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Fast Turnaround Call for Proposals

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May 2019 Call for Proposals

Gemini North and South are accepting proposals for the Fast Turnaround (FT) program. Here, we give information specific to this proposal cycle. Please see the other FT pages - particularly the rules - for general information about the program. FT-specific proposal templates must now be used for all FT proposals; see the "PIT information" section below. The revised 2019B PIT must be used.

We are pleased to announce Gemini North again accepts proposals using the laser guide star system and we encourage Fast Turnaround proposals utilizing it.

Important dates

  • Proposal deadline: 23:59, Hawaiian Standard Time (HST), May 31
  • Please ensure the latest version of the 19B PIT is used for submission.
  • Reviews must be completed by 23:59 HST, June 14. If you have submitted a proposal, but by the 2nd of the month have not received an email from FT regarding reviewing proposals, contact FT as soon as possible.
  • Results will be announced by June 21
  • The deadline for preparing observations (Phase II) is June 30. Accepted programs meeting this deadline will be active from 1 July 2019 until 30 September 2019
  • FT observations will be merged with the queue and observed on queue nights.

Eligibility

  • PIs from all participant countries taking part in the FT program may apply for this cycle.
  • We further welcome Japanese community PI proposals.
  • PIs from participant countries whose FT time for the semester has been used up should not apply for the remainder of the semester. Note that some participant countries only have very small amounts of FT time available each semester. Currently no partners have reached their limit.  See Rule #4 and Q&A for more information.

Acceptable RA ranges

  • Gemini North: Targets from about RA = 12 hrs to 5 hr are acceptable during this cycle. Also note that RAs near 12 hrs will only be accessible for a couple hours during the first half of the first month (July) and only at northern declinations ( Dec> 0). Likewise, RAs near 5 hr will only be accessible for a few hours during the final month (September) and again only in the above declination range. Note Rule #9; an FT program may not fully backload its three-month active period; at least one of its targets must be observable during its first active month.
  • Gemini South: Targets from about RA = 11 hr to 5 hrs are acceptable during this cycle. Note, however, that RAs near 11 will only be accessible for a few hours during the first half of the first month (July) and only at favorable declinations (Dec < 0) . Likewise, RAs near 5 will only be accessible for a few hours during the second half of the final month (September) and again only in the above declination range. Note Rule #9; an FT program may not fully backload its three-month active period; at least one of its targets must be observable during its first active month.

Available instruments and observing modes:

Gemini North

  • Please see the telescope schedule for detailed instrument availabilities.  Please check back later this month for the 19B schedule.
  • Please note that Gemini North is closed for annual maintenance starting July 22 - Aug 25, about a third of this FT cycle.
  • GMOS, NIRI, and GNIRS are offered this cycle.  Please check for the 19B telescope schedule for NIFS availability.
  • LGS is offered with NIRI and GNIRS this cycle. 

Gemini South

  • See the telescope schedule for detailed instrument availabilities. Please check back later this month for the 19B schedule.
  • Please note that Gemini South is closed for annual maintenance during August 12-26. 
  • GMOS-S and Flamingos-2 are otherwise expected to be available during this FT block.
  • A limited amount of GPI time may be available intermittently through the 3-month FT block. Contact the FT team for details.
  • GeMS+GSAOI, and PHOENIX are currently not available for FT.

Both telescopes

  • FT observations may not be executed during classical observing and priority visitor (PV)  blocks, depending on the prevailing conditions.
  • For visiting instruments not listed above, you must contact the FT team before submitting a proposal to check availability (Fast.Turnaround at gemini.edu)
  • For GMOS proposals, please indicate in the Technical section if your program could be carried out with either GMOS (North or South).
  • The R600 grating in each GMOS instrument is NOT offered for FT (or regular queue) observations.
  • MOS observations are available for FT, subject to some caveats/restrictions
  • As discussed in the rules and Q&A, please contact the Fast Turnaround team in advance of the deadline if you would like to propose for an unusual instrument configuration or observing mode.

Time available

  • 20 hrs per month at each telescope is available for FT observations. Very roughly, this implies:
    • 4 hrs of 20%-ile conditions (IQ=20, for example; see this web page)
    • 10 hrs of 50%-ile conditions
    • 14 hrs of 70%-ile conditions
    • 17 hrs of 85%-ile conditions
  • PIs may propose for up to the amount of time in their most restrictive observing conditions, subject to partner's time availability - see rule #4 . For example, a proposal requesting CC50 IQ20 SB50 WVany conditions can request no more than 4 hrs of observing time.

PIT information

  • Proposals must be submitted using the version of the Phase I Tool specified on this web page (in the "Time Requests" tab, select Fast Turnaround Observing at Gemini as the proposal class).
  • In the Time Requests tab, select "Fast Turnaround Observing at Gemini" as the proposal class and specify the reviewer (and mentor, if appropriate). Note that this is where the reviewer is defined; changes cannot be made after the proposal has been submitted.
  • Dedicated LaTeX/Word templates must be used to prepare FT proposals: tex | sty | doc.
  • Submitting the same proposal more than once during a given month (e.g. after correcting/editing a submitted version) should be avoided if at all possible. Only submit when you are sure your proposal is ready to be reviewed.
  • The FT proposal template (which differs somewhat from the queue template) is now compulsory for all FT proposals.

April 2019 Call for Proposals

Gemini North and South are accepting proposals for the Fast Turnaround (FT) program. Here, we give information specific to this proposal cycle. Please see the other FT pages - particularly the rules - for general information about the program. FT-specific proposal templates must now be used for all FT proposals; see the "PIT information" section below. The revised 2019A PIT must be used.

We are pleased to announce Gemini North again accepts proposals using the laser guide star system and we encourage Fast Turnaround proposals utilizing it.

Important dates

  • Proposal deadline: 23:59, Hawaiian Standard Time (HST), April 30
  • Please ensure the latest version of the 19B PIT is used for submission.
  • Reviews must be completed by 23:59 HST, May 14. If you have submitted a proposal, but by the 2nd of the month have not received an email from FT regarding reviewing proposals, contact FT as soon as possible.
  • Results will be announced by May 21
  • The deadline for preparing observations (Phase II) is May 31. Accepted programs meeting this deadline will be active from 1 June 2019 until 31 August 2019
  • FT observations will be merged with the queue and observed on queue nights.

