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Wide-Angle Near-Infrared Surveys of Local Galaxies

  • Bahram Mobasher
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 230)

Abstract

Recently, it has become possible to perform wide-angle galaxy surveys at near-infrared (2.2µm) wavelengths. Such surveys cover limited areas to magnitude limits similar or fainter than that achieved by the DENIS or 2MASS projects. Therefore, the resulting number-magnitude counts can be used to calibrate these datasets. Also, due to the relatively bright magnitude limit of these wide-angle surveys, spectroscopic observations are straightforward and hence, one could construct the local near-ir luminosity function (LF) of galaxies. This could be used to predict the space density of galaxies expected from DENIS or 2MASS, providing reliable control samples for these larger studies.

Keywords

Luminosity Function Spectroscopic Observation Space Density Magnitude Limit Redshift Distribution 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Cowie, L. L., Songaila, A., Hu, E. M., Cohen, J. G. 1996, Astron.J. 112, 839ADSCrossRefGoogle Scholar
  2. Djorgovski, S. et al. 1995, Ap.J., 438, L13ADSCrossRefGoogle Scholar
  3. Efstathiou, G.; Ellis, R. S.; Peterson, B. A. 1988, MNRAS, 232, 431ADSGoogle Scholar
  4. Egami, E.; Hu, E; Cowie, L.L 1996 Ap.J. 112, 73Google Scholar
  5. Gardner, J. P., Sharples, R. M., Carrasco, B. E., Frenk, C. S. 1997, Ap.JL 480, L99ADSCrossRefGoogle Scholar
  6. Glazebrook, K., Peacock, J. A., Collins, C. A. and Miller, L. 1994, MNRAS 266, 65ADSGoogle Scholar
  7. Huang, J. S., Cowie, L. L., Gardner, J. P., Hu, E. M., Songaila, A., Wainscoat, R. J., 1997, Ap.J. 476, 12ADSCrossRefGoogle Scholar
  8. Lynden-Bell, D., 1971, MNRAS, 155, 95ADSGoogle Scholar
  9. Mobasher, B., Ellis, R. S. and Sharples, R. M. 1986, MNRAS 223, 11ADSGoogle Scholar
  10. McLeod, B.A., Bernstein, G.M., Reike, M.J., Tollestrup, E.V. & Fazio, G.G. 1995. Ap.JS 96, 117ADSCrossRefGoogle Scholar
  11. Moustakas, L.A., Davies, M., Graham, J.R., Silk, J., Peterson, B.A. & Yoshii, Y. 1997, Ap.J. 475, 44ADSCrossRefGoogle Scholar
  12. Sandage, A., Tammann, G.A., & Yahil, A., 1979, Ap.J. 232, 352.ADSCrossRefGoogle Scholar
  13. Saracco, P., Iovino, A., Garilli, B., Maccagni, D. & Chincarini, G. 1997, AJ. 114, 887ADSCrossRefGoogle Scholar
  14. SubbaRao, M.U., Connolly, A.J., Szalay, A.S. & Koo, D. C. AJ. 112, 929Google Scholar
  15. Szokoly, G.P., Subbarao, M. U., Connolly, A.J. & Mobasher, B. 1998, Ap.J. 492 (in press)Google Scholar

Copyright information

© Springer Science+Business Media Dordrecht 1998

Authors and Affiliations

  • Bahram Mobasher
    • 1
  1. 1.Astrophysics GroupBlackett Laboratory, Imperial CollegeLondonUK

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