Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_AS/124/559 into FORTRAN code for loading all data files into arrays.
Note that special values are assigned to unknown or unspecified
numbers (also called NULL numbers);
when necessary, the coordinate components making up the right ascension
and declination are converted into floating-point numbers
representing these angles in degrees.
program load_ReadMe
C=============================================================================
C F77-compliant program generated by readme2f_1.81 (2015-09-23), on 2024-Apr-19
C=============================================================================
* This code was generated from the ReadMe file documenting a catalogue
* according to the "Standard for Documentation of Astronomical Catalogues"
* currently in use by the Astronomical Data Centers (CDS, ADC, A&A)
* (see full documentation at URL http://vizier.u-strasbg.fr/doc/catstd.htx)
* Please report problems or questions to
C=============================================================================
implicit none
* Unspecified or NULL values, generally corresponding to blank columns,
* are assigned one of the following special values:
* rNULL__ for unknown or NULL floating-point values
* iNULL__ for unknown or NULL integer values
real*4 rNULL__
integer*4 iNULL__
parameter (rNULL__=--2147483648.) ! NULL real number
parameter (iNULL__=(-2147483647-1)) ! NULL int number
integer idig ! testing NULL number
C=============================================================================
Cat. J/A+AS/124/559 VI photometry of dwarf galaxies (Karanchentsev+ 1997)
*================================================================================
*Revised photometric distances to nearby dwarf galaxies in the
*IC 342/Maffei complex
* Karanchentsev I., Drozdovsky I., Kajsin S., Takalo L.O.,
* Heinamaki P. Valtonen M.
* <Astron. Astrophys. Suppl. Ser. 124, 559 (1997)>
* =1997A&AS..124..559K (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2' ! Photometry of the stars in the galaxy UGCA 105
integer*4 nr__
parameter (nr__=568) ! Number of records
character*38 ar__ ! Full-size record
integer*4 No (nr__) ! Star number
integer*4 Xpos (nr__) ! (pix) X coordinate (1)
integer*4 Ypos (nr__) ! (pix) Y coordinate (1)
real*4 Vmag (nr__) ! (mag) V magnitude
real*4 V_I (nr__) ! (mag) V-I colour index
real*4 V_R (nr__) ! (mag) ? V-R colour index
real*4 SHARP (nr__) ! Image parameter SHARP (2)
integer*4 L (nr__) ! ? [01] Marks the stars inside the visible
* boundary of the galaxy
*Note (1): The XY positions were calculated from the SW corner (X,Y=0,0) of the
* image, with +X going to east and +Y to north. This corner is the
* lower-right corner of the image. 1 pix = 0.176arcsec.
*Note (2): SHARP is a measure of the difference between the observed width of
* the object and the width of the psf model.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3' ! Photometry of the stars in the galaxy UGCA 92
integer*4 nr__1
parameter (nr__1=184) ! Number of records
character*38 ar__1 ! Full-size record
integer*4 No_1 (nr__1) ! Star number
integer*4 Xpos_1 (nr__1) ! (pix) X coordinate (1)
integer*4 Ypos_1 (nr__1) ! (pix) Y coordinate (1)
real*4 Vmag_1 (nr__1) ! (mag) V magnitude
real*4 V_I_1 (nr__1) ! (mag) V-I colour index
real*4 V_R_1 (nr__1) ! (mag) ? V-R colour index
real*4 SHARP_1 (nr__1) ! Image parameter SHARP (2)
integer*4 L_1 (nr__1) ! ? [01] Marks the stars inside the visible
* boundary of the galaxy
*Note (1): The XY positions were calculated from the SW corner (X,Y=0,0) of the
* image, with +X going to east and +Y to north. This corner is the
* lower-right corner of the image. 1 pix = 0.176arcsec.
