Hyper Suprime-Cam (HSC)


Information for S22A applicants


  Schedule of HSC runs in S22A

•  At most four (4) times of HSC observing runs from late April to July.

•  HSC will be NOT available in February, March, and early April due to the TUE overhaul.


  Filter set

Applicants wishing to use the NB391 or NB395 filter must obtain an approval from the filter developer team in advance of the proposal submission. All applicants must explicitly describe the filters they intend to use in the "Instrument Requirements" section of the application form, where the desired set as well as the minimum acceptable set should be clearly specified.


  Default observation mode

Queue mode is the default observing mode for the Normal, Intensive, and Filler programs (see the detail information at the "HSC Queue Mode Webpage"). Applicants wishing a classical mode observation with HSC have to describe why the classical mode is preferred to the queue mode in "Scheduling Requirements" section of the application form. Without any convincing reason, the observation mode may be changed from classical to queue. Note that a proposal requesting the NB387, NB391, or NB395 filter must be submitted as a classical mode program.


  "No-Additional-Target" policy

Requesting additional targets for filling dead time (a.k.a. "Sukima time"), when there is no planned target on the night sky, is not allowed for any HSC observations. "Sukima time" will be exploited as effective as possible depending on the situation (observing priority: (1) observations of standard stars, (2) queue-mode observations for Grade A/B programs, (3) observing applicant's back-up targets, and (4) queue-mode observations for Grade C and F [Filler] programs).


  No service programs

Service observations are not available for HSC.


Last update: July 25, 2021



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Introduction

The Hyper Suprime-Cam (HSC) is a gigantic mosaic CCD camera, which is attached at the prime focus of Subaru Telescope. The HSC uses 104 main science CCDs which cover 1.5-deg field-of-view in diameter with a pixel scale of 0.17 arcseconds, as well as 4 CCDs for auto guider and 8 CCDs for focus monitoring.

It takes about 30 min for changing filters (including a focus check). Before starting a filter exchange, it is necessary to move the telescope to the zenith and rotate the instrument rotator to the appropriate angle. We also have to close the cover of the primary mirror for safety operation.

When you cosider to develop a new HSC filter, please be sure to read the filter policy carefully and contact the Subaru Telescope (contact person: T. Terai [terai_at_naoj.org] ) well before applying for funds. Also, please refer the procedure to determine filters for each HSC run.

We ask for your understanding in advance that the obtained data of which proprietary period (18 months) has not yet expired may be used by Subaru staff without PI's permission for engineering purposes.



Instrument


Observation


Data Analysis and Archive


Tools


Image Quality


Problem Reports


Contact:

Questions regarding HSC should be directed to Satoshi Miyazaki (satoshi_at_naoj.org) and Tsuyoshi Terai (terai_at_naoj.org).

Please note that all numbers on these pages are subject to change as the performance of HSC is better determined.

Last update: November 12, 2021



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