Open Access

Fig. 2.

image

Download original image

Determination of the F444W limiting magnitude. The dependence of the 90% limiting magnitude on circularized effective radii from 0 . 06 $ 0{{\overset{\prime\prime}{.}}}06 $ to 1 . 2 $ 1{{\overset{\prime\prime}{.}}}2 $ is shown for an exponential profile (n = 1, blue solid line) and a de Vaucouleurs profile (n = 4, red solid line), both with null ellipticity (e = 0). In the top right-hand corner, we show the completeness curves for a Sérsic profile n = 1 with size R e = 0 . 42 $ R_{\mathrm{e}}=0{{\overset{\prime\prime}{.}}}42 $ and variable ellipticity and the projection of the 90% completeness on the e = 0 curve that is the most restrictive one. The grey shaded region depicts the FWHM size of the F444W-band. The green solid lines defines the F444W = 25 limiting magnitude as the projection on the most restrictive, while realistic, galaxy size ( R e = 0 . 42 $ R_{\mathrm{e}}=0{{\overset{\prime\prime}{.}}}42 $) and ellipticity (e = 0) at z = 3.5.

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.