Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/651/502 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-19
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/651/502 Spitzer IRAC photometry of M, L, and T dwarfs (Patten+, 2006)
*================================================================================
*Spitzer IRAC photometry of M, L, and T dwarfs.
* Patten B.M., Stauffer J.R., Burrows A., Marengo M., Hora J.L., Luhman K.L.,
* Sonnett S.M., Henry T.J., Raghavan D., Megeath S.T., Liebert J., Fazio G.G.
* <Astrophys. J., 651, 502-516 (2006)>
* =2006ApJ...651..502P
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Sample of late-type M, L, and T dwarfs: basic data
integer*4 nr__
parameter (nr__=86) ! Number of records
character*110 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)
character*15 Name ! Star name
character*1 n_Name ! [b] b: known binary
integer*4 RAh ! (h) Right ascension (J2000)
integer*4 RAm ! (min) Right ascension (J2000)
real*4 RAs ! (s) Right ascension (J2000)
character*1 DE_ ! Declination sign (J2000)
integer*4 DEd ! (deg) Declination (J2000)
integer*4 DEm ! (arcmin) Declination (J2000)
integer*4 DEs ! (arcsec) Declination (J2000)
character*9 SpT ! MK spectral type (1)
integer*4 r_SpT ! Spectral type reference, in refs.dat file
real*8 plx ! (arcsec) ? Parallax
real*8 e_plx ! (arcsec) ? rms uncertainty on plx
integer*4 r_plx ! ? Parallax reference, in refs.dat file
real*4 Jmag ! (mag) J magnitude
real*4 e_Jmag ! (mag) rms uncertainty on Jmag
real*4 Hmag ! (mag) H magnitude
real*4 e_Hmag ! (mag) rms uncertainty on Hmag
real*4 Ksmag ! (mag) Ks magnitude
real*4 e_Ksmag ! (mag) rms uncertainty on Ksmag
integer*4 r_Jmag ! JHK reference, in refs.dat file
character*3 Syst ! Photometry system (2)
*Note (1): Unless otherwise noted, optical spectral types are used for M and
* L dwarfs, and infrared spectral types are used for the T dwarfs.
*Note (2): Photometry system as follows:
* 2MA = 2MASS (Cat. II/246)
* MKO = MKO, Tokunaga et al., 2002PASP..114..180T
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! IRAC photometry and colors of late-type M, L, and
T dwarfs
integer*4 nr__1
parameter (nr__1=86) ! Number of records
character*108 ar__1 ! Full-size record
character*15 Name_1 ! Star name
character*1 n_Name_1 ! [b] b: known binary
character*9 SpT_1 ! MK spectral type
real*4 v_3_6_ ! (mag) IRAC 3.6um magnitude
real*4 e__3_6_ ! (mag) rms uncertainty on [3.6]
integer*4 o__3_6_ ! Number of observations in 3.6um
real*4 v_4_5_ ! (mag) IRAC 4.5um magnitude
real*4 e__4_5_ ! (mag) rms uncertainty on [4.5]
integer*4 o__4_5_ ! Number of observations in 4.5um
real*4 v_5_8_ ! (mag) IRAC 5.8um magnitude
real*4 e__5_8_ ! (mag) rms uncertainty on [5.8]
integer*4 o__5_8_ ! Number of observations in 5.8um
real*4 v_8_0_ ! (mag) IRAC 8.0um magnitude
real*4 e__8_0_ ! (mag) rms uncertainty on [8.0]
integer*4 o__8_0_ ! Number of observations in 8.0um
real*4 v_3_6___4_5_ ! (mag) IRAC [3.6]-[4.5] colour index
real*4 v_4_5___5_8_ ! (mag) IRAC [4.5]-[5.8] colour index
real*4 v_5_8___8_0_ ! (mag) IRAC [5.8]-[8.0] colour index
character*7 Notes ! Notes (1)
*Note (1): Notes as follows:
* 1 = Source saturated in all four IRAC channels in 30s FRAMETIME data;
