2023ApJS..266....9A

Query : 2023ApJS..266....9A

2023ApJS..266....9A - Astrophys. J., Suppl. Ser., 266, 9 (2023/May-0)

The Young Supernova Experiment Data Release 1 (YSE DR1): Light Curves and Photometric Classification of 1975 Supernovae.

ALEO P.D., MALANCHEV K., SHARIEF S., JONES D.O., NARAYAN G., FOLEY R.J., VILLAR V.A., ANGUS C.R., BALDASSARE V.F., BUSTAMANTE-ROSELL M.J., CHATTERJEE D., COLD C., COULTER D.A., DAVIS K.W., DHAWAN S., DROUT M.R., ENGEL A., FRENCH K.D., GAGLIANO A., GALL C., HJORTH J., HUBER M.E., JACOBSON-GALAN W.V., KILPATRICK C.D., LANGEROODI D., MACIAS P., MANDEL K.S., MARGUTTI R., MATASIC F., McGILL P., PIEREL J.D.R., RAMIREZ-RUIZ E., RANSOME C.L., ROJAS-BRAVO C., SIEBERT M.R., SMITH K.W., DE SOTO K.M., STROH M.C., TINYANONT S., TAGGART K., WARD S.M., WOJTAK R., AUCHETTL K., BLANCHARD P.K., DE BOER T.J.L., BOYD B.M., CARROLL C.M., CHAMBERS K.C., DEMARCHI L., DIMITRIADIS G., DODD S.A., EARL N., FARIAS D., GAO H., GOMEZ S., GRAYLING M., GRILLO C., HAYES E.E., HUNG T., IZZO L., KHETAN N., KOLBORG A.N., LAW-SMITH J.A.P., LEBARON N., LIN C.-C., LUO Y., MAGNIER E.A., MATTHEWS D., MOCKLER B., O'GRADY A.J.G., PAN Y.-C., POLITSCH C.A., RAIMUNDO S.I., REST A., RIDDEN-HARPER R., SARANGI A., SCHRODER S.L., SMARTT S.J., TERRERAN G., THORP S., VAZQUEZ J., WAINSCOAT R.J., WANG Q., WASSERMAN A.R., YADAVALLI S.K., YARZA R., ZENATI Y. (The Young Supernova Experiment)

Abstract (from CDS):

We present the Young Supernova Experiment Data Release 1 (YSE DR1), comprised of processed multicolor PanSTARRS1 griz and Zwicky Transient Facility (ZTF) gr photometry of 1975 transients with host-galaxy associations, redshifts, spectroscopic and/or photometric classifications, and additional data products from 2019 November 24 to 2021 December 20. YSE DR1 spans discoveries and observations from young and fast-rising supernovae (SNe) to transients that persist for over a year, with a redshift distribution reaching z ≈ 0.5. We present relative SN rates from YSE's magnitude- and volume-limited surveys, which are consistent with previously published values within estimated uncertainties for untargeted surveys. We combine YSE and ZTF data, and create multisurvey SN simulations to train the ParSNIP and SuperRAENN photometric classification algorithms; when validating our ParSNIP classifier on 472 spectroscopically classified YSE DR1 SNe, we achieve 82% accuracy across three SN classes (SNe Ia, II, Ib/Ic) and 90% accuracy across two SN classes (SNe Ia, core-collapse SNe). Our classifier performs particularly well on SNe Ia, with high (>90%) individual completeness and purity, which will help build an anchor photometric SNe Ia sample for cosmology. We then use our photometric classifier to characterize our photometric sample of 1483 SNe, labeling 1048 (∼71%) SNe Ia, 339 (∼23%) SNe II, and 96 (∼6%) SNe Ib/Ic. YSE DR1 provides a training ground for building discovery, anomaly detection, and classification algorithms, performing cosmological analyses, understanding the nature of red and rare transients, exploring tidal disruption events and nuclear variability, and preparing for the forthcoming Vera C. Rubin Observatory Legacy Survey of Space and Time.

