2021MNRAS.504.2535I

Query : 2021MNRAS.504.2535I

2021MNRAS.504.2535I - Mon. Not. R. Astron. Soc., 504, 2535-2549 (2021/June-3)

The first Hubble diagram and cosmological constraints using superluminous supernovae.

INSERRA C., SULLIVAN M., ANGUS C.R., MACAULAY E., NICHOL R.C., SMITH M., FROHMAIER C., GUTIERREZ C.P., VICENZI M., MOLLER A., BROUT D., BROWN P.J., DAVIS T.M., D'ANDREA C.B., GALBANY L., KESSLER R., KIM A.G., PAN Y.-C., PURSIAINEN M., SCOLNIC D., THOMAS B.P., WISEMAN P., ABBOTT T.M.C., ANNIS J., AVILA S., BERTIN E., BROOKS D., BURKE D.L., CARNERO ROSELL A., CARRASCO KIND M., CARRETERO J., CASTANDER F.J., CAWTHON R., DESAI S., DIEHL H.T., EIFLER T.F., FINLEY D.A., FLAUGHER B., FOSALBA P., FRIEMAN J., GARCIA-BELLIDO J., GAZTANAGA E., GERDES D.W., GIANNANTONIO T., GRUEN D., GRUENDL R.A., GSCHWEND J., GUTIERREZ G., HOLLOWOOD D.L., HONSCHEID K., JAMES D.J., KRAUSE E., KUEHN K., KUROPATKIN N., LI T.S., LIDMAN C., LIMA M., MAIA M.A.G., MARSHALL J.L., MARTINI P., MENANTEAU F., MIQUEL R., PLAZAS MALAGON A.A., ROMER A.K., ROODMAN A., SAKO M., SANCHEZ E., SCARPINE V., SCHUBNELL M., SERRANO S., SEVILLA-NOARBE I., SOARES-SANTOS M., SOBREIRA F., SUCHYTA E., SWANSON M.E.C., TARLE G., THOMAS D., TUCKER D.L., VIKRAM V., WALKER A.R., ZHANG Y., ASOREY J., CALCINO J., CAROLLO D., GLAZEBROOK K., HINTON S.R., HOORMANN J.K., LEWIS G.F., SHARP R., SWANN E., TUCKER B.E. (The DES Collaboration)

Abstract (from CDS):

We present the first Hubble diagram of superluminous supernovae (SLSNe) out to a redshift of two, together with constraints on the matter density, ΩM, and the dark energy equation-of-state parameter, w(≡p/ρ). We build a sample of 20 cosmologically useful SLSNe I based on light curve and spectroscopy quality cuts. We confirm the robustness of the peak-decline SLSN I standardization relation with a larger data set and improved fitting techniques than previous works. We then solve the SLSN model based on the above standardization via minimization of the χ2 computed from a covariance matrix that includes statistical and systematic uncertainties. For a spatially flat Λ cold dark matter (ΛCDM) cosmological model, we find Ω_ M=0.38+0.24^–0.19, with an rms of 0.27 mag for the residuals of the distance moduli. For a w0waCDM cosmological model, the addition of SLSNe I to a 'baseline' measurement consisting of Planck temperature together with Type Ia supernovae, results in a small improvement in the constraints of w0 and wa of 4 per cent. We present simulations of future surveys with 868 and 492 SLSNe I (depending on the configuration used) and show that such a sample can deliver cosmological constraints in a flat ΛCDM model with the same precision (considering only statistical uncertainties) as current surveys that use Type Ia supernovae, while providing a factor of 2-3 improvement in the precision of the constraints on the time variation of dark energy, w0 and wa. This paper represents the proof of concept for superluminous supernova cosmology, and demonstrates they can provide an independent test of cosmology in the high-redshift (z > 1) universe.

Abstract Copyright: © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): transients: supernovae - cosmology: dark matter - cosmology: cosmological parameters

Simbad objects: 31

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Number of rows : 31
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 SN 2011kg SN* 01 39 45.51 +29 55 27.0           SLSN-I 73 1
2 LSQ 12dlf SN* 01 50 29.80 -21 48 45.4           SLSN-I 57 0
3 DES17X1amf SN* 02 17 46.70 -05 36 01.0           SLSN-I 13 0
4 DES17X1blv SN* 02 20 59.64 -04 29 00.8           SLSN-I 8 0
5 DES14X2byo SN* 02 23 46.93 -06 08 12.3           SLSN-I 13 0
6 PS1-12bqf SN* 02 24 54.621 -04 50 22.72           SLSN-I 18 0
7 DES15X3hm SN* 02 26 54.96 -05 03 38.0           SLSN-I 12 0
8 DES15S2nr SN* 02 40 44.62 -00 53 26.4           SLSN-I 14 0
9 DES16C3dmp SN* 03 31 28.35 -28 32 28.3           SLSN-I 11 0
10 PS1-10bzj SN* 03 31 39.826 -27 47 42.17           SLSN-I 55 0
11 DES15C3hav SN* 03 31 52.17 -28 15 09.5           SLSN-I 17 0
12 DES14C1fi SN* 03 33 49.80 -27 03 31.6           SLSN-I 10 0
13 DES16C2nm SN* 03 40 14.83 -29 05 53.5           SLSN-I 17 0
14 DES16C2aix SN* 03 40 41.17 -29 22 48.4           SLSN-I 9 0
15 PS1-11bam SN* 08 41 14.192 +44 01 56.95           SLSN-I 29 0
16 SN 2012il SN* 09 46 12.91 +19 50 28.7           SLSN-I 68 1
17 SN 2017egm SN* 10 19 05.620 +46 27 14.08           SLSN-I 93 0
18 LSQ 14mo ev 10 22 41.53 -16 55 14.4           SLSN-I 58 0
19 SN 2010gx SN* 11 25 46.71 -08 49 41.4           SLSN-I 165 1
20 SN 2016eay SN* 12 02 51.71 +44 15 27.4           SLSN-I 83 0
21 SN 2013dg SN* 13 18 41.35 -07 04 43.0           SLSN-I 42 1
22 SN 2007bi SN* 13 19 20.19 +08 55 44.3       18.3   SLSN-I 228 1
23 SN 2011ke SN* 13 50 57.77 +26 16 42.8     18.6     SLSN-I 92 1
24 SN 2018don SN* 13 55 08.64 +58 29 41.9           SLSN-I 22 0
25 [DAB2006b] J143227.42+333225.1 SN* 14 32 27.395 +33 32 24.83           SLSN-I 116 0
26 SN 2011kf SN* 14 36 57.53 +16 30 56.6           SLSN-I 42 1
27 PTF 09cnd SN* 16 12 08.94 +51 29 16.1           SLSN-I 120 0
28 PS1-11tt SN* 16 12 45.778 +54 04 16.96           SLSN-I 15 0
29 iPTF 13ajg SN* 16 39 03.95 +37 01 38.4           SLSN-I 67 0
30 PS1-10ky SN* 22 13 37.851 +01 14 23.57           SLSN-I 47 0
31 PS1-11aib SN* 22 18 12.217 +01 33 32.01           SLSN-I 16 0

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