Technical Details of the KOSMA telescope (2000)
Technical Details of the KOSMA telescope (2000)
Telescope Type : Cassegrain f-ratio : 10.4 Focal length : 31.2 m Mount : altitude-azimuth Observing ports : 2 Nasmyth foci Max. slew rate : 1 Degree/s Elevation limits : 0-90 Degree Pointing accuracy : 10" Primary reflector parameters Diameter : 3m Shape : parabolic f-ratio : 0.43 Construction : 18 aluminum panels, backstructure CFRP framework Surface accuracy : 5 micron rms (each panel) 20-30 micron rms (telescope) Alignment : actuator at each panel corner Secondary reflector parameters Diameter : 27 cm Shape : hyperbolic Surface : 4 micron rms Construction : aluminum Alignment : 3 linear and 2 angular degrees of freedom with a hexapod Chopper : wobble mechanism in cross-elevation, larger than +-3 arcmin on sky, 4 Hz max. Receiver Dual-channel-SIS receiver Summer Configuration : 230 GHz/345 GHz Winter Configuration : 345 GHz/660 GHz Tuning ranges Receiver Noise Temperature (DSB) [GHz] [K] 210 - 270 150 330 - 365 100 436 - 495 90 - 120 630 - 690 210 780 - 820 800 - 1100 All receivers have an IF of 1.4 GHz with a bandwith of 1 GHz Spectrometer LRS = Low Resolution Acousto-optical Spectrometer MRS = Medium Resolution Acousto-optical Spectrometer HRS = High Resolution Acousto-optical Spectrometer VRS = Variable Resolution Acousto-optical Spectrometer Channels Bandwidth Channel Spacing Reception Resolution Bandwidth Bandwidth [MHz] [kHz] [kHz] [kHz] LRS 1450 1000 688 1800 1150 MRS 1800 300 167 560 360 HRS 2048 59 29 79 53 VRS max. 2048 655-1100 320-700 800-1600 550-1100 For Efficiencies and Beamwidths see here
KOSMA Observing Schedule
References with information about the Observatory
- The University of Cologne 3-m radio telescope. Winnewisser et al. 1986, Astronomy and Astrophysics 167, 207
- CO submillimeter observations from Gornergrat. Winnewisser et al. 1990, Astronomy and Astrophysics 230, 248
- The new KOSMA 3m Telescope. Kramer et al. 1998, In: Proc. SPIE Vol. 3357
- Surveys with the new KOSMA telescope. Kramer et al. 1999, In: "Imaging at Radio through Submillimeter Wavelengths", J. Mangum (ed.), PASP, Tucson/Arizona
