- We recall that every proposal within the Spanish CAT scheme must be led by a principal investigator (PI) affiliated to a Spanish Institution. GTC Spanish/Mex proposals can have either a Spanish or Mexican PI, and must include co-Investigators (co-Is) from both communities (see below).
- The start and end of the semester change with telescope as illustrated next:
- WHT, INT, Stella: August – January.
- NOT, TNG, Mercator: October – March. [Note the new semester for Mercator].
- GTC: September – February. [See “GTC” below].
- Liverpool (LT): July – February (a two-month overlap period is adopted at the start and end of each semester, when proposals from both semesters may be observed in order to reduce problems with under-filled observations queues).
- Large programs are not accepted for GTC in semester 2017B. Large program proposals extending over two semesters (2017B and 2018A) are accepted for WHT and INT (see below for details). Large program proposals extending up to four semesters (2017B through 2019A) with TNG, NOT, LT, Mercator, and/or Stella can be submitted. See below.
Please, read carefully the following information and recommendations made for each telescope and for large programs. There are changes with respect to previous calls for proposals.
To submit proposals, see “how to submit” at the end of this document.
Detailed information about the feature of GTC for this semester can be found on the GTC call for proposals. A short summary is provided next:
- In semester 2017B, no Large Programs are accepted.
- OSIRIS, EMIR, and HiPERCAM are offered in this call. CanariCam and CIRCE are no longer offered.
- EMIR broad- and narrow-band imaging and long-slit spectroscopy are offered. EMIR proposals for 2017B are allowed for execution from July 1st onwards, thus extending the right ascension window of EMIR targets for this call. Because EMIR uses predefined maximum on-source individual integration times per filter and grism (see Table 7 of EMIR users manual), all applicants are recommended to use this tool (which does not include overheads) to optimize the observing time of EMIR targets.
- OSIRIS modes “imaging” (broad-band, SHARDS filters, tunable filters), “spectroscopy” (long-slit, MOS), and “frame transfer and fast photometry” are offered. Multi-Object Spectroscopy (MOS) observations will be part of the observing queue only if the proposals are ranked in the top half (first and second quartiles) of the Spanish CAT final list. However, any proposal in the third and fourth quartiles that has the MOS masks already fabricated from previous semesters will be also included in the observing queue. Applicants must indicate whether their MOS masks are to be fabricated or are available from previous semesters.
- HiPERCAM is a high-speed, multi-band imager and a new GTC visitor instrument (Principal Investigator Vik Dhillon). It is offered on a shared-risk basis to the community quite likely by the end of the semester (January 2018).
- Visitor programs are welcome, but will only be admitted whenever they fall in the top half of the ranked proposal list. The applicants must clearly indicate they are applying for visitor mode. A backup program (in visitor mode) should be defined in the case the observing conditions for the main program are not met.
- Target-of-opportunity proposals are accepted (see here for further details).
- Approved CAT proposals ranked in the first quartile, will be granted an extended life-time of three semesters, or until their completion, whichever comes first. Note that all phase II information must be submitted to the GTC at the deadline corresponding to the semester in which the proposal is accepted.
FILLER PROPOSALS: In order to have an efficient queue-scheduled observations scheme for the GTC, it is useful to have a set of “filler” programs that can be executed under adverse observing conditions (bad seeing, poor sky transmission, etc.) and with targets spanning a wide range in right ascension (RA). Proposers may request filler status for their program, and during the proposal selection process CAT will evaluate their suitability for this category. Such proposals can request a large number of observing hours. In order to be considered as filler proposals they must fulfil the following requirements:
- Their observing requirements should be very relaxed, i.e. little or no restrictions on seeing or cloud coverage.
- The chosen observing mode should be a frequently used mode, specifically broad/narrow-band imaging and long-slit spectroscopy for OSIRIS, and broad-band imaging for CIRCE.
- There is a scientific gain even if only a small fraction of the requested observations are executed.
- A list of targets with a broad RA coverage is provided or, if only few targets are included, they must have good visibility during the semester.
Note that filler proposals have generally been highly successful in the last semesters.
SPANISH/MEX TIME: Up to 2.5% of the GTC observing time is reserved for collaborative proposals between Spanish and Mexican astronomers. To send proposals under this agreement, select the Special Agreement“Spanish/Méx Time” in the CAT application tool.
Detailed information provided by the ING Observatory can be found in the ING call for proposals. All potential applicants must become familiar with the series of changes in instrument availability and of observing time at the WHT and INT driven by the arrival of new survey instruments. The changes are summarized here.
The main changes for 2017B are:
- See the complete list of ING instruments here. Offered instruments for 2017B are:
- WHT: ISIS, ISIS/QUCAMs, LIRIS, ACAM.
- INT: IDS, WFC.
- Not offered instruments: AF2/WYFFOS and INTEGRAL.
- Investigators wishing to submit proposals to use an established WHT visitor instrument (GHaFaS, PAUCam, PN.S) should follow the instructions given in the ING call for proposals.
