Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/143/140 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 2026-Oct-12
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/AJ/143/140 BEST-II periodic variables in CoRoT LRa02 field. II. (Fruth+, 2012)
*================================================================================
*Improved variable star search in large photometric data sets:
*new variables in CoRoT field LRa02 detected by BEST II.
* Fruth T., Kabath P., Cabrera J., Chini R., Csizmadia Sz., Eigmuller P.,
* Erikson A., Kirste S., Lemke R., Murphy M., Pasternacki T., Rauer H.,
* Titz-Weider R.
* <Astron. J., 143, 140 (2012)>
* =2012AJ....143..140F
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Catalog of variable stars detected in CoRoT
field LRa02 after reanalysis of the data set,
sorted by internal BEST II identifiers
integer*4 nr__
parameter (nr__=331) ! Number of records
character*155 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg (nr__) ! (deg) Right Ascension J2000
real*8 DEdeg (nr__) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*6 Field (nr__) ! Field name (LRa02a or LRa02b) (1)
integer*4 BEST (nr__) ! Internal BEST II identifier
character*3 f_BEST (nr__) ! Flag on BEST (c, k, s, ck or cs) (2)
character*17 v2MASS (nr__) ! 2MASS identifier (3)
integer*4 RAh (nr__) ! (h) [6/6] Hour of Right Ascension (J2000) (4)
integer*4 RAm (nr__) ! (min) [47/55] Minute of Right Ascension (J2000) (4)
real*4 RAs (nr__) ! (s) Second of Right Ascension (J2000) (4)
character*1 DE_ (nr__) ! Sign of the Declination (J2000) (4)
integer*4 DEd (nr__) ! (deg) [3/6] Degree of Declination (J2000) (4)
integer*4 DEm (nr__) ! (arcmin) Arcminute of Declination (J2000) (4)
real*4 DEs (nr__) ! (arcsec) Arcsecond of Declination (J2000) (4)
real*4 RBmag (nr__) ! (mag) [12.1/18.9] Observed magnitude (5)
real*8 T0 (nr__) ! (d) [34.587/104.975]? Heliocentric Julian Date of
* minimum brightness; HJD-2454400 (6)
real*8 Per (nr__) ! (d) [0.07167/41]? Period (6)
real*8 e_Per (nr__) ! (d) ? Uncertainty in Per
real*4 Amp (nr__) ! (mag) ? Amplitude of variability (6)
real*4 e_Amp (nr__) ! (mag) ? Uncertainty in Amp
real*8 Js (nr__) ! Stetson's (1996PASP..108..851S) J index
* of variability
character*7 Type (nr__) ! Variable type (from B/gcvs) (7)
character*36 OName (nr__) ! Other names
*Note (1): As the field of view of CoRoT is slightly larger than BEST II, we
* split the field into two subfields (called LRa02a and LRa02b,
* respectively) and pointed at them alternating.
*Note (2): Flag as follows:
* c = contaminated light curve due to overlapping aperture
* of neighboring stars;
* k = known variable (see column "OName" in this table);
* s = suspected variable.
*Note (3): Of closest 2MASS object within a radius of 2 arcseconds.
*Note (4): Derived by an astrometric match of CCD to USNO-A2 coordinates.
*Note (5): BEST II observes without any filter to maximize the photon yield
* (the CCD sensitivity peaks at 650nm and is roughly comparable to the
* Johnson R band).
*Note (6): Derived from the analysis of variance algorithm.
*Note (7): The newly discovered periodic variable stars are classified by
* the shape, amplitude, and period of their folded light curves
* according to the scheme used by the General Catalogue of Variable
* Stars (Cat. B/gcvs). Types of variable are:
* DSCT = Delta Scuti type (pulsating star);
* RR = RR Lyrae type (pulsating star);
* CEP = Cepheid variables (pulsating star);
* EA = Algol type (detached eclipsing binary);
* EB = Beta Lyrae type (semidetached eclipsing binary);
* EW = W Ursae Majoris type (contact eclipsing binary);
* ELL = Stars having sinusoidal-like light curves and showing eclipses
* are marked as rotating ellipsoidal variables;
* SP = Spotted stars (whose characteristic features are exhibited by
* some light curves);
* VAR = The type of variability could not be determined from the light
* curve alone. Further observations are needed to constrain the
* proper physical origin of stellar variability.
* LP = Stars that are variable on timescales longer than the
* observational baseline are classified as long periodic.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! Catalog of periodic variable stars with revised
parameters compared to paper I
(Kabath et al., 2009, Cat. J/A+A/506/569)
integer*4 nr__1
parameter (nr__1=17) ! Number of records
character*155 ar__1 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 (nr__1) ! (deg) Right Ascension J2000
real*8 DEdeg_1 (nr__1) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*6 Field_1 (nr__1) ! Field name (LRa02a or LRa02b) (1)
integer*4 BEST_1 (nr__1) ! Internal BEST II identifier
character*3 f_BEST_1 (nr__1) ! Flag on BEST (c, k, s, ck or cs) (2)
character*17 v2MASS_1 (nr__1) ! 2MASS identifier (3)
integer*4 RAh_1 (nr__1) ! (h) [6/6] Hour of Right Ascension (J2000) (4)
integer*4 RAm_1 (nr__1) ! (min) [47/55] Minute of Right Ascension (J2000) (4)
real*4 RAs_1 (nr__1) ! (s) Second of Right Ascension (J2000) (4)
character*1 DE__1 (nr__1) ! Sign of the Declination (J2000) (4)
integer*4 DEd_1 (nr__1) ! (deg) [3/6] Degree of Declination (J2000) (4)
integer*4 DEm_1 (nr__1) ! (arcmin) Arcminute of Declination (J2000) (4)
real*4 DEs_1 (nr__1) ! (arcsec) Arcsecond of Declination (J2000) (4)
real*4 RBmag_1 (nr__1) ! (mag) [12.1/18.9] Observed magnitude (5)
real*8 T0_1 (nr__1) ! (d) [34.587/104.975]? Heliocentric Julian Date of
* minimum brightness; HJD-2454400 (6)
real*8 Per_1 (nr__1) ! (d) [0.07167/41]? Period (6)
real*8 e_Per_1 (nr__1) ! (d) ? Uncertainty in Per
real*4 Amp_1 (nr__1) ! (mag) ? Amplitude of variability (6)
real*4 e_Amp_1 (nr__1) ! (mag) ? Uncertainty in Amp
real*8 Js_1 (nr__1) ! Stetson's (1996PASP..108..851S) J index
* of variability
character*7 Type_1 (nr__1) ! Variable type (from B/gcvs) (7)
character*36 OName_1 (nr__1) ! Other names
*Note (1): As the field of view of CoRoT is slightly larger than BEST II, we
* split the field into two subfields (called LRa02a and LRa02b,
* respectively) and pointed at them alternating.
