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26 April 2024
 
  » arxiv » 1603.3823

 Article overview



Light Curves of 213 Type Ia Supernovae from the ESSENCE Survey
Gautham Narayan ; Armin Rest ; Brad E. Tucker ; Ryan J. Foley ; W. Michael Wood-Vasey ; Peter Challis ; Christopher W. Stubbs ; Robert P. Kirshner ; Claudio Aguilera ; Andrew C. Becker ; Stephane Blondin ; Alejandro Clocchiatti ; Ricardo Covarrubias ; Guillermo Damke ; Tamara M. Davis ; Alexei V. Filippenko ; Mohan Ganeshalingam ; Arti Garg ; Peter M. Garnavich ; Malcolm Hicken ; Saurabh W. Jha ; Kevin Krisciunas ; Bruno Leibundgut ; Weidong Li ; Thomas Matheson ; Gajus Miknaitis ; Guiliano Pignata ; Jose Luis Prieto ; Adam G. Riess ; Brian P. Schmidt ; Jeffrey M. Silverman ; R. Chris Smith ; Jesper Sollerman ; Jason Spyromilio ; Nicholas B. Suntzeff ; John L. Tonry ; Alfredo Zenteno ;
Date 12 Mar 2016
AbstractThe 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%.
Source arXiv, 1603.3823
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