Abstract Copyright: © 2023. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Supernovae - Surveys - Astronomy databases - Light curves - Light curve classification

VizieR on-line data: <Available at CDS (J/ApJS/266/9): tablec2.dat tablec3.dat lcs/*>

Status at CDS : Objects in title, abstract, text, figures, and all or part of small table(s) being processed in SIMBAD. // All or part of tables of objects will be ingested in SIMBAD with priority 1.

Simbad objects: 32

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Number of rows : 32
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 LEDA 1605946 G 00 10 21.4525477752 +19 48 00.496406592           ~ 4 0
2 SN 2011fu SN* 02 08 21.40 +41 29 12.3           SNII 74 1
3 SN 2002hu SN* 02 18 20.028 +37 27 58.57   16.83       SNIa 55 1
4 SN 2007Y SN* 03 02 35.92 -22 53 50.1     17.5     SNIb 135 1
5 AT 2021ehb ev 03 07 47.806 +40 18 40.57           ~ 42 0
6 SN 2002fk SN* 03 22 05.71 -15 24 03.2     15.7     SNIa 113 1
7 SN 2021hpr SN* 10 16 38.620 +73 24 01.80           SNIa 24 0
8 NGC 3147 Sy2 10 16 53.6388580752 +73 24 02.641798224   11.43 10.61     ~ 533 2
9 SN 2005bf SN* 10 23 56.99 -03 11 29.3     18.0     SNIb 225 1
10 SN 2001N SN* 10 39 58.08 +24 05 26.0     16.3     SNIa 35 1
11 SN 2020fci SN* 10 47 50.010 -00 47 30.30           SNIa 2 0
12 SN 1999aw SN* 11 01 36.37 -06 06 31.6   16.88       SNIa 76 1
13 SN 2017ein SN* 11 52 53.26 +44 07 26.2           SNIc 69 0
14 SN 2006bp SN* 11 53 55.74 +52 21 09.4 14.5 15.8 14.7     SNIIP 191 1
15 NAME Virgo Cluster ClG 12 30 47.8 +12 23 07           ~ 7107 0
16 SN 2011bm SN* 12 56 53.89 +22 22 28.2           SNIc 72 1
17 SN 2020kre SN* 13 10 29.870 -01 18 51.04           SNIa 6 0
18 SN 1996X SN* 13 18 01.13 -26 50 45.3   12.99 13.00     SNIa 198 1
19 SN 1994I SN* 13 29 54.072 +47 11 30.50     12.9     SNIc 645 1
20 SN 2021mnj SN* 14 45 20.590 +38 44 18.56           SNII 1 0
21 PSST 21grp ev 15 18 59.295 -03 11 45.08           ~ 4 0
22 SDSS J152120.08+140410.5 G 15 21 20.0794689096 +14 04 10.555029480           ~ 36 0
23 SN 2020aekp SN* 15 43 11.387 +17 48 47.22           SNIa 10 0
24 AT 2020opy ev 15 56 25.728 +23 22 21.15           ~ 28 0
25 SN 2006cc SN* 16 09 56.470 +43 07 35.90     18.3     SNIa 36 1
26 PTF 10qts SN* 16 41 37.60 +28 58 21.1           SNIc 27 0
27 AT 2020nov ev 16 58 12.970 +02 07 03.04           ~ 17 0
28 SN 2009ip s*b 22 23 08.26 -28 56 52.4           LBV 406 0
29 SN 2007ru SN* 23 07 23.19 +43 35 34.1     17.5     SNIc-BL 62 1
30 SN 2001ic SN* 23 10 43.34 +07 34 10.4     17.4     SNIa 35 1
31 SN 2003jd SN* 23 21 03.38 -04 53 45.5   16.34       SNIc-BL 147 1
32 SN 2006iw SN* 23 21 19.48 +00 15 35.1   19.82 18.97 18.56 18.31 SNIIP 36 1

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