Conversion of standardized ReadMe file for
file /./ftp/cats/II/232 into FORTRAN code for reading data files line by line.
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 2026-Oct-05
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. II/232 UBV photometry of selected regions in the MCs (Braun 2001)
*================================================================================
*Large-scale star formation in the Magellanic Clouds derived from analysis
*of stellar populations.
* Braun J.M.
* <Ph.D. Dissertation, Bonn Univ., Shaker Verlag, Aachen,
* ISBN 3-8265-8325-6, ISSN 0947-7756 (2001)>
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'lmc4c.dat' ! Photometry of the central area of LMC4 (part 1)
integer*4 nr__
parameter (nr__=46749) ! Number of records
character*74 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg ! (deg) Right Ascension J2000
real*8 DEdeg ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*8 FldSeq ! *Field Sequence (1)
integer*4 RAh ! (h) Right Ascension J2000 (hours) (2)
integer*4 RAm ! (min) Right Ascension J2000 (minutes)
real*4 RAs ! (s) Right Ascension J2000 (seconds)
character*1 DE_ ! Declination J2000 (sign) (2)
integer*4 DEd ! (deg) Declination J2000 (degrees)
integer*4 DEm ! (arcmin) Declination J2000 (minutes)
real*4 DEs ! (arcsec) Declination J2000 (seconds)
real*4 Vmag ! (mag) ? V magnitude
real*4 e_Vmag ! (mag) ? Photometric error in V (3)
real*4 B_V ! (mag) ? B-V colour
real*4 e_B_V ! (mag) ? Photometric error in B-V (3)
real*4 U_B ! (mag) ? U-B colour (4)
real*4 e_U_B ! (mag) ? Photometric error in U-B (3)
*Note (1):
* Field Sequence is a floating point derived by field number (1-4) plus
* star sequence number (at most 6 digits) divided by 1000000.
*Note (2):
* The given coordinates are derived by cross identification with MACS stars.
*Note (3):
* Photometric errors from DAOPHOT procedure.
*Note (4):
* These values are not available for all stars due to less deep exposures
* in U or special problems - for the LMC4 ('lmc4c') no U images had been
* taken. All data points had been selected to have B and V photometry.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'n70.dat' ! Photometry of the N70 region (part 2)
integer*4 nr__1
parameter (nr__1=42026) ! Number of records
character*74 ar__1 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 ! (deg) Right Ascension J2000
real*8 DEdeg_1 ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*8 FldSeq_1 ! *Field Sequence (1)
integer*4 RAh_1 ! (h) Right Ascension J2000 (hours) (2)
integer*4 RAm_1 ! (min) Right Ascension J2000 (minutes)
real*4 RAs_1 ! (s) Right Ascension J2000 (seconds)
character*1 DE__1 ! Declination J2000 (sign) (2)
integer*4 DEd_1 ! (deg) Declination J2000 (degrees)
integer*4 DEm_1 ! (arcmin) Declination J2000 (minutes)
real*4 DEs_1 ! (arcsec) Declination J2000 (seconds)
real*4 Vmag_1 ! (mag) ? V magnitude
real*4 e_Vmag_1 ! (mag) ? Photometric error in V (3)
real*4 B_V_1 ! (mag) ? B-V colour
real*4 e_B_V_1 ! (mag) ? Photometric error in B-V (3)
real*4 U_B_1 ! (mag) ? U-B colour (4)
real*4 e_U_B_1 ! (mag) ? Photometric error in U-B (3)
*Note (1):
* Field Sequence is a floating point derived by field number (1-4) plus
* star sequence number (at most 6 digits) divided by 1000000.
*Note (2):
* The given coordinates are derived by cross identification with MACS stars.
*Note (3):
* Photometric errors from DAOPHOT procedure.
