FMOS-COSMOS survey III. 0.7


Authors : Silverman J.D. orcid , Kashino D., Sanders D. (hide) , Kashino D., Sanders D. et..al


CDS Keywords : Galaxies, spectra; Spectra, infrared; Redshifts; Surveys
UAT : Galaxies, Spectroscopy, Infrared astronomy, Spectroscopy, Redshifted, Surveys

Observation (OC)

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Inserted into VizieR : 04-Dec-2015
Last modification : 30-Aug-2017

The FMOS-COSMOS survey of star-forming galaxies at z~1.6. III. Survey design, performance, and sample characteristics. (2015)

Keywords : galaxies general; galaxies: high-redshift; galaxies: ISM; surveys; techniques: spectroscopic

Abstract:We present a spectroscopic survey of galaxies in the COSMOS field using the Fiber Multi-object Spectrograph (FMOS), a near-infrared instrument on the Subaru Telescope. Our survey is specifically designed to detect the H{alpha} emission line that falls within the H-band (1.6-1.8{mu}m) spectroscopic window from star-forming galaxies with 1.4<z<1.7 and M_stellar_>~10^10^M_{sun}_. With the high multiplex capability of FMOS, it is now feasible to construct samples of over 1000 galaxies having spectroscopic redshifts at epochs that were previously challenging. The high-resolution mode (R~2600) effectively separates H{alpha} and [NII]{lambda}6585, thus enabling studies of the gas-phase metallicity and photoionization state of the interstellar ...(more)
Abstract: (hide)
We report on observations carried out between 2012 March and 2013 January with Subaru/FMOS. The central square degree of COSMOS is effectively covered with four FMOS footprints, designated as HR1-HR4 (Figure 1), using both the high-resolution H-long (1.60-1.80um; R~2600) and J-long (1.11-1.35um) gratings.


                
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