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Supernovae at distances <40 Mpc I. Catalogues and fractions of supernovae in a complete sample

文献类型：期刊论文

作者Ma, Xiaoran13; Wang, Xiaofeng12,13; Mo, Jun13; Howell, D. Andrew10,11; Pellegrino, Craig10,11; Zhang JJ(张居甲)8,9; Yan, Shengyu13; Arcavi, Iair7; Chen, Zhihao13; Farah, Joseph10,11
刊名ASTRONOMY & ASTROPHYSICS
出版日期2025-06-26
卷号698
关键词methods: data analysis surveys supernovae: general
ISSN号0004-6361
DOI10.1051/0004-6361/202452684
产权排序第5完成单位
文献子类Article
英文摘要Context. This is the first paper in a series aiming to determine the fractions and birth rates of various types of supernovae (SNe) in the local Universe. Aims. In this paper, we aim to construct a complete sample of SNe in the nearby Universe and provide more precise measurements of subtype fractions. Methods. We carefully selected our SN sample at a distance of less than 40 Mpc mainly from wide-field surveys conducted over the years from 2016 to 2023. Results. The sample contains a total of 211 SNe, including 109 SNe II, 69 SNe Ia, and 33 SNe Ibc. With the aid of sufficient spectra, we obtained relatively accurate subtype classifications for all SNe in this sample. After corrections for the Malmquist bias, this volumelimited sample yielded fractions of SNe Ia, SNe Ibc, and SNe II of 30.4(-11.5)(+3.7) %, 16.3(-7.4)(+3.7) %, and 53.3(-18.7)(+9.5) %, respectively. In the SN Ia sample, the fraction of the 91T-like subtype becomes relatively low (similar to 5.4%), while that of the 02cx-like subtype shows a moderate increase (similar to 6.8%). In the SN Ibc sample, we find significant fractions of broadlined SNe Ic (similar to 18.0%) and SNe Ibn (similar to 8.8%). The fraction of the 87A-like subtype was determined to be similar to 2.3%, indicating rare explosions from blue supergiant stars. We find that SNe Ia show a double peak number distribution in S0- and Sc-type host galaxies, which may serve as straightforward evidence for the presence of prompt and delayed progenitor components that give rise to SN Ia explosions. Several subtypes of SNe such as 02cx-like SNe Ia, broadlined SNe Ic, and SNe IIn (and perhaps SNe Ibn) are found to occur preferentially in less massive spiral galaxies (i.e., with stellar mass <0.5x10(10) M-circle dot), thus favoring their associations with young stellar progenitors. Moreover, the 02cx-like subtype shows a trend of exploding in the outer skirt of their hosts, which is suggestive of metal-poor progenitors.
学科主题天文学 ; 恒星与银河系
URL标识查看原文
出版地17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE
WOS关键词CORE-COLLAPSE SUPERNOVAE ; II-P SUPERNOVA ; IA SUPERNOVA ; LIGHT CURVES ; PHYSICAL-PROPERTIES ; JWST OBSERVATIONS ; MALMQUIST BIAS ; SHOCK BREAKOUT ; MASSIVE STARS ; DATA RELEASE
资助项目National Science Foundation of China[12288102]; National Science Foundation of China[12033003]; China Manned Space Project[CMS-CSST-2021-A12]; Tencent Xplorer prize; NSF[AST-1911225]; NSF[AST-1911151]; UKRI Science and Technology Facilities Council; University of Edinburgh[ST/N002512/1]; Queen's University Belfast[ST/N002520/1]; LSST:UK Science Consortium; National Science Foundation[AST-1440341]; Weizmann Institute for Science; Oskar Klein Center at Stockholm University; University of Washington, Deutsches Elektronen-Synchrotron and Humboldt University, Los Alamos National Laboratories; TANGO Consortium of Taiwan; University of Wisconsin at Milwaukee; Lawrence Berkeley National Laboratories[2000A]; Lawrence Berkeley National Laboratories[.143. . . 