2025PASP..137d4203D

Query : 2025PASP..137d4203D

2025PASP..137d4203D - Publ. Astron. Soc. Pac., 137, part no 4, 4203 (2025/April-0)

Low-luminosity Type IIP Supernovae from the Zwicky Transient Facility Census of the Local Universe. I. Luminosity Function, Volumetric Rate.

DAS K.K., KASLIWAL M.M., FREMLING C., SOLLERMAN J., PERLEY D.A., DE K., TZANIDAKIS A., SIT T., ADAMS S., ANAND S., AHUMUDA T., ANDREONI I., BRENNAN S., BRINK T., BRUCH R.J., CHEN P., CHU M.R., COOK D.O., COVARRUBIAS S., DAHIWALE A., EARLEY N., HO A.Y.Q., GAL-YAM A., GANGOPADHYAY A., HAMMERSTEIN E., HINDS K.-R., KARAMBELKAR V., KONG Y., KULKARNI S.R., JEGOU DU LAZ T., LIU C., MEYNARDIE W., MILLER A.A., NIR G., PATRA K.C., PESSI P.J., RICH R.M., REHEMTULLA N., ROSE S., RUSHOLME B., SCHULZE S., SHARMA Y., SINGH A., SMITH R., STEIN R., SHARMA MANDIGO-STOBA M., STROTJOHANN N.L., QIN Y.-J., WISE J., WOLD A., YAN L., YANG Y., YAO Y. and ZIMMERMAN E.

Abstract (from CDS):

We present the luminosity function and volumetric rate of a sample of Type IIP supernovae (SNe) from the Zwicky Transient Facility Census of the Local Universe survey (CLU). This is the largest sample of Type IIP SNe from a systematic volume-limited survey to-date. The final sample includes 330 Type IIP SNe and 36 low-luminosity Type II (LLIIP) SNe with Mr,peak > -16 mag, which triples the literature sample of LLIIP SNe. The fraction of LLIIP SNe is $1{9}_{-4}^{+3} \% $ of the total CLU Type IIP SNe population (${8}_{-2}^{+1} \% $ of all core-collapse SNe). This implies that while LLIIP SNe likely represent the fate of core-collapse SNe of 8-12 M⊙ progenitors, they alone cannot account for the fate of all massive stars in this mass range. To derive an absolute rate, we estimate the ZTF pipeline efficiency as a function of the apparent magnitude and the local surface brightness. We derive a volumetric rate of $(3.{9}_{-0.4}^{+0.4})\times 1{0}^{4}\,{\mathrm{Gpc}}^{-3}\,{\mathrm{yr}}^{-1}$ for Type IIP SNe and $(7.{3}_{-0.6}^{+0.6})\times 1{0}^{3}\,{\mathrm{Gpc}}^{-3}\,{\mathrm{yr}}^{-1}$ for LLIIP SNe. Now that the rate of LLIIP SNe is robustly derived, the unresolved discrepancy between core-collapse SN rates and star formation rates cannot be explained by LLIIP SNe alone.

Abstract Copyright: © 2025. The Author(s). Published by IOP Publishing Ltd on behalf of the Astronomical Society of the Pacific (ASP).

Journal keyword(s): Supernovae - Core-collapse supernovae - Type II supernovae - Surveys - Transient sources - Massive stars

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

Simbad objects: 25

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Number of rows : 25
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 AT 2008jd ev 00 54 34.16 -37 38 28.6           ~ 134 1
2 SN 2003gd SN* 01 36 42.65 +15 44 19.9     13.2     SNIIP 267 2
3 SN 2013ej SN* 01 36 48.16 +15 45 31.0           SNIIP 248 0
4 SN 2012ec SN* 02 45 59.89 -07 34 25.0         22.32 SNIIP 92 3
5 SN 2022acko SN* 03 19 38.990 -19 23 42.68           SNIIP 28 0
6 SN 2023zaw SN* 04 29 20.235 +70 25 37.52           SNIb 5 0
7 SN 2009kr SN* 05 12 03.30 -15 41 52.2           SNII 93 1
8 SN 2012A SN* 10 25 07.39 +17 09 14.6           SNIIP 135 0
9 NAME Great Attractor SCG 10 32 -46.0           ~ 617 0
10 SN 2012aw SN* 10 43 53.735 +11 40 17.63       15   SNIIP 252 1
11 SN 2009md SN* 10 48 26.28 +12 32 02.8           SNIIP 75 2
12 SPIRITS16tn SN? 11 11 20.40 +55 40 17.3           ~ 11 0
13 SN 2009hd SN* 11 20 16.99 +12 58 46.3           SNII 70 1
14 SN 2018aoq SN* 12 10 38.190 +39 23 47.00           SNIIP 33 0
15 SPIRITS16ix ev 12 29 03.16 +13 11 30.7           ~ 4 0
16 NAME Virgo Cluster ClG 12 30 47.8 +12 23 07           ~ 7107 0
17 SN 2006my SN* 12 43 40.74 +16 23 14.1     15.3     SNIIP 64 1
18 SN 2021inl SN* 13 01 33.245 +27 49 55.12           SNIb 15 0
19 NAME Shapley Supercluster SCG 13 06.0 -33 04           ~ 677 0
20 NAME M51 OT2019-1 ev 13 29 42.394 +47 11 16.99           ~ 30 0
21 SN 2005cs SN* 13 29 53.37 +47 10 28.2   14.5       SNIIP 450 1
22 SN 2004A SN* 16 43 01.90 +36 50 12.5     15.7     SNIIP 90 1
23 SN 2008S ev 20 34 45.33 +60 05 58.4   19.89 18.79 17.93   SNIIn? 253 1
24 SN 2004et SN* 20 35 25.33 +60 07 17.7   12.88       SNIIP 547 1
25 SN 2008bk SN* 23 57 50.42 -32 33 21.5           SNIIP 167 2

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