Fig. 12 from Faint Galaxies in Deep Advanced Camera for Surveys Observations

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

Faint Galaxies in Deep Advanced Camera for Surveys Observations

Authors: N. Benítez, H. Ford, R. Bouwens, F. Menanteau, J. Blakeslee, C. Gronwall, G. Illingworth, G. Meurer, T. J. Broadhurst, M. Clampin, M. Franx, G. F. Hartig, D. Magee, M. Sirianni, D. R. Ardila, F. Bartko, R. A. Brown, C. J. Burrows, E. S. Cheng, N. J. G. Cross, P. D. Feldman, D. A. Golimowski, L. Infante, R. A. Kimble, J. E. Krist, M. P. Lesser, Z. Levay, A. R. Martel, G. K. Miley, M. Postman, P. Rosati, W. B. Sparks, H. D. Tran, Z. I. Tsvetanov, R. L. White, and W. Zheng

Benítez et al. 2004 The Astrophysical Journal Supplement Series 150 1.

Provider: AAS Journals

Caption: Fig. 12.

Fraction of galaxies detected for each of the filters vs. total magnitude. The thick line corresponds to the central region of the VV 29 field, and the thin line corresponds to the outer region of the VV 29 field plus the NGC 4676 field. Note that the X‐axis corresponds to the "total" intrinsic magnitudes.

Other Images in This Article

Copyright and Terms & Conditions