Conversion of standardized ReadMe file for
file /./ftp/cats/V/124 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. V/124 Approximate elements of eclipsing binaries (Svechnikov+, 1990)
*================================================================================
*Catalogue of approximate photometric and absolute elements of eclipsing
*variable stars.
* Svechnikov M.A., Kuznetsova Eh.F.
* <Ural university publication, Sverdlovsk, vols 1,2 (1990)>
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'objects.dat' ! Coordinates of objects
integer*4 nr__
parameter (nr__=3796) ! Number of records
character*39 ar__ ! Full-size record
C J2000.0 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg (nr__) ! (deg) Right Ascension J2000.0
real*8 DEdeg (nr__) ! (deg) Declination J2000.0
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 RAh (nr__) ! (h) ? Right ascension (J2000.0)
integer*4 RAm (nr__) ! (min) ? Right ascension (J2000.0)
real*4 RAs (nr__) ! (s) ? Right ascension (J2000.0)
character*1 DE_ (nr__) ! Declination sign (J2000.0)
integer*4 DEd (nr__) ! (deg) ? Declination (J2000.0)
integer*4 DEm (nr__) ! (arcmin) ? Declination (J2000.0)
integer*4 DEs (nr__) ! (arcsec) ? Declination (J2000.0)
integer*4 Seq (nr__) ! Number of star system
character*9 Name (nr__) ! Object name (1)
*Note (1): GZ Sge and V3476 Sgr have no position.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'catalog.dat' ! Data on photometric and absolute elements of
eclipsing stars
integer*4 nr__1
parameter (nr__1=3796) ! Number of records
character*146 ar__1 ! Full-size record
integer*4 Seq_1 (nr__1) ! Number of star system (1)
character*1 Note (nr__1) ! [*] Remarks on Seq (2)
character*9 Name_1 (nr__1) ! Name of eclipsing binary (3)
real*8 Period (nr__1) ! (d) Orbital period of system
character*1 n_Period (nr__1) ! [*:?] Remark on Period (4)
character*15 Sp (nr__1) ! Spectra SP1+SP2 of the components (5)
character*3 Type (nr__1) ! Eclipsing system type (6)
character*1 u_Type (nr__1) ! [:] Uncertainty flag on Type
character*2 EType (nr__1) ! Evolutionary type (7)
character*1 u_EType (nr__1) ! [:] Uncertainty flag on EType
real*4 q (nr__1) ! Mass ratio of components
real*4 A (nr__1) ! (solRad) Orbital major semiaxis (in solar radii)
real*4 M1 (nr__1) ! (solMass) Mass of first component
real*4 M2 (nr__1) ! (solMass) Mass of second component
real*4 R1 (nr__1) ! (solRad) Radius of first component
real*4 R2 (nr__1) ! (solRad) Radius of second component
real*4 Mbol1 (nr__1) ! (mag) Absolute bolometric magnitude of first
* component (8)
real*4 Mbol2 (nr__1) ! (mag) Absolute bolometric magnitude of second
* component (8)
real*4 r1_1 (nr__1) ! Relative radius of first component in units of
* Orbital major semiaxis A (9)
real*4 r2_1 (nr__1) ! Relative radius of second component in units
* of Orbital major semiaxis A (9)
character*1 l_L1 (nr__1) ! [>] Limit symbol on L1
real*4 L1 (nr__1) ! Relative luminosity of massive component in
* units of L1+L2=1
character*1 u_L1 (nr__1) ! [:] Uncertainty flag on L1
character*1 l_J1_J2 (nr__1) ! [>] Limit symbol on J1/J2
real*8 J1_J2 (nr__1) ! Surface brightness ratio of more massive
* component to one of less massive (J1/J2) (10)
character*1 e_J1_J2 (nr__1) ! [:] Uncertainty in J1/J2
character*1 Band (nr__1) ! [VPvB] Photometric system in J1/J2
character*2 l_Incl (nr__1) ! [>= ~] Limit flag on Incl
real*4 Incl (nr__1) ! (deg) Orbital inclination
integer*4 W (nr__1) ! [0/9] Weight (11)
*Note (1): Numbers beginning from 4001 indicate stars taken from a
* supplementary table (Svechnikov, Kuznetsova 1990, vol.2, p.224).
