Call for Proposals
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Semester S17A: February 1, 2017 -- July 31, 2017
Subaru Telescope, National Astronomical Observatory of Japan
Subaru Telescope invites observing proposals for Semester S17A. Since each instrument has its own specific restrictions/conditions, applicants are required to consult the relevant instrument page when preparing their proposals. Please also refer to How to Submit via webform, Open Use Policy and Telescope webpage.
Open Use Schedule for S17A
|Deadline of Normal/Intensive Program Submission
||September 7 (Wed), 2016 12:00 (Noon) in Japan Standard Time
(i.e., September 7, 3:00 am in UT)
|Deadline of Service/Filler Program Submission
||October 5 (Wed), 2016 12:00 (Noon) in Japan Standard Time
(i.e., October 5, 3:00 am in UT)
|Time Allocation Committee
||late October to early November
|Notification of selection results
Important Notice for S17A
|Downtime due to Repairing Mirror Hatch
||In order to repair the mirror hatch which was accidentally broken on 2016 February 22, the telescope will take some downtime for several nights in S17A. The re-coating work of the primary mirror (which was cancelled in S16B due to this trouble) will be rescheduled in S17B or later.
|Last-Time Availability of Suprime-Cam
||In S17A, Suprime-Cam is offered for open-use in a shared-risk mode.
The observing run will be scheduled only in late May.
Because its auto guider is not available,
images can be taken only with open tracking (without guiding), in which
the length of exposure time will be limited (see the web page for the tracking accuracy). Suprime-Cam is going to be decommissioned after S17A.
|New "Technical Justification" Entry in Service Proposal form
||From S17A, a new entry (Technical Justification) has been arranged in the application form of the service program, in which technical details (such as integration time and so on) should be explained.
|EAO Time in S17A
||In S17A, Subaru Telescope specially provides EAO (East Asian Observatory) researchers with up to 3 nights using Director's Discretionary Time to promote scientific collaborations. Anyone belonging to institutions in China, Korea, Taiwan or Japan is eligible to submit EAO proposals, in which investigators from at least two countries among these should be included.
Applicants are required to explicitly specify "[EAO Time]" in the title head of the proposal. For more details, please see this.
|Status of PI Instrument
||In S17A, CHARIS (to be combined with SCExAO such as like HiCIAO) will be opened in a shared-risk
mode, by which two possibilities (SCExAO+AO188+HiCIAO and SCExAO+AO188+CHARIS) are offtered for observations with
SCExAO+AO188+HiCIAO is available as usual.
Although Kyoto-3DII was already decommissioned in S16B, it will be made specially available for open
use in S17A, because most of the relevant observing nights in
S16A were cancelled due to the mirror hatch accident.
||There will be at most 6 observing runs of HSC in S17A allocated to dark
or dark-gray nights (except for those around late May where Suprime-Cam
observations will be assigned). Since queue-mode observation is regarded
as the primary mode of HSC operation, those wishing to use the classical
observation mode should explicitly account the reason for that choice.
From S17A, we will accept proposals of time critical observations with
HSC queue. Note, however, that queue mode observation is limited to only
normal and filler programs, which will not be offered for intensive program.
Notice for HSC Applicants
|Use of Hyper Suprime-Cam
||In S17A, Hyper Suprime-Cam (HSC) will be offered in a shared-risk mode. HSC proposers requesting to observe the same fields as targeted in the HSC SSP (Subaru Strategic Program) are obliged to clarify the reason for doing so (e.g., how the scientific aim is different from that of SSP). Remote observations conducted from the Hilo Base Facility are not available. Two filters (NB926 and IB945) will be opened in S17A, as well as new r-band filter (HSC-r2) from July 2016. Please see HSC webpage for more detailed information.
|Queue Mode Observation of HSC
||In S17A, queue mode observation with HSC will be
offered only for the normal program and filler program.
Time critical program is possible for this semester. Proposers can request up to 35
hours (= 5 nights in queue mode) in total on-source time without
including overhead. There is no lower limit for requested observing
time, while cadence observations are not allowed.
