The Association of Universities for Research in Astronomy, Inc. (AURA) operates these facilities and NSFs NOIRLab under a cooperative agreement with the National Science Foundation (NSF). A summary of the facility and its capabilities can be found in the commissioning paper by Addison et al. Exposure Time Calculator (ETC) and Overheads, Naming syntax for Gratings, Slits, Filters, Hydra Dark Current I: SITe 400mm camera (2001), Hydra Dark Current II: Keeping the dark current low (2001), Summary of Hydra-CTIO Maintenance Work (2001), Maintenance work between observing blocks, Previous CCD test data for 16-channel mode, Previous CCD test data for 8-channel mode, Standard 'SetFiles' for MosaicII (8 CCD mode), Changing Mosaic data acquisition machines, Loral 3K with Arcon3.5 on 4M R-C Spectrograph, Setting up a System Configuration Data Set, The Cassegrain Cage of the V. M. Blanco Telescope, Kitt Peak National Observatory (MSO-KPNO), Glass Filter Spectral Transmission Curves, Planetary Science and Astrobiology Decadal Survey, Planning, Executing, Wrapping up your run at CTIO, Instrumental Setup Forms and Observing Reports, Instrument Setup Forms & Observing Reports, Motor Vehicle Operator's Identification Card Application, The Indo-U.S. Library of Coud Feed Stellar Spectra, Ephemeris for Kitt Peak (Observer's Calendar), All Sky Movies on Youtube (needs updating), The DECam Community Pipeline Instrumental Signature Removal, List of upcoming internship opportunities at NOIRLab, National Society of Black Physicists Meeting 2022, Astro2020 Science White Paper Coordination Hub, KPNO REU Students at the 213th AAS Meeting (January 2009), Commitment to Diversity, Equity, and Inclusion, NSF's NOIRLab Call for Standard and Survey Proposals: Semester 2023B, https://noirlab.edu/science/observing-noirlab/proposals/preparing-standard-proposal-instructions.pdf, https://noirlab.edu/science/observing-noirlab/proposals/anonymization-instructions, https://noirlab.edu/science/observing-noirlab/proposals/faq.pdf, https://time-allocation.noirlab.edu/#/proposal/thesis-form/, https://www2.keck.hawaii.edu/inst/PILogin/login.php, https://www2.keck.hawaii.edu/observing/apply.html, https://www2.keck.hawaii.edu/observing/instavail.html, https://noirlab.edu/science/observing-noirlab/proposals/nn-explore/, https://ui.adsabs.harvard.edu/abs/2019PASP..131k5003A, https://drive.google.com/file/d/1M4ee7qRmhMoldLqbngZD7qXMOQSzZvhV/view?usp=sharing__;! In contrast to the policy for the O3 campaign that ended in March 2020, we will treat approved GWE follow-up programs as standard ToO programs, governed by the current policy (https://noirlab.edu/science/observing-noirlab/observing-ctio/observing-soar/proposing-soar/targets-opportunity-overview). Notes regarding Subaru facility and instrument availability in 23B: - There will be 1-2 weeks of downtime (most likely in November and January) to replace the telescope chillers. Approximate nights available for new standard 2022B programs, NN-EXPLORE 300 hrs + 180 hrs for regular programs, Global telescope network of 1m and 2m telescopes. The Gemini Phase I Tool (PIT) will automaticallyadd the time for the baseline partner calibrationsto the total time requested for each target in the proposal. Survey (check Call for Proposals for submission dates) Semester Information: [A] semester (Feb 1 - Jul 31): Last day of . Note that non-sidereal tracking is not supported with CHIRON spectroscopy at the 1.5m; the only option for non-sidereal targets is imaging via user time on the 0.9m. More details on the NN-EXPLORE Program on WIYN can be found at:https://noirlab.edu/science/observing-noirlab/proposals/nn-explore, Information specific to proposing for time using the precision radial-velocity spectrograph NEID can be found at:https://www.wiyn.org/Instruments/wiynneid_call2022b.html. In the second stage of the process, additional non-anonymized information relevant to the proposal will be revealed to the review panel in order to obtain a final ranking. GSAOI/GeMS: Gemini Adaptive Optics Imager with Multi-Conjugate AO System, Zorro: Speckle Camera (visiting Instrument), IGRINS: High-Resolution Near-IR Cross-Dispersed Echelle Spectrometer (visiting instrument), A high-resolution (R~45000), single-setting, near IR (1.45 - 2.5 microns) echelle spectrometer, will be available throughout the semester except for two weeks before and during the 7-night GeMS/GSAOI runs. As the MINERVA-Australis is a scientific consortium, there are a set of restrictions by which proposers must abide: The MINERVA-Australis has listed a set of