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The Sloan Digital Sky Survey Reverberation Mapping Project : Hα and Hβ reverberation measurements from first year spectroscopy and photometry

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Figure

Fig. 1.— From top to bottom: The distributions of our sampletion 2.1), andminosity at 5100 of quasars in redshift, i magnitude, median SN-MED (see Sec- λLλ5100 (the host-subtracted quasar continuum lu-A) as a function of redshift.˚
Fig. 2.— The observing cadence for the spectroscopic observa-tions (top panel) and photometric observations (bottom panel).Each vertical black line represents an observed epoch
Fig. 3.—CREAMSDSS J141625.71+535438.5 (RMID 272,stration of the inter-calibration technique
Fig. 4.— Light curves and thebution for SDSS J141018.04+532937.5 (RMID 229,The top two panels show the continuum and Hdisplay purposes, multiple observations within a single night areaveraged and shown as a single point
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