Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJS/119/141 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-Aug-11
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/ApJS/119/141 Oxygen-rich dust shells IR spectral classification (Sloan+ 1998)
*================================================================================
*The infrared spectral classification of oxygen-rich dust shells.
* Sloan G.C., Price S.D.
* <Astrophys. J. Suppl. Ser. 119, 141 (1998)>
* =1998ApJS..119..141S
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! Infrared spectral classifications of the AGB sample
integer*4 nr__
parameter (nr__=546) ! Number of records
character*92 ar__ ! Full-size record
character*10 IRAS ! IRA-PSC (Cat. <II/125>) designation
character*1 m_IRAS ! Multilicity index on IRAS
character*12 Name ! Name
character*9 Var ! Variability type (1)
real*4 Per ! (d) ? Period
character*17 SpType ! Spectral Type
real*4 v12um ! (mag) 12{mu}m magnitude
real*4 v_12___25_ ! (mag) Colour index [12]-[25]
integer*4 LRS ! ? LRS characterisations described in the LRS
* Atlas
real*4 DEC ! Dust emission contrast (2)
real*4 F11_F12 ! Corrected flux ratio F11{mu}m/F12{mu}m
character*5 Dust ! Infrared emission class (3)
*Note (1): M: Mira Ceti-type variables
* Lb: Slow irregular variable of late spectral type
* SRa: Semiregular late-type giants displaying persistent periodicity
* and usually small light amplitudes
* SRb: Semiregular late-type giants with poorly defined periodicity, or
* with alternating intervals of periodic and slow irregular changes,
* and even with light constancy intervals
*Note (2): Ratio of the summed emission from the dust to the summed emission from
* the star over the interval 7.67-14.03{mu}m.
*Note (3): N: Naked (no dust)
* SE: Silicate (and oxygen-rich dust) emission
* SB: Silicate self-absorbed emission
* SA: Silicate absorption
* CE: Carbon-rich dust emission
* H: Very red spectrum (possible H II region)
* P: Peculiar (or noisy)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! Infrared spectral classifications of the supergiants
integer*4 nr__1
parameter (nr__1=65) ! Number of records
character*92 ar__1 ! Full-size record
character*10 IRAS_1 ! IRA-PSC (Cat. <II/125>) designation
character*1 m_IRAS_1 ! Multilicity index on IRAS
character*12 Name_1 ! Name
character*9 Var_1 ! Variability type (1)
real*4 Per_1 ! (d) ? Period
character*17 SpType_1 ! Spectral Type
real*4 v12um_1 ! (mag) 12{mu}m magnitude
real*4 v_12___25__1 ! (mag) Colour index [12]-[25]
integer*4 LRS_1 ! ? LRS characterisations described in the LRS
* Atlas
real*4 DEC_1 ! Dust emission contrast (2)
real*4 F11_F12_1 ! Corrected flux ratio F11{mu}m/F12{mu}m
character*5 Dust_1 ! Infrared emission class (3)
*Note (1): M: Mira Ceti-type variables
* Lb: Slow irregular variable of late spectral type
* SRa: Semiregular late-type giants displaying persistent periodicity
* and usually small light amplitudes
* SRb: Semiregular late-type giants with poorly defined periodicity, or
* with alternating intervals of periodic and slow irregular changes,
* and even with light constancy intervals
*Note (2): Ratio of the summed emission from the dust to the summed emission from
* the star over the interval 7.67-14.03{mu}m.
*Note (3): N: Naked (no dust)
* SE: Silicate (and oxygen-rich dust) emission
* SB: Silicate self-absorbed emission
* SA: Silicate absorption
* CE: Carbon-rich dust emission
* H: Very red spectrum (possible H II region)
* P: Peculiar (or noisy)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6.dat' ! Infrared spectral classifications of the optical
S stars
integer*4 nr__2
parameter (nr__2=24) ! Number of records
character*92 ar__2 ! Full-size record
character*10 IRAS_2 ! IRA-PSC (Cat. <II/125>) designation
character*1 m_IRAS_2 ! Multilicity index on IRAS
character*12 Name_2 ! Name
character*9 Var_2 ! Variability type (1)
real*4 Per_2 ! (d) ? Period
character*17 SpType_2 ! Spectral Type
real*4 v12um_2 ! (mag) 12{mu}m magnitude
real*4 v_12___25__2 ! (mag) Colour index [12]-[25]
integer*4 LRS_2 ! ? LRS characterisations described in the LRS
* Atlas
real*4 DEC_2 ! Dust emission contrast (2)
real*4 F11_F12_2 ! Corrected flux ratio F11{mu}m/F12{mu}m
character*5 Dust_2 ! Infrared emission class (3)
*Note (1): M: Mira Ceti-type variables
* Lb: Slow irregular variable of late spectral type
* SRa: Semiregular late-type giants displaying persistent periodicity
* and usually small light amplitudes
* SRb: Semiregular late-type giants with poorly defined periodicity, or
* with alternating intervals of periodic and slow irregular changes,
* and even with light constancy intervals
*Note (2): Ratio of the summed emission from the dust to the summed emission from
* the star over the interval 7.67-14.03{mu}m.