Eligibility

  • PIs from all participant countries taking part in the FT program may apply for this cycle.
  • We further welcome Japanese community PI proposals.
  • PIs from participant countries whose FT time for the semester has been used up should not apply for the remainder of the semester. Note that some participant countries only have very small amounts of FT time available each semester. Currently no partners have reached their limit.  See Rule #4 and Q&A for more information.

Acceptable RA ranges

  • Gemini North: Targets from about RA = 10.5 hrs to 3.5 hr are acceptable during this cycle. Also note that RAs near 10.5 hrs will only be accessible for a couple hours during the first half of the first month (June) and only at northern declinations ( Dec> 0). Likewise, RAs near 3.5 hr will only be accessible for a few hours during the final month (August) and again only in the above declination range. Note Rule #9; an FT program may not fully backload its three-month active period; at least one of its targets must be observable during its first active month.
  • Gemini South: Targets from about RA = 9.5 hr to 3.5 hrs are acceptable during this cycle. Note, however, that RAs near 9.5 will only be accessible for a few hours during the first half of the first month (June) and only at favorable declinations (Dec < 0) . Likewise, RAs near 3.5 will only be accessible for a few hours during the second half of the final month (August) and again only in the above declination range. Note Rule #9; an FT program may not fully backload its three-month active period; at least one of its targets must be observable during its first active month.

Available instruments and observing modes:

Gemini North

  • Please see the telescope schedule for detailed instrument availabilities.
  • Please note that Gemini North is closed for annual maintenance starting July 22 - Aug 25.
  • There is one GRACES run during this cycle (June 20-27).
  • NIFS is not offered during this cycle as it is currently not scheduled to be on the telescope during this period.
  • LGS is offered with NIRI and GNIRS this cycle. 

Gemini South

  • See the telescope schedule for detailed instrument availabilities.
  • Please note that Gemini South is closed for annual maintenance during August 12-26. 
  • From June 10 to June 25 GMOS South will not be available
  • GMOS-S and Flamingos-2 are otherwise expected to be available during this FT block.
  • A limited amount of GPI time may be available intermittently through the 3-month FT block. Contact the FT team for details.
  • GeMS+GSAOI, and PHOENIX are currently not available for FT.

Both telescopes

  • FT observations may not be executed during classical observing and priority visitor (PV)  blocks, depending on the prevailing conditions.
  • For visiting instruments not listed above, you must contact the FT team before submitting a proposal to check availability (Fast.Turnaround at gemini.edu)
  • For GMOS proposals, please indicate in the Technical section if your program could be carried out with either GMOS (North or South).
  • The R600 grating in each GMOS instrument is NOT offered for FT (or regular queue) observations.
  • MOS observations are available for FT, subject to some caveats/restrictions
  • As discussed in the rules and Q&A, please contact the Fast Turnaround team in advance of the deadline if you would like to propose for an unusual instrument configuration or observing mode.

Time available

  • 20 hrs per month at each telescope is available for FT observations. Very roughly, this implies:
    • 4 hrs of 20%-ile conditions (IQ=20, for example; see this web page)
    • 10 hrs of 50%-ile conditions
    • 14 hrs of 70%-ile conditions
    • 17 hrs of 85%-ile conditions
  • PIs may propose for up to the amount of time in their most restrictive observing conditions, subject to partner's time availability - see rule #4 . For example, a proposal requesting CC50 IQ20 SB50 WVany conditions can request no more than 4 hrs of observing time.

PIT information

  • Proposals must be submitted using the version of the Phase I Tool specified on this web page (in the "Time Requests" tab, select Fast Turnaround Observing at Gemini as the proposal class).
  • In the Time Requests tab, select "Fast Turnaround Observing at Gemini" as the proposal class and specify the reviewer (and mentor, if appropriate). Note that this is where the reviewer is defined; changes cannot be made after the proposal has been submitted.
  • Dedicated LaTeX/Word templates must be used to prepare FT proposals: tex | sty | doc.
  • Submitting the same proposal more than once during a given month (e.g. after correcting/editing a submitted version) should be avoided if at all possible. Only submit when you are sure your proposal is ready to be reviewed.
  • The FT proposal template (which differs somewhat from the queue template) is now compulsory for all FT proposals.

March 2019 Call for Proposals

Gemini North and South are accepting proposals for the Fast Turnaround (FT) program. Here, we give information specific to this proposal cycle. Please see the other FT pages - particularly the rules - for general information about the program. FT-specific proposal templates must now be used for all FT proposals; see the "PIT information" section below. The revised 2019A PIT must be used.

We are pleased to announce Gemini North again accepts proposals using the laser guide star system and we encourage Fast Turnaround proposals utilizing it.

Important dates

  • Proposal deadline: 23:59, Hawaiian Standard Time (HST), March 31
  • Please ensure the latest version of the 19A PIT is used for submission.
  • Reviews must be completed by 23:59 HST, Apr 14. If you have submitted a proposal, but by the 2nd of the month have not received an email from FT regarding reviewing proposals, contact FT as soon as possible.
  • Results will be announced by Apr 21
  • The deadline for preparing observations (Phase II) is Apr 30. Accepted programs meeting this deadline will be active from 1 May 2019 until 31 July 2019
  • FT observations will be merged with the queue and observed on queue nights.

Eligibility

  • PIs from all participant countries taking part in the FT program may apply for this cycle.
  • We further welcome Japanese community PI proposals.
  • PIs from participant countries whose FT time for the semester has been used up should not apply for the remainder of the semester. Note that some participant countries only have very small amounts of FT time available each semester. Currently no partners have reached their limit.  See Rule #4 and Q&A for more information.

Acceptable RA ranges

  • Gemini North: Targets from about RA = 8 hrs to 1.5 hr are acceptable during this cycle. However, note that due to queue filling, only a few hours are available in good conditions at RA 9-11. Also note that RAs near 8 hrs will only be accessible for a couple hours during the first half of the first month (May) and only at northern declinations ( Dec> 0). Likewise, RAs near 1.5 hr will only be accessible for a few hours during the final month (July) and again only in the above declination range. Note Rule #9; an FT program may not fully backload its three-month active period; at least one of its targets must be observable during its first active month.
  • Gemini South: Targets from about RA = 7.5 hr to 2 hrs are acceptable during this cycle. Note, however, that RAs near 7.5 will only be accessible for a few hours during the first half of the first month (May) and only at favorable declinations (Dec < 0) . Likewise, RAs near 2 will only be accessible for a few hours during the second half of the final month (July) and again only in the above declination range. Note Rule #9; an FT program may not fully backload its three-month active period; at least one of its targets must be observable during its first active month.

