Abstract
The total mass distribution of the galaxy cluster CL0024+1654 from the measured source depletion due to lens magnification in the R band was estimated. The luminosity function of CL0024+1654 was computed to estimate the contamination of background source counts from the cluster galaxies. Results showed that the flux magnification effectively enabled to probe deeper than the physical limiting magnitude of the observations in searching for a change of slope in the U band number counts.
Original language | English |
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Pages (from-to) | 12-30 |
Number of pages | 19 |
Journal | Astronomy and Astrophysics |
Volume | 386 |
Issue number | 1 |
DOIs | |
Publication status | Published - Apr 2002 |
Other keywords
- Cosmology: dark matter
- Galaxies: clusters: individual: CL0024+1654
- Gravitational lensing