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The Optical Extragalactic Background Light from Resolved Galaxies

Published online by Cambridge University Press:  13 May 2016

Lucia Pozzetti  and
Piero Madau
Lucia Pozzetti
Affiliation:
Osservatorio Astronomico di Bologna, Via Ranzani 1, Bologna, I-40127, Italy
Piero Madau
Affiliation:
Department of Astronomy and Astrophysics, University of California, Santa Cruz, 95064, USA

Abstract

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We discuss the ultraviolet to near-IR galaxy counts from the deepest imaging surveys, including the northern and southern Hubble Deep Fields. The logarithmic slope of the galaxy number-magnitude relation is flatter than 0.4 in all seven UBVIJHK optical passbands at faint magnitudes, i.e. the light from resolved galaxies has converged from the UV to the near-IR. Most of the galaxy contribution to the extragalactic background light (BEL) comes from relatively bright, low-redshift objects (50% at VAB ≲ 21 and 90% at VAB ≲ 25.5). We find a lower limit to the surface brightness of the optical EBL of about 15 nW m−2 sr−1, comparable to the intensity of the far-IR background from COBE data. Diffuse light, lost because of surface brightness selection effects, may add substantially to the EBL.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 204: The Extragalactic Infrared Background and its Cosmological Implication , 2001 , pp. 71 - 85
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