Available instruments and observing modes:

Gemini North

  • Please see the telescope schedule for detailed instrument availabilities.
  • There is one GRACES run during this cycle (June 20-27).
  • LGS is offered with NIFS and NIRI.  Make sure to check the telescope schedule for the availability of these 2 instruments since they take turns on the telescope.

Gemini South

  • See the telescope schedule for detailed instrument availabilities.
  • GMOS-S and Flamingos-2 are otherwise expected to be available during this FT block.
  • A limited amount of GPI time may be available intermittently through the 3-month FT block. Contact the FT team for details.
  • GeMS+GSAOI, and PHOENIX are currently not available for FT.

Both telescopes

  • FT observations may not be executed during classical observing and priority visitor (PV)  blocks, depending on the prevailing conditions.
  • For visiting instruments not listed above, you must contact the FT team before submitting a proposal to check availability (Fast.Turnaround at gemini.edu)
  • For GMOS proposals, please indicate in the Technical section if your program could be carried out with either GMOS (North or South).
  • The R600 grating in each GMOS instrument is NOT offered for FT (or regular queue) observations.
  • MOS observations are available for FT, subject to some caveats/restrictions
  • As discussed in the rules and Q&A, please contact the Fast Turnaround team in advance of the deadline if you would like to propose for an unusual instrument configuration or observing mode.

Time available

  • 20 hrs per month at each telescope is available for FT observations. Very roughly, this implies:
    • 4 hrs of 20%-ile conditions (IQ=20, for example; see this web page)
    • 10 hrs of 50%-ile conditions
    • 14 hrs of 70%-ile conditions
    • 17 hrs of 85%-ile conditions
  • PIs may propose for up to the amount of time in their most restrictive observing conditions, subject to partner's time availability - see rule #4 . For example, a proposal requesting CC50 IQ20 SB50 WVany conditions can request no more than 4 hrs of observing time.

PIT information

  • Proposals must be submitted using the version of the Phase I Tool specified on this web page (in the "Time Requests" tab, select Fast Turnaround Observing at Gemini as the proposal class).
  • In the Time Requests tab, select "Fast Turnaround Observing at Gemini" as the proposal class and specify the reviewer (and mentor, if appropriate). Note that this is where the reviewer is defined; changes cannot be made after the proposal has been submitted.
  • Dedicated LaTeX/Word templates must be used to prepare FT proposals: tex | sty | doc.
  • Submitting the same proposal more than once during a given month (e.g. after correcting/editing a submitted version) should be avoided if at all possible. Only submit when you are sure your proposal is ready to be reviewed.
  • The FT proposal template (which differs somewhat from the queue template) is now compulsory for all FT proposals.

February 2019 Call for Proposals

Gemini North and South are accepting proposals for the Fast Turnaround (FT) program. Here, we give information specific to this proposal cycle. Please see the other FT pages - particularly the rules - for general information about the program. FT-specific proposal templates must now be used for all FT proposals; see the "PIT information" section below. The revised 2019A PIT must be used.

We are pleased to announce Gemini North again accepts proposals using the laser guide star system and we encourage Fast Turnaround proposals utilizing it.

Important dates

  • Proposal deadline: 23:59, Hawaiian Standard Time (HST), February 28
  • Please ensure the newest version of the PIT is used for submission.
  • Reviews must be completed by 23:59 HST, Mar 14. If you have submitted a proposal, but by the 2nd of the month have not received an email from FT regarding reviewing proposals, contact FT as soon as possible.
  • Results will be announced by Mar 21
  • The deadline for preparing observations (Phase II) is Mar 31. Accepted programs meeting this deadline will be active from 1 April 2019 until 30 June 2019
  • FT observations will be merged with the queue and observed on queue nights.

Eligibility

  • PIs from all participant countries taking part in the FT program may apply for this cycle.
  • We further welcome Japanese community PI proposals.
  • PIs from participant countries whose FT time for the semester has been used up should not apply for the remainder of the semester. Note that some participant countries only have very small amounts of FT time available each semester. Currently no partners have reached their limit.  See Rule #4 and Q&A for more information.

Acceptable RA ranges

  • Gemini North: Targets from about RA = 6 hrs to 1.0 hr are acceptable during this cycle. However, note that due to queue filling, only a few hours are available in good conditions at RA 9-11. Also note that RAs near 6 hrs will only be accessible for a couple hours during the first half of the first month (Apr) and only at northern declinations ( Dec> 0). Likewise, RAs near 1.0 will only be accessible for a few hours during the final month (June) and again only in the above declination range. Note Rule #9; an FT program may not fully backload its three-month active period; at least one of its targets must be observable during its first active month.
  • Gemini South: Targets from about RA = 5.5 hr to 1.5 hrs are acceptable during this cycle. Note, however, that RAs near 5.5 will only be accessible for a few hours during the first half of the first month (Apr) and only at favorable declinations (Dec < 0) . Likewise, RAs near 1. will only be accessible for a few hours during the second half of the final month (June) and again only in the above declination range. Note Rule #9; an FT program may not fully backload its three-month active period; at least one of its targets must be observable during its first active month.

Available instruments and observing modes:

Gemini North

  • Please see the telescope schedule for detailed instrument availabilities.
  • There is one GRACES run during this cycle (Mar 25-31).
  • LGS is offered with NIFS and NIRI.  Make sure to check the telescope schedule for the availability of these 2 instruments since they take turns on the telescope.

Gemini South

  • See the telescope schedule for detailed instrument availabilities.
  • GMOS-S and Flamingos-2 are otherwise expected to be available during this FT block.
  • A limited amount of GPI time may be available intermittently through the 3-month FT block. Contact the FT team for details.
  • GeMS+GSAOI, and PHOENIX are currently not available for FT.

Both telescopes

  • FT observations may not be executed during classical observing and priority visitor (PV)  blocks, depending on the prevailing conditions.
  • For visiting instruments not listed above, you must contact the FT team before submitting a proposal to check availability (Fast.Turnaround at gemini.edu)
  • For GMOS proposals, please indicate in the Technical section if your program could be carried out with either GMOS (North or South).
  • The R600 grating in each GMOS instrument is NOT offered for FT (or regular queue) observations.
  • MOS observations are available for FT, subject to some caveats/restrictions
  • As discussed in the rules and Q&A, please contact the Fast Turnaround team in advance of the deadline if you would like to propose for an unusual instrument configuration or observing mode.