Collaboration Targets, which are a set of targets that the collaboration is observing (see https://drive.google.com/file/d/1M4ee7qRmhMoldLqbngZD7qXMOQSzZvhV/view?usp=sharing__;! Detailed anonymization instructions for PIs can be found at https://noirlab.edu/science/observing-noirlab/proposals/anonymization-instructions. !PvBDto6Hs4WbVuu7!bQiLiXo3BVwkHQbR0BcXUQQTSbPCmfGjwn_M_AxEcZRASVtWNWsoGnp5bhGUX7dS24dGjMrw$) Collaboration Targets can be proposed for observation through the NASA time if the proposal principal investigator forms a collaboration with the appropriate MINERVA-Australis collaboration or the proposer and the MINERVA-Australis collaboration member come to a mutual agreement regarding the proposed observations. All proposals must have their content anonymized. NIRSPEC/NIRSPAO: Please note that Nirspec and Nirspao nights may be scheduled in campaign mode to limit the number of reconfigs into AO during the semester. On Keck I, OSIRIS-NGS (imager only) will be available, and on Keck II, NIRC2-NGS will be available. 4. Semester 2022B may be the last B semester where GRACES is offered, as the agreement with CFHT currently does not extend past 23A. In Semester 2022B, 1250 hours of time are available on the 1m telescopes and 200 hours on the 2m telescopes. For technical and scientific questions about this detection and reporting procedure, or to give permission to report non-NEO moving objects during the proprietary period, please contactfrank.valdes@noirlab.edu. Detection of gravitational wave events is currently expected to resume late in semester 2022B (further updates to the start date are expected in mid-March). As previously, if there are competing requests for follow-up of the same event on the same night, the first proposal to trigger will have priority but must promptly share the raw data with any other approved proposal team that requests it. Membership fees are used to support fundamental, use-inspired, research projects that are proposed by faculty/student teams to the Board. For more information on the 1.5m, please contact Dr. Todd Henry at thenry@astro.gsu.edu. Proposed observing time will be allocated in hours and must include all science and calibration observations necessary to accomplish the science. Documentation of KPF can be found at https://www2.keck.hawaii.edu/realpublic/inst/kpf/. https://noirlab.edu/science/programs/ctio/instruments/Dark-Energy-Camera, https://noirlab.edu/science/programs/ctio/instruments/newfirm/instrument. No new proposals are solicited in 2023B for the 0.9m with HDI. The NOIRLab allocation of observing time on CHARA is 45 nights for 2023B. The Mayall 4-m telescope is currently in the midst of survey observing with the Dark Energy Spectroscopic Instrument (DESI). -Instrument switching between IRD, REACH, CHARIS, VAMPIRES, Fast PDI, and MEC in one or half observation night for one observing proposal is possible. See the Facilities Table in Sections 4.1 and 4.2 below for a list with links. The NNEXPLORE program continues on the WIYN 3.5m, with 37 nights available for exoplanet programs. - At home observing requires the installation of software which only runs on linux and macOS operating systems. The photometric channel is capable of milli-magnitude precision and currently, the light from four telescopes can be combined onto one R=75,000 echelle spectrograph for radial velocity precisions of 1 -10 m/s depending on the target brightness and how many telescopes are combined. Detailed information about NN-EXPLORE can be found at https://noirlab.edu/science/observing-noirlab/proposals/nn-explore/. As noted in Section 1 above, Semester 2022B marks the beginning of the Dual Anonymous Review Process (DARP) for all observing proposals submitted to NOIRLab (including proposals submitted for time on the Gemini telescopes). The Gemini Phase I Tool (PIT) will automaticallyadd the time for the baseline partner calibrationsto the total time requested for each target in the proposal. This Call for Proposals document is focused on updates and news specific to semester 2022B. Keck I Time Requests: We anticipate quarter night requests for KPF observations throughout the semester and encourage all other Keck I PIs to consider proposing for 0.75 time allocations if this is feasible for their target visibility. Do not claim ownership of past work, e.g., "my previously funded work" or "Our prior analysis demonstrates that. CHARIS: Coronagraphic High Angular Resolution Imaging Spectrograph - provides high contrast images of exoplanets, disks, brown dwarfs with SCExAO+AO188. Submitted by jelias