Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/118/1684 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-18
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/AJ/118/1684 UBV photometry of 4 LMC compact OB groups (Walborn+, 1999)
*================================================================================
*HST/FOS spatially resolved spectral classification of compact OB groups
*in the Large Magellanic Cloud.
* Walborn N.R., Drissen L., Parker J.W., Saha A., MacKenty J.W., White R.L.
* <Astron. J. 118, 1684 (1999)>
* =1999AJ....118.1684W
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Observed and derived parameters for the
components of Breysacher 73
integer*4 nr__
parameter (nr__=23) ! Number of records
character*91 ar__ ! Full-size record
integer*4 Seq (nr__) ! Sequential number (1)
real*4 Xpos (nr__) ! (pix) X position (1)
real*4 Ypos (nr__) ! (pix) Y position (1)
real*4 Vmag (nr__) ! (mag) HST/WFPC F569W V magnitude
character*1 n_Vmag (nr__) ! [e] discrepant photometry (2)
real*4 B_V (nr__) ! (mag) ? B-V colour index (F439W-F569W)
real*4 U_B (nr__) ! (mag) ? U-B colour index (F336W-F439W)
real*4 E_B_V (nr__) ! (mag) ? B-V colour excess
character*1 n_E_B_V (nr__) ! [ce] discrepant photometry (2)
real*4 logTe (nr__) ! ([K]) ? Effective temperature
real*4 Mbol (nr__) ! (mag) ? Bolometric magnitude
real*4 BC (nr__) ! (mag) ? Bolometric correction
character*15 SpType (nr__) ! MK spectral type (3)
character*1 n_SpType (nr__) ! [d] Note (3)
character*15 ID (nr__) ! Alternate ID (4)
*Note (1): Running number and detector coordinates from the present photometry,
* to be presented in full by Parker et al. in a subsequent paper.
* * In table1: <Brey 73 NN> in Simbad
* * In table2: <NGC 2044W NN> in Simbad
* * In table3: <LH 10-3209 NN> in Simbad
* * In table4: <HD 32228 NN> in Simbad
*Note (2): Notes as follows:
* c = The colors for these components were discrepant, so the average
* color excess of the other spectroscopically classified
* components was adopted instead
* e = The photometry for this component was discrepant, so the magnitude
* difference from component C in the V deconvolution and the average
* color excess of the other components were adopted for it instead.
*Note (3): Spectroscopy from HST Faint Object Spectrograph, unless
* d = Spectral type from Schild & Testor (1992A&AS...92..729S) or
* Heydari-Malayeri et al. (1993A&A...278...11H)
*Note (4): Alternative IDs refer to:
* * Table1:
* Tes = Testor et al. (1988Msngr..54...43T) with letters added
* here to the numbers to denote subsequently resolved components.
* * Table2:
* H-M = Heydari-Malayeri et al. (1993 A&A...278...11H) with letters
* added here to the numbers to denote subsequently resolved
* components.
* * Table3: See fig. 9 of the paper
* * Table4:
* Sch = Schertl et al. (1995A&A...302..327S)
* H-M = Heydari-Malayeri et al. (1983A&A...118..116H)
* with arabic numerals added here to the letters to denote
* subsequently resolved components.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Observed and derived parameters for the
components of NGC 2044 West
integer*4 nr__1
parameter (nr__1=38) ! Number of records
character*91 ar__1 ! Full-size record
integer*4 Seq_1 (nr__1) ! Sequential number (1)
real*4 Xpos_1 (nr__1) ! (pix) X position (1)
real*4 Ypos_1 (nr__1) ! (pix) Y position (1)
real*4 Vmag_1 (nr__1) ! (mag) HST/WFPC F569W V magnitude
character*1 n_Vmag_1 (nr__1) ! [e] discrepant photometry (2)
real*4 B_V_1 (nr__1) ! (mag) ? B-V colour index (F439W-F569W)
real*4 U_B_1 (nr__1) ! (mag) ? U-B colour index (F336W-F439W)
real*4 E_B_V_1 (nr__1) ! (mag) ? B-V colour excess
character*1 n_E_B_V_1 (nr__1) ! [ce] discrepant photometry (2)
real*4 logTe_1 (nr__1) ! ([K]) ? Effective temperature
real*4 Mbol_1 (nr__1) ! (mag) ? Bolometric magnitude
real*4 BC_1 (nr__1) ! (mag) ? Bolometric correction
character*15 SpType_1 (nr__1) ! MK spectral type (3)
character*1 n_SpType_1 (nr__1) ! [d] Note (3)
character*15 ID_1 (nr__1) ! Alternate ID (4)
*Note (1): Running number and detector coordinates from the present photometry,
* to be presented in full by Parker et al. in a subsequent paper.