*Note (2): SHARP is a measure of the difference between the observed width of
* the object and the width of the psf model.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4' ! Photometry of the stars in the galaxy UGCA 86
integer*4 nr__2
parameter (nr__2=444) ! Number of records
character*38 ar__2 ! Full-size record
integer*4 No_2 (nr__2) ! Star number
integer*4 Xpos_2 (nr__2) ! (pix) X coordinate (1)
integer*4 Ypos_2 (nr__2) ! (pix) Y coordinate (1)
real*4 Vmag_2 (nr__2) ! (mag) V magnitude
real*4 V_I_2 (nr__2) ! (mag) V-I colour index
real*4 V_R_2 (nr__2) ! (mag) ? V-R colour index
real*4 SHARP_2 (nr__2) ! Image parameter SHARP (2)
integer*4 L_2 (nr__2) ! ? [01] Marks the stars inside the visible
* boundary of the galaxy
*Note (1): The XY positions were calculated from the SW corner (X,Y=0,0) of the
* image, with +X going to east and +Y to north. This corner is the
* lower-right corner of the image. 1 pix = 0.176arcsec.
*Note (2): SHARP is a measure of the difference between the observed width of
* the object and the width of the psf model.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5' ! Photometry of the stars in the galaxy NGC 1569
integer*4 nr__3
parameter (nr__3=173) ! Number of records
character*38 ar__3 ! Full-size record
integer*4 No_3 (nr__3) ! Star number
integer*4 Xpos_3 (nr__3) ! (pix) X coordinate (1)
integer*4 Ypos_3 (nr__3) ! (pix) Y coordinate (1)
real*4 Vmag_3 (nr__3) ! (mag) V magnitude
real*4 V_I_3 (nr__3) ! (mag) V-I colour index
real*4 V_R_3 (nr__3) ! (mag) ? V-R colour index
real*4 SHARP_3 (nr__3) ! Image parameter SHARP (2)
integer*4 L_3 (nr__3) ! ? [01] Marks the stars inside the visible
* boundary of the galaxy
*Note (1): The XY positions were calculated from the SW corner (X,Y=0,0) of the
* image, with +X going to east and +Y to north. This corner is the
* lower-right corner of the image. 1 pix = 0.176arcsec.
*Note (2): SHARP is a measure of the difference between the observed width of
* the object and the width of the psf model.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6' ! Photometry of the stars in the galaxy Cas 1
integer*4 nr__4
parameter (nr__4=231) ! Number of records
character*38 ar__4 ! Full-size record
integer*4 No_4 (nr__4) ! Star number
integer*4 Xpos_4 (nr__4) ! (pix) X coordinate (1)
integer*4 Ypos_4 (nr__4) ! (pix) Y coordinate (1)
real*4 Vmag_4 (nr__4) ! (mag) V magnitude
real*4 V_I_4 (nr__4) ! (mag) V-I colour index
real*4 V_R_4 (nr__4) ! (mag) ? V-R colour index
real*4 SHARP_4 (nr__4) ! Image parameter SHARP (2)
integer*4 L_4 (nr__4) ! ? [01] Marks the stars inside the visible
* boundary of the galaxy
*Note (1): The XY positions were calculated from the SW corner (X,Y=0,0) of the
* image, with +X going to east and +Y to north. This corner is the
* lower-right corner of the image. 1 pix = 0.176arcsec.
*Note (2): SHARP is a measure of the difference between the observed width of
* the object and the width of the psf model.
C=============================================================================
C Loading file 'table2' ! Photometry of the stars in the galaxy UGCA 105
C Format for file interpretation
1 format(I3,1X,I4,1X,I4,1X,F5.2,1X,F5.2,1X,F5.2,1X,F4.1,1X,I1)
C Effective file loading
open(unit=1,status='old',file=
+'table2')
write(6,*) '....Loading file: table2'
do i__=1,568
read(1,'(A38)')ar__
read(ar__,1)
+ No(i__),Xpos(i__),Ypos(i__),Vmag(i__),V_I(i__),V_R(i__),
+ SHARP(i__),L(i__)
if(ar__(27:31) .EQ. '') V_R(i__) = rNULL__
if(ar__(38:38) .EQ. '') L(i__) = iNULL__
c ..............Just test output...........
