The Double Imaging Spectrometer (DIS) is a low-resolution optical spectrometer.[8]
KOSMOS, on long-term loan from NOIRLab, is a low-resolution optical spectrometer.
The Near Infrared Camera/Fabry–Pérot Spectrometer (NICFPS) was developed at theUniversity of Colorado. It uses a 1024 × 1024 H1RGHgCdTe infrared detector and a near-infraredFabry–Pérot interferometer. It has many narrow band filters, includingH2,[Fe II], and [SiVI]. It is unique among astronomical Fabry-Pérot devices in that it is cooled withliquid nitrogen.[9]
The Astrophysical Research Consortium Telescope Imaging Camera (ARCTIC) is an optical imaging instrument with a 4096 × 4096 pixel CCD.[10]
TripleSpec (Tspec) is a near infrared spectrograph which provides continuous wavelength coverage over the range 0.94–2.46 μm at moderate resolution (, depending on the choice of slit).[11]
Agile is a high-speed imager with a 1024 × 1024 frame transfer CCD.[citation needed]
The 3.5 m telescope is also used by theApache Point Observatory Lunar Laser-ranging Operation (APOLLO) lunar-ranging project. The APOLLO laser has been operational since October 2005, and routinely accomplishes millimeter-level range accuracy between the Earth and the Moon.[12][13]
Observations using the 3.5 m telescope can be carried out remotely by observers using TUI, the Telescope User Interface, via the internet.[14]
The SDSS 2.5 m (98 in) telescope is used for theSloan Digital Sky Survey, and began operating in 2000. It is a Ritchey-Chretien reflector on an alt-azimuth mount housed under a roll-off enclosure. It was designed with an unusually large 3°field of view to better support its primary task ofsurveying the entire sky.[15]
The NMSU 1.0 m (39 in) telescope is a Ritchey-Chretien reflector set on an alt-azimuth mount, and was completed in 1994.[16][17] A 2048 × 2048 CCD mounted at theNasmyth focus provides at 15.7-arcminute view of the sky.[18]
The ARC Small Aperture Telescope (ARCSAT) was previously called the Photometric Telescope (PT) when it was part of the SDSS project. It is a 0.5 m (20 in) reflecting telescope on anequatorial mount, with a single CCD camera cooled by a CryoTiger unit.[19] It was built in 1991, moved from its previous location in 1998, and used by the SDSS until 2005.[20] It is currently used for small research projects.
A 0.6 m (24 in) reflecting telescope was built in 1993 to monitor sky conditions for the SDSS project. It never operated in a satisfactory manner, and was replaced with the 0.5 m PT.[20]
^"Annual Reports of Astronomical Observatories and Departments: Apache Point Observatory, Astrophysical Research Consortium".Bulletin of the American Astronomical Society.24: 17. 1992.Bibcode:1992BAAS...24...17.
^York, D. G. (1994). "University of Chicago, Apache Point Observatory/Department of Astronomy and Astrophysics, Chicago, Illinois 60637".Bulletin of the Astronomical Society.26 (1): 58.Bibcode:1994BAAS...26...58Y.
^"Annual Reports of Astronomical Observatories and Departments: Astrophysical Research Consortium, Apache Point Observatory".Bulletin of the American Astronomical Society.27: 9. 1995.Bibcode:1995BAAS...27....9.