*Note (4):
* These values are not available for all stars due to less deep exposures
* in U or special problems - for the LMC4 ('lmc4c') no U images had been
* taken. All data points had been selected to have B and V photometry.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'lmc2s.dat' ! Photometry of the strip inside LMC2 (part 2)
integer*4 nr__2
parameter (nr__2=66901) ! Number of records
character*74 ar__2 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_2 ! (deg) Right Ascension J2000
real*8 DEdeg_2 ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*8 FldSeq_2 ! *Field Sequence (1)
integer*4 RAh_2 ! (h) Right Ascension J2000 (hours) (2)
integer*4 RAm_2 ! (min) Right Ascension J2000 (minutes)
real*4 RAs_2 ! (s) Right Ascension J2000 (seconds)
character*1 DE__2 ! Declination J2000 (sign) (2)
integer*4 DEd_2 ! (deg) Declination J2000 (degrees)
integer*4 DEm_2 ! (arcmin) Declination J2000 (minutes)
real*4 DEs_2 ! (arcsec) Declination J2000 (seconds)
real*4 Vmag_2 ! (mag) ? V magnitude
real*4 e_Vmag_2 ! (mag) ? Photometric error in V (3)
real*4 B_V_2 ! (mag) ? B-V colour
real*4 e_B_V_2 ! (mag) ? Photometric error in B-V (3)
real*4 U_B_2 ! (mag) ? U-B colour (4)
real*4 e_U_B_2 ! (mag) ? Photometric error in U-B (3)
*Note (1):
* Field Sequence is a floating point derived by field number (1-4) plus
* star sequence number (at most 6 digits) divided by 1000000.
*Note (2):
* The given coordinates are derived by cross identification with MACS stars.
*Note (3):
* Photometric errors from DAOPHOT procedure.
*Note (4):
* These values are not available for all stars due to less deep exposures
* in U or special problems - for the LMC4 ('lmc4c') no U images had been
* taken. All data points had been selected to have B and V photometry.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'lmc2o.dat' ! Photometry of the LMC2 outer field (part 2)
integer*4 nr__3
parameter (nr__3=17672) ! Number of records
character*74 ar__3 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_3 ! (deg) Right Ascension J2000
real*8 DEdeg_3 ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*8 FldSeq_3 ! *Field Sequence (1)
integer*4 RAh_3 ! (h) Right Ascension J2000 (hours) (2)
integer*4 RAm_3 ! (min) Right Ascension J2000 (minutes)
real*4 RAs_3 ! (s) Right Ascension J2000 (seconds)
character*1 DE__3 ! Declination J2000 (sign) (2)
integer*4 DEd_3 ! (deg) Declination J2000 (degrees)
integer*4 DEm_3 ! (arcmin) Declination J2000 (minutes)
real*4 DEs_3 ! (arcsec) Declination J2000 (seconds)
real*4 Vmag_3 ! (mag) ? V magnitude
real*4 e_Vmag_3 ! (mag) ? Photometric error in V (3)
real*4 B_V_3 ! (mag) ? B-V colour
real*4 e_B_V_3 ! (mag) ? Photometric error in B-V (3)
real*4 U_B_3 ! (mag) ? U-B colour (4)
real*4 e_U_B_3 ! (mag) ? Photometric error in U-B (3)
*Note (1):
* Field Sequence is a floating point derived by field number (1-4) plus
* star sequence number (at most 6 digits) divided by 1000000.
*Note (2):
* The given coordinates are derived by cross identification with MACS stars.
*Note (3):
* Photometric errors from DAOPHOT procedure.
*Note (4):
* These values are not available for all stars due to less deep exposures
* in U or special problems - for the LMC4 ('lmc4c') no U images had been
* taken. All data points had been selected to have B and V photometry.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'n171.dat' ! Photometry of the N171 region (part 2)
integer*4 nr__4
parameter (nr__4=27920) ! Number of records
character*74 ar__4 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_4 ! (deg) Right Ascension J2000
real*8 DEdeg_4 ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*8 FldSeq_4 ! *Field Sequence (1)
integer*4 RAh_4 ! (h) Right Ascension J2000 (hours) (2)
integer*4 RAm_4 ! (min) Right Ascension J2000 (minutes)
real*4 RAs_4 ! (s) Right Ascension J2000 (seconds)
character*1 DE__4 ! Declination J2000 (sign) (2)
integer*4 DEd_4 ! (deg) Declination J2000 (degrees)
integer*4 DEm_4 ! (arcmin) Declination J2000 (minutes)
real*4 DEs_4 ! (arcsec) Declination J2000 (seconds)
real*4 Vmag_4 ! (mag) ? V magnitude
real*4 e_Vmag_4 ! (mag) ? Photometric error in V (3)
real*4 B_V_4 ! (mag) ? B-V colour
real*4 e_B_V_4 ! (mag) ? Photometric error in B-V (3)
real*4 U_B_4 ! (mag) ? U-B colour (4)
real*4 e_U_B_4 ! (mag) ? Photometric error in U-B (3)
*Note (1):
* Field Sequence is a floating point derived by field number (1-4) plus
* star sequence number (at most 6 digits) divided by 1000000.
