| M33N 2015-12b | 2457382.45 | 1 33 54.17 | 30 26 10.8 | 16.8 w | Fe II | CBAT TOCP; Williams & Darnley 2016 (ATel 8511) | |
| M33N 2016-12a | 2457726.05 | 1 34 01.57 | 30 42 39.9 | 16.8 w | He/N | AT 2016irp | TNS 2016irp; CBAT TOCP; CBAT TOCP; Williams & Darnley 2016 (ATel 9828) |
| M33N 2017-10a | 2458054.92 | 1 33 07.85 | 30 33 09.1 | 19.0 w | AT 2017hqh | TNS 2017hqh | |
| M33N 2019-01a | 2458489.03 | 1 33 56.94 | 30 32 33.7 | 17.0 o | Fe IIb | AT 2019gc | CBAT TOCP; TNS 2019gc; Cappellaro et al. 2019 (ATel 12361) |
| M33N 2019-06a | 2458654.95 | 1 32 32.41 | 30 35 21.5 | 19.1 r | AT 2019iby | TNS 2019iby; Lasair ZTF19aawtdov | |
| M33N 2019-09a | 2458747.12 | 1 33 52.73 | 30 44 36.2 | 17.6 w | AT 2019qml | TNS 2019qml; CBAT TOCP | |
| M33N 2019-11a | 2458814.15 | 1 34 33.20 | 30 39 05.2 | 20.7 w | AT 2019vub | TNS 2019vub | |
| M33N 2019-11b | 2458818.16 | 1 33 13.98 | 30 27 50.3 | 19.3 w | AT 2019xuw | TNS 2019xuw | |
| M33N 2020-06a | 2459022.39 | 1 33 27.69 | 30 32 08.7 | 18.3 w | CBAT TOCP | ||
| M33N 2020-09a | 2459117.79 | 1 34 05.62 | 30 57 29.4 | 18.4 r | Fe II | AT 2020upt | Lasair ZTF20aceeeuz; TNS 2020upt; Reguitti et al. 2020 (ATel 14189) |
| M33N 2021-01a | 2459218.15 | 1 33 22.00 | 30 33 01.2 | 17.9 w | Nova | AT 2021bl; t3 < 5 d | XOSS XM48MZ; TNS 2021bl; Bryan & Shafter 2021 (ATel 14355); CBAT TOCP; Karambelkar 2021 (TNS Classification Report); Rochester Extragalactic Novae 2021 |
| M33N 2021-07a | 2459416.20 | 1 33 38.54 | 30 35 36.4 | 17.5 w | AT 2021wcf | CBAT TOCP; TNS 2021wcf; Gaia21duh | |
| M33N 2021-08b | 2459438.95 | 1 34 25.81 | 30 55 18.9 | 20.9 g | AT 2021wjl; ZTF21absjpej | ZTF (TNS 2021wjl) | |
| M33N 2021-08a | 2459443.58 | 1 35 01.94 | 30 43 19.8 | 19.6 g | RN; 2nd eruption of M33N 2011-10a; AT 2021wfc | BAA observation database (2021 Aug 18); ZTF (TNS 2021wfc); Shafter et al. 2025 (ATel 17435) | |
| M33N 2021-09a | 2459485.38 | 1 33 40.0 | 30 29 59 | 18.5 w | AT 2021zsv; unconfirmed; not detected in ATLAS or ZTF forced photometry (including positions up to 6" either side in R.A.) | Conjat (TNS 2021zsv) | |
| M33N 2022-12a | 2459914.65 | 1 33 56.38 | 30 40 25.6 | 20.1 r | AT 2022acki; ZTF18adicrrs; probable LPV (recurring red brightenings in ZTF, about every 400 d) | ZTF (TNS 2022acki) | |
| M33N 2023-02a | 2459986.29 | 1 34 52.97 | 30 47 14.5 | 16.8 g | Nova? | AT 2023bne; classified "CV in outburst?" from its color and an early featureless spectrum, but probably a nova (g-r reddens a few days later; no other outburst 2015-2026) | Castellani et al. (TNS 2023bne); Poidevin & Perez-Fournon 2023 (ATel 15899); Castellani 2023 (TNS Classification Report) |
| M33N 2023-07a | 2460145.94 | 1 33 56.43 | 30 43 35.7 | 16.7 w | AT 2023nou; not a nova? (not detected in ATLAS or ZTF forced photometry) | GEOTS (TNS 2023nou); David's Astronomy Pages (2023 Jul 31 – Oct 3) | |
| M33N 2023-11a | 2460278.11 | 1 32 54.00 | 30 21 38.7 | 18.2 w | Fe II? | AT 2023ypg; narrow Balmer lines | XOSS (TNS 2023ypg); Zhao 2023 (TNS Classification Report) |
| AT 2024pwl | 2460511.86 | 1 34 15.33 | 30 30 45.2 | 19.5 r | ZTF23aaapxqa; LPV | ZTF (TNS 2024pwl) | |
| M33N 2024-08a | 2460537.87 | 1 34 02.81 | 30 42 40.6 | 17.2 w | AT 2024sgd; not a nova? (not detected in ATLAS or ZTF forced photometry) | GEOTS (TNS 2024sgd) | |
| M33N 2024-09a | 2460564.86 | 1 33 13.12 | 30 38 27.5 | 19.5 r | Nova | AT 2024vfg; ZTF24abhbdph | ZTF (TNS 2024vfg); Wise 2024 (TNS Classification Report) |
| M33N 2024-11a | 2460635.91 | 1 33 16.60 | 30 21 44.6 | 16.1 o | Fe IIb? | AT 2024abqt; ATLAS24qiq; broad Hα | ATLAS (TNS 2024abqt); Garcia Lozano et al. 2024 (ATel 16918); Balcon 2024 (TNS Classification Report) |
| M33N 2024-12a | 2460674.95 | 1 33 10.38 | 30 45 34.3 | 17.6 w | He/N? | AT 2024afyi; Hα FWHM ~6250 km/s, double-peaked (He/N or very broad-lined Fe IIb) | Itagaki (TNS 2024afyi); Chamoli et al. 2025 (ATel 16965) |
| M33N 2025-05a | 2460825.37 | 1 34 01.66 | 30 49 05.2 | 17.8 w | AT 2025mmr | XOSS (TNS 2025mmr) | |
| M33N 2025-06a | 2460844.35 | 1 34 28.03 | 31 05 19.2 | 16.7 w | Nova | AT 2025ofe | ATLAS (TNS 2025ofe); Balcon 2025 (TNS Classification Report) |
| AT 2025yal | 2460938.50 | 1 32 10.0 | 30 29 11 | 18.0 w | LPV maximum | Lorrai (TNS 2025yal) | |
| M33N 2025-09a | 2460940.20 | 1 33 24.34 | 30 37 36.9 | 18.2 w | AT 2025yhk; TNS position may be off by ~1-2" (ZTF forced photometry) | XOSS (TNS 2025yhk) | |
| M33N 2025-10a | 2460951.15 | 1 35 01.97 | 30 43 20.2 | 18.4 w | He/N | RN; 3rd eruption of M33N 2011-10a | Shafter et al. 2025 (ATel 17435); Xu & Gao (CBAT TOCP); Darnley et al. 2025 (ATel 17432) |
*Data through 2021 August are from the MPE M33 Catalog. Last updated 2 November 2026; table maintenance is now being assisted by AI (Claude Opus 5.5).