- Applicants are encouraged to submit proposals for large time allocations, even within one semester.
- Large program proposals requiring WHT and specially INT observing time over two semesters (2017B and 2018A) can be submitted. Any instrument can be requested in this category. The number of nights available for large programs on the WHT and INT are indicated below.
- At the INT, service observations of approved CAT programs are offered through collaboration with the INT student support astronomers. Details are provided in page 3 of the ING call for proposals.
About 35% of the observing time at the WHT is managed by CAT. Starting from semester 2013B, 20% of the time is distributed to the best-ranked proposals from the Spanish community, and the remaining 15% will be reserved for proposals led by PIs affiliated to the IAC.
Offered instruments are listed here. Updates with respect to previous semesters are as follows:
- A new detector has been installed in FIES, which provides low-fringing and high efficiency in the red. The new CCD (e2V CCD231-42) is about 10% larger than the old one, thus allowing to sample further into the infrared part of the spectrum Current wavelength coverage is 364-911 nm with the high-resolution fiber.
- A new fiber bundle is planned to be installed in FIES in the coming months. With this new bundle, the radial velocity stability with the high-resolution fiber is expected to improve from 8-10 m/s to ~3 m/s.
- The SOFIN high-resolution Echelle spectrograph is available. It offers a resolution of R = 27,000-170,000. Applicants that require this instrument are strongly requested to read the NOT web pages, since this is not a common-user instrument.
The instruments WiFSIP and SES are offered:
- WiFSIP will receive a new CCD detector of equal size, but with a readout time of only 30 seconds for full frame. This new setup will be ready for 2017B, which may be of interest to long-term programs. The Hbeta filters will be replaced eventually.
- SES has no change with respect to previous calls for proposals.
- involve novel ideas, opportunities for great advance, or legacy programs,
- span between two and four semesters,
- publicly release their final high-level products in an appropriate format, and
- be led by a Spanish institution (a large fraction of the team should be affiliated to a Spanish institution).
Considering the time allocated to on-going large-programs, in 2017B the following time is available for Large Programs:
- TNG: 10 nights in 2017B and subsequent semesters.
- WHT: 5 nights in 2017B and 15 nights in 2018A (only two semesters).
- INT: 11 nights in 2017B and 25 nights in 2018A (only two semesters).
- NOT: 10 nights per semester.
- Mercator: 15 nights per semester.
- Liverpool: 10 h in 2017B, 80 h in subsequent semesters.
- Stellar-SES and Stella-WiFSIP: 100 h per robotic telescope and per semester.
All large programs will be evaluated by the CAT and advised by external expert referees, based on the above criteria. Yearly progress reports are expected, and a final report to the CAT is due at the end of the project. Raw data from long-term programs will follow the same proprietary period as regular proposals. Up to 66% of the time distributed by the CAT on the Liverpool (LT), Mercator, STELLA, and INT, up to 33% of the time on NOT and TNG, and up to 15% of the time on the WHT may be assigned to large programs.
Applicants must ensure that their proposals comply with the required page limits and layout indicated below. The use of English is recommended for normal proposals. Large program proposals must be written in English. To send proposals, use the night time CAT application tool at http://cat.iac.es. A simple manual to learn how to deal with this application is available in this pdf document. To submit a proposal, the PI and co-Is need to be registered. If you are already registered but you do not remember your password, please do NOT register twice (in order to avoid confusions for statistical purposes). You can find instructions about how to reset your password in the same webpage.
Remember to use the latest LaTeX style, which is available at ftp://ftp.iac.es/pub/research/cat/cat.tar.z. The form is also available in Word format at ftp://ftp.iac.es/pub/research/cat/cat_word.docNote also that the time request in the on-line application tool has changed, as one should now specify the time requested for each semester by creating as many “Observations” as needed.
In the evaluation of proposals, CAT will take into account the publications derived from previous observations with the CAT telescopes. Therefore, in the BIBCodes menu of the application tool, remember to update the fields Comment and Bibliographic code for all proposals approved in the last two years.
Before the deadline expires, please check that the uploaded pdf file contain the latest version of your proposal, and that it prints correctly. No replacement or updating of the proposal content will be made after the deadline, and those proposals which do not correctly print out or lack relevant sections will be automatically withdrawn from the evaluation process. Those proposals where the font size (10pt) has been reduced or the text of the scientific justification exceeds limitations (one page for common/regular proposals and two pages for large programmes) will also be withdrawn. Figures and Tables cited in the scientific justification should fit a maximum of one page (normal proposals) and two pages (large programs). It is advised to follow the instructions described at http://cat.iac.es/faces/ayuda/pdf_latex.jsf
To send GTC proposals under the Spain-México agreement, select the Special Agreement“Spanish/Méx Time” in the CAT application tool.
UPDATED on 9 Mar 2017.
Contact e-mail: catiac at iac.es.