*Note (2):
* The given coordinates are derived by cross identification with MACS stars.
*Note (3):
* Photometric errors from DAOPHOT procedure.
*Note (4):
* These values are not available for all stars due to less deep exposures
* in U or special problems - for the LMC4 ('lmc4c') no U images had been
* taken. All data points had been selected to have B and V photometry.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'n214.dat' ! Photometry of the southern N214 region (part 2)
integer*4 nr__5
parameter (nr__5=39435) ! Number of records
character*74 ar__5 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_5 ! (deg) Right Ascension J2000
real*8 DEdeg_5 ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*8 FldSeq_5 ! *Field Sequence (1)
integer*4 RAh_5 ! (h) Right Ascension J2000 (hours) (2)
integer*4 RAm_5 ! (min) Right Ascension J2000 (minutes)
real*4 RAs_5 ! (s) Right Ascension J2000 (seconds)
character*1 DE__5 ! Declination J2000 (sign) (2)
integer*4 DEd_5 ! (deg) Declination J2000 (degrees)
integer*4 DEm_5 ! (arcmin) Declination J2000 (minutes)
real*4 DEs_5 ! (arcsec) Declination J2000 (seconds)
real*4 Vmag_5 ! (mag) ? V magnitude
real*4 e_Vmag_5 ! (mag) ? Photometric error in V (3)
real*4 B_V_5 ! (mag) ? B-V colour
real*4 e_B_V_5 ! (mag) ? Photometric error in B-V (3)
real*4 U_B_5 ! (mag) ? U-B colour (4)
real*4 e_U_B_5 ! (mag) ? Photometric error in U-B (3)
*Note (1):
* Field Sequence is a floating point derived by field number (1-4) plus
* star sequence number (at most 6 digits) divided by 1000000.
*Note (2):
* The given coordinates are derived by cross identification with MACS stars.
*Note (3):
* Photometric errors from DAOPHOT procedure.
*Note (4):
* These values are not available for all stars due to less deep exposures
* in U or special problems - for the LMC4 ('lmc4c') no U images had been
* taken. All data points had been selected to have B and V photometry.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'smc1.dat' ! Photometry inside SGS SMC1 (part 3)
integer*4 nr__6
parameter (nr__6=8705) ! Number of records
character*74 ar__6 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_6 ! (deg) Right Ascension J2000
real*8 DEdeg_6 ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*8 FldSeq_6 ! *Field Sequence (1)
integer*4 RAh_6 ! (h) Right Ascension J2000 (hours) (2)
integer*4 RAm_6 ! (min) Right Ascension J2000 (minutes)
real*4 RAs_6 ! (s) Right Ascension J2000 (seconds)
character*1 DE__6 ! Declination J2000 (sign) (2)
integer*4 DEd_6 ! (deg) Declination J2000 (degrees)
integer*4 DEm_6 ! (arcmin) Declination J2000 (minutes)
real*4 DEs_6 ! (arcsec) Declination J2000 (seconds)
real*4 Vmag_6 ! (mag) ? V magnitude
real*4 e_Vmag_6 ! (mag) ? Photometric error in V (3)
real*4 B_V_6 ! (mag) ? B-V colour
real*4 e_B_V_6 ! (mag) ? Photometric error in B-V (3)
real*4 U_B_6 ! (mag) ? U-B colour (4)
real*4 e_U_B_6 ! (mag) ? Photometric error in U-B (3)
*Note (1):
* Field Sequence is a floating point derived by field number (1-4) plus
* star sequence number (at most 6 digits) divided by 1000000.
*Note (2):
* The given coordinates are derived by cross identification with MACS stars.
