All Tables
- Table 1:
The list of Vilnius photoelectric standard stars
observed in the studied fields and used for calibration.
- Table 2:
The fitting results in each pass-band for the stars
common to both the observed fields.
- Table 3:
A selection of the color-excess EB-V of M 92 from
several authors in the literature (in order of publication).
- Table 4:
The [Fe/H] ratios measured for each color excess in
both fields M92C and M92W with the corresponding rms error and
the number of stars involved in computing each value.
- Table 5:
The results of the statistical analysis. The values of
median, skewness, kurtosis-excess are indicated for each set of
metallicity measurements, in each field (C for M92C and W for
M92W). The values listed in Cols. 4 and 6 give the limit for
the
skewness and the kurtosis-excess to be considered significantly equal
to zero (see the text).
- Table 6:
Some [Fe/H] determinations of the globular cluster M 92
measured by different authors in different epochs.
- Table A.1:
CCD photometry in M92C.
- Table A.2:
CCD photometry in M92W.
- Table A.3:
The identification numbers Nc and Nw for
the 64 stars common to both the observed regions M92C and M92W. The
corresponding numbers are taken from Tables A.1 and A.2.
- Table A.4:
In Cols. 1 and 2 the identification numbers of
M92C stars Nc and the corresponding Sandage & Walker numbers (1966)
Ns. In Cols. 3 and 4 the Vc and Vs magnitudes and in Cols. 5 and 6 the
(B-V) color indices. The color-index (B-V) in Col. 5 is determined
by transformations of linear combinations of Vilnius color-indices (see
text).
- Table A.5:
In Cols. 1 and 2 the identification numbers of M92W
stars Nw and the corresponding Sandage & Walker numbers (1966)
Ns. In Cols. 3 and 4 the Vw and Vs magnitudes and in Cols. 5 and 6 the B-V color
indices. The color-index (B-V) in Col. 5 is determined by transformations
of linear combinations of Vilnius color-indices (see text).
- Table A.6:
The V magnitudes and the (B-V) color-indices of 17 stars observed by Sandage & Walker (1966) and re-observed by Sandage
(1969).
- Table A.7:
In Col. 1 are the id. numbers of
the sample of stars selected in the M92C field. In Cols. 2-4
the measured values of [Fe/H] are shown.
- Table A.8:
In Col. 1 are the id. numbers of
the sample of stars selected in the M92W field. In Cols. 2-4
the measured values of [Fe/H] are shown.