J/ApJ/933/172ivo://CDS.VizieR/J/ApJ/933/172doi:10.26093/cds/vizier/ba-x5-5cCDSJones D.O.Mandel K.S.Kirshner R.P.Thorp S.Challis P.M.,Avelino A.Brout D.Burns C.Foley R.J.Pan Y.-C.Scolnic D.M.,Siebert M.R.Chornock R.Freedman W.L.Friedman A.Frieman J.,Galbany L.Hsiao E.Kelsey L.Marion G.H.Nichol R.C.Nugent P.E.,Phillips M.M.Rest A.Riess A.G.Sako M.Smith M.Wiseman P.,Wood-Vasey W.M.2026-07-02T11:58:42Z2025-03-24T13:05:13ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frsupernovaehst-photometryinfrared-astronomyredshiftedsurveysvisible-astronomyType Ia supernovae (SNe Ia) are more precise standardizable candles when measured in the near-infrared (NIR) than in the optical. With this motivation, from 2012 to 2017 we embarked on the RAISIN program with the Hubble Space Telescope (HST) to obtain rest-frame NIR light curves for a cosmologically distant sample of 37 SNe Ia (0.2<~z<~0.6) discovered by Pan-STARRS and the Dark Energy Survey. By comparing higher-z HST data with 42 SNe Ia at z<0.1 observed in the NIR by the Carnegie Supernova Project, we construct a Hubble diagram from NIR observations (with only time of maximum light and some selection cuts from optical photometry) to pursue a unique avenue to constrain the dark energy equation-of-state parameter, w. We analyze the dependence of the full set of Hubble residuals on the SN Ia host galaxy mass and find Hubble residual steps of size ~0.06-0.1mag with 1.5{sigma}-2.5{sigma} significance depending on the method and step location used. Combining our NIR sample with cosmic microwave background constraints, we find 1+w=-0.17+/-0.12 (statistical + systematic errors). The largest systematic errors are the redshift-dependent SN selection biases and the properties of the NIR mass step. We also use these data to measure H_0_=75.9+/-2.2km/s/Mpc from stars with geometric distance calibration in the hosts of eight SNe Ia observed in the NIR versus H_0_=71.2+/-3.8km/s/Mpc using an inverse distance ladder approach tied to Planck. Using optical data, we find 1+w=-0.10+/-0.09, and with optical and NIR data combined, we find 1+w=-0.06+/-0.07; these shifts of up to ~0.11 in w could point to inconsistency in the optical versus NIR SN models. There will be many opportunities to improve this NIR measurement and better understand systematic uncertainties through larger low-z samples, new light-curve models, calibration improvements, and eventually by building high-z samples from the Roman Space Telescope.2022ApJ...933..172Jhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/933/172CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toB/hst : HST Archived Exposures Catalog (STScI, 2007)II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016)II/357 : The Dark Energy Survey (DES): Data Release 1 (Abbott+, 2018)V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)II/371 : The Dark Energy Survey (DES): Data Release 2 (Abbott+, 2021)J/ApJ/659/122 : Improved distances to type Ia supernovae (Jha+, 2007)J/AJ/136/2306 : SDSS-II Supernova survey, 2005 (Holtzman+, 2008)J/ApJ/689/377 : SNe Ia as NIR std candles from PAIRITEL (Wood-Vasey+, 2008)J/AJ/139/519 : Carnegie supernova project. SNe Ia (Contreras+, 2010)J/AJ/139/120 : Low-redshift Type-Ia supernovae (Folatelli+, 2010)J/A+A/523/A7 : Light curves of type Ia supernovae in SNLS (Guy+, 2010)J/ApJ/722/566 : Host gal. of SNe Ia in SDSS-II SN survey (Lampeitl+, 2010)J/MNRAS/406/782 : Type Ia supernovae luminosities (Sullivan+, 2010)J/MNRAS/416/2840 : The 2M++ galaxy redshift catalogue (Lavaux+, 2011)J/ApJ/731/120 : Intrinsic SN Ia light curves (Mandel+, 2011)J/AJ/142/156 : The CSP (DR2): photometry of SNe Ia (Stritzinger+, 2011)J/ApJS/199/25 : CLASH sources for MACS1149.6+2223 (Postman+, 2012)J/A+A/568/A22 : Joint analysis of the SDSS-II & SNLS SNe Ia (Betoule+, 2014)J/MNRAS/438/1391 : Host galaxies of Type Ia SN from PTF (Pan+, 2014)J/ApJ/795/44 : PS1 SNe Ia (0.02<z<0.7) griz light curves (Rest+, 2014)J/AJ/148/13 : Redshifts of 65 CANDELS supernovae (Rodney+, 2014)J/ApJS/220/9 : CfAIR2: NIR light curves of Type Ia SNe (Friedman+, 2015)J/ApJ/812/31 : Local Star Formation effects on type Ia SNe (Jones+, 2015)J/ApJ/826/56 : HST/WFC3 obs. of Cepheids in SN Ia host gal. (Riess+, 2016)J/AJ/154/211 : CSP (DR3): photometry of low-z SNe Ia (Krisciunas+, 2017)J/ApJ/869/56 : Updated calibration of CSP-I SNe Ia sample (Burns+, 2018)J/A+A/611/A58 : SN 2007on and SN 2011iv light curves (Gall+, 2018)J/ApJ/867/108 : Masses & rest-frame u-g colors of SNIa (Jones+, 2018)J/ApJ/857/51 : Measuring DE properties with PS1 SNe. II. (Jones+, 2018)J/ApJ/854/24 : Environmental dependence of