The Properties of Faint Ly-alpha Emitters at z~6: Results from a Wide-Field Spectroscopic Survey

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

Some feedback models suggest Reionization effectively extinguishes star formation in low mass galaxies. Yet, the brightest galaxies discovered at redshifts z~6 do not, alone, provide enough ionizing photons to maintain the ionization of the intergalactic medium. Accounting for all the ionizing photons requires a significant extrapolation of the galaxy luminosity function to fainter galaxies. To better constrain the properties of this star-forming population, we carried out a blind, spectroscopic Ly-alpha redshift survey at redshifts z~6 using the wide field IMACS f/2 spectrograph at Magellan. Among over 200 emission- line galaxies discovered, we identified interlopers via the presence of multiple emission lines or broad-band photometry (i.e. the paucity of a Lyman break). Roughly 10% of the sample passes these tests. We have recently obtained higher resolution spectra of these objects to constrain their physical properties. We will present our constraints on the galaxy luminosity function and discuss the properties of these Ly-alpha selected galaxies.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

The Properties of Faint Ly-alpha Emitters at z~6: Results from a Wide-Field Spectroscopic Survey does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Properties of Faint Ly-alpha Emitters at z~6: Results from a Wide-Field Spectroscopic Survey, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Properties of Faint Ly-alpha Emitters at z~6: Results from a Wide-Field Spectroscopic Survey will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1783871

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.