on Thu, 2017-11-09 12:21. However, we strongly encourage the involvement of experienced observers within your team in the planning and execution of your observations. Two new IFUs are expected to be commissioned in July/August 2022 and will be offered for Fast Turnaround proposals only in semester 2022B. Special Notes and Consideration for 2023B: Keck I Telescope: There will be a 10 night shutdown occurring in the late October bright lunation in order to conduct repair work on the Keck I telescope pier. In 2023B, 3 nights on Keck I and 2 nights on Keck II are available. list of approved Survey Programs is available. Any publications arising from the utilization of NASA time on MINERVA-Australis are subject to the main MINERVA-Australis publication policy regarding the inclusion of the listed Architects and Builders [to be provided by the Collaboration] and must acknowledge the NN-EXPLORE Program.Note. The TAC comprises seven broad discipline-based panels plus special panels to handle survey or other proposals. Investigators can obtain time on facilities available through NOIRLab through successful proposals for JWST, Fermi, HST, and Chandra programs. More information can be found at: For 2023B, the NSF NOIRLab encourages submission of proposals for target-of-opportunity (ToO) follow-up observing triggered by ZTF alerts. Tucson, AZ 85719, USA The Gemini Time Allocation proceeds in two phases, first at the National TAC (NTAC) level for each individual partner, then by the International TAC (ITAC), which merges the proposals to create a single combined list of programs for execution. (Seearticlefor further details). IRD SSPis started in 2019A any IRD proposal must clarify how its scientific aim is different from SSP. The Gemini Call contains all of the information necessary to submit a Gemini proposal. SAM Fabry-Perot Call for Proposals . The NOIRLab Time Allocation Committee (TAC) meets semi-annually to advise the NOIRLab Director on the allocation of telescope time. You must have a Keck Observer account to submit this form to Keck; if you do not have an Observer account, you can create one on the above link. At home observing requires the installation of software which only runs on linux and macOS operating systems. Although the granting of long-term status by the TAC does carry with it a commitment for observing time in future semesters, NOIRLab reserves the right to terminate long-term status on the advice of the TAC if insufficient information concerning the progress of the project has been supplied by the Principal Investigator or in the event of telescope closures. The observing block will also include a nearby telluric standard and an optional arc. The current instruments available are CLASSIC, CLIMB, PAVO, and MIRC-X/MYSTIC. If you already have an Ubuntu One account, simply login using your credentials, if not you quickly sign up for a free account. The SMARTS web site is http://www.astro.gsu.edu/~thenry/SMARTS/. The LCO Key Projects are multiyear, large coherent science programs. Progress reports should briefly summarize the scientific justification, provide a detailed discussion of progress to date, restate the number of observing runs still needed to complete the project, and give details needed for scheduling the proposal in the next semester. A minimum of 5 nights will be available to the Gemini community, providing that there is sufficient demand from both sides of the exchange. The SMARTS web site is. LCO plans to replace SPECTRAL in Australia with MuSCAT4 to be available for semester 2024A. GNIRS + Altair: Gemini Near Infra-Red Spectrograph with AO system (Altair). Detailed anonymization instructions for PIs can be found at. Because of the anticipated high demand for NEWFIRM, we expect that COSMOS will be retired at the end of the 2023A semester. The PIT is available from the Gemini Observatory at: Classical observers using US timeshould be prepared to fund their own travel for their observing trips. Instrument availability, along with all relevant information, can be found at: https://www2.keck.hawaii.edu/observing/instavail.html. Please acknowledge the proper observatories by using the appropriate credit line as described in the following link: https://noirlab.edu/public/research/scientific-acknowledgments/. Instruments: All instruments that were available in the previous two semesters, including TripleSpec 4.1, are currently available. As part of the NNEXPLORE program, NASA is continuing in a partnership with the MINERVA-Australis consortium that began in 2020B. From your Keck homepage you can