*Note (3): N: Naked (no dust)
* SE: Silicate (and oxygen-rich dust) emission
* SB: Silicate self-absorbed emission
* SA: Silicate absorption
* CE: Carbon-rich dust emission
* H: Very red spectrum (possible H II region)
* P: Peculiar (or noisy)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table9.dat' ! MS (oxygen-rich AGB or supergiant) stars
integer*4 nr__3
parameter (nr__3=18) ! Number of records
character*10 ar__3 ! Full-size record
character*10 IRAS_3 ! IRAS-PSC designation
C=============================================================================
C Loading file 'table4.dat' ! Infrared spectral classifications of the AGB sample
C Format for file interpretation
1 format(
+ A10,A1,1X,A12,1X,A9,1X,F6.2,1X,A17,1X,F5.2,1X,F5.2,1X,I3,1X,
+ F5.2,1X,F4.2,1X,A5)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,546
read(1,'(A92)')ar__
read(ar__,1)
+ IRAS,m_IRAS,Name,Var,Per,SpType,v12um,v_12___25_,LRS,DEC,
+ F11_F12,Dust
if(ar__(36:41) .EQ. '') Per = rNULL__
if(ar__(73:75) .EQ. '') LRS = iNULL__
c ..............Just test output...........
write(6,1)
+ IRAS,m_IRAS,Name,Var,Per,SpType,v12um,v_12___25_,LRS,DEC,
+ F11_F12,Dust
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table5.dat' ! Infrared spectral classifications of the supergiants
C Format for file interpretation
2 format(
+ A10,A1,1X,A12,1X,A9,1X,F6.2,1X,A17,1X,F5.2,1X,F5.2,1X,I3,1X,
+ F5.2,1X,F4.2,1X,A5)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,65
read(1,'(A92)')ar__1
read(ar__1,2)
+ IRAS_1,m_IRAS_1,Name_1,Var_1,Per_1,SpType_1,v12um_1,
+ v_12___25__1,LRS_1,DEC_1,F11_F12_1,Dust_1
if(ar__1(36:41) .EQ. '') Per_1 = rNULL__
if(ar__1(73:75) .EQ. '') LRS_1 = iNULL__
c ..............Just test output...........
write(6,2)
+ IRAS_1,m_IRAS_1,Name_1,Var_1,Per_1,SpType_1,v12um_1,
+ v_12___25__1,LRS_1,DEC_1,F11_F12_1,Dust_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table6.dat' ! Infrared spectral classifications of the optical
* S stars
C Format for file interpretation
3 format(
+ A10,A1,1X,A12,1X,A9,1X,F6.2,1X,A17,1X,F5.2,1X,F5.2,1X,I3,1X,
+ F5.2,1X,F4.2,1X,A5)
C Effective file loading
open(unit=1,status='old',file=
+'table6.dat')
write(6,*) '....Loading file: table6.dat'
do i__=1,24
read(1,'(A92)')ar__2
read(ar__2,3)
+ IRAS_2,m_IRAS_2,Name_2,Var_2,Per_2,SpType_2,v12um_2,
+ v_12___25__2,LRS_2,DEC_2,F11_F12_2,Dust_2
if(ar__2(36:41) .EQ. '') Per_2 = rNULL__
if(ar__2(73:75) .EQ. '') LRS_2 = iNULL__
c ..............Just test output...........
write(6,3)
+ IRAS_2,m_IRAS_2,Name_2,Var_2,Per_2,SpType_2,v12um_2,
+ v_12___25__2,LRS_2,DEC_2,F11_F12_2,Dust_2
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table9.dat' ! MS (oxygen-rich AGB or supergiant) stars
C Format for file interpretation
4 format(A10)
C Effective file loading
open(unit=1,status='old',file=
+'table9.dat')
write(6,*) '....Loading file: table9.dat'
do i__=1,18
read(1,'(A10)')ar__3
read(ar__3,4)IRAS_3
c ..............Just test output...........
write(6,4)IRAS_3
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end