Hostname: page-component-cc8bf7c57-ksm4s Total loading time: 0 Render date: 2024-12-12T05:02:24.698Z Has data issue: false hasContentIssue false
  • English
  • Français

ABRIXAS

Published online by Cambridge University Press:  25 May 2016

G. Hasinger ,
J. Trümper  and
R. Staubert
G. Hasinger
Affiliation:
Astrophysikalisches Institut, D-14482 Potsdam
J. Trümper
Affiliation:
Max-Planck-Inst. f. extrat. Physik, D-85740 Garching
R. Staubert
Affiliation:
Institut für Astronomie und Astrophysik, Astronomie, D-72076 Tűbingen

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

All Sky Surveys are very useful for several reasons: Firstly, their unbiased view provides the potential for new discoveries. Secondly, they yield large unbiased samples of a variety of objects which can be used for statistical investigations. And thirdly, the unlimited field of view of telescopic sky surveys allows to study extended objects and large scale structures.

Type
Session 2: Future Space Programs
Information
Symposium - International Astronomical Union , Volume 188: The Hot Universe , 1998 , pp. 83 - 86
Copyright
Copyright © Kluwer 1998 

References

Comastri, A., Setti, G., Zamorani, G., Hasinger, G. 1995, A&A 296, 1 Google Scholar
Döhring, T., Friedrich, P., Aschenbach, B., et al., 1998, AN 319, in press CrossRefGoogle Scholar
Friedrich, P., Hasinger, G., Richter, G., et al., 1996, MPE report 263, 681 Google Scholar
Matt, G., Fabian, A.C., 1994, MNRAS 267, 187 CrossRefGoogle Scholar
Trümper, J.E., Hasinger, G., Staubert, R., 1998, AN 319, in press CrossRefGoogle Scholar