Time available

  • 20 hrs per month at each telescope is available for FT observations. Very roughly, this implies:
    • 4 hrs of 20%-ile conditions (IQ=20, for example; see this web page)
    • 10 hrs of 50%-ile conditions
    • 14 hrs of 70%-ile conditions
    • 17 hrs of 85%-ile conditions
  • PIs may propose for up to the amount of time in their most restrictive observing conditions, subject to partner's time availability - see rule #4 . For example, a proposal requesting CC50 IQ20 SB50 WVany conditions can request no more than 4 hrs of observing time.

PIT information

  • Proposals must be submitted using the version of the Phase I Tool specified on this web page (in the "Time Requests" tab, select Fast Turnaround Observing at Gemini as the proposal class).
  • In the Time Requests tab, select "Fast Turnaround Observing at Gemini" as the proposal class and specify the reviewer (and mentor, if appropriate). Note that this is where the reviewer is defined; changes cannot be made after the proposal has been submitted.
  • Dedicated LaTeX/Word templates must be used to prepare FT proposals: tex | sty | doc.
  • Submitting the same proposal more than once during a given month (e.g. after correcting/editing a submitted version) should be avoided if at all possible. Only submit when you are sure your proposal is ready to be reviewed.
  • The FT proposal template (which differs somewhat from the queue template) is now compulsory for all FT proposals.

January 2019 Call for Proposals

Gemini North and South are accepting proposals for the Fast Turnaround (FT) program. Here, we give information specific to this proposal cycle. Please see the other FT pages - particularly the rules - for general information about the program. FT-specific proposal templates must now be used for all FT proposals; see the "PIT information" section below. The revised 2019A PIT must be used.

We are pleased to announce Gemini North again accepts proposals using the laser guide star system and we encourage Fast Turnaround proposals utilizing it.

Important dates

  • Proposal deadline: 23:59, Hawaiian Standard Time (HST), January 31
  • Please ensure the newest version of the PIT is used for submission.
  • Reviews must be completed by 23:59 HST, Feb 14. If you have submitted a proposal, but by the 2nd of the month have not received an email from FT regarding reviewing proposals, contact FT as soon as possible.
  • Results will be announced by Feb 21
  • The deadline for preparing observations (Phase II) is Feb 28. Accepted programs meeting this deadline will be active from 1 March 2019 until 31 May 2019
  • FT observations will be merged with the queue and observed on queue nights.

Eligibility

  • PIs from all participant countries taking part in the FT program may apply for this cycle.
  • We further welcome Japanese community PI proposals.
  • PIs from participant countries whose FT time for the semester has been used up should not apply for the remainder of the semester. Note that some participant countries only have very small amounts of FT time available each semester. Currently no partners have reached their limit.  See Rule #4 and Q&A for more information.

Acceptable RA ranges

  • Gemini North: Targets from about RA = 4 hrs to 22.5 hr are acceptable during this cycle. However, note that due to queue filling, only a few hours are available in good conditions at RA 9-11. Also note that RAs near 4 hrs will only be accessible for a couple hours during the first half of the first month (Mar) and only at northern declinations ( Dec> 0). Likewise, RAs near 22.5 will only be accessible for a few hours during the final month (May) and again only in the above declination range. Note Rule #9; an FT program may not fully backload its three-month active period; at least one of its targets must be observable during its first active month.
  • Gemini South: Targets from about RA = 4.5 hr to 22.5 hrs are acceptable during this cycle. Note, however, that RAs near 4.5 will only be accessible for a few hours during the first half of the first month (Mar) and only at favorable declinations (Dec < 0) . Likewise, RAs near 22.5 will only be accessible for a few hours during the second half of the final month (May) and again only in the above declination range. Note Rule #9; an FT program may not fully backload its three-month active period; at least one of its targets must be observable during its first active month.

Available instruments and observing modes:

Gemini North

  • Please see the telescope schedule for detailed instrument availabilities.
  • There is one GRACES run during this cycle (Mar 25-31).
  • LGS is offered with NIFS and NIRI.  Make sure to check the telescope schedule for the availability of these 2 instruments since they take turns on the telescope.

Gemini South

  • See the telescope schedule for detailed instrument availabilities.
  • GMOS-S and Flamingos-2 are otherwise expected to be available during this FT block.
  • A limited amount of GPI time may be available intermittently through the 3-month FT block. Contact the FT team for details.
  • GeMS+GSAOI, and PHOENIX are currently not available for FT.

Both telescopes

  • FT observations may not be executed during classical observing and priority visitor (PV)  blocks, depending on the prevailing conditions.
  • For visiting instruments not listed above, you must contact the FT team before submitting a proposal to check availability (Fast.Turnaround at gemini.edu)
  • For GMOS proposals, please indicate in the Technical section if your program could be carried out with either GMOS (North or South).
  • The R600 grating in each GMOS instrument is NOT offered for FT (or regular queue) observations.
  • MOS observations are available for FT, subject to some caveats/restrictions
  • As discussed in the rules and Q&A, please contact the Fast Turnaround team in advance of the deadline if you would like to propose for an unusual instrument configuration or observing mode.

Time available

  • 20 hrs per month at each telescope is available for FT observations. Very roughly, this implies:
    • 4 hrs of 20%-ile conditions (IQ=20, for example; see this web page)
    • 10 hrs of 50%-ile conditions
    • 14 hrs of 70%-ile conditions
    • 17 hrs of 85%-ile conditions
  • PIs may propose for up to the amount of time in their most restrictive observing conditions, subject to partner's time availability - see rule #4 . For example, a proposal requesting CC50 IQ20 SB50 WVany conditions can request no more than 4 hrs of observing time.

PIT information

  • Proposals must be submitted using the version of the Phase I Tool specified on this web page (in the "Time Requests" tab, select Fast Turnaround Observing at Gemini as the proposal class).
  • In the Time Requests tab, select "Fast Turnaround Observing at Gemini" as the proposal class and specify the reviewer (and mentor, if appropriate). Note that this is where the reviewer is defined; changes cannot be made after the proposal has been submitted.
  • Dedicated LaTeX/Word templates must be used to prepare FT proposals: tex | sty | doc.
  • Submitting the same proposal more than once during a given month (e.g. after correcting/editing a submitted version) should be avoided if at all possible. Only submit when you are sure your proposal is ready to be reviewed.
  • The FT proposal template (which differs somewhat from the queue template) is now compulsory for all FT proposals.