Please see HSC queue mode web page
for more detailed information.
|Classical Mode Observation of HSC
||In S17A, proposers wishing to use the classical observation mode of HSC have to
describe why the classical mode is preferred to the queue mode in Entry 13.(Scheduling Requirements). Unless
any convincing reason, proposers may be asked if it is possible to change the observation mode from classical
|"No-Additional-Target" Policy for HSC
||In S17A, requesting additional targets is not allowed for any HSC observations during the semester.
The dead time ("Sukima" time), when there is no planned target on the night sky, will be exploited as effectively as possible depending on the situation (observing priority: 1. observations of standard stars, 2. queue-mode observations for Grade A/B/C, 3. observing user's back-up targets, and 4. queue-mode observations for Grade F).
Notice About Nasmyth/Cassegrain Instruments
|Notice for HDS Applicants
||HDS often has to be combined with the Subaru
infrared secondary mirror (with which throughput at <3800Å is considerably deteriorated),
in order to accommodate as many HDS programs as possible.
So, if blue or UV regions are crucially needed for your program, it should be
explicitly described in Entry 16 (Instrument Requirements).
|Shared-Risk Operation for MOIRCS
||The MOIRCS observations in S17A will be executed under the shared-risk
policy. Please check MOIRCS website for more information.
||IRCS observations will be conducted always in combination with AO188 optics, regardless of the use of AO correction.
Polarimetry mode of IRCS+AO188 has been partially opened for
open use in a shared-risk mode.
The available modes are Y-, J-, H-, and K-bands imaging polarimetry and
zJH, HK spectropolarimetry modes.
Please see the "Polarimetry" section of IRCS page for more detailed information.
Grism and Echelle spectroscopy modes of IRCS+AO188 are available also in service programs. Please see the Service program page for more detailed information.
|Dark Nights Essentially Due to HSC
||Since almost all dark nights will be allocated to Hyper Suprime-Cam, using dark nights with other instruments would be hardly possible.
Notice About Time-Exchange Programs
|Time Exchange Programs with Gemini and Keck
||According to the inter-observatory time-exchange agreement, we accept proposals of observations with
Gemini (North & South) and Keck telescopes, which will be screened by Subaru TAC within the framework of
Subaru Call for Proposals. Maximum several nights (for each of Keck I and Keck II) and minimum 5 nights (Gemini) are available in S17A for this purpose. Those who have direct access to Gemini or Keck time must refrain from applying for Gemini/Keck observing time by this program.|
Please refer to Subaru/Gemini Time Exchange page and Subaru/Keck Time Exchange page for more details.
|Application from Gemini/Keck Community
||We strongly recommend that non-Japanese PIs who wish to use the Subaru Telescope but have access
to Gemini or Keck telescope time apply through the time-exchange programs provided by Gemini or
Keck. In case that such non-Japanese PIs directly submit their proposals to the Subaru Call for Proposals, they must provide a clear justification in their proposals why they have decided to do so.
|New Arrangement between Subaru and Gemini
||From S16B, researchers belonging to Gemini Community can apply for Subaru Intensive Program through the time exchange program, and inversely those belonging to Subaru Community for Gemini Large and Long Programs as a new arrangement in the time exchange program between Subaru and Gemini. Similarly, Subaru Community can apply for Fast Turnaround Programs, in which up to 5 nights per semester are available for researchers belonging to Subaru Community.
Required Clarification in Proposals
|Necessity of FOCAS Preimaging
||FOCAS/MOS users are required to describe explicitly about the pre-imaging
observation with FOCAS in Entry 16 (Instrument Requirements) when it is necessary
for their MOS mask design. Please check the instrument web page for details.
|Set of Hyper Suprime-Cam(or Suprime-Cam) Filters
||Hyper Suprime-Cam(or Suprime-Cam) users must explicitly describe the filters they intend to use in Entry 16
, where the desired set as well as
the minimum acceptable set should be clearly specified.
|Number of MOIRCS/MOS Masks
||MOIRCS/MOS users must explicitly describe the
required number of masks in Entry 16,
where the desired number as well as the minimum acceptable number should be clearly specified.
|Moon-affected Unacceptable Dates
||When one particular source or several sources whose coordinates are concentrated to a particular sky region are planned to be observed on bright or grey nights, observations may be severely affected by the Moon in some particular nights. In such cases, those inconvenient or unacceptable dates should be explicitly indicated in Entry 13 (Scheduling Requirements).
|Service Program Similar to Normal Program
Service Program applicants are required to clarify whether they have submitted similar Normal/Intensive Program proposals for this semester.
