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MRSP - The Muenster Redshift Project

Published online by Cambridge University Press:  03 August 2017

P Schuecker ,
H Horstmann  and
W Seitter
P Schuecker
Affiliation:
Astronomical Institute of Muenster University, F.R.G.
H Horstmann
Affiliation:
Astronomical Institute of Muenster University, F.R.G.
W Seitter
Affiliation:
Astronomical Institute of Muenster University, F.R.G.

Extract

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ESO/SRC-J-Atlas plates (film copies) and film copies of UK-Schmidt objective prism J-plates (dispersion 246nm/mm at Hγ) were scanned with the microdensitometer PDS 2020 GM and reduced automatically with the software package ADAS developed at the Astronomical Institute of Muenster University. In a single field (30 square degrees) near the South Galactic Pole 150 000 objects are found up to the limiting magnitude Stars and galaxies are separated. Algorithms for quasar search among the star-like objects are applied and radial velocities determined from the identified emission lines. Follow-up observations with the ESO 3.6m telescope show fair agreement between the redshifts determined from the objective prism plate and from the slit spectra.

Type
Appendix 1: Poster Papers
Information
Symposium - International Astronomical Union , Volume 130: Large Scale Structures of the Universe , 1988 , pp. 526 - 527
Copyright
Copyright © Reidel 1988 

References

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