December 2018 Call for Proposals

Gemini North and South are accepting proposals for the Fast Turnaround (FT) program. Here, we give information specific to this proposal cycle. Please see the other FT pages - particularly the rules - for general information about the program. FT-specific proposal templates must now be used for all FT proposals; see the "PIT information" section below. The revised 2019A PIT must be used.

We are pleased to announce Gemini North again accepts proposals using the laser guide star system and we encourage Fast Turnaround proposals utilizing it.

Important dates

  • Proposal deadline: 23:59, Hawaiian Standard Time (HST), December 31
  • Please ensure the newest version of the PIT is used for submission.
  • Reviews must be completed by 23:59 HST, Jan 14. If you have submitted a proposal, but by the 2nd of the month have not received an email from FT regarding reviewing proposals, contact FT as soon as possible.
  • Results will be announced by Jan 21
  • The deadline for preparing observations (Phase II) is Jan 31. Accepted programs meeting this deadline will be active from 1 February 2019 until 30 April 2019
  • FT observations will be merged with the queue and observed on queue nights.

Eligibility

  • PIs from all participant countries taking part in the FT program may apply for this cycle.
  • We further welcome Japanese community PI proposals.
  • PIs from participant countries whose FT time for the semester has been used up should not apply for the remainder of the semester. Note that some participant countries only have very small amounts of FT time available each semester. Currently no partners have reached their limit. However, Argentina has used up 4.35 of their 6 hours. See Rule #4 and Q&A for more information.

Acceptable RA ranges

  • Gemini North: Targets from about RA = 1 hrs to 21.5 hr are acceptable during this cycle. However, note that due to queue filling, only a few hours are available in good conditions at RA~1 and at RA 9-11. Also note that RAs near 1 will only be accessible for a couple hours during the first half of the first month (Feb) and only at northern declinations ( Dec> 0). Likewise, RAs near 21.5 will only be accessible for a few hours during the final month (Apr) and again only in the above declination range. Note Rule #9; an FT program may not fully backload its three-month active period; at least one of its targets must be observable during its first active month.
  • Gemini South: Targets from about RA = 2.5 hr to 22 hrs are acceptable during this cycle . Note, however, that RAs near 2.5 will only be accessible for a few hours during the first half of the first month (Feb) and only at favorable declinations (Dec < 0) . Likewise, RAs near 22 will only be accessible for a few hours during the second half of the final month (Apr) and again only in the above declination range. Note Rule #9; an FT program may not fully backload its three-month active period; at least one of its targets must be observable during its first active month.

Available instruments and observing modes:

Gemini North

  • Please see the telescope schedule for detailed instrument availabilities.
  • The next GRACES run is currently not scheduled. This will be known during this call. Please contact the FT team for more information.
  • LGS is offered with NIFS and NIRI.

Gemini South

  • See the telescope schedule for detailed instrument availabilities.
  • GMOS-S and Flamingos-2 are otherwise expected to be available during this FT block.
  • A limited amount of GPI time may be available intermittently through the 3-month FT block. Contact the FT team for details.
  • GeMS+GSAOI, and PHOENIX are currently not available for FT.

Both telescopes

  • FT observations may not be executed during classical observing, priority visitor (PV) and Korean blocks, depending on the prevailing conditions.
  • For visiting instruments not listed above, you must contact the FT team before submitting a proposal to check availability (Fast.Turnaround at gemini.edu)
  • For GMOS proposals, please indicate in the Technical section if your program could be carried out with either GMOS (North or South).
  • The R600 grating in each GMOS instrument is NOT offered for FT (or regular queue) observations.
  • MOS observations are available for FT, subject to some caveats/restrictions
  • As discussed in the rules and Q&A, please contact the Fast Turnaround team in advance of the deadline if you would like to propose for an unusual instrument configuration or observing mode.

Time available

  • 20 hrs per month at each telescope is available for FT observations. Very roughly, this implies:
    • 4 hrs of 20%-ile conditions (IQ=20, for example; see this web page)
    • 10 hrs of 50%-ile conditions
    • 14 hrs of 70%-ile conditions
    • 17 hrs of 85%-ile conditions
  • PIs may propose for up to the amount of time in their most restrictive observing conditions, subject to partner's time availability - see rule #4 . For example, a proposal requesting CC50 IQ20 SB50 WVany conditions can request no more than 4 hrs of observing time.

PIT information

  • Proposals must be submitted using the version of the Phase I Tool specified on this web page (in the "Time Requests" tab, select Fast Turnaround Observing at Gemini as the proposal class).
  • In the Time Requests tab, select "Fast Turnaround Observing at Gemini" as the proposal class and specify the reviewer (and mentor, if appropriate). Note that this is where the reviewer is defined; changes cannot be made after the proposal has been submitted.
  • Dedicated LaTeX/Word templates must be used to prepare FT proposals: tex | sty | doc.
  • Submitting the same proposal more than once during a given month (e.g. after correcting/editing a submitted version) should be avoided if at all possible. Only submit when you are sure your proposal is ready to be reviewed.
  • The FT proposal template (which differs somewhat from the queue template) is now compulsory for all FT proposals.

November 2018 Call for Proposals

Gemini North and South are accepting proposals for the Fast Turnaround (FT) program. Here, we give information specific to this proposal cycle. Please see the other FT pages - particularly the rules - for general information about the program. FT-specific proposal templates must now be used for all FT proposals; see the "PIT information" section below. The revised 2019A PIT must be used.

Important dates

  • Proposal deadline: 23:59, Hawaiian Standard Time (HST), November 30
  • Please ensure the newest version of the PIT is used for submission.
  • Reviews must be completed by 23:59 HST, Dec 14. If you have submitted a proposal, but by the 2nd of the month have not received an email from FT regarding reviewing proposals, contact FT as soon as possible.
  • Results will be announced by Dec 21
  • The deadline for preparing observations (Phase II) is Dec 31. Accepted programs meeting this deadline will be active from 1 January 2019 until 31 March 2019
  • FT observations will be merged with the queue and observed on queue nights.