* * In table1: <Brey 73 NN> in Simbad
* * In table2: <NGC 2044W NN> in Simbad
* * In table3: <LH 10-3209 NN> in Simbad
* * In table4: <HD 32228 NN> in Simbad
*Note (2): Notes as follows:
* c = The colors for these components were discrepant, so the average
* color excess of the other spectroscopically classified
* components was adopted instead
* e = The photometry for this component was discrepant, so the magnitude
* difference from component C in the V deconvolution and the average
* color excess of the other components were adopted for it instead.
*Note (3): Spectroscopy from HST Faint Object Spectrograph, unless
* d = Spectral type from Schild & Testor (1992A&AS...92..729S) or
* Heydari-Malayeri et al. (1993A&A...278...11H)
*Note (4): Alternative IDs refer to:
* * Table1:
* Tes = Testor et al. (1988Msngr..54...43T) with letters added
* here to the numbers to denote subsequently resolved components.
* * Table2:
* H-M = Heydari-Malayeri et al. (1993 A&A...278...11H) with letters
* added here to the numbers to denote subsequently resolved
* components.
* * Table3: See fig. 9 of the paper
* * Table4:
* Sch = Schertl et al. (1995A&A...302..327S)
* H-M = Heydari-Malayeri et al. (1983A&A...118..116H)
* with arabic numerals added here to the letters to denote
* subsequently resolved components.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Observed and derived parameters for the
components of LH 10-3209
integer*4 nr__2
parameter (nr__2=6) ! Number of records
character*91 ar__2 ! Full-size record
integer*4 Seq_2 (nr__2) ! Sequential number (1)
real*4 Xpos_2 (nr__2) ! (pix) X position (1)
real*4 Ypos_2 (nr__2) ! (pix) Y position (1)
real*4 Vmag_2 (nr__2) ! (mag) HST/WFPC F569W V magnitude
character*1 n_Vmag_2 (nr__2) ! [e] discrepant photometry (2)
real*4 B_V_2 (nr__2) ! (mag) ? B-V colour index (F439W-F569W)
real*4 U_B_2 (nr__2) ! (mag) ? U-B colour index (F336W-F439W)
real*4 E_B_V_1 (nr__2) ! (mag) ? B-V colour excess
character*1 n_E_B_V_1 (nr__2) ! [ce] discrepant photometry (2)
real*4 logTe_2 (nr__2) ! ([K]) ? Effective temperature
real*4 Mbol_2 (nr__2) ! (mag) ? Bolometric magnitude
real*4 BC_2 (nr__2) ! (mag) ? Bolometric correction
character*15 SpType_2 (nr__2) ! MK spectral type (3)
character*1 n_SpType_2 (nr__2) ! [d] Note (3)
character*15 ID_2 (nr__2) ! Alternate ID (4)
*Note (1): Running number and detector coordinates from the present photometry,
* to be presented in full by Parker et al. in a subsequent paper.
* * In table1: <Brey 73 NN> in Simbad
* * In table2: <NGC 2044W NN> in Simbad
* * In table3: <LH 10-3209 NN> in Simbad
* * In table4: <HD 32228 NN> in Simbad
*Note (2): Notes as follows:
* c = The colors for these components were discrepant, so the average
* color excess of the other spectroscopically classified
* components was adopted instead
* e = The photometry for this component was discrepant, so the magnitude
* difference from component C in the V deconvolution and the average
* color excess of the other components were adopted for it instead.
*Note (3): Spectroscopy from HST Faint Object Spectrograph, unless
* d = Spectral type from Schild & Testor (1992A&AS...92..729S) or
* Heydari-Malayeri et al. (1993A&A...278...11H)
*Note (4): Alternative IDs refer to:
* * Table1:
* Tes = Testor et al. (1988Msngr..54...43T) with letters added
* here to the numbers to denote subsequently resolved components.
* * Table2:
* H-M = Heydari-Malayeri et al. (1993 A&A...278...11H) with letters
* added here to the numbers to denote subsequently resolved
* components.
