Commit d3230bd7 authored by Emmanuel Bertin's avatar Emmanuel Bertin
Browse files

Removed obsolete measurement parameters. 

Pushed version number to 2.8.6
parent a14d0e27

configure.ac

+1 −1
Original line number Diff line number Diff line
@@ -6,7 +6,7 @@ define([AC_CACHE_LOAD],) 
define([AC_CACHE_SAVE],)



# This is your standard Bertin source code...

AC_INIT(sextractor, 2.8.5, [bertin@iap.fr])

AC_INIT(sextractor, 2.8.6, [bertin@iap.fr])

AC_CONFIG_SRCDIR(src/makeit.c)

AC_CONFIG_AUX_DIR(autoconf)

AM_CONFIG_HEADER(config.h)

src/param.h

+8 −5
Original line number Diff line number Diff line
@@ -9,7 +9,7 @@ 
*

*	Contents:	parameter list for catalog data.

*

*	Last modify:	18/05/2008

*	Last modify:	08/04/2009

*

*%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%

*/
@@ -135,23 +135,23 @@ keystruct objkey[] = { 
	&outobj2.vector_somfit, H_FLOAT, T_FLOAT, "%5.2f", "",

	"src.morph.param", "", 1, &prefs.somfit_vectorsize},



/* The following would use Principal Component fitting.

   This has been obsoleted by bona fide model fitting.



  {"FLUX_GALFIT", "Flux derived from the galaxy fit",

	&outobj2.flux_galfit, H_FLOAT, T_FLOAT, "%12.7g", "count",

	"phot.flux;stat.fit.param", "ct"},

/*

  {"FLUXERR_GALFIT", "RMS error for GALFIT flux",

	&outobj2.fluxerr_galfit, H_FLOAT, T_FLOAT, "%12.7g", "count"},

*/

  {"MAG_GALFIT", "Magnitude derived from galaxy fit",

	&outobj2.mag_galfit, H_FLOAT, T_FLOAT, "%8.4f", "mag",

	"phot.mag;stat.fit.param", "mag"},



/*

  {"MAGERR_GALFIT", "Magnitude error derived from galaxy fit",

	&outobj2.magerr_galfit, H_FLOAT, T_FLOAT, "%8.4f", "mag"},

  {"ERROR_GALFIT", "Reduced Chi-square error of the galaxy fit",

	&outobj2.stderr_galfit, H_FLOAT, T_FLOAT, "%10g", ""},

*/



  {"GALDANG_IMAGE", "Galaxy disk position angle  from the galaxy fit",

	&outobj2.gdposang, H_FLOAT, T_FLOAT, "%5.1f", "deg",

	"pos.posAng;stat.fit.param", "deg"},
@@ -179,6 +179,7 @@ keystruct objkey[] = { 
  {"GALBASPEC_IMAGE", "Galaxy bulge aspect ratio from the galaxy fit",

	&outobj2.gbaspect, H_FLOAT, T_FLOAT, "%5.3f", "",

	"phys.size.axisRatio;stat.fit.param", ""},

*/



  {"KRON_RADIUS", "Kron apertures in units of A or B",

	&outobj2.kronfactor, H_FLOAT, T_FLOAT, "%5.2f", "",
@@ -831,6 +832,7 @@ keystruct objkey[] = { 
	&outobj2.poserrtheta1950_psf, H_FLOAT, T_FLOAT, "%5.1f", "deg",

	"pos.posAng;pos.errorEllipse", "deg"},



/* Temporarily (at least) deactivated not to confuse users with model-fitting

  {"X2PC_IMAGE", "PC variance along x",

	&outobj2.mx2_pc, H_EXPO, T_DOUBLE, "%15.10e", "pixel**2",

	"src.impactParam;instr.det", "pix2"},
@@ -853,6 +855,7 @@ keystruct objkey[] = { 
  {"PC", "Principal components",

	&outobj2.vector_pc, H_FLOAT, T_FLOAT, "%15.10e", "",

	"src.morph.param", "", 1, &prefs.pc_vectorsize},

*/



#include "paramprofit.h"