Euclid - I. Overview of the Euclid mission | Astronomy & Astrophysics (A&A)

Open Access

Fig. 27

VIS view of a $2_{\cdot}^{'} 5$ $\[2^{\prime}_\cdot5\]$ × $2_{\cdot}^{'} 0$ $\[2^{\prime}_\cdot0\]$ wide area of Euclid’s self-calibration field (Sect. 4.2.3) taken during the PV phase. Left: an unprocessed single exposure, where cosmic rays are clearly visible. Right: aVIS-processed stack using 42 exposures, or about 10 times the exposure time of the EWS. The ability of Euclid to reveal low-surface-brightness features is evident.

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.