Conversion of standardized ReadMe file for
file /./ftp/cats/II/232 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 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 (nr__) ! (deg) Right Ascension J2000
real*8 DEdeg (nr__) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*8 FldSeq (nr__) ! *Field Sequence (1)
integer*4 RAh (nr__) ! (h) Right Ascension J2000 (hours) (2)
integer*4 RAm (nr__) ! (min) Right Ascension J2000 (minutes)
real*4 RAs (nr__) ! (s) Right Ascension J2000 (seconds)
character*1 DE_ (nr__) ! Declination J2000 (sign) (2)
integer*4 DEd (nr__) ! (deg) Declination J2000 (degrees)
integer*4 DEm (nr__) ! (arcmin) Declination J2000 (minutes)
real*4 DEs (nr__) ! (arcsec) Declination J2000 (seconds)
real*4 Vmag (nr__) ! (mag) ? V magnitude
real*4 e_Vmag (nr__) ! (mag) ? Photometric error in V (3)
real*4 B_V (nr__) ! (mag) ? B-V colour
real*4 e_B_V (nr__) ! (mag) ? Photometric error in B-V (3)
real*4 U_B (nr__) ! (mag) ? U-B colour (4)
real*4 e_U_B (nr__) ! (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 (nr__1) ! (deg) Right Ascension J2000
real*8 DEdeg_1 (nr__1) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*8 FldSeq_1 (nr__1) ! *Field Sequence (1)
integer*4 RAh_1 (nr__1) ! (h) Right Ascension J2000 (hours) (2)
integer*4 RAm_1 (nr__1) ! (min) Right Ascension J2000 (minutes)
real*4 RAs_1 (nr__1) ! (s) Right Ascension J2000 (seconds)
character*1 DE__1 (nr__1) ! Declination J2000 (sign) (2)
integer*4 DEd_1 (nr__1) ! (deg) Declination J2000 (degrees)
integer*4 DEm_1 (nr__1) ! (arcmin) Declination J2000 (minutes)
real*4 DEs_1 (nr__1) ! (arcsec) Declination J2000 (seconds)
real*4 Vmag_1 (nr__1) ! (mag) ? V magnitude
real*4 e_Vmag_1 (nr__1) ! (mag) ? Photometric error in V (3)
real*4 B_V_1 (nr__1) ! (mag) ? B-V colour
real*4 e_B_V_1 (nr__1) ! (mag) ? Photometric error in B-V (3)
real*4 U_B_1 (nr__1) ! (mag) ? U-B colour (4)
real*4 e_U_B_1 (nr__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 (nr__2) ! (deg) Right Ascension J2000
real*8 DEdeg_2 (nr__2) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*8 FldSeq_2 (nr__2) ! *Field Sequence (1)
integer*4 RAh_2 (nr__2) ! (h) Right Ascension J2000 (hours) (2)
integer*4 RAm_2 (nr__2) ! (min) Right Ascension J2000 (minutes)
real*4 RAs_2 (nr__2) ! (s) Right Ascension J2000 (seconds)
character*1 DE__2 (nr__2) ! Declination J2000 (sign) (2)
integer*4 DEd_2 (nr__2) ! (deg) Declination J2000 (degrees)
integer*4 DEm_2 (nr__2) ! (arcmin) Declination J2000 (minutes)
real*4 DEs_2 (nr__2) ! (arcsec) Declination J2000 (seconds)
real*4 Vmag_2 (nr__2) ! (mag) ? V magnitude
real*4 e_Vmag_2 (nr__2) ! (mag) ? Photometric error in V (3)
real*4 B_V_2 (nr__2) ! (mag) ? B-V colour
real*4 e_B_V_2 (nr__2) ! (mag) ? Photometric error in B-V (3)
real*4 U_B_2 (nr__2) ! (mag) ? U-B colour (4)
real*4 e_U_B_2 (nr__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 (nr__3) ! (deg) Right Ascension J2000
real*8 DEdeg_3 (nr__3) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*8 FldSeq_3 (nr__3) ! *Field Sequence (1)
integer*4 RAh_3 (nr__3) ! (h) Right Ascension J2000 (hours) (2)
integer*4 RAm_3 (nr__3) ! (min) Right Ascension J2000 (minutes)
real*4 RAs_3 (nr__3) ! (s) Right Ascension J2000 (seconds)
