Issue |
A&A
Volume 508, Number 3, December IV 2009
|
|
---|---|---|
Page(s) | 1173 - 1191 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361/200810644 | |
Published online | 27 October 2009 |
Online Material
Table 9:
accuracy derived from simulations for
galaxies in the spectroscopic sample, based on the GR code.
Table 10:
accuracy expected for the faintest galaxies in the
EDisCS sample, based on the GR code.
![]() |
Figure 16:
Comparison between spectroscopic and photometric redshifts
for the low-z sample, obtained with Hyperz ( top panel) and
GR ( central panel)
codes. Solid (red) circles, open (blue) circles, and crosses correspond
to objects with good (type 1), medium (type 2) and tentative
(type 3) spectroscopic redshift determinations, respectively.
Dot-dashed lines display
|
Open with DEXTER |
![]() |
Figure 17:
(Comparison between spectroscopic and photometric redshifts
for the high-z sample, obtained with Hyperz ( top panel) and
GR ( central panel)
codes. Solid (red) circles, open (blue) circles, and crosses correspond
to objects with good (type 1), medium (type 2) and tentative
(type 3) spectroscopic redshift determinations, respectively.
Dot-dashed lines display
|
Open with DEXTER |
![]() |
Figure 18:
A comparison of
|
Open with DEXTER |
![]() |
Figure 19: Same as Fig. 18 but for the clusters with VRIJK photometry. |
Open with DEXTER |
![]() |
Figure 20:
The histogram of
|
Open with DEXTER |
![]() |
Figure 21: Same as Fig. 14 except for Cl1420-1236. |
Open with DEXTER |
![]() |
Figure 22: Same as Fig. 14 except for Cl1040-1155. |
Open with DEXTER |
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