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Home All issues Volume 501 / No 3 (July III 2009) A&A, 501 3 (2009) 851-864 Full HTML
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Table 4:

WINGS-NIR catalogs useful parametersa.
Cluster DM Band $m_{\lim}$ ${\mu}_{\rm thresh}$ Cum Stars Gals Notes
    mag mag mag/''2 Det Det Clas Det Clas  
A119 36.46 K 21.2 21.02 20.0 19.8 18.2 19.3 19.0  
A376 36.66 J 21.5 22.11 20.2 20.4 19.0 20.0 19.6 1
    J 21.6 21.93 21.0 20.0 18.0 19.6 19.2 1, 2
A500 37.40 K 20.8 21.02 19.7 19.2 17.7 18.7 18.3 2, 4
A602 37.22 K 21.2 21.68 20.0 20.3 18.7 19.3 19.2 1, 3
    J 21.5 22.11 20.3 20.3 18.5 19.8 19.4 2, 4
A957x 36.43 K 21.1 21.49 20.0 20.0 18.7 19.7 19.4  
    J 21.8 22.31 21.0 20.6 18.6 20.0 19.5 2
A970 37.10 K 20.9 21.13 19.7 19.5 17.7 18.9 18.5 1, 4
    J 21.9 21.95 21.2 20.2 18.6 19.8 19.5 5, 6
A1069 37.33 K 20.6 21.32 19.2 20.3 18.7 19.7 19.4  
    J 21.8 22.37 21.0 21.1 19.2 20.3 20.2  
A1291 36.85 K 20.6 21.29 19.5 19.5 18.2 19.0 18.8 1, 2, 5
    J 21.2 22.09 20.0 20.1 18.5 19.5 19.1  
A1631a 36.56 K 20.7 21.02 19.1 19.7 18.4 19.3 18.7 1, 3
    J 21.8 21.98 20.2 20.7 19.2 20.0 19.6 1, 4
A1644 36.61 K 20.6 20.90 19.0 19.5 18.1 18.9 18.7 1, 4, 6
    J 22.0 22.27 21.5 20.1 18.0 19.8 18.0 2, 5
A1795 37.24 K 20.8 21.07 19.0 19.1 18.0 18.7 18.5 2
    J 21.7 22.34 21.1 21.0 19.5 20.5 20.1 6
A1831 37.20 K 20.5 21.19 19.3 19.3 17.5 19.0 18.6 1, 6
    J 21.9 22.63 20.6 21.0 19.5 20.3 20.0 1, 4
A1983 36.43 K 20.2 20.74 18.9 19.0 18.0 18.5 18.5 4
A1991 37.10 J 21.7 22.10 21.1 20.8 19.0 20.0 19.5  
    J 21.7 22.22 21.2 20.7 19.1 20.0 19.6 2
A2107 36.30 K 20.8 21.08 19.2 19.2 18.0 19.3 19.1 1, 4
    J 21.7 22.29 21.2 20.2 18.7 20.0 19.7  
A2124 37.35 K 21.1 21.36 20.0 19.8 18.3 19.2 19.1  
A2149 37.43 K 20.9 21.11 20.0 19.7 18.3 19.3 19.0 6
    J 21.7 22.14 21.0 20.8 19.1 20.1 19.8  
A2169 37.09 K 20.6 20.99 19.7 19.5 18.2 19.3 18.9  
A2382 37.21 K 20.3 20.57 19.5 19.2 17.7 18.8 18.3 2
A2399 37.07 K 20.8 21.04 19.6 19.5 18.2 19.2 18.6 1, 4
A2457 37.12 K 20.9 21.14 19.8 19.7 18.0 19.3 18.7 4
A2572a 36.25 K 21.0 21.25 19.9 19.7 18.4 19.3 19.2 2, 5
A2589 36.31 K 21.1 21.36 20.0 19.8 18.0 19.5 18.8 2, 5
    J 21.5 21.83 20.4 20.5 19.0 19.8 19.0 1, 2, 4
IIZW108 36.70 K 21.03 21.32 19.8 19.8 18.3 19.5 19.0 1, 4, 6
    J 21.9 22.56 20.5 21.0 19.6 20.3 20.0 1
MKW3s 36.50 K 21.0 21.35 20.0 19.7 18.3 19.3 18.7 2, 4
    J 21.5 22.10 20.2 20.5 18.9 19.9 19.6 2
RX1022 36.69 K 21.2 21.53 20.1 19.8 18.2 19.3 19.2 2
RX1740 36.40 K 20.6 20.86 19.1 19.1 17.8 18.7 18.2 1, 2, 4
    J 21.7 22.16 20.9 20.7 19.2 20.0 19.9 2
Z8338 36.61 K 20.7 21.06 19.5 19.6 18.6 19.3 18.9  
a The Cluster column identifies the cluster, the DM column is the cluster distance modulus in magnitudes, the $m_{\lim}$ column is the theoretical magnitude detection limit calculated with Eq. (2), ${\mu}_{\rm thresh}$ column is the minimum surface brightness at the detection threshold cut calculate with Eq. (4), the cumulative detection column (``Cum Det'') lists the turnover magnitude of the number counts diagram for all the detected sources (see Fig. 9), ``Stars'' and ``Gals'' columns represent the average 90% completeness detection and classification limits for stars and galaxies as deduced from simulations.
Notes legend:
1:= patchy and/or noisy background; 2:= strongly variable PSF; 3:= many spurious detections; 4:= excess of classified stars; 5:= deficient in classified stars; 6:= exceptionally bright star(s).

Source LaTeX | All tables | In the text

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