character*1 DE__3 (nr__3) ! Declination J2000 (sign) (2)
integer*4 DEd_3 (nr__3) ! (deg) Declination J2000 (degrees)
integer*4 DEm_3 (nr__3) ! (arcmin) Declination J2000 (minutes)
real*4 DEs_3 (nr__3) ! (arcsec) Declination J2000 (seconds)
real*4 Vmag_3 (nr__3) ! (mag) ? V magnitude
real*4 e_Vmag_3 (nr__3) ! (mag) ? Photometric error in V (3)
real*4 B_V_3 (nr__3) ! (mag) ? B-V colour
real*4 e_B_V_3 (nr__3) ! (mag) ? Photometric error in B-V (3)
real*4 U_B_3 (nr__3) ! (mag) ? U-B colour (4)
real*4 e_U_B_3 (nr__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 (nr__4) ! (deg) Right Ascension J2000
real*8 DEdeg_4 (nr__4) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*8 FldSeq_4 (nr__4) ! *Field Sequence (1)
integer*4 RAh_4 (nr__4) ! (h) Right Ascension J2000 (hours) (2)
integer*4 RAm_4 (nr__4) ! (min) Right Ascension J2000 (minutes)
real*4 RAs_4 (nr__4) ! (s) Right Ascension J2000 (seconds)
character*1 DE__4 (nr__4) ! Declination J2000 (sign) (2)
integer*4 DEd_4 (nr__4) ! (deg) Declination J2000 (degrees)
integer*4 DEm_4 (nr__4) ! (arcmin) Declination J2000 (minutes)
real*4 DEs_4 (nr__4) ! (arcsec) Declination J2000 (seconds)
real*4 Vmag_4 (nr__4) ! (mag) ? V magnitude
real*4 e_Vmag_4 (nr__4) ! (mag) ? Photometric error in V (3)
real*4 B_V_4 (nr__4) ! (mag) ? B-V colour
real*4 e_B_V_4 (nr__4) ! (mag) ? Photometric error in B-V (3)
real*4 U_B_4 (nr__4) ! (mag) ? U-B colour (4)
real*4 e_U_B_4 (nr__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 (nr__5) ! (deg) Right Ascension J2000
real*8 DEdeg_5 (nr__5) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*8 FldSeq_5 (nr__5) ! *Field Sequence (1)
integer*4 RAh_5 (nr__5) ! (h) Right Ascension J2000 (hours) (2)
integer*4 RAm_5 (nr__5) ! (min) Right Ascension J2000 (minutes)
real*4 RAs_5 (nr__5) ! (s) Right Ascension J2000 (seconds)
character*1 DE__5 (nr__5) ! Declination J2000 (sign) (2)
integer*4 DEd_5 (nr__5) ! (deg) Declination J2000 (degrees)
integer*4 DEm_5 (nr__5) ! (arcmin) Declination J2000 (minutes)
real*4 DEs_5 (nr__5) ! (arcsec) Declination J2000 (seconds)
real*4 Vmag_5 (nr__5) ! (mag) ? V magnitude
real*4 e_Vmag_5 (nr__5) ! (mag) ? Photometric error in V (3)
real*4 B_V_5 (nr__5) ! (mag) ? B-V colour
real*4 e_B_V_5 (nr__5) ! (mag) ? Photometric error in B-V (3)
real*4 U_B_5 (nr__5) ! (mag) ? U-B colour (4)
real*4 e_U_B_5 (nr__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 (nr__6) ! (deg) Right Ascension J2000
real*8 DEdeg_6 (nr__6) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*8 FldSeq_6 (nr__6) ! *Field Sequence (1)
integer*4 RAh_6 (nr__6) ! (h) Right Ascension J2000 (hours) (2)
integer*4 RAm_6 (nr__6) ! (min) Right Ascension J2000 (minutes)
real*4 RAs_6 (nr__6) ! (s) Right Ascension J2000 (seconds)
character*1 DE__6 (nr__6) ! Declination J2000 (sign) (2)
integer*4 DEd_6 (nr__6) ! (deg) Declination J2000 (degrees)
integer*4 DEm_6 (nr__6) ! (arcmin) Declination J2000 (minutes)
real*4 DEs_6 (nr__6) ! (arcsec) Declination J2000 (seconds)
real*4 Vmag_6 (nr__6) ! (mag) ? V magnitude
real*4 e_Vmag_6 (nr__6) ! (mag) ? Photometric error in V (3)
real*4 B_V_6 (nr__6) ! (mag) ? B-V colour
real*4 e_B_V_6 (nr__6) ! (mag) ? Photometric error in B-V (3)
real*4 U_B_6 (nr__6) ! (mag) ? U-B colour (4)
