Apache Point Observatory

Apache Point Observatory

File:Apache Point Observatory.jpg Site operations of the Apache Point Observatory.
Alternative names	APO
Organization	Astrophysical Research Consortium
Observatory code	705, 645
Location	Sunspot, New Mexico, USA
Coordinates	32°46′49″N 105°49′13″W
Altitude	2,788 m (9,147 ft)
Established	1998
Website	[1]
Telescopes
Astrophysical Research Consortium telescope 3.5 m reflector Sloan Digital Sky Survey telescope 2.5 m reflector New Mexico State University telescope 1 m reflector
Location of Apache Point Observatory
Related media on Commons

The Apache Point Observatory is located in the Sacramento Mountains in Sunspot, New Mexico (USA) 18 miles south of Cloudcroft. The observatory consists of the Astrophysical Research Consortium's 3.5-meter telescope, the Sloan Digital Sky Survey 2.5-m telescope with a 20" photometric telescope, and New Mexico State University's 1.0-m telescope. Access to the telescopes and buildings is restricted, but the public is welcomed to stroll the grounds. The visitor's center at Sun Spot (the National Solar Observatory) includes a model of Apache Point's 3.5 meter telescope and actual filter plates for the Sloan telescope.

The 3.5 m telescope hosts the 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.

Observations at APO are often carried out remotely by observers using TUI, the Telescope User Interface, via the internet.

Instruments

There are a variety of optical and near-infrared instruments at APO.

NICFPS

The Near Infrared Camera/Fabry–Pérot Spectrometer was developed at the University of Colorado. It uses a 1024x1024 H1RG HgCdTe infrared detector and a near-infrared Fabry–Pérot interferometer. It has many narrow band filters, including H2, [Fe II], and [SiVI]. It is unique among astronomical Fabry-Perot devices in that it is cooled with liquid nitrogen.

DIS

The Double Imaging Spectrometer is a low-resolution optical spectrometer.

Echelle

The echelle spectrometer at APO uses a 2048 x 2048 pixel CCD and has a resolution of 30,000.

SPIcam

The Seaver Prototype Imaging camera is an optical imaging instrument with a 2048x2048 pixel CCD.

Photometric telescope

The Photometric Telescope, or PT, is an (usually) automated telescope used by the Sloan Digital Sky Survey (SDSS). The telescope is a 20" reflector telescope with a single CCD camera, cooled by a CryoTiger unit.

During normal operations of the SDSS 2.5m telescope the PT is under automated control. While the SDSS obtains photometric or spectroscopic data, the PT will image patches of the sky that lie along the drift paths of the SDSS. These patches are used to calibrate the SDSS data, correcting for nightly atmospheric extinction as well as calibrating the data to the ugriz photometric system zero points. This process is required because while the ugriz system is tied to USNO standard stars, the SDSS cannot image directly these stars because they are too bright. Instead the PT records transfer patches which are compared to SDSS data.

The PT uses u'g'r'i'z' filters. These filters were intended to be identical to the SDSS ugriz, however physical differences do exist. Works is ongoing to accurately tie the PT to the SDSS, which is important for the future use of SDSS.

See also

• List of observatories, including a nearby solar observatory

References

1. "Apache Point Observatory Homepage". APO Home Page. Retrieved November 14, 2007.

Further reading

• Holtzman, Jon; et al. (2009-03-15). Apache Point Observatory: Facilities, Operations, and Partnerships. Astro2010: The Astronomy and Astrophysics Decadal Survey publisher=National Academies (Report). Retrieved 2009-08-14. {{cite report}}: Explicit use of et al. in: |last= (help); Missing pipe in: |work= (help)

External links

• Apache Point Clear Sky Clock Weather forecasts for observing conditions.