write(6,1)
+ No(i__),Xpos(i__),Ypos(i__),Vmag(i__),V_I(i__),V_R(i__),
+ SHARP(i__),L(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3' ! Photometry of the stars in the galaxy UGCA 92
C Format for file interpretation
2 format(I3,1X,I4,1X,I4,1X,F5.2,1X,F5.2,1X,F5.2,1X,F4.1,1X,I1)
C Effective file loading
open(unit=1,status='old',file=
+'table3')
write(6,*) '....Loading file: table3'
do i__=1,184
read(1,'(A38)')ar__1
read(ar__1,2)
+ No_1(i__),Xpos_1(i__),Ypos_1(i__),Vmag_1(i__),V_I_1(i__),
+ V_R_1(i__),SHARP_1(i__),L_1(i__)
if(ar__1(27:31) .EQ. '') V_R_1(i__) = rNULL__
if(ar__1(38:38) .EQ. '') L_1(i__) = iNULL__
c ..............Just test output...........
write(6,2)
+ No_1(i__),Xpos_1(i__),Ypos_1(i__),Vmag_1(i__),V_I_1(i__),
+ V_R_1(i__),SHARP_1(i__),L_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4' ! Photometry of the stars in the galaxy UGCA 86
C Format for file interpretation
3 format(I3,1X,I4,1X,I4,1X,F5.2,1X,F5.2,1X,F5.2,1X,F4.1,1X,I1)
C Effective file loading
open(unit=1,status='old',file=
+'table4')
write(6,*) '....Loading file: table4'
do i__=1,444
read(1,'(A38)')ar__2
read(ar__2,3)
+ No_2(i__),Xpos_2(i__),Ypos_2(i__),Vmag_2(i__),V_I_2(i__),
+ V_R_2(i__),SHARP_2(i__),L_2(i__)
if(ar__2(27:31) .EQ. '') V_R_2(i__) = rNULL__
if(ar__2(38:38) .EQ. '') L_2(i__) = iNULL__
c ..............Just test output...........
write(6,3)
+ No_2(i__),Xpos_2(i__),Ypos_2(i__),Vmag_2(i__),V_I_2(i__),
+ V_R_2(i__),SHARP_2(i__),L_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table5' ! Photometry of the stars in the galaxy NGC 1569
C Format for file interpretation
4 format(I3,1X,I4,1X,I4,1X,F5.2,1X,F5.2,1X,F5.2,1X,F4.1,1X,I1)
C Effective file loading
open(unit=1,status='old',file=
+'table5')
write(6,*) '....Loading file: table5'
do i__=1,173
read(1,'(A38)')ar__3
read(ar__3,4)
+ No_3(i__),Xpos_3(i__),Ypos_3(i__),Vmag_3(i__),V_I_3(i__),
+ V_R_3(i__),SHARP_3(i__),L_3(i__)
if(ar__3(27:31) .EQ. '') V_R_3(i__) = rNULL__
if(ar__3(38:38) .EQ. '') L_3(i__) = iNULL__
c ..............Just test output...........
write(6,4)
+ No_3(i__),Xpos_3(i__),Ypos_3(i__),Vmag_3(i__),V_I_3(i__),
+ V_R_3(i__),SHARP_3(i__),L_3(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table6' ! Photometry of the stars in the galaxy Cas 1
C Format for file interpretation
5 format(I3,1X,I4,1X,I4,1X,F5.2,1X,F5.2,1X,F5.2,1X,F4.1,1X,I1)
C Effective file loading
open(unit=1,status='old',file=
+'table6')
write(6,*) '....Loading file: table6'
do i__=1,231
read(1,'(A38)')ar__4
read(ar__4,5)
+ No_4(i__),Xpos_4(i__),Ypos_4(i__),Vmag_4(i__),V_I_4(i__),
+ V_R_4(i__),SHARP_4(i__),L_4(i__)
if(ar__4(27:31) .EQ. '') V_R_4(i__) = rNULL__
if(ar__4(38:38) .EQ. '') L_4(i__) = iNULL__
c ..............Just test output...........
write(6,5)
+ No_4(i__),Xpos_4(i__),Ypos_4(i__),Vmag_4(i__),V_I_4(i__),
+ V_R_4(i__),SHARP_4(i__),L_4(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end