real*4 e_U_B_6 (nr__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 (nr__7) ! (deg) Right Ascension J2000
real*8 DEdeg_7 (nr__7) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*8 FldSeq_7 (nr__7) ! *Field Sequence (1)
integer*4 RAh_7 (nr__7) ! (h) Right Ascension J2000 (hours) (2)
integer*4 RAm_7 (nr__7) ! (min) Right Ascension J2000 (minutes)
real*4 RAs_7 (nr__7) ! (s) Right Ascension J2000 (seconds)
character*1 DE__7 (nr__7) ! Declination J2000 (sign) (2)
integer*4 DEd_7 (nr__7) ! (deg) Declination J2000 (degrees)
integer*4 DEm_7 (nr__7) ! (arcmin) Declination J2000 (minutes)
real*4 DEs_7 (nr__7) ! (arcsec) Declination J2000 (seconds)
real*4 Vmag_7 (nr__7) ! (mag) ? V magnitude
real*4 e_Vmag_7 (nr__7) ! (mag) ? Photometric error in V (3)
real*4 B_V_7 (nr__7) ! (mag) ? B-V colour
real*4 e_B_V_7 (nr__7) ! (mag) ? Photometric error in B-V (3)
real*4 U_B_7 (nr__7) ! (mag) ? U-B colour (4)
real*4 e_U_B_7 (nr__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(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Vmag(i__),e_Vmag(i__),B_V(i__),e_B_V(i__),
+ U_B(i__),e_U_B(i__)
if(ar__(37:42) .EQ. '') Vmag(i__) = rNULL__
if(ar__(44:48) .EQ. '') e_Vmag(i__) = rNULL__
if(ar__(50:55) .EQ. '') B_V(i__) = rNULL__
if(ar__(57:61) .EQ. '') e_B_V(i__) = rNULL__
if(ar__(63:68) .EQ. '') U_B(i__) = rNULL__
if(ar__(70:74) .EQ. '') e_U_B(i__) = rNULL__
RAdeg(i__) = rNULL__
DEdeg(i__) = rNULL__
c Derive coordinates RAdeg and DEdeg from input data
c (RAdeg and DEdeg are set to rNULL__ when unknown)
if(RAh(i__) .GT. -180) RAdeg(i__)=RAh(i__)*15.
if(RAm(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAm(i__)/4.
if(RAs(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAs(i__)/240.
if(DEd(i__) .GE. 0) DEdeg(i__)=DEd(i__)
if(DEm(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEm(i__)/60.
if(DEs(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEs(i__)/3600.
if(DE_(i__).EQ.'-'.AND.DEdeg(i__).GE.0) DEdeg(i__)=-DEdeg(i__)
c ..............Just test output...........
write(6,1)
+ FldSeq(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Vmag(i__),e_Vmag(i__),B_V(i__),e_B_V(i__),
+ U_B(i__),e_U_B(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
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(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),Vmag_1(i__),e_Vmag_1(i__),
+ B_V_1(i__),e_B_V_1(i__),U_B_1(i__),e_U_B_1(i__)
if(ar__1(37:42) .EQ. '') Vmag_1(i__) = rNULL__
if(ar__1(44:48) .EQ. '') e_Vmag_1(i__) = rNULL__
if(ar__1(50:55) .EQ. '') B_V_1(i__) = rNULL__
if(ar__1(57:61) .EQ. '') e_B_V_1(i__) = rNULL__
if(ar__1(63:68) .EQ. '') U_B_1(i__) = rNULL__
if(ar__1(70:74) .EQ. '') e_U_B_1(i__) = rNULL__
RAdeg_1(i__) = rNULL__
DEdeg_1(i__) = 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(i__) .GT. -180) RAdeg_1(i__)=RAh_1(i__)*15.
if(RAm_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAm_1(i__)/4.
if(RAs_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAs_1(i__)/240.
if(DEd_1(i__) .GE. 0) DEdeg_1(i__)=DEd_1(i__)
if(DEm_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEm_1(i__)/60.
if(DEs_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEs_1(i__)/3600.
if(DE__1(i__).EQ.'-'.AND.DEdeg_1(i__).GE.0) DEdeg_1(i__)=-DEdeg_1(i__)
c ..............Just test output...........
