The data obtained are automatically transfered to the Hawaii Observatory in Hilo and stored in the Subaru Telescope ARchive System (STARS), as well as in OBCP. Users are allowed to access their own data in STARS.
The data in STARS will be opened to public use 18 months following the observation. Publicly available data are stored in the Subaru-Mitaka-Okayama-Kiso Archive system SMOKA, and the Japanese Virtual Observatory JVO.
For the purpose of evaluating the data obtained during the observation, the following two tools for ``quick-look'' are prepared on OBC and on the computer for data analysis (ANA).
A quick reduction with IRAF is possible on the summit, using scripts
adopted specifically for the HDS (see Section ![[*]](crossref.png)
).
Two-dimensional image data and a cross-cut image at a given CCD line can be displayed. The count per pixel for data that are obtained can be estimated immediately.
Two-dimensional image data and a cross-cut image at a given CCD line can be displayed. Spectra of individual orders are shown by the order trace using the data written in the ASCII extension table (T.B.D).