Eligibility

  • PIs from all participant countries taking part in the FT program may apply for this cycle.
  • We further welcome Japanese community PI proposals.
  • PIs from participant countries whose FT time for the semester has been used up should not apply for the remainder of the semester. Note that some participant countries only have very small amounts of FT time available each semester. Currently no partners have reached their limit. However, Argentina has used up 4.35 of their 6 hours. See Rule #4 and Q&A for more information.

Acceptable RA ranges

  • Gemini North: Targets from about RA = 22.5 hrs to 19.5 hr are acceptable during this cycle. However, note that due to queue filling, only a few hours are available in good conditions at RA~0 Also note that RAs near 20 will only be accessible for a couple hours during the first half of the first month (Jan) and only at northern declinations ( Dec> 0). Likewise, RAs near 16.5 will only be accessible for a few hours during the final month (Mar) and again only in the above declination range. Note Rule #9; an FT program may not fully backload its three-month active period; at least one of its targets must be observable during its first active month.
  • Gemini South: Targets from about RA = 00.5 hr to 18.5 hrs are acceptable during this cycle . Note, however, that RAs near 0.5 will only be accessible for a few hours during the first half of the first month (Jan) and only at favorable declinations (Dec < 0) . Likewise, RAs near 18.5 will only be accessible for a few hours during the second half of the final month (Mar) and again only in the above declination range. Note Rule #9; an FT program may not fully backload its three-month active period; at least one of its targets must be observable during its first active month.

Available instruments and observing modes:

Gemini North

  • Please see the telescope schedule for detailed instrument availabilities.
  • The next GRACES run is scheduled for Jan 15-22. This is subject to change pending repairs to the instrument. Please contact the FT team for more information.
  • LGS is NOT offered at this time. However, please check back here or contact the FT team for updates later this month.

Gemini South

  • See the telescope schedule for detailed instrument availabilities.
  • GMOS-S and Flamingos-2 are otherwise expected to be available during this FT block.
  • A limited amount of GPI time may be available intermittently through the 3-month FT block. Contact the FT team for details.
  • GeMS+GSAOI, and PHOENIX are currently not available for FT.

Both telescopes

  • FT observations may not be executed during classical observing, priority visitor (PV) and Korean blocks, depending on the prevailing conditions.
  • For visiting instruments not listed above, you must contact the FT team before submitting a proposal to check availability (Fast.Turnaround at gemini.edu)
  • For GMOS proposals, please indicate in the Technical section if your program could be carried out with either GMOS (North or South).
  • The R600 grating in each GMOS instrument is NOT offered for FT (or regular queue) observations.
  • MOS observations are available for FT, subject to some caveats/restrictions
  • As discussed in the rules and Q&A, please contact the Fast Turnaround team in advance of the deadline if you would like to propose for an unusual instrument configuration or observing mode.

Time available

  • 20 hrs per month at each telescope is available for FT observations. Very roughly, this implies:
    • 4 hrs of 20%-ile conditions (IQ=20, for example; see this web page)
    • 10 hrs of 50%-ile conditions
    • 14 hrs of 70%-ile conditions
    • 17 hrs of 85%-ile conditions
  • PIs may propose for up to the amount of time in their most restrictive observing conditions, subject to partner's time availability - see rule #4 . For example, a proposal requesting CC50 IQ20 SB50 WVany conditions can request no more than 4 hrs of observing time.

PIT information

  • Proposals must be submitted using the version of the Phase I Tool specified on this web page (in the "Time Requests" tab, select Fast Turnaround Observing at Gemini as the proposal class).
  • In the Time Requests tab, select "Fast Turnaround Observing at Gemini" as the proposal class and specify the reviewer (and mentor, if appropriate). Note that this is where the reviewer is defined; changes cannot be made after the proposal has been submitted.
  • Dedicated LaTeX/Word templates must be used to prepare FT proposals: tex | sty | doc.
  • Submitting the same proposal more than once during a given month (e.g. after correcting/editing a submitted version) should be avoided if at all possible. Only submit when you are sure your proposal is ready to be reviewed.
  • The FT proposal template (which differs somewhat from the queue template) is now compulsory for all FT proposals.

October 2018 Call for Proposals

Gemini North and South are accepting proposals for the Fast Turnaround (FT) program. Here, we give information specific to this proposal cycle. Please see the other FT pages - particularly the rules - for general information about the program. FT-specific proposal templates must now be used for all FT proposals; see the "PIT information" section below. The revised 2018B PIT must be used

Important dates

  • Proposal deadline: 23:59, Hawaiian Standard Time (HST), October 31
  • Please ensure the new version of the PIT is used for submission (version 2.2).
  • Reviews must be completed by 23:59 HST, Nov 14. If you have submitted a proposal, but by the 2nd of the month have not received an email from FT regarding reviewing proposals, contact FT as soon as possible.
  • Results will be announced by Nov 21;
  • The deadline for preparing observations (Phase II) is Nov 30. Accepted programs meeting this deadline will be active from 1 December 2018 until 28 February 2019;
  • FT observations will be merged with the queue and observed on queue nights.

Eligibility

  • PIs from all participant countries taking part in the FT program may apply for this cycle.
  • We further welcome Japanese community PI proposals.
  • PIs from participant countries whose FT time for the semester has been used up should not apply for the remainder of the semester. Note that some participant countries only have very small amounts of FT time available each semester. Currently no partners have reached their limit. However, Argentina has used up 4.35 of their 6 hours. See Rule #4 and Q&A for more information.

Acceptable RA ranges

  • Gemini North: Targets from about RA = 20 hrs to 16.5 hr are acceptable during this cycle. However, note that due to queue filling, only a few hours are available in good conditions at RA~0. Also note that RAs near 20 will only be accessible for a couple hours during the first half of the first month (Dec) and only at northern declinations ( Dec> 0). Likewise, RAs near 16.5 will only be accessible for a few hours during the final month (Feb) and again only in the above declination range. Note Rule #9; an FT program may not fully backload its three-month active period; at least one of its targets must be observable during its first active month.
  • Gemini South: Targets from about RA = 22.5 hr to 16.5 hrs are acceptable during this cycle . Note, however, that RAs near 22.5 will only be accessible for a few hours during the first half of the first month (Dec) and only at favorable declinations (Dec < 0) . Likewise, RAs near 16.5 will only be accessible for a few hours during the second half of the final month (Feb) and again only in the above declination range. Note Rule #9; an FT program may not fully backload its three-month active period; at least one of its targets must be observable during its first active month.

