WFC - Photometric Calibration

Results from a reduction by Derek Jones of standards taken for the INT WFC survey during Semester 98B/99A/99B. These zero-points are predicated on the fact that the data has been processed through the WFS pipeline (see pipeline processing for more details). The individual colour terms have now been replaced by averaged colour terms taken from a simulataneous fit to all the data over these two semesters and the zero-points appropriately adjusted for the definitive colour terms. For ease of cross-calibration we are providing photometry based in the Landolt (1992, AJ 104, 340) and SDSS systems. There is evidence for colour term non-linearity in the SDSS-Landolt cross-calibration which has been ignored for the moment.

Errors in the zero-points are generally less than 1-2% except where ":" denotes 5% or more uncertainties, usually due to a limited amount of photometric conditions. For users who have accessed the previous version of this page click here to compare with the original table which used individual WFS run colour terms.

Provisional Photometric Zero-Points & Colour Terms
(Landolt, SDSS)

Passband Zero-Point Colour terms Date Zero-Point Colour terms
RGO U 22.36 -0.055 U-B Oct 98 - +0.005 u'-g'
- 22.28 (+/-0.021) Dec 98 - (+/-0.016)
- 22.30 - Feb 99 - -
- 22.30 - Jun 99 - -
- 22.43: - Jul 99 - -
- 22.36 - Aug 99 - -
KPNO B 24.68 -0.129 B-V Oct 98 - +0.191 g'-r'
- 24.63 (+/-0.016) Dec 98 - (+/-0.016)
- 24.56 - Feb 99 - -
- 24.52 - Mar 99 - -
- 24.53 - Apr 99 - -
- 24.44 - Jun 99 - -
Harris B 24.12: - Nov 98 - -
- 24.25 - May 99 - -
Harris V 24.49 -0.009 V-R Oct 98 - -0.566 g'-r'
- 24.33 (+/-0.018) Nov 98 - (+/-0.005)
- 24.43 - Dec 98 - -
- 24.38 - Feb 99 - -
- 24.34 - May 99 - -
Harris R 24.45 +0.010 V-R Oct 98 - -0.214 r'-i'
- 24.17: (+/-0.010) Dec 98 - (+/-0.015)
- 24.36 - Feb 99 - -
RGO I 23.74 -0.062 R-I Oct 98 - -0.377 i'-z'
- 23.58 (+/-0.016) Nov 98 - (+/-0.020)
- 23.64: - Dec 98 - -
- 23.63 - May 99 - -
RGO z' 22.24 -0.381 R-I Oct 98 - +0.053 i'-z'
- 22.11: (+/-0.039) Dec 98 - (+/-0.064)
- 22.21 - Feb 99 - -
- 22.25 - Apr 99 - -
- 22.19 - Jun 99 - -
- 22.13 - Jul 99 - -
- 22.05: - Aug 99 - -
SDSS g' 24.88 -0.521 B-V Jun 99 - -0.139 g'-r'
- 24.83 (+/-0.004) Jul 99 - (+/-0.005)
- 24.80 - Aug 99 - -
SDSS r' 24.33 +0.245 V-R Mar 99 - -0.005 r'-i'
- 24.34 (+/-0.016) Apr 99 - (+/-0.012)
- 24.23: - Jun 99 - -
- 24.37 - Jul 99 - -
- 24.35 - Aug 99 - -
SDSS i' 23.73 +0.211 R-I Feb 99 - +0.020 i'-z'
- 23.57: (+/-0.006) Jun 99 - (+/-0.025)
- 23.73 - Jul 99 - -
- 23.68 - Aug 99 - -

Notes to table:

An example use of the zero points and colour terms for each passband is given below:
B'_ccd = 24.52 - 2.5 log10(counts/s) = B - 0.129 B-V
where B'_ccd is the natural CCD + filter system and B, B-V are on Landolt's 1992 system.

Average extinction coefficients for La Palma of:
U = 0.49, B = 0.25, V = 0.15, R = 0.11, I = 0.07, Z = 0.08, g' = 0.22, r' = 0.12, i' = 0.08,
have been assumed for the photometric nights used to derive the zero-points and colour terms. For details of nightly individual extinction measurements and more information regarding the La Palma extinction curve see the Carlsberg Meridian Telescope extinction measurements.

The Z-band Landolt zero-point is in the natural WFC filter + CCD passband and has been approximately normalised to the Vega system using an extrapolated colour correction for the Landolt photometry.

The effective gain (e-/ADU) of the system is 3.12 so to convert the zero-points to photons/s add 1.24 magnitudes.

An attempt was made to use only photometric nights in deriving the zero-points but this was not possible for some runs eg. Dec 98 R-band, usually denoted by ":" after the zero-point.


Last modified: Tue Jan 18 13:02:56 2000