Unless otherwise noted, images should be credited to Fermilab Visual Media Services. Click on any of the links below to download a larger version of the image thumbnails.
This is the bottom of the 2.5-meter survey telescope, where the instrument package (either mosaic camera or spectrograph) is mounted.
Looking inside the base of the 2.5-meter survey telescope. The stack of rings sits just above the primary mirror and serves to shield the instruments below from stray light.
The SDSS survey telescope stands out against the breaktaking backdrop of the Sacramento Mountains.
The telescope enclosure building (above) and instrument room (below) jut out from the mountainside. The SDSS telescope facility was designed this way to provide the calmest and coldest possible air above and around the survey telescope.
A look down inside the 2.5-meter survey telescope reveals the primary mirror (the reflective surface at the bottom) as well as the secondary mirror (center), all surrounded by the wind baffle.
This photo shows the two-story enclosure building for the 2.5-meter telescope.
In the foreground is the dome for the photometric telescope. The enclosure for the 2.5-meter survey telescope is in the background.
The 2.5-meter diameter primary mirror of the SDSS telescope. This photo was taken with the telescope horizontally on its side, pointing into the trees.
The SDSS 2.5-meter telescope.
A half-moon (left) rises over the SDSS and APO telescopes in the Sacramento Mountains.
This photo shows the two-story enclosure building for the 2.5-meter telescope. The staircase in the foreground leads to the photometric telescope.
The SDSS 2.5-meter telescope is shown here, framed by the staircase and support beams for the photometric telescope building.
(Image credit: Reidar Hahn, Fermilab)
SDSS Project Director John Peoples with the 2.5-meter Survey telescope in the background.
(Image credit: Reidar Hahn, Fermilab)
SDSS Project Director John Peoples poses at sunset in front of the 2.5-meter Survey telescope, located at Apache Point Observatory in New Mexico.
(Image credit: Dan Long, Apache Point Observatory)
Constance Rockosi, a graduate student at the University of Chicago and a member of the multi-institutional team that built the digital scanning camera for the Sloan Digital Sky Survey, checks the status of the instrument during its first on-the-sky trial runs in May 1998.
The 2.5-meter reflecting telescope of the Sloan Digital Sky Survey. The box-like structure protects the separately mounted telescope from being buffeted by the wind.
Apache Point Observatory in the Sacramento Mountains of New Mexico. The Sloan Digital Sky Survey's 2.5-meter telescope is on the left. White Sands National Monument is visible in the distance, above the telescope. The monitor telescope, used for calibrations, is inside the small dome to the right of center. Optical fibers for spectroscopy are pre-positioned each day in the building on the right (behind the trees). The building in the center rolls on rails to cover the 2.5-meter telescope when i t is not in use.
A photo of the 2.5-meter SDSS telescope, with its wind baffle.
A view of the dome for the 0.6-meter photometric telescope.
A view of the 2.5-meter telescope inside the wind baffle, looking up toward the secondary mirror.
The secondary mirror of the 2.5-meter telescope.
Connie Rockosi, examining the instrument package on the base of the 2.5-meter survey telescope.
Inside the control room.
Bruce Gillespie at the Apache Point Observatory.
Members of the SDSS collaboration from Fermilab unfurl the 30 foot image of the sky from the 2.5-meter telescope's first light.
(Image credit: Fred Ullrich, Fermilab)
The mount (left), for the Sloan Digital Sky Survey's 2.5-meter telescope at the Apache Point Observatory in the Sacramento Mountains of New Mexico. The telescope will achieve first light in May 1998. The garage-like structure in the foreground rol ls forward to cover the telescope when it is not in use. At right is the Sky Survey's monitor telescope.
Astrophysicist Rich Kron, of the University of Chicago and Fermilab, inserts optical fibers into a pre-drilled "plug-plate," part of the Sloan Digital Sky Survey's unique spectrographic system for determining the distances to stars, galaxies and qu asars.
(Image credit: Thomas Nash)
This is a view of a plug plate that's been drilled, fitted with optical fibers, and mounted on the spectograph assembly. This entire package will be flipped upside down and mounted to the underside of the 2.5-meter telescope at its focal plane.
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