An additonal 5 nights are available to the community through NN-EXPLORE (see Section 3.1) on the precision radial-velocity spectrograph, Veloce, for exoplanet research.
Proposals for this time should be submitted through the NOAO proposal form. The proposals will be reviewed by the NOAO TAC, and the successful proposals submitted to the AAO for scheduling. Note also that proposals for AAT time through the regular AAT open call, submitted by the AAO deadline of 15 September 2018 at 17:00 (AEDT) using the AAO form, are also encouraged by the AAO. These will be assessed only by the Australian Time Assignment Committee.
The following updatess to instrumentation at all facilities available through NOAO are noted here to alert investigators preparing proposals.
The other opportunities for NN-EXPLORE continue: WIYN with its full instrument complement, along with 400 hours (the equivalent of 40 nights) on the CTIO/SMARTS 1.5m with the precision radial-velocity spectrometer CHIRON.
The Gemini Call contains all of the information necessary to submit a Gemini proposal. It is usggested that you read the Gemini CfP if youare requesting Gemini time.
Gemini and Subaru are continuing their time-exchange program. A desired minimum of five classically-scheduled nights will be available to the Gemini community, providing that there is sufficient demand from both sides of the exchange. Please see the Gemini call for proposals for more information. Proposers requesting Subaru time must use the Gemini Phase-I Tool (PIT).
Instruments avasilable: In 2019B, CTIO will be offering the Dark Energy Camera (DECam) and the Cerro Tololo Ohio State Multi-Object Spectrograph (COSMOS).
Nights available in 2019B: Approximately 66.
The SOAR website is located at:
Several special opportunities are available for SOAR in 2019B - interested parties should visit the SOAR home page for details beyond the summary below:
TSpec availability: The TripleSpec instrument (ex-ARCOIRIS, re-baptized TripleSpec 4.1) is being commissioned in March, with possible science verification in April and June. People interested in proposing can do so using performance information from the Blanco telescope (http://www.ctio.noao.edu/noao/content/Arcoiris). Any time granted in 2019B will be shared-risk, of course. See the SOAR web pages for further details.All instruments that were available in the previous semester are currently available.
Queue scheduling opportunity: We hope to schedule a modest fraction of SOAR nights in queue mode in 2019B. Programs that would be included in this program must meet the following conditions:
- Programs must be feasible in SOAR's current remote/classical mode
- Proposers require observations at a cadence of 2-4 weeks, set by the scheduled queue nights
- Proposers can use the Goodman spectrograph with the red camera and 400 l/mm grating
- Proposers have prior experience with the telescope and instrument
- For further details, including how to express interest in participation, please see the SOAR web pages, which include appropriate contact information.
We will only provide this mode if we are confident it is working reliably; this is why proposals must be feasible without queue scheduling.
Time on the small telescopes at CTIO will be available to NOAO users in 2019B via the usual proposal process. The telescopes are operated by the SMARTS consortium with up to 15% of time available to the NOAO community.
Note that time on the 1.3m is not avaialble in 2019B.
The 0.9m + CFCCD is available in user mode only. It is being operated on a part time basis (operating on up to 60% of nights), during the 2018B semester. As a result up to 18 nights will be available for allocation by the NOAO TAC For more information on the 0.9m, please contact Dr. Todd Henry at email@example.com.
Non-sidereal tracking is no longer supported as service or queue observing. The only option for non-sidereal is user time on the 0.9m.
The 1.5m + CHIRON (fiber-fed cross-dispersed echelle). 400 hours is available for the NN-EXPLORE program, and we anticipate that ~180 hrs will be available for scheduling by the NOAO TAC for non-NN-EXPLORE programs. For more information on the 1.5m, please contact Dr. Todd Henry at firstname.lastname@example.org.
