... are coupled to images formed by the SDSS 2.5-m telescope by 640 optical fibers ... to manufacture (SDSST TN19961022, 2.5-m telescope spectrographic optical design ... CMM) with an accuracy specified at +/-2.5 ?m (0.0001") was used for the measurements ...
... Support and adjustment of the SDSS 2.5-m telescope conical baffle . Contents . ... The Sloan Digital Sky Survey (SDSS) 2.5-m telescope is based on a wide-field fast ...
... Plate uw0111 uw0112 (?m) (?m) Points 3 3 Mean x 28.3 21.5 Mean y -2.5 -3.4 Mean t 8.9 22.7 Std Deviation r 26.4 17.2 Std Deviation t 23.4 20.4 . ...
... LOG . MAXV vel ( * ) . MAXVEL vel ( * ) . M [pos [vel [time]]] ( * ) . MOVE . MOVE pos ( * ) . MOVE pos vel ( * ) . ... Alias: MAXV . Sets the maximum allowed velocity. Alias: M . Stops the axis at the current position (overshoots and returns). ...
... Conference Proceedings, 2002 Page 17 of 32 Revised 4/11/07 Bowen, D. V., Tripp, T. M., Jenkins, E. B., Brinks, E., and Huchtmeier, W., "Damped Lyman-alpha Absorption from the Nearby Low Surface Brightness Galaxy SBS 1543+593: A Summary", 2002 ...
... A better value for this effect for the 3.5 m telescope main axes should be available in the near future. ... mas RMS) Az axis wobble Drive disk high freq. error 200 17.17 Guide roller error 50 8.58 Lower bearing high freq./nonrep. error ...
... H) x 4112(V) 15 µm square 61.4 mm x 61.4 mm 4 63.0 x 69.0 mm silicon carbide with two Package format flexi connectors Focal plane height, above base 15.0 mm Height tolerance ±10 µm Connectors two 37-way micro-D Flatness <20 µm (peak to valley) Amplifier ...
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