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Chapter 2     Surface photometry of nearby field galaxies


63

from which we find after substitution of each of these equations into each other:

  µB(r) = { (1 - pc2) · P1 + pc1 · P2 } / { 1 + pc1 - pc2 } (2.3a)
and
  µR(r) = { (1 + pc1) · P2 + pc2 · P1 } / { 1 + pc1 - pc2 } (2.3b)

Equations (2.3) represent the solutions for the surface brightness profiles, corrected for the color term, in each of the two filters. Similar equations hold for U and R and corresponding color (U-R). This procedure avoids the introduction of additional correlated errors in the radial surface brightness profiles due to the two filters used in the color term correction, that one expects when propagating errors in the more commonly applied iterative methods.
For completeness we give also the equations used to find the formal random errors on the surface brightness profiles thus derived:

  nm   =   1/{1+pc1-pc2}
\sigmaµR(r)   =   nm · { (1 - pc2\sigmaP1² + pc1² \sigmaP2² + (µB²(r) + P1²) · \sigmapc2² + (µB²(r) + P2²) · \sigmapc1² }½
(2.4)
and
  µR(r) = { (1 + pc1) · P2 + pc2 · P1 } / { 1 + pc1 - pc2 } (2.3b)
(...)

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