4.1 Facilities List
4.2 Telescope and Instrument Lists (with Instrument Proposal Code and Web-link)
GMOS-N: Gemini Optical Imager, Multi-Object Spectrograph and IFU
GNIRS: Gemini Near Infra-Red Spectrograph
GNIRS + Altair: Gemini Near Infra-Red Spectrograph with NGS, LGS, or LGS+PWFS1 AO systems (Altair)
NIFS: Near-IR IFU Spectrograph
NIFS + Altair: Near-IR IFU Spectrograph with NGS, LGS, or LGS+PWFS1 AO systems (Altair)
NIRI: Near-Infrared Imager
NIRI + Altair: Near-IR Imager with NGS, LGS, LGS+PWFS1 AO systems
'Alopeke: Speckle Camera (visiting instrument)
GRACES: Gemini Remote Access to CFHT ESPaDOnS Spectrograph (visiting instrument)
POLISH-2: High-precision optical polarimeter (visiting instrument)
TEXES: a high resolution (R ~4,000-100,000) mid-infrared (5-25 micron) spectrometer. Schedule will be based on demand (visiting instrument) https://www.gemini.edu/sciops/instruments/texes-north
FLAMINGOS-2: Near-Infrared Wide Field Imager and Spectrometer (imaging and longslit modes only)
GMOS-S: Gemini Optical Imager, Multi-Object Spectrograph and IFU
GPI: Gemini Planet Imager
GSAOI/GeMS: Gemini Adaptive Optics Imager with Multi-Conjugate AO System
DSSI: Speckle Camera (visiting Instrument)
Phoenix: High-Resolution Near-IR Echelle Spectrometer (visiting instrument)
Subaru (Gemini Exchange time)
COMICS: Cooled Mid-IR Camera and Spectrometer
FOCAS: Faint Object Camera and Spectrograph
HDS: High Dispersion Spectrograph
HSC: Hyper Suprime-Cam Wide-Field Optical Imager
IRCS: IR Camera and Spectrograph
IRCS+AO188: IRCS + Natural and Laser Guide Star AO
MOIRCS: Multi-Object IR Camera and Spectrograph
Visiting Instruments on Subaru (Observing proposals using the visiting instruments must include the relevant instrument PIs as a Co-investigators)
CHARIS: Coronagraphic High Angular Resolution Imaging Spectrograph - provides high contrast images of exoplanets, disks, brown dwarfs with SCExAO+AO188. https://scholar.princeton.edu/charis
SCExAO: Subaru Coronagraphic Extreme Adaptive Optics - delivers high contrast images of the innermost surrounding of bright sources to CHARIS. The VAMPIRES module in SCExAO is also available for science observations in 2019B. https://www.naoj.org/Projects/SCEXAO/scexaoWEB/000home.web/indexm.html
IRD: Infrared high-dispersion, high resolution (up to 70,000) fiber-fed spectrometer. IRD provides high spectral resolution echelle spectroscopy and radial velocity measurements from 0.97 to 1.75 um simultaneously combined with AO188. IRD is available with NGS-AO only in shared-risk. IRD SSP started in 2019A – any IRD proposal must clarify how its scientific aim is different from SSP. http://ird.mtk.nao.ac.jp/IRDpub/index_tmp.html
CTIO 4m Blanco
DECam: Wide-Field Optical Imager
COSMOS: CTIO Ohio State Multi-Object Spectrograph
Goodman: Goodman Spectrograph
SOI: SOAR Optical Imager
TripleSpec4.1 (ex-ARCOIRIS): Cross-dispersed, single-object, longslit, IR imaging spectrograph
Spartan: Spartan IR Imager
SAM: SOAR Adaptive Module
HRCAM: High-Resolution Camera
SAMHR: SAM + HRCAM
SIFS: SOAR Integral Field 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
WHIRC: WIYN High Resolution IR Camera
GRDPK: GradPak IFU
HEXPK: HexPak IFU
NESSI: NASA Exoplanet Star (and) Speckle Imager
Large Binocular Telescope
LBC: Large Binocular Cameras, Red and Blue
LUCI: LBT Utility Cameras in the Infrared
MODS: Multi-Object Double Spectrographs
CLASSIC: IR (H or K) Imaging
CLIMB: IR (H or K) Imaging
MIRC: Low-resolution H-band Spectroscopy
PAVO: Low-resolution Optical Spectroscopy
VEGA: Medium-resolution and High-resolution Optical Spectroscopy
LCO-2m Global Network
Spectral: Optical Imager
FLOYDS: Cross-dispersed Low-resolution Spectrograph
LCO-1m Global Network
Sinistro: Optical Imager
NRES: High-resolution Fiber-fed Echelle Spectrograph
CHIRON: High-resolution Fiber-fed Cross-dispersed Echelle Spectrograph for Precision RV
CFIM+T2K: Cass Direct + SITe 2K CCD
HDI: Half-Degree Imager
5. How to Acknowledge Use of NOAO Facilities
There are a variety of credit lines which are appropriate for citing the use of data from one or more of the NOAO facilities. Please acknowledge the proper observatories by using the appropriate credit line as discussed below.
