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Light Curves of 213 Type Ia Supernovae from the ESSENCE Survey

Authors :
Narayan, Gautham
Rest, Armin
Tucker, Brad E.
Foley, Ryan J.
Wood-Vasey, W. Michael
Challis, Peter
Stubbs, Christopher W.
Kirshner, Robert P.
Aguilera, Claudio
Becker, Andrew C.
Blondin, Stephane
Clocchiatti, Alejandro
Covarrubias, Ricardo
Damke, Guillermo
Davis, Tamara M.
Filippenko, Alexei V.
Ganeshalingam, Mohan
Garg, Arti
Garnavich, Peter M.
Hicken, Malcolm
Jha, Saurabh W.
Krisciunas, Kevin
Leibundgut, Bruno
Li, Weidong
Matheson, Thomas
Miknaitis, Gajus
Pignata, Guiliano
Prieto, Jose Luis
Riess, Adam G.
Schmidt, Brian P.
Silverman, Jeffrey M.
Smith, R. Chris
Sollerman, Jesper
Spyromilio, Jason
Suntzeff, Nicholas B.
Tonry, John L.
Zenteno, Alfredo
Publication Year :
2016

Abstract

The ESSENCE survey discovered 213 Type Ia supernovae at redshifts 0.1 < z < 0.81 between 2002 and 2008. We present their R and I-band photometry, measured from images obtained using the MOSAIC II camera at the CTIO 4 m Blanco telescope, along with rapid-response spectroscopy for each object. We use our spectroscopic follow-up observations to determine an accurate, quantitative classification and a precise redshift. Through an extensive calibration program we have improved the precision of the CTIO Blanco natural photometric system. We use several empirical metrics to measure our internal photometric consistency and our absolute calibration of the survey. We assess the effect of various potential sources of systematic bias on our measured fluxes, and we estimate that the dominant term in the systematic error budget from the photometric calibration on our absolute fluxes is ~1%.<br />Comment: (40 pages, 21 figures, accepted for publication in ApJS)

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.1603.03823
Document Type :
Working Paper
Full Text :
https://doi.org/10.3847/0067-0049/224/1/3