*Note (3):
* Photometric errors from DAOPHOT procedure.
*Note (4):
* These values are not available for all stars due to less deep exposures
* in U or special problems - for the LMC4 ('lmc4c') no U images had been
* taken. All data points had been selected to have B and V photometry.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'lmc7.dat' ! Photometry of the central area of LMC7 (part 4)
integer*4 nr__7
parameter (nr__7=44286) ! Number of records
character*74 ar__7 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_7 ! (deg) Right Ascension J2000
real*8 DEdeg_7 ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*8 FldSeq_7 ! *Field Sequence (1)
integer*4 RAh_7 ! (h) Right Ascension J2000 (hours) (2)
integer*4 RAm_7 ! (min) Right Ascension J2000 (minutes)
real*4 RAs_7 ! (s) Right Ascension J2000 (seconds)
character*1 DE__7 ! Declination J2000 (sign) (2)
integer*4 DEd_7 ! (deg) Declination J2000 (degrees)
integer*4 DEm_7 ! (arcmin) Declination J2000 (minutes)
real*4 DEs_7 ! (arcsec) Declination J2000 (seconds)
real*4 Vmag_7 ! (mag) ? V magnitude
real*4 e_Vmag_7 ! (mag) ? Photometric error in V (3)
real*4 B_V_7 ! (mag) ? B-V colour
real*4 e_B_V_7 ! (mag) ? Photometric error in B-V (3)
real*4 U_B_7 ! (mag) ? U-B colour (4)
real*4 e_U_B_7 ! (mag) ? Photometric error in U-B (3)
*Note (1):
* Field Sequence is a floating point derived by field number (1-4) plus
* star sequence number (at most 6 digits) divided by 1000000.
*Note (2):
* The given coordinates are derived by cross identification with MACS stars.
*Note (3):
* Photometric errors from DAOPHOT procedure.
*Note (4):
* These values are not available for all stars due to less deep exposures
* in U or special problems - for the LMC4 ('lmc4c') no U images had been
* taken. All data points had been selected to have B and V photometry.
C=============================================================================
C Loading file 'lmc4c.dat' ! Photometry of the central area of LMC4 (part 1)
C Format for file interpretation
1 format(
+ F9.6,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F5.2,1X,F6.3,1X,
+ F5.3,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3)
C Effective file loading
open(unit=1,status='old',file=
+'lmc4c.dat')
write(6,*) '....Loading file: lmc4c.dat'
do i__=1,46749
read(1,'(A74)')ar__
read(ar__,1)
+ FldSeq,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Vmag,e_Vmag,B_V,e_B_V,U_B,
+ e_U_B
if(ar__(37:42) .EQ. '') Vmag = rNULL__
if(ar__(44:48) .EQ. '') e_Vmag = rNULL__
if(ar__(50:55) .EQ. '') B_V = rNULL__
if(ar__(57:61) .EQ. '') e_B_V = rNULL__
if(ar__(63:68) .EQ. '') U_B = rNULL__
if(ar__(70:74) .EQ. '') e_U_B = rNULL__
RAdeg = rNULL__
DEdeg = rNULL__
c Derive coordinates RAdeg and DEdeg from input data
c (RAdeg and DEdeg are set to rNULL__ when unknown)
if(RAh .GT. -180) RAdeg=RAh*15.
if(RAm .GT. -180) RAdeg=RAdeg+RAm/4.
if(RAs .GT. -180) RAdeg=RAdeg+RAs/240.
if(DEd .GE. 0) DEdeg=DEd
if(DEm .GE. 0) DEdeg=DEdeg+DEm/60.
if(DEs .GE. 0) DEdeg=DEdeg+DEs/3600.
if(DE_.EQ.'-'.AND.DEdeg.GE.0) DEdeg=-DEdeg
c ..............Just test output...........