* Systems 1043, 1143, 1970, 2860, 3598 are excluded from the electronic
* version according to Svechnikov's notes (2004, private communication).
*Note (2): Asterisk indicates the presence of this system in the notes.dat file.
*Note (3): The systems are placed in the catalogue by constellations as in
* GCVS IV.
*Note (4): The symbol means the following:
* : = period is uncertain
* * = variable period
* ? = probably variable period
*Note (5): SP1 is given from GCVS IV or from another (as usually, later)
* literature. In the last case the spectra from GCVS IV is given in
* remarks. The spectral types of components computed from the
* observational values of J1/J2 in assumption that both components
* radiate as the black bodies are given in the square brackets.
*
* If SP1 is not known from the available literature and it is evaluated
* from the statistical dependences for the eclipsing binaries of
* different types we put it in brackets ().
*
* If there is in literature only spectral class (for example A or F)
* without spectral subclass, then we put in brackets () supposed
* spectral subclass (for example A(3)).
*Note (6): Eclipsing system type taken from GCVS IV or from other
* literatures (E, EA, EB, EW or ELL (rotating))
*Note (7): Evolutionary type according to Svechnikov's classification [2,3,4]:
* DM = detached main sequence systems. Both components are main sequence
* stars, which do not fill their inner Roche lobes.
* SD = semi-detached systems, where more massive component is main
* sequence star, and less massive secondary component is subgiant
* which fills (or nearly fills) its Roche lobe.
* DS = detached systems with subgiant secondary. The less massive
* subgiant component distinctly does not fill its Roche lobe.
* KE = contact systems of early spectra, both components are close to
* their Roche lobes, spectra of the more massive component are
* not later about F0.
* KW = contact systems of W UMa-type with the periods shorter than
* 0.5 days and with SP1 later than about F0.
* DW = systems, similar to W UMa-stars, where both components do not
* fill their Roche lobes and their physical characteristics
* are similar to those of KW-systems [2,8].
* Lately designation of these eclipsing binaries as
* "short-periodic RS CVN-type systems" is widely applied [10,11].
*Note (8): The effective temperature scale given in [12,13]
*Note (9): Radii or the small equatorial semiaxes for ellipsoidal star
* (in units of Orbital major semiaxis A).
* The index "1" always is related to more massive star.
*Note (10): As a rule, in the color of amplitudes of minima A1 and A2
* given in GCVS IV)
*Note (11): Weight characterizes the reliability of evaluation of
* photometric and absolute elements in 10-ball scale (highly unreliable
* elements have weight 0; elements, evaluated with reliability,
* approaching to reliability of the evaluation of elements by exact
* methods over their light curves and radial velocity curves have W=9.
* For systems with certain meaning of SP1 the elements are defined more
* certainly and they have weight essentially larger than systems with
* uncertain component spectrum.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'notes.dat' ! Notes
integer*4 nr__2
parameter (nr__2=806) ! Number of records
character*426 ar__2 ! Full-size record
integer*4 Seq_2 (nr__2) ! Sequential number
character*9 Name_2 (nr__2) ! Name
character*409 Text (nr__2) ! Text of the note
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'refs.dat' ! References
integer*4 nr__3
parameter (nr__3=18) ! Number of records
character*180 ar__3 ! Full-size record
integer*4 Ref (nr__3) ! Reference number
character*175 Text_1 (nr__3) ! Text of reference
C=============================================================================
C Loading file 'objects.dat' ! Coordinates of objects
C Format for file interpretation
1 format(I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,4X,I4,2X,A9)
C Effective file loading
open(unit=1,status='old',file=
+'objects.dat')
write(6,*) '....Loading file: objects.dat'
do i__=1,3796
read(1,'(A39)')ar__
read(ar__,1)
+ RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),
+ DEs(i__),Seq(i__),Name(i__)
if(ar__(1:2) .EQ. '') RAh(i__) = iNULL__
if(ar__(4:5) .EQ. '') RAm(i__) = iNULL__
if(ar__(7:10) .EQ. '') RAs(i__) = rNULL__
if(ar__(13:14) .EQ. '') DEd(i__) = iNULL__
if(ar__(16:17) .EQ. '') DEm(i__) = iNULL__
if(ar__(19:20) .EQ. '') DEs(i__) = iNULL__
RAdeg(i__) = rNULL__
DEdeg(i__) = rNULL__
c Derive coordinates RAdeg and DEdeg from input data
c (RAdeg and DEdeg are set to rNULL__ when unknown)
if(RAh(i__) .GT. -180) RAdeg(i__)=RAh(i__)*15.