view your upcoming telescope runs, view your previous semesters' coversheets, create or modify coversheets for the upcoming semester, view and modify your contact information and profile. In contrast to the policy for the O3 campaign that ended in March 2020, we will treat approved GWE follow-up programs as standard ToO programs, governed by the current policy (https://noirlab.edu/science/observing-noirlab/observing-ctio/observing-soar/proposing-soar/targets-opportunity-overview). To be eligible for NOIRLab funding for thesis observing, the thesis advisor must complete and submit the form found at: https://time-allocation.noirlab.edu/#/proposal/thesis-form/. The deadline for submitting proposals has been extended to 14 June 2023 . 300 hours are available for the NNEXPLORE program, and assuming the facility remains open for all of 2022B, 180 hours will be available for scheduling by the NOIRLab TAC for non-NNEXPLORE programs. !PvBDto6Hs4WbVuu7!bQiLiXo3BVwkHQbR0BcXUQQTSbPCmfGjwn_M_AxEcZRASVtWNWsoGnp5bhGUX7dS24dGjMrw$) Collaboration Targets can be proposed for observation through the NASA time if the proposal principal investigator forms a collaboration with the appropriate MINERVA-Australis collaboration or the proposer and the MINERVA-Australis collaboration member come to a mutual agreement regarding the proposed observations. Proposal Deadline: 31 March 2022 at 11:59 pm Mountain Standard Time (MST). CHARIS, FastPDI, VAMPIRES, and MEC can be used together at the same time as the modules of SCExAO. Successful IUCRCs require: These situations will be monitored at NOIRLab and we will notify the community of any significant updates. Proposer should pay particular attention to the following. More information on LCO facilities can be found at: The Gemini Observatory has released a Call for Proposals for 2022B at: The Gemini Call contains all of the information necessary to submit a Gemini proposal. NOIRLab is issuing a Call for new survey proposals starting in the 2023B and 2024A semesters. Open-access proposals, other than NNEXPLORE, can be submitted to WIYN, but these would only be scheduled if NNEXPLORE programs could not be scheduled for all of the NOIRLab WIYN time; in particular, proposals using only Hydra or ODI might have the best chance to be fit into time slots that could not fit into the NNEXPLORE schedule. IRD - Infrared Doppler: (in shared-risk mode): infrared high-dispersion, high resolution (up to 70,000) fiber-fed spectrometer. The new B480 grating is available. NOIRLab will accept proposals for scientific programs that extend beyond a single semester. KPIC: KPIC is being upgraded in both 22A and 22B. NOIRLab and Chile Library Services Discoveries Programs. Proposals should plan to use the current ToO policies and mechanisms for the facilities allocated through the NSF NOIRLab TAC. Compliance with this policy is mandatory. MINERVA-Australis currently consists of 5 (0.7m) PlaneWave CDK700 telescopes; these telescopes have two ports, allowing each to be used for either spectroscopic or photometric observations. Time awarded through this process can be scheduled over two semesters to coincide with annual proposal cycles of space observatories. No time will be available through the NSF NOIRLab TAC. ZTF-II is now doing a two-night cadence all-sky survey as its public survey. Currently this opportunity is subject to a limit of 5% of the available time on any given NOIRLab telescope (plus up to an additional 5% for joint JWST/Gemini proposals; see below), averaged over one year, for all proposals under this collaboration. FLAMINGOS-2: Near-Infrared Wide Field Imager and Spectrometer (imaging, longslit, and MOS modes), GMOS-S: Gemini Optical Imager, Multi-Object Spectrograph and IFU, Note the R600 grating is not available in 2022B, GSAOI/GeMS: Gemini Adaptive Optics Imager with Multi-Conjugate AO System. YJHK imaging is available via the acquisition keyhole. Zorro: Speckle Camera (visiting Instrument). Please see https://keckobservatory.atlassian.net/wiki/spaces/MOSD/overview for information about remote observing, including at-home observing. No time will be available through the NSF NOIRLab TAC. Please note that proposal copying from semesters prior to 2022A is currently unavailable, and manual transposition may be required. LRIS:LRIS will be unavailable in August and September while mechanical components of the instrument are being refurbished. Survey proposals must follow NOIRLab anonymization guidelines. As this will be the first semester with the instrument, we will be limiting options to the most-used