write(6,1)
+ FldSeq,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Vmag,e_Vmag,B_V,e_B_V,U_B,
+ e_U_B
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'n70.dat' ! Photometry of the N70 region (part 2)
C Format for file interpretation
2 format(
+ F9.6,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F5.2,1X,F6.3,1X,
+ F5.3,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3)
C Effective file loading
open(unit=1,status='old',file=
+'n70.dat')
write(6,*) '....Loading file: n70.dat'
do i__=1,42026
read(1,'(A74)')ar__1
read(ar__1,2)
+ FldSeq_1,RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,Vmag_1,
+ e_Vmag_1,B_V_1,e_B_V_1,U_B_1,e_U_B_1
if(ar__1(37:42) .EQ. '') Vmag_1 = rNULL__
if(ar__1(44:48) .EQ. '') e_Vmag_1 = rNULL__
if(ar__1(50:55) .EQ. '') B_V_1 = rNULL__
if(ar__1(57:61) .EQ. '') e_B_V_1 = rNULL__
if(ar__1(63:68) .EQ. '') U_B_1 = rNULL__
if(ar__1(70:74) .EQ. '') e_U_B_1 = rNULL__
RAdeg_1 = rNULL__
DEdeg_1 = rNULL__
c Derive coordinates RAdeg_1 and DEdeg_1 from input data
c (RAdeg_1 and DEdeg_1 are set to rNULL__ when unknown)
if(RAh_1 .GT. -180) RAdeg_1=RAh_1*15.
if(RAm_1 .GT. -180) RAdeg_1=RAdeg_1+RAm_1/4.
if(RAs_1 .GT. -180) RAdeg_1=RAdeg_1+RAs_1/240.
if(DEd_1 .GE. 0) DEdeg_1=DEd_1
if(DEm_1 .GE. 0) DEdeg_1=DEdeg_1+DEm_1/60.
if(DEs_1 .GE. 0) DEdeg_1=DEdeg_1+DEs_1/3600.
if(DE__1.EQ.'-'.AND.DEdeg_1.GE.0) DEdeg_1=-DEdeg_1
c ..............Just test output...........
write(6,2)
+ FldSeq_1,RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,Vmag_1,
+ e_Vmag_1,B_V_1,e_B_V_1,U_B_1,e_U_B_1
write(6,'(6H Pos: 2F8.4)') RAdeg_1,DEdeg_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'lmc2s.dat' ! Photometry of the strip inside LMC2 (part 2)
C Format for file interpretation
3 format(
+ F9.6,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F5.2,1X,F6.3,1X,
+ F5.3,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3)
C Effective file loading
open(unit=1,status='old',file=
+'lmc2s.dat')
write(6,*) '....Loading file: lmc2s.dat'
do i__=1,66901
read(1,'(A74)')ar__2
read(ar__2,3)
+ FldSeq_2,RAh_2,RAm_2,RAs_2,DE__2,DEd_2,DEm_2,DEs_2,Vmag_2,
+ e_Vmag_2,B_V_2,e_B_V_2,U_B_2,e_U_B_2
if(ar__2(37:42) .EQ. '') Vmag_2 = rNULL__
if(ar__2(44:48) .EQ. '') e_Vmag_2 = rNULL__
if(ar__2(50:55) .EQ. '') B_V_2 = rNULL__
if(ar__2(57:61) .EQ. '') e_B_V_2 = rNULL__
if(ar__2(63:68) .EQ. '') U_B_2 = rNULL__
if(ar__2(70:74) .EQ. '') e_U_B_2 = rNULL__
RAdeg_2 = rNULL__
DEdeg_2 = rNULL__
c Derive coordinates RAdeg_2 and DEdeg_2 from input data
c (RAdeg_2 and DEdeg_2 are set to rNULL__ when unknown)
if(RAh_2 .GT. -180) RAdeg_2=RAh_2*15.
if(RAm_2 .GT. -180) RAdeg_2=RAdeg_2+RAm_2/4.
if(RAs_2 .GT. -180) RAdeg_2=RAdeg_2+RAs_2/240.
if(DEd_2 .GE. 0) DEdeg_2=DEd_2
if(DEm_2 .GE. 0) DEdeg_2=DEdeg_2+DEm_2/60.
if(DEs_2 .GE. 0) DEdeg_2=DEdeg_2+DEs_2/3600.
if(DE__2.EQ.'-'.AND.DEdeg_2.GE.0) DEdeg_2=-DEdeg_2
c ..............Just test output...........