NOAO generic press release
The National Optical Astronomy Observatory (NOAO) consists of Kitt Peak National Observatory near Tucson, Arizona, Cerro Tololo Inter-American Observatory near La Serena, Chile, and the NOAO System Science Center. NOAO is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation.
Observers should also note their NOAO proposal ID and observing dates in their publications either in a footnote, or in the observations section or acknowledgments sections of their papers.
Visitors are asked to add a Kitt Peak byline on the title page, as a footnote to the author, that reads:
Visiting Astronomer, Kitt Peak National Observatory, National Optical Astronomy Observatory, which is operated by the Association of Universities for Research in Astronomy (AURA) under cooperative agreement with the National Science Foundation.
NOAO staff members are asked to add a footnote after their names on the title page that reads: Kitt Peak National Observatory, National Optical Astronomy Observatory, which is operated by the Association of Universities for Research in Astronomy (AURA) under cooperative agreement with the National Science Foundation.
In addition to the Kitt Peak credit line, Case Western Reserve University has requested that a special acknowledgement be included on papers resulting from observations obtained with the Burrell Schmidt telescope:
Observations made with the Burrell Schmidt of the Warner and Swasey Observatory, Case Western Reserve University.
In addition to the Kitt Peak Credit line, the WIYN Observatory Corporation has requested that the following acknowledgement be included in any paper using WIYN data. The acknowledgement should be included as a footnote on the title page. The WIYN Board also encourages the mention of WIYN in the title or abstract of the paper:
The WIYN Observatory is a joint facility of the University of Wisconsin-Madison, Indiana University, Yale University, and the National Optical Astronomy Observatory.
For publications resulting from NN-EXPLORE telescope time, please include this text: "Data presented herein were obtained at the WIYN Observatory from telescope time allocated to NN-EXPLORE through the scientific partnership of the National Aeronautics and Space Administration, the National Science Foundation, and the National Optical Astronomy Observatory."
It is expected that visiting observers making use of CTIO facilities will utilize the observations they obtain for the preparation of a publication describing their research activity. Publications by visiting observers should carry the following credit lines:
Visiting astronomer, Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, which are operated by the Association of Universities for Research in Astronomy, under contract with the National Science Foundation.
Visiting observers who use CTIO facilities for only a small part of a larger program should include suitable acknowledgement to the Observatory in their publication or dissertation.
To properly acknowledge the use of data obtained with the SOAR telescope in publications, whether partially or entirely based on SOAR data, please include an asterisk by the paper title referring to a footnote stating:
"Based on observations obtained at the Southern Astrophysical Research (SOAR) telescope, which is a joint project of the Ministério da Ciência, Tecnologia, e Inovação (MCTI) da República Federativa do Brasil, the U.S. National Optical Astronomy Observatory (NOAO), the University of North Carolina at Chapel Hill (UNC), and Michigan State University (MSU)."
Papers containing data from the Gemini telescopes (e.g., an ApJ paper) should include the following general acknowledgment as a footnote on the first page or in the last section before the references:
Based on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Ministério da Ciência e Tecnologia (Brazil) and Ministerio de Ciencia, Tecnología e Innovación Productiva (Argentina).
If appropriate, please also acknowledge the provision of visiting instrument(s) as described in the relevant "documents" web pages for that instrument.
Authors are also asked to give the identification number ("Program ID") of the program(s) under which their data were obtained, e.g. GN-2004A-Q-10, or GS-2003B-C- 1, or GN-2002B-SV-78 or GS-2005A-DD-96. We recommend that this reference to the Program ID be made in the acknowledgement section at the end of the paper or in the Observations section of the paper.
Please acknowledge NSF-TSIP support by including the following in all publications relating to TSIP observing time (preferably as a footnote on the title page): “[Keck, MMT, or Magellan] telescope time was granted by NOAO, through the Telescope System Instrumentation Program (TSIP). TSIP is funded by NSF.” Observers should also note their NOAO proposal ID and observing dates in their publications either in the same footnote, or in the observations section or acknowledgments sections of their papers.
In addition for Keck time, please include the standard Keck acknowledgements at http://www2.keck.hawaii.edu/observing/keck_authors.html
Any publication that results from NOAO-allocated time on the 200-inch Hale telescope should acknowledge the NSF/NOAO ReSTAR program, in addition to a Hale/Palomar acknowledgment. The requested wording for ReSTAR acknowledgements is:
"This material is based upon work supported by AURA through the National Science Foundation under AURA Cooperative Agreement AST 0132798 as amended."