J/ApJ/738/162     SN Ia candidates from the SDSS-II SN Survey     (Sako+, 2011)

Photometric type Ia supernova candidates from the three-year SDSS-II SN Survey data. Sako M., Bassett B., Connolly B., Dilday B., Cambell H., Frieman J.A., Gladney L., Kessler R., Lampeitl H., Marriner J., Miquel R., Nichol R.C., Schneider D.P., Smith M., Sollerman J. <Astrophys. J., 738, 162 (2011)> =2011ApJ...738..162S 2011ApJ...738..162S
ADC_Keywords: Extinction ; Redshifts ; Supernovae ; Photometry ; Surveys Keywords: cosmology: observations - supernovae: general - surveys Abstract: We analyze the three-year Sloan Digital Sky Survey II (SDSS-II) Supernova (SN) Survey data and identify a sample of 1070 photometric Type Ia supernova (SN Ia) candidates based on their multiband light curve data. This sample consists of SN candidates with no spectroscopic confirmation, with a subset of 210 candidates having spectroscopic redshifts of their host galaxies measured while the remaining 860 candidates are purely photometric in their identification. We describe a method for estimating the efficiency and purity of photometric SN Ia classification when spectroscopic confirmation of only a limited sample is available, and demonstrate that SN Ia candidates from SDSS-II can be identified photometrically with ∼91% efficiency and with a contamination of ∼6%. Although this is the largest uniform sample of SN candidates to date for studying photometric identification, we find that a larger spectroscopic sample of contaminating sources is required to obtain a better characterization of the background events. A Hubble diagram using SN candidates with no spectroscopic confirmation, but with host galaxy spectroscopic redshifts, yields a distance modulus dispersion that is only ∼20%-40% larger than that of the spectroscopically confirmed SN Ia sample alone with no significant bias. A Hubble diagram with purely photometric classification and redshift-distance measurements, however, exhibits biases that require further investigation for precision cosmology. Description: The SDSS-II SN Survey was conducted during the September-November months of 2005-2007. A 300deg2 region along the celestial equator was observed using the SDSS 2.5m telescope with an average cadence of four days. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 89 210 SDSS-II zhost-Ia Candidates table4.dat 92 860 SDSS-II Photo-Ia Candidates -------------------------------------------------------------------------------- See also: B/sn : Asiago Supernova Catalogue (Barbon et al., 1999-) J/A+A/526/A28 : SDSS-II supernovae NTT and NOT spectroscopy (Oestman+, 2011) J/ApJ/713/1026 : SN Ia rate at redshift ≲0.3 from SDSS-II (Dilday+, 2010) J/ApJ/722/566 : Host galaxies of SNIa in SDSS-II SN survey (Lampeitl+, 2010) J/AJ/139/519 : Carnegie supernova project. SNe Ia (Contreras+, 2010) J/MNRAS/406/782 : Type Ia supernovae luminosities (Sullivan+, 2010) J/ApJ/700/331 : Light curves of type Ia supernovae (CfA3) (Hicken+, 2009) J/ApJS/185/32 : First-year SDSS-II SN results (Kessler+, 2009) J/AJ/136/2306 : SDSS-II Supernova survey, 2005 (Holtzman+, 2008) J/AJ/135/1766 : Sloan Digital Sky Survey-II supernova survey (Zheng+, 2008) J/AJ/135/348 : SDSS-II SNe survey: search and follow-up (Sako+, 2008) J/MNRAS/389/1871 : Type Ia supernovae candidates from SDSS (Horesh+, 2008) Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- CID [703/22006] Internal SDSS-II SN candidate designation 7- 16 F10.6 deg RAdeg [-53/58.7] Right ascension (J2000) 18- 26 F9.6 deg DEdeg [-1.3/1.3] Declination (J2000) 28- 33 F6.4 --- z [0.10/0.50] Spectroscopic redshift 35- 40 F6.4 --- e_z [0/0.01] Uncertainty in z 42- 46 F5.2 mag AV [-0.68/2.37] V-band extinction 48- 52 F5.2 mag B_AV The 1σ upper V-band extinction limit 54- 58 F5.2 mag b_AV The 1σ lower V-band extinction limit 60- 63 F4.2 mag dm15 [0.61/1.74] Phillips Δm15(B) (G1) 65- 69 F5.2 mag B_dm15 The 1σ upper Phillips Δm15(B) limit 71- 75 F5.2 mag b_dm15 The 1σ lower Phillips Δm15(B) limit 77- 81 F5.3 --- PzIa Bayesian SN Ia probability (1) 83- 86 F4.2 --- chi2 [0.74/1.8] Best-fit reduced chi-squared 87- 89 A3 --- --- [000] -------------------------------------------------------------------------------- Note (1): With spectroscopic redshift prior. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- CID [822/21890] Internal SDSS-II SN candidate designation 7- 16 F10.6 deg RAdeg [-58.2/58.8] Right Ascension (J2000) 18- 26 F9.6 deg DEdeg [-1.3/1.3] Declination (J2000) 28- 32 F5.3 --- zph [0.01/0.7] Photometric redshift 34- 39 F6.3 --- B_zph The 1σ upper photometric redshift 41- 46 F6.3 --- b_zph The 1σ lower photometric redshift 48- 52 F5.2 mag AV [-0.94/5] V-band extinction 54- 58 F5.2 mag B_AV The 1σ upper V-band extinction limit 60- 64 F5.2 mag b_AV The 1σ lower V-band extinction limit 66- 69 F4.2 mag dm15 [0.6/1.77] Phillips Δm15(B) (G1) 71- 75 F5.2 mag B_dm15 The 1σ upper Phillips Δm15(B) limit 77- 81 F5.2 mag b_dm15 The 1σ lower Phillips Δm15(B) limit 83- 87 F5.3 --- PIa Bayesian SN Ia probability (1) 89- 92 F4.2 --- chi2 [0.51/1.6] Best-fit reduced chi-squared -------------------------------------------------------------------------------- Note (1): With flat redshift prior. -------------------------------------------------------------------------------- Golbal Notes: Note (G1): Decline rate parameter defined by Philips (1999AJ....118.1766P 1999AJ....118.1766P): Δm15(B)=B(+15days)-B(max) History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 23-Jan-2013
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