write(6,3)
+ FldSeq_2,RAh_2,RAm_2,RAs_2,DE__2,DEd_2,DEm_2,DEs_2,Vmag_2,
+ e_Vmag_2,B_V_2,e_B_V_2,U_B_2,e_U_B_2
write(6,'(6H Pos: 2F8.4)') RAdeg_2,DEdeg_2
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'lmc2o.dat' ! Photometry of the LMC2 outer field (part 2)
C Format for file interpretation
4 format(
+ F9.6,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F5.2,1X,F6.3,1X,
+ F5.3,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3)
C Effective file loading
open(unit=1,status='old',file=
+'lmc2o.dat')
write(6,*) '....Loading file: lmc2o.dat'
do i__=1,17672
read(1,'(A74)')ar__3
read(ar__3,4)
+ FldSeq_3,RAh_3,RAm_3,RAs_3,DE__3,DEd_3,DEm_3,DEs_3,Vmag_3,
+ e_Vmag_3,B_V_3,e_B_V_3,U_B_3,e_U_B_3
if(ar__3(37:42) .EQ. '') Vmag_3 = rNULL__
if(ar__3(44:48) .EQ. '') e_Vmag_3 = rNULL__
if(ar__3(50:55) .EQ. '') B_V_3 = rNULL__
if(ar__3(57:61) .EQ. '') e_B_V_3 = rNULL__
if(ar__3(63:68) .EQ. '') U_B_3 = rNULL__
if(ar__3(70:74) .EQ. '') e_U_B_3 = rNULL__
RAdeg_3 = rNULL__
DEdeg_3 = rNULL__
c Derive coordinates RAdeg_3 and DEdeg_3 from input data
c (RAdeg_3 and DEdeg_3 are set to rNULL__ when unknown)
if(RAh_3 .GT. -180) RAdeg_3=RAh_3*15.
if(RAm_3 .GT. -180) RAdeg_3=RAdeg_3+RAm_3/4.
if(RAs_3 .GT. -180) RAdeg_3=RAdeg_3+RAs_3/240.
if(DEd_3 .GE. 0) DEdeg_3=DEd_3
if(DEm_3 .GE. 0) DEdeg_3=DEdeg_3+DEm_3/60.
if(DEs_3 .GE. 0) DEdeg_3=DEdeg_3+DEs_3/3600.
if(DE__3.EQ.'-'.AND.DEdeg_3.GE.0) DEdeg_3=-DEdeg_3
c ..............Just test output...........
write(6,4)
+ FldSeq_3,RAh_3,RAm_3,RAs_3,DE__3,DEd_3,DEm_3,DEs_3,Vmag_3,
+ e_Vmag_3,B_V_3,e_B_V_3,U_B_3,e_U_B_3
write(6,'(6H Pos: 2F8.4)') RAdeg_3,DEdeg_3
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'n171.dat' ! Photometry of the N171 region (part 2)
C Format for file interpretation
5 format(
+ F9.6,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F5.2,1X,F6.3,1X,
+ F5.3,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3)
C Effective file loading
open(unit=1,status='old',file=
+'n171.dat')
write(6,*) '....Loading file: n171.dat'
do i__=1,27920
read(1,'(A74)')ar__4
read(ar__4,5)
+ FldSeq_4,RAh_4,RAm_4,RAs_4,DE__4,DEd_4,DEm_4,DEs_4,Vmag_4,
+ e_Vmag_4,B_V_4,e_B_V_4,U_B_4,e_U_B_4
if(ar__4(37:42) .EQ. '') Vmag_4 = rNULL__
if(ar__4(44:48) .EQ. '') e_Vmag_4 = rNULL__
if(ar__4(50:55) .EQ. '') B_V_4 = rNULL__
if(ar__4(57:61) .EQ. '') e_B_V_4 = rNULL__
if(ar__4(63:68) .EQ. '') U_B_4 = rNULL__
if(ar__4(70:74) .EQ. '') e_U_B_4 = rNULL__
RAdeg_4 = rNULL__
DEdeg_4 = rNULL__
c Derive coordinates RAdeg_4 and DEdeg_4 from input data
c (RAdeg_4 and DEdeg_4 are set to rNULL__ when unknown)
if(RAh_4 .GT. -180) RAdeg_4=RAh_4*15.
