Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/599/A70 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-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/A+A/599/A70 Young moving group M-dwarf multiplicity (Janson+, 2017)
*================================================================================
*Binaries among low-mass stars in nearby young moving groups.
* Janson M., Durkan S., Hippler S., Dai X., Brandner W., Schlieder J.,
* Bonnefoy M., Henning T.
* <Astron. Astrophys. 599, A70 (2017)>
* =2017A&A...599A..70J (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Full sample summary
integer*4 nr__
parameter (nr__=181) ! Number of records
character*66 ar__ ! Full-size record
character*17 v2MASS (nr__) ! 2MASS identifier (JHHMMSSss+DDMMSSs)
character*4 SpType (nr__) ! Spectral type
character*4 YMG (nr__) ! Young Moving Group assignment
character*4 r_YMG (nr__) ! Reference for the YMG assignment (1)
real*4 Jmag (nr__) ! (mag) Apparent J-band magnitude from 2MASS
real*4 pmRA (nr__) ! (mas/yr) Proper motion along right ascension
real*4 pmDE (nr__) ! (mas/yr) Proper motion along declination
real*4 Dist (nr__) ! (pc) Distance to the target
character*4 Method (nr__) ! Method for determining the distance (2)
integer*4 Mult (nr__) ! Multiplicity count (3)
*Note (1): Reference for the association allocation as follows:
* BII = Re-evaluation in this work with BANYANII, based on ambiguous
* classification in previous works
* GBII = Re-evaluation based on GAIA data
* G15 = Gagne et al., 2015ApJ...798...73G
* K14 = Kraus et al., 2014AJ....147..146K
* M13 = Malo et al., 2013ApJ...762...88M
* M14 = Malo et al., 2014ApJ...788...81M
*Note (2): Method of distance estimation as follows:
* Plx = Parallax
* Kin = Kinematics
* Spec = Spectroscopic
*Note (3): The number of components seen in the AstraLux images
* (i.e. 1 is single, etc).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Astrometric properties
integer*4 nr__1
parameter (nr__1=70) ! Number of records
character*61 ar__1 ! Full-size record
character*17 v2MASS_1 (nr__1) ! 2MASS identifier
character*5 Pair (nr__1) ! Pair identifier (1)
real*4 Sep (nr__1) ! (arcsec) Separation at the given epoch
real*4 e_Sep (nr__1) ! (arcsec) Separation error
real*4 PA (nr__1) ! (deg) Position angle at the given epoch
real*4 e_PA (nr__1) ! (deg) Position angle error
real*8 Epoch (nr__1) ! (yr) Epoch of observation
character*1 CPM (nr__1) ! Common Proper Motion flag (2)
character*3 r_CPM (nr__1) ! Reference for CPM determination (3)
*Note (1): Pair displays false triple effect -- possibly subject to a
* 180 deg ambiguity.
*Note (2): Flag for CPM as follows:
* Y = if proven CPM
* N = if non-CPM
* U = if undetermined
* I = if implied (see paper)
*Note (3): CPM reference as follows:
* TP = This paper
* WDS = The Washington Double Star catalogue (Mason et al., 2001, Cat. I/281/)
* B15 = Bowler et al., 2015ApJS..216....7B
* C10 = Chauvin et al., 2010A&A...509A..52C
* D99 = Delfosse et al., 1999A&A...350L..39D
* D13 = Delorme et al., 2013A&A...553L...5D
* E15 = Elliott et al., 2015A&A...580A..88E
* J01 = Jayawardhana & Brandeker, 2001ApJ...561L.111J
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Photometric properties
integer*4 nr__2
parameter (nr__2=51) ! Number of records
character*51 ar__2 ! Full-size record
character*17 v2MASS_2 (nr__2) ! 2MASS identifier
character*2 Pair_1 (nr__2) ! Pair identifier
real*4 dzmag (nr__2) ! (mag) z'-band magnitude difference
real*4 e_dzmag (nr__2) ! (mag) z'-band magnitude error
real*4 M1 (nr__2) ! (Msun) Estimated mass of the primary
real*4 M2 (nr__2) ! (Msun) Estimated mass of the secondary
integer*4 a (nr__2) ! (AU) Estimated semi-major axis
integer*4 Porb (nr__2) ! (yr) Estimated orbital period
C=============================================================================
C Loading file 'table1.dat' ! Full sample summary
C Format for file interpretation
1 format(
+ A17,1X,A4,1X,A4,1X,A4,1X,F5.2,1X,F6.1,1X,F6.1,1X,F6.1,1X,A4,
+ 1X,I1)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,181
read(1,'(A66)')ar__
read(ar__,1)
+ v2MASS(i__),SpType(i__),YMG(i__),r_YMG(i__),Jmag(i__),
+ pmRA(i__),pmDE(i__),Dist(i__),Method(i__),Mult(i__)
c ..............Just test output...........
write(6,1)
+ v2MASS(i__),SpType(i__),YMG(i__),r_YMG(i__),Jmag(i__),
+ pmRA(i__),pmDE(i__),Dist(i__),Method(i__),Mult(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Astrometric properties
C Format for file interpretation
2 format(
+ A17,1X,A5,2X,F6.3,1X,F5.3,1X,F5.1,1X,F3.1,1X,F7.2,1X,A1,1X,A3)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,70
read(1,'(A61)')ar__1
read(ar__1,2)
+ v2MASS_1(i__),Pair(i__),Sep(i__),e_Sep(i__),PA(i__),e_PA(i__),
+ Epoch(i__),CPM(i__),r_CPM(i__)
c ..............Just test output...........
write(6,2)
+ v2MASS_1(i__),Pair(i__),Sep(i__),e_Sep(i__),PA(i__),e_PA(i__),
+ Epoch(i__),CPM(i__),r_CPM(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Photometric properties
C Format for file interpretation
3 format(A17,1X,A2,1X,F4.2,1X,F4.2,1X,F4.2,1X,F5.3,1X,I3,1X,I5)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,51
read(1,'(A51)')ar__2
read(ar__2,3)
+ v2MASS_2(i__),Pair_1(i__),dzmag(i__),e_dzmag(i__),M1(i__),
+ M2(i__),a(i__),Porb(i__)
c ..............Just test output...........
write(6,3)
+ v2MASS_2(i__),Pair_1(i__),dzmag(i__),e_dzmag(i__),M1(i__),
+ M2(i__),a(i__),Porb(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end