SN Ia luminosities (Kim+, 2018)J/A+A/615/A68 : Type Ia supernova luminosities (Roman+, 2018)J/ApJ/859/101 : The supernovae Ia Pantheon sample (Scolnic+, 2018)J/A+A/615/A45 : NIR K-corrections (Stanishev+, 2018)J/AJ/155/201 : SweetSpot DR1: SNIa with WIYN+WHIRC (Weyant+, 2018)J/ApJ/874/150 : The first 3yrs of DES-SN (DES-SN3YR) (Brout+, 2019)J/MNRAS/486/5785 : Type Ia supernova (Siebert+, 2019)J/ApJ/889/5 : HST obs. of Miras in the SNIa host NGC1559 (Huang+, 2020)J/A+A/644/A176 : Sample of 141 SNe Ia (Rigault+, 2020)J/ApJ/905/94 : Classif. for PS1-MDS SNe with SuperRAENN (Villar+, 2020)J/MNRAS/495/4040 : SN host galaxies in the DES I (Wiseman+, 2020)J/ApJ/923/237 : Opt and NIR phot. follow-up of iPTF SNIa (Johansson+, 2021)J/ApJ/923/197 : SNIa observed in H-band with UV-opt. LCs (Ponder+, 2021)J/ApJS/258/24 : H-band LC for 7 DEHVILS Milky Way Cepheids (Konchady+, 2022)http://des.ncsa.illinois.edu/releases/sn : Dark Energy Survey SN homepagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/933/172https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/933/172http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/933/172https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/933/172https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/933/172http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/933/172GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/933/172/raisin (The RAISIN sample, redshifts and discovery dates (Table 5) and distances and cuts (Table 7))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/933/172/raisin?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/933/172/raisin?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/933/172/raisin?GETtext/xml+votable180.050000true149.80061253.221543060.0055555555555555566/6517 6519 7200 10150 10981-10982 11425 17671 17682 17686 17688 17692 17694 17712 17745-17746 17750 18787-18790 19030 19036 27245 27247 27345 35387-35390 35932 35934 35956 35958 36104 36107https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/933/172?format=asciiOpticalInfrareddefaultJ/ApJ/933/172/raisinThe RAISIN sample, redshifts and discovery dates (Table 5) and distances and cuts (Table 7)SimbadNameSimbad column added by the CDSmeta.idcharnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDName of the SNmeta.id;meta.maincharprimaryRAJ2000Hour of Right Ascension (J2000) (1)pos.eq.ra;meta.mainDEJ2000Degree of Declination (J2000) (1)pos.eq.dec;meta.mainzhelio[0.2/0.7] Redshift in the heliocentric framesrc.redshift;pos.heliocentricfloatzCMB[0.2/0.7] Cosmic Microwave Background redshiftsrc.redshift;pos.cmbfloatzsourceSource of redshift: "host" or "SN" (2)meta.note;src.redshiftcharMJD[55243/57694] Modified Julian date of the discovery (the first S/N>5 detection)time.epochintDist[40/43]? Raw distance modulus (3)magphot.mag.distModfloatnullablee_Dist[0.02/0.078]? Raw distance modulus uncertaintymagstat.error;phot.mag.distModfloatnullableBandRest-frame bands (Y, J and/or i) (4)magmeta.code;instr.filtercharBias[0.004/0.08]? Bias correctionmagphot.mag;arith.difffloatnullableSigtmax[0.05/2] time of maximum light dispersion, {sigma}_tmax_dtime;arith.difffloatSigphot[0/0.3] Average {sigma}_phot_magstat.errorfloatCutsReasons for removalmeta.notecharDES-SN3YRDisplay data from the DES-SN 3yrs (Brout+ 2019, J/ApJ/874/150) within 3"meta.ref.urlnullableDESDisplay data from the DES DR1 (II/357) and DR2 (II/371) within 1.5"meta.ref.urlnullablePantheonDisplay data from the Pantheon sample (Scolnic+ 2018, J/ApJ/859/101) within 3"meta.ref.urlintnullablePS1-MDSDisplay data from PS1-MDS (Jones+ 2018, J/ApJ/857/51 and Villar+ 2020, J/ApJ/905/94) within 3"meta.ref.urlintnullableNpNumber of photometry measurements for this SN (link to Table 6)meta.numberintnullableLCInteractive LC Plotmeta.ref.urlcharJ/ApJ/933/172/table6HST photometry for the RAISIN sampleIDSN identifiermeta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMJD[56229/57731] Modified Julian datetime.epochintFilterHST/WFC3 "F125W" or "F160W" filtermeta.id;instr.filtercharSNmag[22.33/26] SN apparent magnitudemagphot.magfloate_SNmag[0.03/0.4] SNmag uncertaintymagstat.error;phot.magfloats_SNmag[0.018/0.31] SN dispersion of magnitude, {sigma}_SN_magstat.error;phot.magfloatHostmag[19.5/29.3]? Host apparent magnitudemagphot.magfloatnullables_Hostmag[0.01/0.288]? Host dispersion of magnitude, {sigma}_host_magstat.error;phot.magfloatnullableSigc[0/0.018] {sigma}_c_ valuearcsecstat.errorfloatDelmtmpl[0/0.05]? Template difference magnitude, {Delta}^tmpl^_m_magphot.mag;arith.difffloatnullableSigtmpl[0/0.03]? {sigma}_tmpl_ valuemagstat.errorfloatnullable