2008/02/17 by Crystal L. Martin, Marcin Sawicki, Alan Dressler +2
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Astrophysics and Cosmic Phenomena #Emission spectrum #Galaxies: Formation, Evolution, Phenomena #Galaxy #Line (geometry) #Luminosity #Luminosity function #Physics #Population #Quasar #Redshift #Spectral line #astro-ph
paper · pdf · doi:10.1086/586729
Accepted for publication in May 20 Astrophysical Journal; Also available at http://www.physics.ucsb.edu/~cmartin/publications.html
arxiv created 2008/02/17 · openalex publication_date 2008/05/30 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/06
We present results from a blind, spectroscopic survey for z ∼ 5.7 Lyα-emitting galaxies (LAEs) using the Inamori Magellan Areal Camera and Spectrograph. A total of ~200 arcmin 2 were observed in the COSMOS and LCIRS fields using a narrowband filter, which transmits between atmospheric emission lines at 8190 Å, and a mask with 100 long slits. This observing technique provides higher emission-line sensitivity than narrowband imaging and probes larger volumes than strong lensing. We find 170 emission-line galaxies and identify their redshifts spectroscopically. We confirm three LAEs, the first discovered using multislit narrowband spectroscopy. Their line profiles are narrow, but fitted models suggest intrinsic, unattenuated widths ~400 km s −1 FWHM. The red wing of the line profiles presents features consistent with galactic winds. The star formation rates of these galaxies are at least 5-7 M ☉ yr −1 and likely a factor of 2 higher. We estimate that the number density of L ⩾ 5 × 10 42 erg s −1 LAEs is 9.0 −4 +12 × 10 −5 h 70 3 Mpc −3 at redshift 5.7 and constrain the Schechter function parameters describing this population. Galaxies fainter than our detection limit may well be the primary source of ionizing photons at z ∼ 6. We argue, however, that the break luminosity L *,Ly α is not yet well constrained. If this break luminosity is near our detection limit, and somewhat lower than previous estimates, then the detected LAE population could be responsible for ionizing the intergalactic gas at redshift z ∼ 6. We discuss the potential of multislit narrowband spectroscopy for deeper emission-line surveys.