write(6,2)
+ FldSeq_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),Vmag_1(i__),e_Vmag_1(i__),
+ B_V_1(i__),e_B_V_1(i__),U_B_1(i__),e_U_B_1(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__)
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(i__),RAh_2(i__),RAm_2(i__),RAs_2(i__),DE__2(i__),
+ DEd_2(i__),DEm_2(i__),DEs_2(i__),Vmag_2(i__),e_Vmag_2(i__),
+ B_V_2(i__),e_B_V_2(i__),U_B_2(i__),e_U_B_2(i__)
if(ar__2(37:42) .EQ. '') Vmag_2(i__) = rNULL__
if(ar__2(44:48) .EQ. '') e_Vmag_2(i__) = rNULL__
if(ar__2(50:55) .EQ. '') B_V_2(i__) = rNULL__
if(ar__2(57:61) .EQ. '') e_B_V_2(i__) = rNULL__
if(ar__2(63:68) .EQ. '') U_B_2(i__) = rNULL__
if(ar__2(70:74) .EQ. '') e_U_B_2(i__) = rNULL__
RAdeg_2(i__) = rNULL__
DEdeg_2(i__) = 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(i__) .GT. -180) RAdeg_2(i__)=RAh_2(i__)*15.
if(RAm_2(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAm_2(i__)/4.
if(RAs_2(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAs_2(i__)/240.
if(DEd_2(i__) .GE. 0) DEdeg_2(i__)=DEd_2(i__)
if(DEm_2(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEm_2(i__)/60.
if(DEs_2(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEs_2(i__)/3600.
if(DE__2(i__).EQ.'-'.AND.DEdeg_2(i__).GE.0) DEdeg_2(i__)=-DEdeg_2(i__)
c ..............Just test output...........
write(6,3)
+ FldSeq_2(i__),RAh_2(i__),RAm_2(i__),RAs_2(i__),DE__2(i__),
+ DEd_2(i__),DEm_2(i__),DEs_2(i__),Vmag_2(i__),e_Vmag_2(i__),
+ B_V_2(i__),e_B_V_2(i__),U_B_2(i__),e_U_B_2(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_2(i__),DEdeg_2(i__)
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(i__),RAh_3(i__),RAm_3(i__),RAs_3(i__),DE__3(i__),
+ DEd_3(i__),DEm_3(i__),DEs_3(i__),Vmag_3(i__),e_Vmag_3(i__),
+ B_V_3(i__),e_B_V_3(i__),U_B_3(i__),e_U_B_3(i__)
if(ar__3(37:42) .EQ. '') Vmag_3(i__) = rNULL__
if(ar__3(44:48) .EQ. '') e_Vmag_3(i__) = rNULL__
if(ar__3(50:55) .EQ. '') B_V_3(i__) = rNULL__
if(ar__3(57:61) .EQ. '') e_B_V_3(i__) = rNULL__
if(ar__3(63:68) .EQ. '') U_B_3(i__) = rNULL__
if(ar__3(70:74) .EQ. '') e_U_B_3(i__) = rNULL__
RAdeg_3(i__) = rNULL__
DEdeg_3(i__) = 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(i__) .GT. -180) RAdeg_3(i__)=RAh_3(i__)*15.
if(RAm_3(i__) .GT. -180) RAdeg_3(i__)=RAdeg_3(i__)+RAm_3(i__)/4.
if(RAs_3(i__) .GT. -180) RAdeg_3(i__)=RAdeg_3(i__)+RAs_3(i__)/240.
if(DEd_3(i__) .GE. 0) DEdeg_3(i__)=DEd_3(i__)
if(DEm_3(i__) .GE. 0) DEdeg_3(i__)=DEdeg_3(i__)+DEm_3(i__)/60.
if(DEs_3(i__) .GE. 0) DEdeg_3(i__)=DEdeg_3(i__)+DEs_3(i__)/3600.
if(DE__3(i__).EQ.'-'.AND.DEdeg_3(i__).GE.0) DEdeg_3(i__)=-DEdeg_3(i__)
c ..............Just test output...........
