2020ApJ...896L..13S


Query : 2020ApJ...896L..13S

2020ApJ...896L..13S - Astrophys. J., 896, L13-L13 (2020/June-2)

Supernova siblings: assessing the consistency of properties of Type Ia supernovae that share the same parent galaxies.

SCOLNIC D., SMITH M., MASSIAH A., WISEMAN P., BROUT D., KESSLER R., DAVIS T.M., FOLEY R.J., GALBANY L., HINTON S.R., HOUNSELL R., KELSEY L., LIDMAN C., MACAULAY E., MORGAN R., NICHOL R.C., MOLLER A., POPOVIC B., SAKO M., SULLIVAN M., THOMAS B.P., TUCKER B.E., ABBOTT T.M.C., AGUENA M., ALLAM S., ANNIS J., AVILA S., BECHTOL K., BERTIN E., BROOKS D., BURKE D.L., CARNERO ROSELL A., CAROLLO D., CARRASCO KIND M., CARRETERO J., COSTANZI M., DA COSTA L.N., DE VICENTE J., DESAI S., DIEHL H.T., DOEL P., DRLICA-WAGNER A., ECKERT K., EIFLER T.F., EVERETT S., FLAUGHER B., FOSALBA P., FRIEMAN J., GARCIA-BELLIDO J., GAZTANAGA E., GERDES D.W., GLAZEBROOK K., GRUEN D., GRUENDL R.A., GSCHWEND J., GUTIERREZ G., HARTLEY W.G., HOLLOWOOD D.L., HONSCHEID K., JAMES D.J., KUEHN K., KUROPATKIN N., LEWIS G.F., LI T.S., LIMA M., MAIA M.A.G., MARSHALL J.L., MENANTEAU F., MIQUEL R., PALMESE A., PAZ-CHINCHON F., PLAZAS A.A., PURSIAINEN M., SANCHEZ E., SCARPINE V., SCHUBNELL M., SERRANO S., SEVILLA-NOARBE I., SOMMER N.E., SUCHYTA E., SWANSON M.E.C., TARLE G., VARGA T.N., WALKER A.R., WILKINSON R. (The DES Collaboration)

Abstract (from CDS):

While many studies have shown a correlation between properties of the light curves of SNe Ia and properties of their host galaxies, it remains unclear what is driving these correlations. We introduce a new direct method to study these correlations by analyzing "parent" galaxies that host multiple SNe Ia "siblings." Here, we search the Dark Energy Survey SN sample, one of the largest samples of discovered SNe, and find eight galaxies that hosted two likely SNe Ia. Comparing the light-curve properties of these SNe and recovered distances from the light curves, we find no better agreement between properties of SNe in the same galaxy as any random pair of galaxies, with the exception of the SN light-curve stretch. We show at 2.8σ significance that at least one-half of the intrinsic scatter of SNe Ia distance modulus residuals is not from common host properties. We also discuss the robustness with which we could make this evaluation with LSST, which will find 100x more pairs of galaxies, and pave a new line of study on the consistency of SNe Ia in the same parent galaxies. Finally, we argue that it is unlikely that some of these SNe are actually single, lensed SN with multiple images.

Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.

Journal keyword(s): Observational cosmology

Simbad objects: 26

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Number of rows : 26
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 DES13E1wu SN* 00 27 16.8 -42 34 26           SNIa 2 0
2 DES14E1uti SN* 00 27 16.8 -42 34 24           SNIa 2 0
3 DES15X2nku SN* 02 21 38.1 -05 45 56           SNIa 2 0
4 DES15X2mlr SN* 02 21 38.5 -05 45 56           SNIa 2 0
5 DES13S2dlj SN* 02 43 27.3 -01 36 06           SNIa 2 0
6 DES14S2pkz SN* 02 43 27.378 -01 36 13.12           SNIa 8 0
7 DES15S2okk SN* 02 47 02.7 -01 22 41           SNIa 2 0
8 DES17S2alm SN* 02 47 02.8 -01 22 41           SNIa 2 0
9 SN 1981D SN* 03 22 38.381 -37 13 57.79   12.59 12.33     SNIa 103 1
10 SN 2006dd SN* 03 22 41.64 -37 12 13.2   14.5 15.0     SNIa 87 1
11 NGC 1316 rG 03 22 41.789 -37 12 29.52 9.81 9.15 8.53 7.66   ~ 1491 1
12 SN 2006mr SN* 03 22 42.84 -37 12 28.5     15.6     SNIap 78 1
13 SN 1980N SN* 03 23 00.319 -37 12 49.90   12.5 12.37     SNIa 159 1
14 NAME DES16C3nd0 SN* 03 28 52.4 -27 34 28           SNIa 2 0
15 NAME DES16C3nd1 SN* 03 28 52.4 -27 34 28           SNIa 2 0
16 DES16C3nd ev 03 28 52.4 -27 34 28           SNIa 2 0
17 DES15C3edd SN* 03 33 10.671 -27 57 27.96           SNIa 11 0
18 DES14C3zym SN* 03 33 10.8 -27 57 26           SNIa 2 0
19 DES14C2iku SN* 03 37 37.1 -28 18 37           SNIa 2 0
20 DES17C2jjb SN* 03 37 37.2 -28 18 37           SNIa 2 0
21 ACO S 373 ClG 03 38 29.4 -35 27 08           ~ 2029 0
22 NGC 1404 rG 03 38 51.917 -35 35 39.81 11.53 10.69 10.00 9.03   ~ 787 1
23 DES15C2mky SN* 03 40 34.8 -28 37 41           SNIa 2 0
24 DES16C2cqh SN* 03 40 35.0 -28 37 40           SNIa 2 0
25 SN 2013aa SN* 14 32 33.88 -44 13 27.8           SNIa 81 1
26 SN 2017cbv SN* 14 32 34.420 -44 08 02.74           SNIa 146 0

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