Available instruments and observing modes
 

  • Gemini North
    • Please see the telescope schedule for detailed instrument availabilities.
    • The next GRACES run is scheduled for Jan 15-22. This is subject to change pending repairs to the instrument. Please contact the FT team for more information.
    • LGS is NOT offered at this time.
  • Gemini South
    • See the telescope schedule for detailed instrument availabilities.
    • GMOS-S and Flamingos-2 are otherwise expected to be available during this FT block.
    • A limited amount of GPI time may be available intermittently through the 3-month FT block. Contact the FT team for details.
    • GeMS+GSAOI, and PHOENIX are currently not available for FT.
  • Both telescopes
    • FT observations may not be executed during classical observing, priority visitor (PV) and Korean blocks, depending on the prevailing conditions.
    • For visiting instruments not listed above, you must contact the FT team before submitting a proposal to check availability (Fast.Turnaround at gemini.edu)
    • For GMOS proposals, please indicate in the Technical section if your program could be carried out with either GMOS (North or South).
    • The R600 grating in each GMOS instrument is NOT offered for FT (or regular queue) observations.
    • MOS observations are available for FT, subject to some caveats/restrictions
    • As discussed in the rules and Q&A, please contact the Fast Turnaround team in advance of the deadline if you would like to propose for an unusual instrument configuration or observing mode.

Time available

  • 20 hrs per month at each telescope is available for FT observations. Very roughly, this implies:
    • 4 hrs of 20%-ile conditions (IQ=20, for example; see this web page)
    • 10 hrs of 50%-ile conditions
    • 14 hrs of 70%-ile conditions
    • 17 hrs of 85%-ile conditions
  • PIs may propose for up to the amount of time in their most restrictive observing conditions, subject to partner's time availability - see rule #4 . For example, a proposal requesting CC50 IQ20 SB50 WVany conditions can request no more than 4 hrs of observing time.

PIT information

  • Proposals must be submitted using the version of the Phase I Tool specified on this web page (in the "Time Requests" tab, select Fast Turnaround Observing at Gemini as the proposal class).
  • In the Time Requests tab, select "Fast Turnaround Observing at Gemini" as the proposal class and specify the reviewer (and mentor, if appropriate). Note that this is where the reviewer is defined; changes cannot be made after the proposal has been submitted.
  • Dedicated LaTeX/Word templates must be used to prepare FT proposals: tex | sty | doc.
  • Submitting the same proposal more than once during a given month (e.g. after correcting/editing a submitted version) should be avoided if at all possible. Only submit when you are sure your proposal is ready to be reviewed.
  • The FT proposal template (which differs somewhat from the queue template) is now compulsory for all FT proposals.

September 2018 Call for Proposals

Gemini North and South are accepting proposals for the Fast Turnaround (FT) program. Here, we give information specific to this proposal cycle. Please see the other FT pages - particularly the rules - for general information about the program. FT-specific proposal templates must now be used for all FT proposals; see the "PIT information" section below. The revised 2018B PIT must be used

Important dates

  • Proposal deadline: 23:59, Hawaiian Standard Time (HST), September 30
  • Please ensure the new version of the PIT is used for submission (version 2.2).
  • Reviews must be completed by 23:59 HST, Oct 14. If you have submitted a proposal, but by the 2nd of the month have not received an email from FT regarding reviewing proposals, contact FT as soon as possible.
  • Results will be announced by Oct 21;
  • The deadline for preparing observations (Phase II) is Oct 31. Accepted programs meeting this deadline will be active from 1 November 2018 until 31 January 2019;
  • FT observations will be merged with the queue and observed on queue nights.

Eligibility

  • PIs from all participant countries taking part in the FT program may apply for this cycle.
  • We further welcome Japanese community PI proposals.
  • PIs from participant countries whose FT time for the semester has been used up should not apply for the remainder of the semester. Note that some participant countries only have very small amounts of FT time available each semester. Currently no partners have reached their limit. See Rule #4 and Q&A for more information.

Acceptable RA ranges

  • Gemini North: Targets from about RA = 19 hrs to 14.5 hr are acceptable during this cycle. However, note that due to queue filling, only a few hours are available in good conditions at RA~0. Also note that RAs near 19 will only be accessible for a couple hours during the first half of the first month (Nov) and only at northern declinations ( Dec> 0). Likewise, RAs near 14.5 will only be accessible for a few hours during the final month (Jan) and again only in the above declination range. Note Rule #9; an FT program may not fully backload its three-month active period; at least one of its targets must be observable during its first active month.
  • Gemini South: Targets from about RA = 20.5 hr to 14 hrs are acceptable during this cycle . Note, however, that RAs near 20.5 will only be accessible for a few hours during the first half of the first month (Nov) and only at favorable declinations (Dec < 0) . Likewise, RAs near 14 will only be accessible for a few hours during the second half of the final month (Jan) and again only in the above declination range. Note Rule #9; an FT program may not fully backload its three-month active period; at least one of its targets must be observable during its first active month.

Available instruments and observing modes
 

  • Gemini North
    • Please see the telescope schedule for detailed instrument availabilities.
    • The next GRACES run is scheduled for Jan 15-22. This is subject to change pending repairs to the instrument. Please contact the FT team for more information.
    • LGS is NOT offered at this time.
  • Gemini South
    • See the telescope schedule for detailed instrument availabilities.
    • GMOS-S and Flamingos-2 are otherwise expected to be available during this FT block.
    • A limited amount of GPI time may be available intermittently through the 3-month FT block. Contact the FT team for details.
    • GeMS+GSAOI, and PHOENIX are currently not available for FT.
  • Both telescopes
    • FT observations may not be executed during classical observing, priority visitor (PV) and Korean blocks, depending on the prevailing conditions.
    • For visiting instruments not listed above, you must contact the FT team before submitting a proposal to check availability (Fast.Turnaround at gemini.edu)
    • For GMOS proposals, please indicate in the Technical section if your program could be carried out with either GMOS (North or South).
    • The R600 grating in each GMOS instrument is NOT offered for FT (or regular queue) observations.
    • MOS observations are available for FT, subject to some caveats/restrictions
    • As discussed in the rules and Q&A, please contact the Fast Turnaround team in advance of the deadline if you would like to propose for an unusual instrument configuration or observing mode.

