Call for Proposals for the NASA Infrared Telescope Facility

DEADLINE: Monday 01 October 2018

NASA Infrared Telescope Facility Observing Proposals. The due date for the 2019A semester (February 1, 2019 to July 31, 2019) is Monday, October 1, 2018. See our online submission form, which is available for proposal submission from 12:00AM on September 01, 2018 until 5:00PM on October 01, 2018 HST. The deadline on a world clock listing is available here.

Available facility instruments include:

(1) SpeX, a 0.7 – 5.3 micron cross-dispersed medium-resolution spectrograph (up to R=2,500) and imager. The 0.8 micron cut-on dichroic was replaced with a 0.7 micron dichroic during semester 2017A. This will increase the spectral wavelength grasp for optically guided solar system targets. Sub-arrays and movie mode are working again in the IR guider. Electronic observing logs are now automatically generated.

(2) MORIS, a 512x512 pixel Andor CCD camera (60"x60" field-of-view) mounted at the side-facing window of the SpeX cryostat that can be used simultaneously with SpeX. Electronic observing logs are now automatically generated.

(3) iSHELL, a 1.06 – 5.3 micron cross-dispersed echelle spectrograph (up to R=75,000) and imager. Wedged order-sorting filters are being procured to remove slight fringing in the spectra. We expect to install new filters covering the K-, L- and M-band modes in early 2019A, during which time iSHELL will be unavailable for one month. For semester 2019A we are again limiting the number of proposals requiring radial velocity precisions less than about 100 m/s since the results from commissioning runs are still being analyzed and the limiting precision is not yet know. The data reduction tool for iSHELL is now available; it is part of the Spextool package. We have developed a version of xtellcor that uses atmospheric models instead of standard stars to remove telluric absorption lines in iSHELL spectra. For now we recommend that observers still take standard stars until they have compared both methods. For more details see http://irtfweb.ifa.hawaii.edu/research/dr_resources.

(4) MIRSI/MOC, a 5 – 20 micron camera and grism spectrograph. MIRSI was recently upgraded by IR Labs with a closed-cycle cooler to replace its liquid nitrogen and liquid helium cryostat. It is currently being further refurbished by IRTF with a new array controller and an optical channel similar to MORIS (MOC) with a 60"x60" field-of-view. For 2019A we are offering MIRSI and MOC in shared risk mode. . A new chopping secondary mirror should also be available for use with MIRSI. Remote observing will be available with MIRSI and MOC.

Information on available instruments and performance can be found at: http://irtfweb.ifa.hawaii.edu/instruments. Exposure time calculators for SpeX and iSHELL are available on the respective instrument webpages.

PI-led visitor instruments (available on a collaborative basis with the instrument team) include: TEXES (5-20 micron high-resolution spectrograph; contact Tommy Greathouse at tgreathouse@swri.edu for more information), BASS (3-14 micron spectrometer; contact Jon Mauerhan at jon.c.mauerhan@aero.org for more information), and HIPWAC (7-17 micron heterodyne spectrograph; contact Tim Livengood at timothy.a.livengood@nasa.gov for more information).

Following feedback from the IRTF TAC, investigators are asked to make a clear statement about the connection between the proposed observations and the overall science goal. It is important to concisely articulate the big science picture. Be specific about the number of targets needed, and for continuing proposals, what is needed for the program to be considered complete. Figures need to be legible - no small print. Target visibility plots are not required. We encourage proposals that will provide data for thesis work. The student should be listed as PI or at least as Co-I. You will be asked to provide details of the thesis on the proposal form including the anticipated year of graduation.

Investigators are reminded that any significant changes to the TAC approved observing program must be pre-approved by the IRTF Director.

Observers may apply for Target of Opportunity (ToO) programs on IRTF, but the total time that can be allocated to ToO programs is 12 hours for Solar System and 12 hours for non-Solar System proposals. Each ToO interrupt is limited to 3 hours length. The proposal must clearly define the criteria by which a ToO interrupt would be initiated. Time for ToO interrupts will be taken from scheduled, non-time critical observing programs. Programs affected by ToO interrupts will be offered make-up time from Director Discretionary Time (engineering time) when possible.

Remote observing is available with SpeX, MORIS, and iSHELL. Requests for remote observing must be made in the proposal application – later requests will be considered if requested at least one month ahead of time. If you wish to observe from your home institution, you must comply with the requirements for video conferencing and instrument operation provided on the Remote Observers Information page. (A working three-button mouse is required.) Observers are strongly encouraged to contact Miranda Hawarden-Ogata (hawarden@hawaii.edu) to set up a test of the video link and user interface at least one month prior to their observing run. We cannot guarantee a successful remote observing connection on short notice since we have no control of hardware and software compatibility on the user’s side. It is the responsibility of the PI to provide up to date observing contact information through submission of the online Observing Requirements Form (ORF).

To keep our bibliography up to date, and to ensure future funding of the IRTF, we ask that you send us citations to your latest IRTF publications. You can check your publications using our website bibliography page for refereed papers:

http://irtfweb.ifa.hawaii.edu/research/biblio/publications.php

Please send any missing references to Bobby Bus (sjb@ifa.hawaii.edu), and please continue to include in your paper the acknowledgement to the IRTF and the name of the instrument used as described at:

http://irtfweb.ifa.hawaii.edu/research/acknowledge.php

We are in the process of compiling a list of PhD Dissertations that have utilized observations obtained with the IRTF. If you (or your student) has written a dissertation based on IRTF data that is not yet included in this list, please send the appropriate information (including a web link to the dissertation, if possible) to Bobby Bus (sjb@ifa.hawaii.edu):

http://irtfweb.ifa.hawaii.edu/research/biblio/dissertations.html

The IRTF Data archive is now open for use, and is being hosted by the NASA/IPAC Infrared Science Archive (IRSA) at: https//irsa.ipac.caltech.edu/Missions/irtf.html. Raw data files taken with SpeX beginning Aug. 1, 2016, and with iSHELL beginning Feb. 1, 2017, are now publicly available via this site after a proprietary period of 18 months from the date of observation. As part of the archive process, the abstract field on the observing proposal form is being preserved and provided as metadata when data files are searched for or downloaded from the archive.

On Dec. 1, 2017 we announced that IRTF data for the years 2001 to 2016 would be made available on request following a proprietary period of 18 months, i.e. ‘legacy’ data will be available from June 1, 2019. It is planned that starting in June 2019, IRTF legacy data will be searchable via a web page, and data will be downloadable via a script generated by the webserver.