if(RAm_4 .GT. -180) RAdeg_4=RAdeg_4+RAm_4/4.
if(RAs_4 .GT. -180) RAdeg_4=RAdeg_4+RAs_4/240.
if(DEd_4 .GE. 0) DEdeg_4=DEd_4
if(DEm_4 .GE. 0) DEdeg_4=DEdeg_4+DEm_4/60.
if(DEs_4 .GE. 0) DEdeg_4=DEdeg_4+DEs_4/3600.
if(DE__4.EQ.'-'.AND.DEdeg_4.GE.0) DEdeg_4=-DEdeg_4
c ..............Just test output...........
write(6,5)
+ FldSeq_4,RAh_4,RAm_4,RAs_4,DE__4,DEd_4,DEm_4,DEs_4,Vmag_4,
+ e_Vmag_4,B_V_4,e_B_V_4,U_B_4,e_U_B_4
write(6,'(6H Pos: 2F8.4)') RAdeg_4,DEdeg_4
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'n214.dat' ! Photometry of the southern N214 region (part 2)
C Format for file interpretation
6 format(
+ F9.6,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F5.2,1X,F6.3,1X,
+ F5.3,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3)
C Effective file loading
open(unit=1,status='old',file=
+'n214.dat')
write(6,*) '....Loading file: n214.dat'
do i__=1,39435
read(1,'(A74)')ar__5
read(ar__5,6)
+ FldSeq_5,RAh_5,RAm_5,RAs_5,DE__5,DEd_5,DEm_5,DEs_5,Vmag_5,
+ e_Vmag_5,B_V_5,e_B_V_5,U_B_5,e_U_B_5
if(ar__5(37:42) .EQ. '') Vmag_5 = rNULL__
if(ar__5(44:48) .EQ. '') e_Vmag_5 = rNULL__
if(ar__5(50:55) .EQ. '') B_V_5 = rNULL__
if(ar__5(57:61) .EQ. '') e_B_V_5 = rNULL__
if(ar__5(63:68) .EQ. '') U_B_5 = rNULL__
if(ar__5(70:74) .EQ. '') e_U_B_5 = rNULL__
RAdeg_5 = rNULL__
DEdeg_5 = rNULL__
c Derive coordinates RAdeg_5 and DEdeg_5 from input data
c (RAdeg_5 and DEdeg_5 are set to rNULL__ when unknown)
if(RAh_5 .GT. -180) RAdeg_5=RAh_5*15.
if(RAm_5 .GT. -180) RAdeg_5=RAdeg_5+RAm_5/4.
if(RAs_5 .GT. -180) RAdeg_5=RAdeg_5+RAs_5/240.
if(DEd_5 .GE. 0) DEdeg_5=DEd_5
if(DEm_5 .GE. 0) DEdeg_5=DEdeg_5+DEm_5/60.
if(DEs_5 .GE. 0) DEdeg_5=DEdeg_5+DEs_5/3600.
if(DE__5.EQ.'-'.AND.DEdeg_5.GE.0) DEdeg_5=-DEdeg_5
c ..............Just test output...........
write(6,6)
+ FldSeq_5,RAh_5,RAm_5,RAs_5,DE__5,DEd_5,DEm_5,DEs_5,Vmag_5,
+ e_Vmag_5,B_V_5,e_B_V_5,U_B_5,e_U_B_5
write(6,'(6H Pos: 2F8.4)') RAdeg_5,DEdeg_5
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'smc1.dat' ! Photometry inside SGS SMC1 (part 3)
C Format for file interpretation
7 format(
+ F9.6,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F5.2,1X,F6.3,1X,
+ F5.3,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3)
C Effective file loading
open(unit=1,status='old',file=
+'smc1.dat')
write(6,*) '....Loading file: smc1.dat'
do i__=1,8705
read(1,'(A74)')ar__6
read(ar__6,7)
+ FldSeq_6,RAh_6,RAm_6,RAs_6,DE__6,DEd_6,DEm_6,DEs_6,Vmag_6,
+ e_Vmag_6,B_V_6,e_B_V_6,U_B_6,e_U_B_6
if(ar__6(37:42) .EQ. '') Vmag_6 = rNULL__
if(ar__6(44:48) .EQ. '') e_Vmag_6 = rNULL__
if(ar__6(50:55) .EQ. '') B_V_6 = rNULL__
if(ar__6(57:61) .EQ. '') e_B_V_6 = rNULL__
if(ar__6(63:68) .EQ. '') U_B_6 = rNULL__
if(ar__6(70:74) .EQ. '') e_U_B_6 = rNULL__
RAdeg_6 = rNULL__
DEdeg_6 = rNULL__
c Derive coordinates RAdeg_6 and DEdeg_6 from input data
c (RAdeg_6 and DEdeg_6 are set to rNULL__ when unknown)
if(RAh_6 .GT. -180) RAdeg_6=RAh_6*15.