if(RAm(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAm(i__)/4.
if(RAs(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAs(i__)/240.
if(DEd(i__) .GE. 0) DEdeg(i__)=DEd(i__)
if(DEm(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEm(i__)/60.
if(DEs(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEs(i__)/3600.
if(DE_(i__).EQ.'-'.AND.DEdeg(i__).GE.0) DEdeg(i__)=-DEdeg(i__)
c ..............Just test output...........
write(6,1)
+ RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),
+ DEs(i__),Seq(i__),Name(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'catalog.dat' ! Data on photometric and absolute elements of
* eclipsing stars
C Format for file interpretation
2 format(
+ I4,A1,1X,A9,1X,F13.9,1X,A1,1X,A15,1X,A3,A1,1X,A2,A1,1X,F5.3,
+ 1X,F6.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F6.2,1X,F6.2,1X,
+ F5.3,1X,F5.3,1X,A1,F4.2,A1,A1,F7.2,A1,1X,A1,1X,A2,F4.1,1X,I1)
C Effective file loading
open(unit=1,status='old',file=
+'catalog.dat')
write(6,*) '....Loading file: catalog.dat'
do i__=1,3796
read(1,'(A146)')ar__1
read(ar__1,2)
+ Seq_1(i__),Note(i__),Name_1(i__),Period(i__),n_Period(i__),
+ Sp(i__),Type(i__),u_Type(i__),EType(i__),u_EType(i__),q(i__),
+ A(i__),M1(i__),M2(i__),R1(i__),R2(i__),Mbol1(i__),Mbol2(i__),
+ r1_1(i__),r2_1(i__),l_L1(i__),L1(i__),u_L1(i__),l_J1_J2(i__),
+ J1_J2(i__),e_J1_J2(i__),Band(i__),l_Incl(i__),Incl(i__),W(i__)
c ..............Just test output...........
write(6,2)
+ Seq_1(i__),Note(i__),Name_1(i__),Period(i__),n_Period(i__),
+ Sp(i__),Type(i__),u_Type(i__),EType(i__),u_EType(i__),q(i__),
+ A(i__),M1(i__),M2(i__),R1(i__),R2(i__),Mbol1(i__),Mbol2(i__),
+ r1_1(i__),r2_1(i__),l_L1(i__),L1(i__),u_L1(i__),l_J1_J2(i__),
+ J1_J2(i__),e_J1_J2(i__),Band(i__),l_Incl(i__),Incl(i__),W(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'notes.dat' ! Notes
C Format for file interpretation
3 format(I4,1X,A9,3X,A409)
C Effective file loading
open(unit=1,status='old',file=
+'notes.dat')
write(6,*) '....Loading file: notes.dat'
do i__=1,806
read(1,'(A426)')ar__2
read(ar__2,3)Seq_2(i__),Name_2(i__),Text(i__)
c ..............Just test output...........
write(6,3)Seq_2(i__),Name_2(i__),Text(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'refs.dat' ! References
C Format for file interpretation
4 format(1X,I2,2X,A175)
C Effective file loading
open(unit=1,status='old',file=
+'refs.dat')
write(6,*) '....Loading file: refs.dat'
do i__=1,18
read(1,'(A180)')ar__3
read(ar__3,4)Ref(i__),Text_1(i__)
c ..............Just test output...........
write(6,4)Ref(i__),Text_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end