Time available

  • 20 hrs per month at each telescope is available for FT observations. Very roughly, this implies:
    • 4 hrs of 20%-ile conditions (IQ=20, for example; see this web page)
    • 10 hrs of 50%-ile conditions
    • 14 hrs of 70%-ile conditions
    • 17 hrs of 85%-ile conditions
  • PIs may propose for up to the amount of time in their most restrictive observing conditions, subject to partner's time availability - see rule #4 . For example, a proposal requesting CC50 IQ20 SB50 WVany conditions can request no more than 4 hrs of observing time.

PIT information

  • Proposals must be submitted using the version of the Phase I Tool specified on this web page (in the "Time Requests" tab, select Fast Turnaround Observing at Gemini as the proposal class).
  • In the Time Requests tab, select "Fast Turnaround Observing at Gemini" as the proposal class and specify the reviewer (and mentor, if appropriate). Note that this is where the reviewer is defined; changes cannot be made after the proposal has been submitted.
  • Dedicated LaTeX/Word templates must be used to prepare FT proposals: tex | sty | doc.
  • Submitting the same proposal more than once during a given month (e.g. after correcting/editing a submitted version) should be avoided if at all possible. Only submit when you are sure your proposal is ready to be reviewed.
  • The FT proposal template (which differs somewhat from the queue template) is now compulsory for all FT proposals.

August 2018 Call for Proposals

Gemini North and South are accepting proposals for the Fast Turnaround (FT) program. Here, we give information specific to this proposal cycle. Please see the other FT pages - particularly the rules - for general information about the program. FT-specific proposal templates must now be used for all FT proposals; see the "PIT information" section below. The revised 2018B PIT must be used

Important dates

  • Proposal deadline: 23:59, Hawaiian Standard Time (HST), August 31
  • Proposal deadline: 23:59, Hawaiian Standard Time (HST), Sep 3
  • Please ensure the new version of the PIT is used for submission (version 2.2).
  • Reviews must be complete by 23:59 HST, Sep 14. If you have submitted a proposal, but by the 2nd of the month have not received an email from FT regarding reviewing proposals, contact FT as soon as possible.
  • Results will be announced by Sep 21;
  • The deadline for preparing observations (Phase II) is Sep 30. Accepted programs meeting this deadline will be active from 1 October 2018 until 31 December 2018;
  • FT observations will be merged with the queue and observed on queue nights.

Eligibility

  • PIs from all participant countries taking part in the FT program may apply for this cycle.
  • We further welcome Japanese community PI proposals.
  • PIs from participant countries whose FT time for the semester has been used up should not apply for the remainder of the semester. Note that some participant countries only have very small amounts of FT time available each semester. Currently no partners have reached their limit. See Rule #4 and Q&A for more information.

Acceptable RA ranges

  • Gemini North: Targets from about RA = 15.5 hrs to 10.5 hr are acceptable during this cycle. Note, however, that RAs near 15.5 will only be accessible for a couple hours during the first half of the first month (Oct) and only at northern declinations ( Dec> 0) . Likewise, RAs near 10.5 will only be accessible for a few hours during the final month (Dec) and again only in the above declination range. Note Rule #9; an FT program may not fully backload its three-month active period; at least one of its targets must be observable during its first active month.
  • Gemini South: Targets from about RA = 19.0 hr to 12.5 hrs are acceptable during this cycle . Note, however, that RAs near 19.0 will only be accessible for a few hours during the first half of the first month (Oct) and only at favorable declinations (Dec < 0) . Likewise, RAs near 12.5 will only be accessible for a few hours during the second half of the final month (Dec) and again only in the above declination range. Note Rule #9; an FT program may not fully backload its three-month active period; at least one of its targets must be observable during its first active month.

Available instruments and observing modes
 

  • Gemini North
    • Please see the telescope schedule for detailed instrument availabilities.
    • For GRACES, check the schedule to confirm if and when GRACES will be available.
    • LGS is NOT offered at this time.
  • Gemini South
    • See the telescope schedule for detailed instrument availabilities.
    • GMOS-S and Flamingos-2 are otherwise expected to be available during this FT block.
    • A limited amount of GPI time may be available intermittently through the 3-month FT block. Contact the FT team for details.
    • GeMS+GSAOI, and PHOENIX are currently not available for FT.
  • Both telescopes
    • FT observations may not be executed during classical observing, priority visitor (PV) and Korean blocks, depending on the prevailing conditions.
    • For visiting instruments not listed above, you must contact the FT team before submitting a proposal to check availability (Fast.Turnaround at gemini.edu)
    • For GMOS proposals, please indicate in the Technical section if your program could be carried out with either GMOS (North or South).
    • The R600 grating in each GMOS instrument is NOT offered for FT (or regular queue) observations.
    • MOS observations are now available for FT, subject to some caveats/restrictions
    • As discussed in the rules and Q&A, please contact the Fast Turnaround team in advance of the deadline if you would like to propose for an unusual instrument configuration or observing mode.

Time available

  • 20 hrs per month at each telescope is available for FT observations. Very roughly, this implies:
    • 4 hrs of 20%-ile conditions (IQ=20, for example; see this web page)
    • 10 hrs of 50%-ile conditions
    • 14 hrs of 70%-ile conditions
    • 17 hrs of 85%-ile conditions
  • PIs may propose for up to the amount of time in their most restrictive observing conditions, subject to partner's time availability - see rule #4 . For example, a proposal requesting CC50 IQ20 SB50 WVany conditions can request no more than 4 hrs of observing time.

PIT information

  • Proposals must be submitted using the version of the Phase I Tool specified on this web page (in the "Time Requests" tab, select Fast Turnaround Observing at Gemini as the proposal class).
  • In the Time Requests tab, select "Fast Turnaround Observing at Gemini" as the proposal class and specify the reviewer (and mentor, if appropriate). Note that this is where the reviewer is defined; changes cannot be made after the proposal has been submitted.
  • Dedicated LaTeX/Word templates must be used to prepare FT proposals: tex | sty | doc.
  • Submitting the same proposal more than once during a given month (e.g. after correcting/editing a submitted version) should be avoided if at all possible. Only submit when you are sure your proposal is ready to be reviewed.
  • The FT proposal template (which differs somewhat from the queue template) is now compulsory for all FT proposals.

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