Adelberger, K.L., & Steidel, C.C. 2000, ApJ, in press.Google Scholar
Armand, C., Milliard, B., & Deharveng, J.-M. 1994, A&A, 284, 12 Google Scholar
Bernstein, R. A., 1999, in the Low Surface Brightness Universe, ASP Conference Series 170, ed. Davies, J. I., Impey, C., and Phillipps, S., 341 Google Scholar
Bernstein, R. A., Freedman, W. L., & Madore, B. F. 2000, submitted.Google Scholar
Bowyer, S., 1991, ARA&A, 29, 59 Google Scholar
Bruzual, A. C., & Charlot, S. 1993, ApJ, 405, 538 CrossRefGoogle Scholar
Cimatti, A., et al. 1999, A&A, 352, L45 Google Scholar
Connolly, A.J., Szalay, A.S., Dickinson, M., SubbaRao, M.U., Brunner, R.J., 1997, ApJ, 486, L11 CrossRefGoogle Scholar
Daddi, E., Cimatti, A., Pozzetti, L., et al. 2000, A&A 361, 535 Google Scholar
Dube, R.R., Wickes, W.W., Wilkinson, D.T., 1979, ApJ, 232, 333 CrossRefGoogle Scholar
Dwek, E., & Arendt, R. G. 1998, ApJ, 508, L9 Google Scholar
Dwek, E., et al. 1998, ApJ, 508, 106 CrossRefGoogle Scholar
Elbaz, D., et al. 1999, A&A, 351, L37 Google Scholar
Ellis, R. S., Colless, M., Broadhurst, T., Heyl, J., & Glazebrook, K. 1996, MNRAS, 280, 235 Google Scholar
Ferguson, H.C., & Babul, A. 1998, MNRAS, 296, 585 Google Scholar
Finkbeiner, D. P., Davis, M., Schlegel, D. 2000, this volume.Google Scholar
Fixsen, D. J., et al. 1998, ApJ, 508, 123 Google Scholar
Fukugita, M., Hogan, C. J., & Peebles, P. J. E. 1998, ApJ, 503, 518 CrossRefGoogle Scholar
Gallego, J., Zamorano, J., Aragon-Salamanca, A., Rego, M. 1995, ApJ, 455, L1 Google Scholar
Gardner, J.P., Brown, T.M., & Ferguson, H.C. 2000, ApJ, 542, L19 CrossRefGoogle Scholar
Gardner, J.P., Sharpies, R.M., Frenk, C.S., Carrasco, B.E. 1997, ApJ, 480, L99 CrossRefGoogle Scholar
Gispert, R., Lagache, G., Puget, J.L. 2000, A&A 361, 1 Google Scholar
Glazebrook, K., Blake, C., Economou, F., Lilly, S., Colless, M. 1999, MNRAS, 308, 459 Google Scholar
Gorjian, V., Wright, E.L., Chary, R.R. 2000, ApJ, 536, 500 Google Scholar
Hasinger, G. 2000, in the ESO Deep Fields Workshop, Munich 2000 Google Scholar
Hauser, M. G., et al. 1998, ApJ, 508, 25 Google Scholar
Hu, E.M., & Ridgway, S. E., 1994, AJ 107, 1303 Google Scholar
Hughes, D., et al. 1998 Nature, 398, 241 Google Scholar
Lagache, G., Abergel, A., Boulanger, F., Desert, F. X., & Puget, J.-L. 1999, A&A, 344, 322 Google Scholar
Lagache, G.G., Haffner, L.M., Reynolds, R.J., Tufte, S.L. 2000, A&A 354, 247 Google Scholar
Lilly, S.J., Le Fevre, O., Hammer, F., Crampton, D. 1996, ApJ, 460, L1 Google Scholar
Madau, P., Ferguson, H.C., Dickinson, M.E., Giavalisco, M., Steidel, C.C., Fruchter, A. 1996, MNRAS, 283, 1388 Google Scholar
Madau, P. 1999, in After the Dark Ages: When Galaxies were Young (the Universe at 2<z<5), eds. Holt, S. and Smith, E. (AIP Press), 299 Google Scholar
Madau, P., Pozzetti, L., & Dickinson, M. 1998, ApJ, 498, 106 Google Scholar
Madau, P., & Pozzetti, L., 2000, MNRAS, 312, L9 CrossRefGoogle Scholar
McCracken, H.J., Metcalfe, N., Shanks, T., Campos, A., Gardner, J.P., 2000, MNRAS, 311, 707 CrossRefGoogle Scholar
Moriondo, G., Cimatti, A., Daddi, E. 2000, A&A, in press.Google Scholar
Pozzetti, L., Madau, P., Zamorani, G., Ferguson, H. C., & Bruzual, A. G. 1998, MNRAS, 298, 1133 Google Scholar
Puget, J.-L., Abergel, A., Bernard, J.-P., Boulanger, F., Burton, W. B., Desert, F.-X., & Hartmann, D. 1996, A&A, 308, L5 Google Scholar
Soifer, B.T., & Neugebauer, G. 1991, ApJ, 101, 354 Google Scholar
Somerville, R. S., Primack, J. R., 1999, MNRAS, 310, 1087 Google Scholar
Steidel, C.C., Adelberger, K.L., Giavalisco, M., Dickinson, M., Pettini, M. 1999, ApJ, 519, 1 CrossRefGoogle Scholar
Steidel, C.C., Giavalisco, M., Pettini, M., Dickinson, M.E., & Adelberger, K. 1996, ApJ, 462, L17 CrossRefGoogle Scholar
Toller, G.N., 1983, ApJ, 266, L79 Google Scholar
Totani, T., Yoshii, Y. 2000, ApJ, 540, 81 CrossRefGoogle Scholar
Tresse, L., & Maddox, S. J. 1998, ApJ, 495, 691 Google Scholar
Treyer, M.A., et al. 1998, MNRAS, 300, 303 Google Scholar
Vaisanen, P., & Tollestrup, E.V. 1999, in the Low Surface Brightness Universe, ASP Conference Series 170, eds. Davies, J.I., Impey, C., and Phillipps, S., 365 Google Scholar
Volonteri, M., Saracco, P., Chincarini, G., Bolozonella, M. 2000, A&A 362, 487 Google Scholar
Vogeley, M. S. 1997, AAS, 191, 304 Google Scholar
Williams, R. E., et al. 1996, AJ, 112, 1335 Google Scholar
Wright, E.L. 2000, in press (astro-ph/0004192).Google Scholar
Yoshii, Y. 1993, ApJ, 403, 552 Google Scholar