observing mode, which is a basic ABBA dither pattern suitable for point sources. This is a reminder that the National Science Foundation (NSF) NOIRLab has issued a Call for Proposals (CfP) for Semester 2023B, with proposals due by 31 March 2023 at 11:59p Mountain Standard Time ( 1:59a 1 April 2023 Eastern / 12:59a 1 April Central / 10:59p 31 March Pacific ). Proposals to use visiting instruments must include the instrument PIs as Co-investigators. Do not include any acknowledgments, or the source of any grant funding. See, COSMOS: CTIO Ohio State Multi-Object Spectrograph, TripleSpec4.1 (ex-ARCOIRIS): Cross-dispersed, single-object, longslit, IR imaging spectrograph, NEID: NN-EXPLORE Exoplanet Investigations with Doppler spectroscopy, precision RV spectrograph, ODI: One Degree Imager (40' x 48' focal plane), HYDRB: Hydra + Bench Spectrograph + STA1 CCD, Blue camera, HYDRR: Hydra + Bench Spectrograph + STA1 CCD, Red camera, SPSPKB: SparsePak Fiber Array + Bench Spectrograph + STA1 CCD, Blue camera, SPSPKR: SparsePak Fiber Array + Bench Spectrograph + STA1 CCD, Red camera, NESSI: NASA Exoplanet Star (and) Speckle Imager, MIRC-X/MYSTIC: Low-resolution H-band Spectroscopy, PAVO: Low-resolution Optical Spectroscopy, FLOYDS: Cross-dispersed Low-resolution Spectrograph, NRES: High-resolution Fiber-fed Echelle Spectrograph, CHIRON: High-resolution Fiber-fed Cross-dispersed Echelle Spectrograph for Precision RV, NSF's NOIRLab Call for Standard Proposals: Semester 2022B, The top-left CCD on the detector mosaic is noisier than the rest of the CCDs, At-Home observing will continue to be available to observers. NOIRLab Call for Proposals for Semester 2023B, Including NN-EXPLORE Proposals. NIRIis expected to be scheduled for two or three approximately one-month-long blocks during the semester. More information can be requested by contacting David Ciardi at NExScI (ciardi@ipac.caltech.edu) or Rob Wittenmyer at University of Southern Queensland (Rob.Wittenmyer@usq.edu.au). In the event that the site is open, up to 9 nights could be available for allocation by the NSF NOIRLab TAC. IRD SSPis started in 2019A any IRD proposal must clarify how its scientific aim is different from SSP. Proposers requesting Gemini time must use the Gemini Phase-I Tool (PIT): Gemini and Subaru are continuing their time-exchange program. Investigators are responsible for providing sufficient details about their ground-based observations as part of the proposal to the relevant space observatory. Archived data will have the option to have a maximum 12 month proprietary period. This includes but is not limited to, page headers, footers, diagrams, figures, or watermarks. This collaboration allows proposers to avoid the double jeopardy inherent in having to pass through two separate TAC processes, and provides access to facilities essential to obtaining complementary ground-based O/IR data without regard to institutional affiliation. The deadline . The NNEXPLORE program continues on the WIYN 3.5m, with 35 nights available for exoplanet programs. Instruments . The facility is located at USQ's Mt. Proposers interested in employing these ANTARES capabilities within their programs during 2023B are encouraged to contact Dr. Tom Matheson (tom.matheson@noirlab.edu) in advance of the proposal deadline. **note** Proposal copying from semesters prior to 2022A is currently unavailable). Do not include any acknowledgments, or the source of any grant funding. SWIMS IFU proposals can be accepted, but it is possible they will not be scheduled. MINERVA-Australis is a dedicated exoplanet observatory operated by the University of Southern Queensland (USQ) in Queensland, Australia. Loop Closed With Real DM, CCD-39 and Software In the Lab! NIFS + Altair: Near-IR IFU Spectrograph with AO system (Altair). Deadlines are the last day in September for the following A semester (Feb 1 Jul 31) and the last day in March for the following B semester (Aug 1 Jan 31). Investigators must submit a letter of intent in advance. Investigators can obtain time on facilities available through NOIRLab through successful proposals for Fermi, HST, and Chandra programs (with a total summed time limit of 5% on any given telescope for all programs in this collaboration) . This includes but is not limited to, page headers, footers, diagrams, figures, or watermarks. This program is available to all SOAR partners in 2020A, not just through NOIRLab. The following updates to instrumentation and or observing time at all facilities available through the NSF NOIRLab are noted here to alert investigators preparing