* 2s FRAMETIME data used instead
* 2 = GTO program PID 33 target; 2s FRAMETIME data
* 3 = GTO program PID 33 target; 0.6s FRAMETIME data
* 4 = Channel 1 saturated for 30s FRAMETIME data; used 2s FRAMETIME
* data for this channel
* 5 = Channel 2 saturated for 30s FRAMETIME data; used 2s FRAMETIME
* data for this channel
* 6 = GTO program PID 33 target
* 7 = Target source aperture possibly contaminated by flux from
* another nearby source
* 8 = Target in crowded field; some contamination of source aperture by
* other nearby sources possible
* 9 = Spitzer AOR target name incorrectly reads 2MA 1410+1804
* 10 = Wings of GJ 1001 PSF may contaminate source aperture for target;
* however, 2s FRAMETIME data for channels 1 and 2 agree well with
* the 30s FRAMETIME data
* 11 = Strong nebulosity in background, especially in channel 4
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'refs.dat' ! References
integer*4 nr__2
parameter (nr__2=41) ! Number of records
character*76 ar__2 ! Full-size record
integer*4 Ref ! Reference code
character*19 BibCode ! BibCode
character*20 Aut ! Authot's name
character*30 Com ! Comments
C=============================================================================
C Loading file 'table1.dat' ! Sample of late-type M, L, and T dwarfs: basic data
C Format for file interpretation
1 format(
+ A15,1X,A1,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,1X,A9,1X,
+ I2,1X,F7.5,1X,F7.5,1X,I2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,
+ F5.2,1X,F4.2,1X,I2,1X,A3)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,86
read(1,'(A110)')ar__
read(ar__,1)
+ Name,n_Name,RAh,RAm,RAs,DE_,DEd,DEm,DEs,SpT,r_SpT,plx,e_plx,
+ r_plx,Jmag,e_Jmag,Hmag,e_Hmag,Ksmag,e_Ksmag,r_Jmag,Syst
if(ar__(53:59) .EQ. '') plx = rNULL__
if(ar__(61:67) .EQ. '') e_plx = rNULL__
if(ar__(69:70) .EQ. '') r_plx = iNULL__
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)
+ Name,n_Name,RAh,RAm,RAs,DE_,DEd,DEm,DEs,SpT,r_SpT,plx,e_plx,
+ r_plx,Jmag,e_Jmag,Hmag,e_Hmag,Ksmag,e_Ksmag,r_Jmag,Syst
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! IRAC photometry and colors of late-type M, L, and
* T dwarfs
C Format for file interpretation
2 format(
+ A15,1X,A1,1X,A9,1X,F5.2,1X,F4.2,1X,I2,1X,F5.2,1X,F4.2,1X,I2,
+ 1X,F5.2,1X,F4.2,1X,I2,1X,F5.2,1X,F4.2,1X,I2,1X,F5.2,1X,F5.2,
+ 1X,F4.2,1X,A7)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,86
read(1,'(A108)')ar__1
read(ar__1,2)
+ Name_1,n_Name_1,SpT_1,v_3_6_,e__3_6_,o__3_6_,v_4_5_,e__4_5_,
+ o__4_5_,v_5_8_,e__5_8_,o__5_8_,v_8_0_,e__8_0_,o__8_0_,
+ v_3_6___4_5_,v_4_5___5_8_,v_5_8___8_0_,Notes
c ..............Just test output...........
write(6,2)
+ Name_1,n_Name_1,SpT_1,v_3_6_,e__3_6_,o__3_6_,v_4_5_,e__4_5_,
+ o__4_5_,v_5_8_,e__5_8_,o__5_8_,v_8_0_,e__8_0_,o__8_0_,
+ v_3_6___4_5_,v_4_5___5_8_,v_5_8___8_0_,Notes
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'refs.dat' ! References
C Format for file interpretation
3 format(I2,1X,A19,1X,A20,3X,A30)
C Effective file loading
open(unit=1,status='old',file=
+'refs.dat')
write(6,*) '....Loading file: refs.dat'
do i__=1,41
read(1,'(A76)')ar__2
read(ar__2,3)Ref,BibCode,Aut,Com
c ..............Just test output...........
write(6,3)Ref,BibCode,Aut,Com
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end