NTT and NOT Spectroscopy of SDSS-II Supernovae

Journal Article · Tue Feb 01 04:00:00 EST 2011 · Astron.Astrophys.

DOI:https://doi.org/10.1051/0004-6361/201015704· OSTI ID:2520115

Ostman, L. ^[1]; Nordin, J. ^[2]; Goobar, A. ^[2]; Amanullah, R. ^[2]; Smith, M. ^[3]; Sollerman, J. ^[4]; Stanishev, V. ^[5]; Stritzinger, M. D. ^[6]; Bassett, B. A. ^[7]; Davis, T. M. ^[8]; Edmondson, E. ^[9]; Frieman, J. A. ^[10]; Garnavich, P. M. ^[11]; Lampeitl, H. ^[9]; Leloudas, G. ^[12]; Marriner, J. ^[13]; Nichol, R. C. ^[9]; Romer, K. ^[14]; Sako, M. ^[15]; Schneider, D. P. ^[16] ; Zheng, C. ^[17]

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1. Stockholm U.; Barcelona, IFAE; Stockholm U., OKC
2. Stockholm U.; Stockholm U., OKC
3. Portsmouth U.; Cape Town U., Dept. Math.
4. Stockholm U., OKC; Stockholm U.; Bohr Inst.
5. Lisbon, IST
6. Stockholm U., OKC; Bohr Inst.; Carnegie Inst. Observ.
7. Cape Town U., Dept. Math.; South African Astron. Observ.; African Inst. Math. Sci., Cape Town
8. Bohr Inst.; Queensland U.
9. Portsmouth U.
10. Fermilab; Chicago U., KICP
11. Notre Dame U.
12. Bohr Inst.
13. Fermilab
14. Sussex U.
15. Pennsylvania U.
16. Penn State U.
17. Stanford U., Phys. Dept.

Context. The SDSS-II Supernova Survey, conducted between 2005 and 2007, was designed to detect a large number of Type Ia supernovae (SNe Ia) around z~0.2, the redshift "gap" between low-z and high-z SN searches. The survey has provided multi-band photometric lightcurves for variable targets, and SN candidates were scheduled for spectroscopic observations, primarily to provide SN classification and accurate redshifts. We present SN spectra obtained in 2006 and 2007 using the NTT and the NOT. Aims. We provide an atlas of SN spectra in the range z =0.03-0.32 that complements the well-sampled lightcurves from SDSS-II in the forthcoming three-year SDSS SN cosmology analysis. The sample can, for example, be used for spectral studies of SNe Ia, which are critical for understanding potential systematic effects when SNe are used to determine cosmological distances. Methods. The spectra were reduced in a uniform manner, and special care was taken in estimating the uncertainties for the different processing steps. Host-galaxy light was subtracted when possible and the SN type fitted using the SuperNova IDentification code (SNID). We also present comparisons between spectral and photometric dating using SALT lightcurve fits to the photometry from SDSS-II, as well as the global distribution of our sample in terms of the lightcurve parameters: stretch and colour. Results. We report new spectroscopic data from 141 SNe Ia, mainly between -9 and +15 days from lightcurve maximum, including a few cases of multi-epoch observations. This homogeneous, host-galaxy subtracted, SN Ia spectroscopic sample is among the largest such data sets and unique in its redshift interval. The sample includes two potential SN 1991T-like SNe (SN 2006on and SN 2007ni) and one potential SN 2002cx-like SN (SN 2007ie). In addition, the new compilation includes spectra from 23 confirmed Type II and 8 Type Ib/c SNe.

• Research Organization: Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
• Sponsoring Organization: USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
• DOE Contract Number: 89243024CSC000002
• OSTI ID: 2520115
• Report Number(s): FERMILAB-PUB-10-598-A; arXiv:1011.5869; oai:inspirehep.net:880270
• Journal Information: Astron.Astrophys., Journal Name: Astron.Astrophys. Vol. 526
• Country of Publication: United States
• Language: English

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79 ASTRONOMY AND ASTROPHYSICS