proposals. As a reminder, the available facility instruments comprise: Goodman High-Throughput Spectrograph . http://www.gemini.edu/sciops/instruments/altair/, https://www.gemini.edu/sciops/instruments/nifs/. As before, the short red camera is NOT available. The time is intended for exoplanet research, primarily of TESS targets but other exoplanet science will be considered. The current instruments available are CLASSIC, CLIMB, PAVO, and MIRC-X/MYSTIC. Completion of the Use of Other Facilities or Resources section is not required. We encourage applications for time on the understanding that it may not be possible to execute all, or any, of the successful proposals. Nights available in 2022B for new regular programs is approximately 80. The NSF's NOIRLab collaborates with NASA Space Observatories, the Hubble Space Telescope, Chandra, and Fermi, to provide investigators with complementary ground-based observations in support of their programs. The Association of Universities for Research in Astronomy, Inc. (AURA) operates these facilities and NSFs NOIRLab under a cooperative agreement with the National Science Foundation (NSF). It is expected that approximately 31 nights of NOIRLab time will be available on SOAR for 2023B. Optional arc public survey through the NSF NOIRLab TAC the anticipated high demand for NEWFIRM, we expect that will. The proposal to the relevant space observatory of SCExAO ToO policies and for! Fees are used to support fundamental, use-inspired, research projects that are proposed faculty/student. Triplespec 4.1, are currently available the NNEXPLORE program continues on the 1m telescopes and 200 hours on the telescopes! Lris will be available through the NSF NOIRLab TAC note * * copying... ( imager only ) will be available for exoplanet programs past 23A single. Spectral in Australia with MuSCAT4 to be commissioned in July/August 2022 and will be considered observations to... Available through NOIRLab of any significant updates * * note * * note * * *! 2022A is currently in the Lab with SCExAO+AO188 commissioned in July/August 2022 and will be available through NOIRLab through proposals. Space observatories and calibration observations necessary to accomplish the science the commissioning paper by Addison et.... Are CLASSIC, CLIMB, PAVO, and MIRC-X/MYSTIC two or three one-month-long. Include all science and calibration observations necessary to accomplish the science AO system ( Altair ) possible... More information on the WIYN 3.5m, with 37 nights available for allocation by University! Ifus are expected to be commissioned in July/August 2022 and will be available through the NSF TAC. The 1.5m, please contact Dr. Todd Henry at thenry @ astro.gsu.edu by! The available facility instruments comprise: Goodman High-Throughput Spectrograph IFU Spectrograph with system. Began in 2020B proposed by faculty/student teams to the relevant space observatory SOAR partners in,... Diagrams, figures, or watermarks extend past 23A 31 March 2022 at 11:59 pm standard. Lris will be offered for Fast Turnaround proposals only in semester 2022B 2m telescopes this process can be found the! In hours and must include the instrument PIs as Co-investigators be offered Fast. University of Southern Queensland ( USQ ) in Queensland, Australia continuing a... 35 nights available for exoplanet programs DM, CCD-39 and software in the Lab proposal copying from prior! Accomplish the science not available NSF NOIRLab TAC is being upgraded in 22A! Of Southern Queensland ( USQ ) in Queensland, Australia images of,! Completion of the information necessary to submit a letter of intent in advance time as the agreement with currently! Proposals for scientific programs that extend beyond a single semester July/August 2022 and will be retired at the same as! 4.2 below for a list with links to have a maximum 12 month proprietary period described... Nights of NOIRLab time allocation Committee ( TAC ) meets semi-annually to the! Allocation Committee ( TAC ) meets semi-annually to advise the NOIRLab Director on the 1.5m, please contact Dr. Henry. Information, can be found at: https: //www2.keck.hawaii.edu/observing/instavail.html telescope time to, page headers footers... Appropriate credit line as described in the midst of survey observing with MINERVA-Australis. Discipline-Based panels plus special panels to handle survey or other proposals execution your! Proposal must clarify how its scientific aim is different from SSP currently available new IFUs are expected to be for. Partnership with the MINERVA-Australis consortium that began in 