* * Table3: See fig. 9 of the paper
* * Table4:
* Sch = Schertl et al. (1995A&A...302..327S)
* H-M = Heydari-Malayeri et al. (1983A&A...118..116H)
* with arabic numerals added here to the letters to denote
* subsequently resolved components.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! Observed and derived parameters for the
components of HD 32228
integer*4 nr__3
parameter (nr__3=71) ! Number of records
character*91 ar__3 ! Full-size record
integer*4 Seq_3 (nr__3) ! Sequential number (1)
real*4 Xpos_3 (nr__3) ! (pix) X position (1)
real*4 Ypos_3 (nr__3) ! (pix) Y position (1)
real*4 Vmag_3 (nr__3) ! (mag) HST/WFPC F569W V magnitude
character*1 n_Vmag_3 (nr__3) ! [e] discrepant photometry (2)
real*4 B_V_3 (nr__3) ! (mag) ? B-V colour index (F439W-F569W)
real*4 U_B_3 (nr__3) ! (mag) ? U-B colour index (F336W-F439W)
real*4 E_B_V_1 (nr__3) ! (mag) ? B-V colour excess
character*1 n_E_B_V_1 (nr__3) ! [ce] discrepant photometry (2)
real*4 logTe_3 (nr__3) ! ([K]) ? Effective temperature
real*4 Mbol_3 (nr__3) ! (mag) ? Bolometric magnitude
real*4 BC_3 (nr__3) ! (mag) ? Bolometric correction
character*15 SpType_3 (nr__3) ! MK spectral type (3)
character*1 n_SpType_3 (nr__3) ! [d] Note (3)
character*15 ID_3 (nr__3) ! Alternate ID (4)
*Note (1): Running number and detector coordinates from the present photometry,
* to be presented in full by Parker et al. in a subsequent paper.
* * In table1: <Brey 73 NN> in Simbad
* * In table2: <NGC 2044W NN> in Simbad
* * In table3: <LH 10-3209 NN> in Simbad
* * In table4: <HD 32228 NN> in Simbad
*Note (2): Notes as follows:
* c = The colors for these components were discrepant, so the average
* color excess of the other spectroscopically classified
* components was adopted instead
* e = The photometry for this component was discrepant, so the magnitude
* difference from component C in the V deconvolution and the average
* color excess of the other components were adopted for it instead.
*Note (3): Spectroscopy from HST Faint Object Spectrograph, unless
* d = Spectral type from Schild & Testor (1992A&AS...92..729S) or
* Heydari-Malayeri et al. (1993A&A...278...11H)
*Note (4): Alternative IDs refer to:
* * Table1:
* Tes = Testor et al. (1988Msngr..54...43T) with letters added
* here to the numbers to denote subsequently resolved components.
* * Table2:
* H-M = Heydari-Malayeri et al. (1993 A&A...278...11H) with letters
* added here to the numbers to denote subsequently resolved
* components.
* * Table3: See fig. 9 of the paper
* * Table4:
* Sch = Schertl et al. (1995A&A...302..327S)
* H-M = Heydari-Malayeri et al. (1983A&A...118..116H)
* with arabic numerals added here to the letters to denote
* subsequently resolved components.
C=============================================================================
C Loading file 'table1.dat' ! Observed and derived parameters for the
* components of Breysacher 73
C Format for file interpretation
1 format(
+ I2,1X,F6.2,1X,F6.2,1X,F5.2,A1,F5.2,1X,F5.2,1X,F5.2,A1,F5.3,1X,
+ F6.2,1X,F5.2,1X,A15,A1,A15)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,23
read(1,'(A91)')ar__
read(ar__,1)
+ Seq(i__),Xpos(i__),Ypos(i__),Vmag(i__),n_Vmag(i__),B_V(i__),
+ U_B(i__),E_B_V(i__),n_E_B_V(i__),logTe(i__),Mbol(i__),BC(i__),
+ SpType(i__),n_SpType(i__),ID(i__)
if(ar__(24:28) .EQ. '') B_V(i__) = rNULL__
if(ar__(30:34) .EQ. '') U_B(i__) = rNULL__
if(ar__(36:40) .EQ. '') E_B_V(i__) = rNULL__
if(ar__(42:46) .EQ. '') logTe(i__) = rNULL__
if(ar__(48:53) .EQ. '') Mbol(i__) = rNULL__
if(ar__(55:59) .EQ. '') BC(i__) = rNULL__
c ..............Just test output...........
write(6,1)
+ Seq(i__),Xpos(i__),Ypos(i__),Vmag(i__),n_Vmag(i__),B_V(i__),
+ U_B(i__),E_B_V(i__),n_E_B_V(i__),logTe(i__),Mbol(i__),BC(i__),
+ SpType(i__),n_SpType(i__),ID(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Observed and derived parameters for the
* components of NGC 2044 West
C Format for file interpretation
2 format(
+ I2,1X,F6.2,1X,F6.2,1X,F5.2,A1,F5.2,1X,F5.2,1X,F5.2,A1,F5.3,1X,
+ F6.2,1X,F5.2,1X,A15,A1,A15)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,38
read(1,'(A91)')ar__1
read(ar__1,2)
+ Seq_1(i__),Xpos_1(i__),Ypos_1(i__),Vmag_1(i__),n_Vmag_1(i__),
+ B_V_1(i__),U_B_1(i__),E_B_V_1(i__),n_E_B_V_1(i__),
+ logTe_1(i__),Mbol_1(i__),BC_1(i__),SpType_1(i__),
+ n_SpType_1(i__),ID_1(i__)
if(ar__1(24:28) .EQ. '') B_V_1(i__) = rNULL__
if(ar__1(30:34) .EQ. '') U_B_1(i__) = rNULL__
if(ar__1(36:40) .EQ. '') E_B_V_1(i__) = rNULL__
if(ar__1(42:46) .EQ. '') logTe_1(i__) = rNULL__
if(ar__1(48:53) .EQ. '') Mbol_1(i__) = rNULL__
if(ar__1(55:59) .EQ. '') BC_1(i__) = rNULL__
c ..............Just test output...........
