Table 7
Redshift and redshift-dependent parameters.
| maxBCG | zMrk668 | zLe Phare | log Pcore, 1.4 GHz | log Ptot, 1.4 GHz | LAS | LLS | |
| (W Hz-1) | (W Hz-1) | (′′) | (Mpc) | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | |
|
|
|||||||
| 2596 | 0.56 | ... | 24.21 | 25.93 | 42 | 0.27 | |
| 3131 | 1.03 | 1.57 |
24.73 | 26.29 | 27 | 0.22 | |
| 6167 | 1.13 | 1.00 |
... | 26.63 | 36 | 0.30 | |
| 8495 | 0.96 | 0.88 |
... | 26.20 | 39 | 0.31 | |
| 10942 | 1.71 | ... | 25.32 | 27.14 | 51 | 0.44 | |
| 11079 | 3.18 | ... | 26.10 | 28.19 | 39 | 0.30 | |
| 11390 | 1.28 | ... | ... | 26.00 | 24 | 0.21 | |
| 11780 | 0.05 | ... | 21.37 | 23.12 | 36 | 0.04 | |
Notes. Column 1: the radio source corresponding to the SDSS maxBCG cluster field: identification number is the sequential number (Koester et al. 2007). Column 2: redshift estimate assuming Mrk 668 as a template. Column 3: redshift estimate using the Le Phare photometric redshift code and Stripe 82 photometry in conjunction with our NIR data. Column 4: the logarithm of the “core” rest-frame monochromatic radio luminosity. The radio “core” power is estimated using funtools on circular regions of approximately the same size (~2 arcsec) and centered on the NIR emission regions N. We have not included a k-correction. Column 5: the logarithm of the total FIRST rest-frame monochromatic radio luminosity. The radio power is estimated from sum of the integrated flux densities of all the FIRST components. We have not included a k-correction. Column 6: FIRST projected largest angular size. Column 7: FIRST projected largest linear size.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.