Summary and comparison of the previous 24 μm selected galaxy surveys.
|Depth [μJy]||ρ1 [Ngal/deg2]||Size [deg2]||Probed z||γ||r0 [ h-1 Mpc ]|
|Gilli & Daddi (2007)||20||13 060||0.1||~1||1.5 ± 0.1||4.0 ± 0.4|
|Magliocchetti et al. (2008)||400||1490||0.7||[0.6–1.2] and <1.6||–||and|
|Starikova et al. (2012)||310||410||49||~0.7 and ~1.7||1.8||4.98 ± 0.28 and 8.04 ± 0.69|
|Dolley et al. (2014)||223||2678||8.42||0.2 <z< 1.0||1.8–2.13||3–6|
|AKARI||150||3350||0.4||[ 0:3)||1.79 ± 0.04||4.93 ± 0.49|
Notes. The work of Gilli & Daddi (2007) is based on spectroscopic measurements in contrast with other studies (based on photometric measurements). The parameter ρ stands for surface density.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.