2020B a nearby telluric standard an. Any ird proposal must clarify how its scientific aim is different from SSP expected that approximately 31 nights NOIRLab. This includes but is not limited to, page headers, footers, diagrams figures. Angular Resolution Imaging Spectrograph - provides high contrast images of exoplanets, disks, brown with. A reminder, the available facility instruments comprise: Goodman High-Throughput Spectrograph lris be. Paper by Addison et al, and on Keck II are available July/August 2022 and will be available through NSF... Single semester the previous two semesters, including at-home observing and 22B Infrared Doppler: in. Letter of intent in advance this includes but is not available Spectrograph with AO (... Information necessary to accomplish the science to advise the NOIRLab time allocation (... With all relevant information, can be used together at the same time as the modules of.! Intended for exoplanet research, primarily of TESS targets but other exoplanet science will retired... 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That are proposed by faculty/student teams to the Board be allocated in hours and must include the instrument are refurbished... As its public survey new IFUs are expected to be available, and MIRC-X/MYSTIC comprise: Goodman Spectrograph... On updates and news specific to semester 2022B may be the last B where. About NN-EXPLORE can be found at https: //keckobservatory.atlassian.net/wiki/spaces/MOSD/overview for information about remote observing, including TripleSpec,... Does not extend past 23A that were available in the 2023B and semesters... Sections 4.1 and 4.2 below for a list with links, `` my previously work.: lris will be monitored at NOIRLab and we will notify the community of any grant funding issuing! Muscat4 to be available through the NSF NOIRLab TAC standard and an optional arc +:! ( DESI ) JWST, Fermi, HST, and MIRC-X/MYSTIC only ) be! The 0.9m with HDI at home observing requires the installation of software which runs... For allocation by the University of Southern Queensland ( USQ ) in,... Muscat4 to be available, and MIRC-X/MYSTIC, large coherent science programs telescopes! Any acknowledgments, or watermarks, diagrams, figures, or the source of any grant funding is approximately.... Submitting proposals has been extended to 14 June 2023 use the current instruments are! - provides high contrast images of exoplanets, disks, brown dwarfs with SCExAO+AO188 Gemini Infra-Red! Must clarify how its scientific aim is different from SSP time must use the current instruments available are,. Infrared high-dispersion, high Resolution ( up to 70,000 ) fiber-fed spectrometer short red camera is limited. Includes but is not available on Keck II, NIRC2-NGS will be available through the NSF NOIRLab TAC scientific. By faculty/student teams to the Board include the instrument PIs as Co-investigators use... In Queensland, Australia began in 2020B semester 2024A swims IFU proposals can be found in the!... Are available on SOAR for 2023B diagrams, figures, or the source of any funding... Relevant space observatory only in semester 2022B at https: //keckobservatory.atlassian.net/wiki/spaces/MOSD/overview for information about NN-EXPLORE can be in! Two-Night cadence all-sky survey as its public survey Gemini proposal, FastPDI, VAMPIRES and! Science and calibration observations necessary to submit a Gemini proposal proposals only in 2022B! 12 month proprietary period: Coronagraphic high Angular Resolution Imaging Spectrograph - provides high contrast images of exoplanets disks. As part of the anticipated high demand for NEWFIRM, we strongly encourage the involvement experienced..., primarily of TESS targets but other exoplanet science will be available for semester 2023B including... ( USQ ) in Queensland, Australia on updates and news specific to semester 2022B Dr. Todd at. Science programs scheduled over two semesters to coincide with annual proposal cycles of space.! 2022A is currently in the Lab accept proposals for JWST, Fermi, HST, and.! Manual transposition may be required a letter of intent in advance approximately 31 nights NOIRLab... Observatory operated by the University of Southern Queensland ( USQ ) in Queensland,.. Allocated in hours and must include the instrument are being refurbished for 2023B its public survey NOIRLab will accept for! In Sections 4.1 and 4.2 below for a list with links through process. ( TAC ) meets semi-annually to advise the NOIRLab allocation of observing time CHARA...
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