write(6,4)
+ FldSeq_3(i__),RAh_3(i__),RAm_3(i__),RAs_3(i__),DE__3(i__),
+ DEd_3(i__),DEm_3(i__),DEs_3(i__),Vmag_3(i__),e_Vmag_3(i__),
+ B_V_3(i__),e_B_V_3(i__),U_B_3(i__),e_U_B_3(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_3(i__),DEdeg_3(i__)
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(i__),RAh_4(i__),RAm_4(i__),RAs_4(i__),DE__4(i__),
+ DEd_4(i__),DEm_4(i__),DEs_4(i__),Vmag_4(i__),e_Vmag_4(i__),
+ B_V_4(i__),e_B_V_4(i__),U_B_4(i__),e_U_B_4(i__)
if(ar__4(37:42) .EQ. '') Vmag_4(i__) = rNULL__
if(ar__4(44:48) .EQ. '') e_Vmag_4(i__) = rNULL__
if(ar__4(50:55) .EQ. '') B_V_4(i__) = rNULL__
if(ar__4(57:61) .EQ. '') e_B_V_4(i__) = rNULL__
if(ar__4(63:68) .EQ. '') U_B_4(i__) = rNULL__
if(ar__4(70:74) .EQ. '') e_U_B_4(i__) = rNULL__
RAdeg_4(i__) = rNULL__
DEdeg_4(i__) = 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(i__) .GT. -180) RAdeg_4(i__)=RAh_4(i__)*15.
if(RAm_4(i__) .GT. -180) RAdeg_4(i__)=RAdeg_4(i__)+RAm_4(i__)/4.
if(RAs_4(i__) .GT. -180) RAdeg_4(i__)=RAdeg_4(i__)+RAs_4(i__)/240.
if(DEd_4(i__) .GE. 0) DEdeg_4(i__)=DEd_4(i__)
if(DEm_4(i__) .GE. 0) DEdeg_4(i__)=DEdeg_4(i__)+DEm_4(i__)/60.
if(DEs_4(i__) .GE. 0) DEdeg_4(i__)=DEdeg_4(i__)+DEs_4(i__)/3600.
if(DE__4(i__).EQ.'-'.AND.DEdeg_4(i__).GE.0) DEdeg_4(i__)=-DEdeg_4(i__)
c ..............Just test output...........
write(6,5)
+ FldSeq_4(i__),RAh_4(i__),RAm_4(i__),RAs_4(i__),DE__4(i__),
+ DEd_4(i__),DEm_4(i__),DEs_4(i__),Vmag_4(i__),e_Vmag_4(i__),
+ B_V_4(i__),e_B_V_4(i__),U_B_4(i__),e_U_B_4(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_4(i__),DEdeg_4(i__)
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(i__),RAh_5(i__),RAm_5(i__),RAs_5(i__),DE__5(i__),
+ DEd_5(i__),DEm_5(i__),DEs_5(i__),Vmag_5(i__),e_Vmag_5(i__),
+ B_V_5(i__),e_B_V_5(i__),U_B_5(i__),e_U_B_5(i__)
if(ar__5(37:42) .EQ. '') Vmag_5(i__) = rNULL__
if(ar__5(44:48) .EQ. '') e_Vmag_5(i__) = rNULL__
if(ar__5(50:55) .EQ. '') B_V_5(i__) = rNULL__
if(ar__5(57:61) .EQ. '') e_B_V_5(i__) = rNULL__
if(ar__5(63:68) .EQ. '') U_B_5(i__) = rNULL__
if(ar__5(70:74) .EQ. '') e_U_B_5(i__) = rNULL__
RAdeg_5(i__) = rNULL__
DEdeg_5(i__) = 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(i__) .GT. -180) RAdeg_5(i__)=RAh_5(i__)*15.
if(RAm_5(i__) .GT. -180) RAdeg_5(i__)=RAdeg_5(i__)+RAm_5(i__)/4.
if(RAs_5(i__) .GT. -180) RAdeg_5(i__)=RAdeg_5(i__)+RAs_5(i__)/240.
if(DEd_5(i__) .GE. 0) DEdeg_5(i__)=DEd_5(i__)
if(DEm_5(i__) .GE. 0) DEdeg_5(i__)=DEdeg_5(i__)+DEm_5(i__)/60.
if(DEs_5(i__) .GE. 0) DEdeg_5(i__)=DEdeg_5(i__)+DEs_5(i__)/3600.
if(DE__5(i__).EQ.'-'.AND.DEdeg_5(i__).GE.0) DEdeg_5(i__)=-DEdeg_5(i__)
c ..............Just test output...........