Reminder About Basic Rules
||From S16B, the size of Intensive Program has been expanded up to 40 nights over maximum 6 consecutive semesters (with maximum 20 nights in a semester).
|Proposals for Unspecified Targets
||Proposals in which targets are not specified at the time of proposal submission should be
submitted to Normal Program, not to Service Program.
|2nd Choice Instruments
||If your science goal could (fully or partly) be achieved by other
instruments (of Subaru/Keck/Gemini) instead of your 1st choice instrument,
we recommend you to describe such alternative instruments,
which may be usable/acceptable to attain
your science goal, as 2nd choice instrument(s).
|Description of Acceptable Observing Date Range
||Even though your preferred observing dates are rather limited,
you should make your acceptable date range as wide as possible.
Your proposal would be automatically rejected, in case that
we cannot find an observing slot for your program in your
acceptable range (even if your proposal is above the borderline
|Abstract of Accepted Proposals Going to Be Opened
||It has been decided that the complete text of the abstract
of all the accepted Subaru proposals from S15B semester
will be open to the public at the same time of the data release
(i.e., when the proprietary period of 18 months has expired).
||In principle, cancelled observation time due to unexpected telescope/instrumentation failure will not be compensated.
|Using PI Instruments
||Any proposal using PI instruments must include the relevant instrument PI as a Co-investigator. In principle, the use of each PI instrument at the infrared Nasmyth focus is limited to only one observing run in a semester.
|Target Check in Subaru Archive Data
||Applicants are required to check their targets in SMOKA database (Public Data Archive) before submission. If the objects have already been observed by Subaru in the past, the reason why they need to be observed again must be described.
|Duplicated Submission Unallowable
||An identical proposal of the same science and targets using the same instrument and telescope should not be submitted twice at the same time through different TAC processes. For example, if a proposal using Keck or Gemini was once submitted to Subaru time-exchange program, it should not be applied to the ordinary proposal selection on Keck or Gemini side at the same semester. (And vice versa.)
|One Proposal for One Project
||Even if you intend to carry out observations by using different Subaru instruments
(or even by using different telescopes, such as Subaru+Keck or Subaru+Gemini) for the same scientific project(s),
you must describe them only in "one" proposal, because separate submission of two or more proposals belonging to
the same project brings about considerable confusion.
You can specify several different instruments in Entry 12 (Observing Run) and describe your detailed observing plan of how to use them in Entry 16 (Instrument Requirements) or Entry 15 (Observing Method and Technical Details).
Especially, if you want to use two telescopes (Subaru+Gemini or Subaru+Keck) for the same project(s), please summarize your plan in one proposal and select the relevant option in the webform.
|Time Allocation Basically One-night Unit
||Telescope time allocation (except for queue observations) is basically made in unit of one night, though
half night allocation may be exceptionally possible, if a suitable
program can be found for the other half night.
|Travel Support for Japanese Researchers
||NAOJ provides travel support for researchers belonging to Japanese institutions for accepted program observations. It is in principle limited up to 2 researchers belonging to the team (i.e., PI or Co-I of the proposal) for each observing run to Hawaii, and up to 3 researchers including Mitaka remote observations.
||Remote observations from Mitaka Headquarter (remote-M) are allowed for all instruments under the approval of relevant support astronomer.
Meanwhile, remote observations conducted from Hilo Base Facility
(remote-H) may be allowed for IRCS (NGS mode only), HDS,
and MOIRCS (only imaging mode). Those who wish to perform the observations remotely should check the box in Entry 13 (Scheduling Requirements), though such a request may not necessarily be granted, depending on the instrument status and/or scheduling limitations.
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