33B]; Lawrence Berkeley National Laboratories[2014ASPC]; Asteroid Terrestrial Impact Last Alert System (ATLAS) project; Asteroid Terrestrial Impact Last Alert System; NASA[NN12AR55G]; NASA[80NSSC18K0284]; NASA[80NSSC18K1575]; NASA[J1944/80NSSC19K0112]; NASA[HST GO-15889]; STFC[ST/T000198/1]; STFC[ST/S006109/1]; South African Astronomical Observatory; ESA Gaia, DPAC; National Natural Science Foundation of China (NSFC)[12403061]; Innovative project of Caiyun Post-doctoral Project of Yunnan Province
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001518016800001
出版者EDP SCIENCES S A
资助机构National Science Foundation of China[12288102, 12033003] ; China Manned Space Project[CMS-CSST-2021-A12] ; Tencent Xplorer prize ; NSF[AST-1911225, AST-1911151] ; UKRI Science and Technology Facilities Council ; University of Edinburgh[ST/N002512/1] ; Queen's University Belfast[ST/N002520/1] ; LSST:UK Science Consortium ; National Science Foundation[AST-1440341] ; Weizmann Institute for Science ; Oskar Klein Center at Stockholm University ; University of Washington, Deutsches Elektronen-Synchrotron and Humboldt University, Los Alamos National Laboratories ; TANGO Consortium of Taiwan ; University of Wisconsin at Milwaukee ; Lawrence Berkeley National Laboratories[2000A, .143. . . 33B, 2014ASPC] ; Asteroid Terrestrial Impact Last Alert System (ATLAS) project ; Asteroid Terrestrial Impact Last Alert System ; NASA[NN12AR55G, 80NSSC18K0284, 80NSSC18K1575, J1944/80NSSC19K0112, HST GO-15889] ; STFC[ST/T000198/1, ST/S006109/1] ; South African Astronomical Observatory ; ESA Gaia, DPAC ; National Natural Science Foundation of China (NSFC)[12403061] ; Innovative project of Caiyun Post-doctoral Project of Yunnan Province
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/28386]  
专题云南天文台_丽江天文观测站（南方基地）
通讯作者Wang, Xiaofeng
作者单位1.Beijing Planetarium, Beijing Academy of Sciences and Technology, Beijing, 100044, China
2.School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 101408, China;
3.Key Laboratory of Space Astronomy and Technology, National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Beijing 100101, China;
4.School of Physics and Information Engineering, Jiangsu Second Normal University, Nanjing 211200, China;
5.The NSF AI Institute for Artificial Intelligence and Fundamental Interactions, USA;
6.Center for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138-1516, USA;
7.School of Physics and Astronomy, Tel Aviv University, Tel Aviv 69978, Israel;
8.International Centre of Supernovae, Yunnan Key Laboratory, Kunming 650216, PR China;
9.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, China;
10.Department of Physics, University of California, Santa Barbara, CA 93106-9530, USA;
推荐引用方式
GB/T 7714		 Ma, Xiaoran,Wang, Xiaofeng,Mo, Jun,et al. Supernovae at distances <40 Mpc I. Catalogues and fractions of supernovae in a complete sample[J]. ASTRONOMY & ASTROPHYSICS,2025,698.
APA Ma, Xiaoran.,Wang, Xiaofeng.,Mo, Jun.,Howell, D. Andrew.,Pellegrino, Craig.,...&Zhang, Tianmeng.(2025).Supernovae at distances <40 Mpc I. Catalogues and fractions of supernovae in a complete sample.ASTRONOMY & ASTROPHYSICS,698.
MLA Ma, Xiaoran,et al."Supernovae at distances <40 Mpc I. Catalogues and fractions of supernovae in a complete sample".ASTRONOMY & ASTROPHYSICS 698(2025).

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