if(RAm_6 .GT. -180) RAdeg_6=RAdeg_6+RAm_6/4.
if(RAs_6 .GT. -180) RAdeg_6=RAdeg_6+RAs_6/240.
if(DEd_6 .GE. 0) DEdeg_6=DEd_6
if(DEm_6 .GE. 0) DEdeg_6=DEdeg_6+DEm_6/60.
if(DEs_6 .GE. 0) DEdeg_6=DEdeg_6+DEs_6/3600.
if(DE__6.EQ.'-'.AND.DEdeg_6.GE.0) DEdeg_6=-DEdeg_6
c ..............Just test output...........
write(6,7)
+ FldSeq_6,RAh_6,RAm_6,RAs_6,DE__6,DEd_6,DEm_6,DEs_6,Vmag_6,
+ e_Vmag_6,B_V_6,e_B_V_6,U_B_6,e_U_B_6
write(6,'(6H Pos: 2F8.4)') RAdeg_6,DEdeg_6
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'lmc7.dat' ! Photometry of the central area of LMC7 (part 4)
C Format for file interpretation
8 format(
+ F9.6,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F5.2,1X,F6.3,1X,
+ F5.3,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3)
C Effective file loading
open(unit=1,status='old',file=
+'lmc7.dat')
write(6,*) '....Loading file: lmc7.dat'
do i__=1,44286
read(1,'(A74)')ar__7
read(ar__7,8)
+ FldSeq_7,RAh_7,RAm_7,RAs_7,DE__7,DEd_7,DEm_7,DEs_7,Vmag_7,
+ e_Vmag_7,B_V_7,e_B_V_7,U_B_7,e_U_B_7
if(ar__7(37:42) .EQ. '') Vmag_7 = rNULL__
if(ar__7(44:48) .EQ. '') e_Vmag_7 = rNULL__
if(ar__7(50:55) .EQ. '') B_V_7 = rNULL__
if(ar__7(57:61) .EQ. '') e_B_V_7 = rNULL__
if(ar__7(63:68) .EQ. '') U_B_7 = rNULL__
if(ar__7(70:74) .EQ. '') e_U_B_7 = rNULL__
RAdeg_7 = rNULL__
DEdeg_7 = rNULL__
c Derive coordinates RAdeg_7 and DEdeg_7 from input data
c (RAdeg_7 and DEdeg_7 are set to rNULL__ when unknown)
if(RAh_7 .GT. -180) RAdeg_7=RAh_7*15.
if(RAm_7 .GT. -180) RAdeg_7=RAdeg_7+RAm_7/4.
if(RAs_7 .GT. -180) RAdeg_7=RAdeg_7+RAs_7/240.
if(DEd_7 .GE. 0) DEdeg_7=DEd_7
if(DEm_7 .GE. 0) DEdeg_7=DEdeg_7+DEm_7/60.
if(DEs_7 .GE. 0) DEdeg_7=DEdeg_7+DEs_7/3600.
if(DE__7.EQ.'-'.AND.DEdeg_7.GE.0) DEdeg_7=-DEdeg_7
c ..............Just test output...........
write(6,8)
+ FldSeq_7,RAh_7,RAm_7,RAs_7,DE__7,DEd_7,DEm_7,DEs_7,Vmag_7,
+ e_Vmag_7,B_V_7,e_B_V_7,U_B_7,e_U_B_7
write(6,'(6H Pos: 2F8.4)') RAdeg_7,DEdeg_7
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end