Figure 1 from A COMPREHENSIVE STUDY OF DETECTABILITY AND CONTAMINATION IN DEEP RAPID OPTICAL SEARCHES FOR GRAVITATIONAL WAVE COUNTERPARTS

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A COMPREHENSIVE STUDY OF DETECTABILITY AND CONTAMINATION IN DEEP RAPID OPTICAL SEARCHES FOR GRAVITATIONAL WAVE COUNTERPARTS

Authors: P. S. Cowperthwaite and E. Berger

2015 The Astrophysical Journal 814 25.

Provider: AAS Journals

Caption: Figure 1.

Top: kilonova spectra from Barnes & Kasen (2013) at ∼1 day and ∼1 week with ejecta properties of M_ej = 10⁻² M_⊙ and β_ej = 0.2. Bottom: light curve for the same model parameters computed at a fiducial distance of 200 Mpc in the DECam r-, i-, and z-band filters.

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