write(6,6)
+ FldSeq_5(i__),RAh_5(i__),RAm_5(i__),RAs_5(i__),DE__5(i__),
+ DEd_5(i__),DEm_5(i__),DEs_5(i__),Vmag_5(i__),e_Vmag_5(i__),
+ B_V_5(i__),e_B_V_5(i__),U_B_5(i__),e_U_B_5(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_5(i__),DEdeg_5(i__)
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(i__),RAh_6(i__),RAm_6(i__),RAs_6(i__),DE__6(i__),
+ DEd_6(i__),DEm_6(i__),DEs_6(i__),Vmag_6(i__),e_Vmag_6(i__),
+ B_V_6(i__),e_B_V_6(i__),U_B_6(i__),e_U_B_6(i__)
if(ar__6(37:42) .EQ. '') Vmag_6(i__) = rNULL__
if(ar__6(44:48) .EQ. '') e_Vmag_6(i__) = rNULL__
if(ar__6(50:55) .EQ. '') B_V_6(i__) = rNULL__
if(ar__6(57:61) .EQ. '') e_B_V_6(i__) = rNULL__
if(ar__6(63:68) .EQ. '') U_B_6(i__) = rNULL__
if(ar__6(70:74) .EQ. '') e_U_B_6(i__) = rNULL__
RAdeg_6(i__) = rNULL__
DEdeg_6(i__) = 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(i__) .GT. -180) RAdeg_6(i__)=RAh_6(i__)*15.
if(RAm_6(i__) .GT. -180) RAdeg_6(i__)=RAdeg_6(i__)+RAm_6(i__)/4.
if(RAs_6(i__) .GT. -180) RAdeg_6(i__)=RAdeg_6(i__)+RAs_6(i__)/240.
if(DEd_6(i__) .GE. 0) DEdeg_6(i__)=DEd_6(i__)
if(DEm_6(i__) .GE. 0) DEdeg_6(i__)=DEdeg_6(i__)+DEm_6(i__)/60.
if(DEs_6(i__) .GE. 0) DEdeg_6(i__)=DEdeg_6(i__)+DEs_6(i__)/3600.
if(DE__6(i__).EQ.'-'.AND.DEdeg_6(i__).GE.0) DEdeg_6(i__)=-DEdeg_6(i__)
c ..............Just test output...........
write(6,7)
+ FldSeq_6(i__),RAh_6(i__),RAm_6(i__),RAs_6(i__),DE__6(i__),
+ DEd_6(i__),DEm_6(i__),DEs_6(i__),Vmag_6(i__),e_Vmag_6(i__),
+ B_V_6(i__),e_B_V_6(i__),U_B_6(i__),e_U_B_6(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_6(i__),DEdeg_6(i__)
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(i__),RAh_7(i__),RAm_7(i__),RAs_7(i__),DE__7(i__),
+ DEd_7(i__),DEm_7(i__),DEs_7(i__),Vmag_7(i__),e_Vmag_7(i__),
+ B_V_7(i__),e_B_V_7(i__),U_B_7(i__),e_U_B_7(i__)
if(ar__7(37:42) .EQ. '') Vmag_7(i__) = rNULL__
if(ar__7(44:48) .EQ. '') e_Vmag_7(i__) = rNULL__
if(ar__7(50:55) .EQ. '') B_V_7(i__) = rNULL__
if(ar__7(57:61) .EQ. '') e_B_V_7(i__) = rNULL__
if(ar__7(63:68) .EQ. '') U_B_7(i__) = rNULL__
if(ar__7(70:74) .EQ. '') e_U_B_7(i__) = rNULL__
RAdeg_7(i__) = rNULL__
DEdeg_7(i__) = 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(i__) .GT. -180) RAdeg_7(i__)=RAh_7(i__)*15.
if(RAm_7(i__) .GT. -180) RAdeg_7(i__)=RAdeg_7(i__)+RAm_7(i__)/4.
if(RAs_7(i__) .GT. -180) RAdeg_7(i__)=RAdeg_7(i__)+RAs_7(i__)/240.
if(DEd_7(i__) .GE. 0) DEdeg_7(i__)=DEd_7(i__)
if(DEm_7(i__) .GE. 0) DEdeg_7(i__)=DEdeg_7(i__)+DEm_7(i__)/60.
if(DEs_7(i__) .GE. 0) DEdeg_7(i__)=DEdeg_7(i__)+DEs_7(i__)/3600.
if(DE__7(i__).EQ.'-'.AND.DEdeg_7(i__).GE.0) DEdeg_7(i__)=-DEdeg_7(i__)
c ..............Just test output...........
write(6,8)
+ FldSeq_7(i__),RAh_7(i__),RAm_7(i__),RAs_7(i__),DE__7(i__),
+ DEd_7(i__),DEm_7(i__),DEs_7(i__),Vmag_7(i__),e_Vmag_7(i__),
+ B_V_7(i__),e_B_V_7(i__),U_B_7(i__),e_U_B_7(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_7(i__),DEdeg_7(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end