Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/636/1098 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 2024-Apr-20
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/ApJ/636/1098 Debris disks around solar-type stars (Bryden+, 2006)
*================================================================================
*Frequency of debris disks around solar-type stars: first results from a Spitzer
*MIPS survey.
* Bryden G., Beichman C.A., Trilling D.E., Rieke G.H., Holmes E.K.,
* Lawler S.M., Stapelfeldt K.R., Werner M.W., Gautier T.N., Blaylock M.,
* Gordon K.D., Stansberry J.A., Su K.Y.L.
* <Astrophys. J., 636, 1098-1113 (2006)>
* =2006ApJ...636.1098B
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! FGK survey stars
integer*4 nr__
parameter (nr__=127) ! Number of records
character*92 ar__ ! Full-size record
integer*4 HD ! The HD number (Cat. III/135)
character*3 n_HD ! [ab] a = Observed, b = Known planet-bearing star.
character*8 SpType ! SIMBAD MK spectral type
real*4 Vmag ! (mag) SIMBAD visual magnitude (2)
real*4 Age ! (Gyr) ? The Wright et al. (2004, Cat. J/ApJS/152/261)
* age (3)
real*4 AgeMin ! (Gyr) ? Minimum age
real*4 AgeMax ! (Gyr) ? Maximum age
character*14 r_Age ! Reference(s) for Age
real*4 v_Fe_H_ ! ([Sun]) ? The average [Fe/H] abundance
real*4 e__Fe_H_ ! ([Sun]) ? Dispersion in Abund
integer*4 o__Fe_H_ ! Number of estimates in Abund
character*21 Refs ! Additional reference(s)
*Note (2): Typically from the Hipparcos satellite.
*Note (3): Or an average of other estimates if Wright data is unavailable.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'refs.dat' ! References
integer*4 nr__1
parameter (nr__1=31) ! Number of records
character*113 ar__1 ! Full-size record
character*2 Ref ! Reference code
character*19 Bibcode ! Bibcode
character*24 Aut ! Author's name
character*65 Com ! Comment
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Measured and predicted fluxes at 24 and 70{mu}m
integer*4 nr__2
parameter (nr__2=69) ! Number of records
character*72 ar__2 ! Full-size record
integer*4 HD_1 ! The HD number
character*1 n_HD_1 ! [de] Note on IR excess (1)
real*4 MIPS24um ! (mJy) Measured MIPS 24{mu}m flux density
real*4 Star24um ! (mJy) Predicted 24{mu}m flux density
real*4 Rat24um ! The MIPS/predicted 24{mu}m flux density ratio
real*4 MIPS70um ! (mJy) Measured MIPS 70{mu}m flux density
real*4 e_MIPS70um ! (mJy) Uncertainty in MIPS70um
real*4 Star70um ! (mJy) Predicted 70{mu}m flux density
real*4 Rat70um ! The MIPS/predicted 70{mu}m flux density ratio
real*4 S_N ! The 70{mu}m signal-to-noise ratio
real*4 chi70 ! Significance of excess (Eq. 1)
real*4 FDust ! (mJy) ? Dust flux density at 70{mu}m (2)
character*1 l_LDust ! Limit flag on LDust
real*4 LDust ! Dust luminosity from 70{mu}m emission (3)
*Note (1): Flag on HD, defined as follows:
* d = star with excess 70{mu}m emission;
* e = star with excess 24{mu}m emission.
*Note (2): 70{mu}m dust fluxes have been color corrected by 15%, appropriate
* for ~50K emission.
*Note (3): See Eq. 3. In units of the stellar luminosity
C=============================================================================
C Loading file 'table1.dat' ! FGK survey stars
C Format for file interpretation
1 format(
+ 3X,I6,1X,A3,1X,A8,1X,F4.2,1X,F4.1,1X,F4.2,1X,F4.1,1X,A14,1X,
+ F5.2,1X,F4.2,1X,I1,1X,A21)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,127
read(1,'(A92)')ar__
read(ar__,1)
+ HD,n_HD,SpType,Vmag,Age,AgeMin,AgeMax,r_Age,v_Fe_H_,e__Fe_H_,
+ o__Fe_H_,Refs
if(ar__(29:32) .EQ. '') Age = rNULL__
if(ar__(34:37) .EQ. '') AgeMin = rNULL__
if(ar__(39:42) .EQ. '') AgeMax = rNULL__
if(ar__(59:63) .EQ. '') v_Fe_H_ = rNULL__
if(ar__(65:68) .EQ. '') e__Fe_H_ = rNULL__
c ..............Just test output...........
write(6,1)
+ HD,n_HD,SpType,Vmag,Age,AgeMin,AgeMax,r_Age,v_Fe_H_,e__Fe_H_,
+ o__Fe_H_,Refs
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'refs.dat' ! References
C Format for file interpretation
2 format(A2,1X,A19,1X,A24,1X,A65)
C Effective file loading
open(unit=1,status='old',file=
+'refs.dat')
write(6,*) '....Loading file: refs.dat'
do i__=1,31
read(1,'(A113)')ar__1
read(ar__1,2)Ref,Bibcode,Aut,Com
c ..............Just test output...........
write(6,2)Ref,Bibcode,Aut,Com
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Measured and predicted fluxes at 24 and 70{mu}m
C Format for file interpretation
3 format(
+ I6,1X,A1,1X,F6.1,1X,F6.1,1X,F4.2,1X,F5.1,1X,F4.1,1X,F5.1,1X,
+ F3.1,1X,F4.1,1X,F4.1,1X,F5.1,1X,A1,E6.2)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,69
read(1,'(A72)')ar__2
read(ar__2,3)
+ HD_1,n_HD_1,MIPS24um,Star24um,Rat24um,MIPS70um,e_MIPS70um,
+ Star70um,Rat70um,S_N,chi70,FDust,l_LDust,LDust
if(ar__2(60:64) .EQ. '') FDust = rNULL__
c ..............Just test output...........
write(6,3)
+ HD_1,n_HD_1,MIPS24um,Star24um,Rat24um,MIPS70um,e_MIPS70um,
+ Star70um,Rat70um,S_N,chi70,FDust,l_LDust,LDust
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end