D. Toomey | Semantic Scholar
SpeX: A Medium‐Resolution 0.8–5.5 Micron Spectrograph and Imager for the NASA Infrared Telescope Facility
- John T. RaynerD. Toomey S. Wang
- 1 March 2003
Physics, Engineering
We present the design, construction, and performance of SpeX, a medium‐resolution 0.8–5.5 μm cryogenic spectrograph and imager, now in operation at the 3.0 m NASA Infrared Telescope Facility (IRTF)…
SpeX: a medium-resolution IR spectrograph for IRTF
- J. RaynerD. Toomey Shu-i Wang
- 21 August 1998
Physics, Engineering
SpeX is a medium-resolution 0.8-5.5 micrometers cryogenic spectrograph being built at the Institute for Astronomy, University of Hawaii, for the NASA IR Telescope Facility on Mauna Kea. SpeX was…
A Redetermination of the Mass of Procyon
- T. GirardH. Wu D. Pourbaix
- 1 May 2000
Physics
The parallax and astrometric orbit of Procyon have been redetermined from PDS measurements of over 250 photographic plates spanning 83 years, with roughly 600 exposures used in the solution. These…
CSHELL: a high spectral resolution 1-5-μm cryogenic echelle spectrograph for the IRTF
- T. GreeneA. TokunagaD. ToomeyJ. Carr
- 20 October 1993
Physics, Engineering
Defense, Security, and Sensing
A 1 - 5.4 micrometers Cryogenic Echelle Spectrograph (CSHELL) for the NASA Infrared Telescope Facility is described. It achieves a resolving power of 5,000 to 40,000 using slits ranging from 4.0' to…
Design for a 1--5-um cryogenic echelle spectrograph for the NASA IRTF
- A. TokunagaD. ToomeyJ. CarrD. HallH. Epps
- 1 July 1990
Physics, Engineering
The design of an infrared cryogenic echelle spectrograph for use on the NASA Infrared Telescope Facility is described. The resolving power achieved over the range 1-5.4 microns is 1-40,000 with slit…
THE GEMINI/NICI PLANET-FINDING CAMPAIGN: THE FREQUENCY OF PLANETS AROUND YOUNG MOVING GROUP STARS
- B. BillerMichael C. Liu D. Toomey
- 5 September 2013
Physics
We report results of a direct imaging survey for giant planets around 80 members of the β Pic, TW Hya, Tucana-Horologium, AB Dor, and Hercules-Lyra moving groups, observed as part of the Gemini/NICI…
NSFCAM: a new infrared array camera for the NASA Infrared Telescope Facility
- M. ShureD. ToomeyJ. RaynerP. OnakaA. Denault
- 1 December 1993
Physics, Engineering
We have just recently commissioned a new 1.0-5.5 micrometers IR array camera for the NASA IR Telescope Facility based upon the Santa Barbara Research Center 256x256 InSb array. The primary features…
Revised Fluxes for Gliese 229B
- S. LeggettD. ToomeyT. GeballeR. H. Brown
- 28 March 1999
Physics
We have used the coronagraphic instrument CoCo with the Infrared Telescope Facility's camera, NSFCAM, to obtain improved photometry at JHKL' of the giant planet/brown dwarf Gliese 229B. We have…
THE GEMINI NICI PLANET-FINDING CAMPAIGN: DISCOVERY OF A CLOSE SUBSTELLAR COMPANION TO THE YOUNG DEBRIS DISK STAR PZ Tel
- B. BillerMichael C. Liu D. Toomey
- 27 July 2010
Physics
We report the discovery of a tight substellar companion to the young solar analog PZ Tel, a member of the β Pic moving group observed with high-contrast adaptive optics imaging as part of the Gemini…
THE GEMINI NICI PLANET-FINDING CAMPAIGN: THE FREQUENCY OF GIANT PLANETS AROUND YOUNG B AND A STARS
- E. NielsenMichael C. Liu D. Toomey
- 1 June 2013
Physics
We have carried out high contrast imaging of 70 young, nearby B and A stars to search for brown dwarf and planetary companions as part of the Gemini NICI Planet-Finding Campaign. Our survey…