write(6,2)
+ Seq_1(i__),Xpos_1(i__),Ypos_1(i__),Vmag_1(i__),n_Vmag_1(i__),
+ B_V_1(i__),U_B_1(i__),E_B_V_1(i__),n_E_B_V_1(i__),
+ logTe_1(i__),Mbol_1(i__),BC_1(i__),SpType_1(i__),
+ n_SpType_1(i__),ID_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Observed and derived parameters for the
* components of LH 10-3209
C Format for file interpretation
3 format(
+ I2,1X,F6.2,1X,F6.2,1X,F5.2,A1,F5.2,1X,F5.2,1X,F5.2,A1,F5.3,1X,
+ F6.2,1X,F5.2,1X,A15,A1,A15)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,6
read(1,'(A91)')ar__2
read(ar__2,3)
+ Seq_2(i__),Xpos_2(i__),Ypos_2(i__),Vmag_2(i__),n_Vmag_2(i__),
+ B_V_2(i__),U_B_2(i__),E_B_V_1(i__),n_E_B_V_1(i__),
+ logTe_2(i__),Mbol_2(i__),BC_2(i__),SpType_2(i__),
+ n_SpType_2(i__),ID_2(i__)
if(ar__2(24:28) .EQ. '') B_V_2(i__) = rNULL__
if(ar__2(30:34) .EQ. '') U_B_2(i__) = rNULL__
if(ar__2(36:40) .EQ. '') E_B_V_1(i__) = rNULL__
if(ar__2(42:46) .EQ. '') logTe_2(i__) = rNULL__
if(ar__2(48:53) .EQ. '') Mbol_2(i__) = rNULL__
if(ar__2(55:59) .EQ. '') BC_2(i__) = rNULL__
c ..............Just test output...........
write(6,3)
+ Seq_2(i__),Xpos_2(i__),Ypos_2(i__),Vmag_2(i__),n_Vmag_2(i__),
+ B_V_2(i__),U_B_2(i__),E_B_V_1(i__),n_E_B_V_1(i__),
+ logTe_2(i__),Mbol_2(i__),BC_2(i__),SpType_2(i__),
+ n_SpType_2(i__),ID_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4.dat' ! Observed and derived parameters for the
* components of HD 32228
C Format for file interpretation
4 format(
+ I2,1X,F6.2,1X,F6.2,1X,F5.2,A1,F5.2,1X,F5.2,1X,F5.2,A1,F5.3,1X,
+ F6.2,1X,F5.2,1X,A15,A1,A15)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,71
read(1,'(A91)')ar__3
read(ar__3,4)
+ Seq_3(i__),Xpos_3(i__),Ypos_3(i__),Vmag_3(i__),n_Vmag_3(i__),
+ B_V_3(i__),U_B_3(i__),E_B_V_1(i__),n_E_B_V_1(i__),
+ logTe_3(i__),Mbol_3(i__),BC_3(i__),SpType_3(i__),
+ n_SpType_3(i__),ID_3(i__)
if(ar__3(24:28) .EQ. '') B_V_3(i__) = rNULL__
if(ar__3(30:34) .EQ. '') U_B_3(i__) = rNULL__
if(ar__3(36:40) .EQ. '') E_B_V_1(i__) = rNULL__
if(ar__3(42:46) .EQ. '') logTe_3(i__) = rNULL__
if(ar__3(48:53) .EQ. '') Mbol_3(i__) = rNULL__
if(ar__3(55:59) .EQ. '') BC_3(i__) = rNULL__
c ..............Just test output...........
write(6,4)
+ Seq_3(i__),Xpos_3(i__),Ypos_3(i__),Vmag_3(i__),n_Vmag_3(i__),
+ B_V_3(i__),U_B_3(i__),E_B_V_1(i__),n_E_B_V_1(i__),
+ logTe_3(i__),Mbol_3(i__),BC_3(i__),SpType_3(i__),
+ n_SpType_3(i__),ID_3(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end