eBOSS ELG Target Selection with Deep Photometry
|Universidad Autónoma de Madrid, Spain|
Photometry deeper than SDSS was used to assess algorithms for selection of Emission Line Galaxies (ELG) for spectroscopic observations
An object whose
ANCILLARY_TARGET2 value includes one or more of the bitmasks in the following table was targeted for spectroscopy as part of this ancillary target program. See SDSS bitmasks to learn how to use these values to identify objects in this ancillary target program.
|Program (bit name)||Bit number||Target Description||Number of Fibers|
|FAINT_ELG||18||Blue star-forming galaxy selected from CFHT-LS photometry||2,588|
This program used photometry extending to fainter limits than SDSS to select emission line galaxy (ELG) candidates, with the goal of assessing target selection algorithms for eBOSS. The sample was defined to help evaluate the completeness of the targeting sample and redshift success rates near the faint end of the ELG target population.
Data from this ancillary science program are described in Comparat et al. (2014), which measured the evolution of the bright end of the [OII] emission line luminosity function. Favole et al. (2015, in preparation) use these data to derive halo occupation statistics of emission line galaxies.
Blue star-forming galaxies in the redshift range 0.6 < z < 1.2 were selected from the Canada-France-Hawaii Telescope Legacy Survey (CFHTLS) Wide W3 field photometric redshift catalog T0007 (Ilbert et al. 2006; Coupon et al. 2009). Three plates were observed centered on the same position, and targets were selected at a density of nearly 400 objects per square degree.
Selected objects satised the following constraints:
- 20 < g < 22.8
- -0.5 < (u – r) < 0.7(g – i) + 0.1
All photometry was based on CFHTLS MAG_AUTO magnitudes on the AB system. Objects with known redshift were excluded. A target was excluded if a redshift already existed from previous observations.
Comparat, J., et al. (2014), arXiv:1408.1523
Coupon, J., et al. 2009, A&A, 500, 981
Ilbert, O., et al. 2006, A&A, 457, 841