*Note (2): Flag as follows:
* c = contaminated light curve due to overlapping aperture
* of neighboring stars;
* k = known variable (see column "OName" in this table);
* s = suspected variable.
*Note (3): Of closest 2MASS object within a radius of 2 arcseconds.
*Note (4): Derived by an astrometric match of CCD to USNO-A2 coordinates.
*Note (5): BEST II observes without any filter to maximize the photon yield
* (the CCD sensitivity peaks at 650nm and is roughly comparable to the
* Johnson R band).
*Note (6): Derived from the analysis of variance algorithm.
*Note (7): The newly discovered periodic variable stars are classified by
* the shape, amplitude, and period of their folded light curves
* according to the scheme used by the General Catalogue of Variable
* Stars (Cat. B/gcvs). Types of variable are:
* DSCT = Delta Scuti type (pulsating star);
* RR = RR Lyrae type (pulsating star);
* CEP = Cepheid variables (pulsating star);
* EA = Algol type (detached eclipsing binary);
* EB = Beta Lyrae type (semidetached eclipsing binary);
* EW = W Ursae Majoris type (contact eclipsing binary);
* ELL = Stars having sinusoidal-like light curves and showing eclipses
* are marked as rotating ellipsoidal variables;
* SP = Spotted stars (whose characteristic features are exhibited by
* some light curves);
* VAR = The type of variability could not be determined from the light
* curve alone. Further observations are needed to constrain the
* proper physical origin of stellar variability.
* LP = Stars that are variable on timescales longer than the
* observational baseline are classified as long periodic.
C=============================================================================
C Loading file 'table3.dat' ! Catalog of variable stars detected in CoRoT
* field LRa02 after reanalysis of the data set,
* sorted by internal BEST II identifiers
C Format for file interpretation
1 format(
+ A6,1X,I5,1X,A3,1X,A17,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,
+ F4.1,1X,F5.2,1X,F7.3,1X,F9.6,1X,F8.6,1X,F5.3,1X,F5.3,1X,F7.4,
+ 1X,A7,1X,A36)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,331
read(1,'(A155)')ar__
read(ar__,1)
+ Field(i__),BEST(i__),f_BEST(i__),v2MASS(i__),RAh(i__),
+ RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),DEs(i__),
+ RBmag(i__),T0(i__),Per(i__),e_Per(i__),Amp(i__),e_Amp(i__),
+ Js(i__),Type(i__),OName(i__)
if(ar__(65:71) .EQ. '') T0(i__) = rNULL__
if(ar__(73:81) .EQ. '') Per(i__) = rNULL__
if(ar__(83:90) .EQ. '') e_Per(i__) = rNULL__
if(ar__(92:96) .EQ. '') Amp(i__) = rNULL__
if(ar__(98:102) .EQ. '') e_Amp(i__) = rNULL__
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)
+ Field(i__),BEST(i__),f_BEST(i__),v2MASS(i__),RAh(i__),
+ RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),DEs(i__),
+ RBmag(i__),T0(i__),Per(i__),e_Per(i__),Amp(i__),e_Amp(i__),
+ Js(i__),Type(i__),OName(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 'table4.dat' ! Catalog of periodic variable stars with revised
* parameters compared to paper I
* (Kabath et al., 2009, Cat. J/A+A/506/569)
C Format for file interpretation
2 format(
+ A6,1X,I5,1X,A3,1X,A17,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,
+ F4.1,1X,F5.2,1X,F7.3,1X,F9.6,1X,F8.6,1X,F5.3,1X,F5.3,1X,F7.4,
+ 1X,A7,1X,A36)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,17
read(1,'(A155)')ar__1
read(ar__1,2)
+ Field_1(i__),BEST_1(i__),f_BEST_1(i__),v2MASS_1(i__),
+ RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),DEd_1(i__),
+ DEm_1(i__),DEs_1(i__),RBmag_1(i__),T0_1(i__),Per_1(i__),
+ e_Per_1(i__),Amp_1(i__),e_Amp_1(i__),Js_1(i__),Type_1(i__),
+ OName_1(i__)
if(ar__1(65:71) .EQ. '') T0_1(i__) = rNULL__
if(ar__1(73:81) .EQ. '') Per_1(i__) = rNULL__
if(ar__1(83:90) .EQ. '') e_Per_1(i__) = rNULL__
if(ar__1(92:96) .EQ. '') Amp_1(i__) = rNULL__
if(ar__1(98:102) .EQ. '') e_Amp_1(i__) = rNULL__
RAdeg_1(i__) = rNULL__
DEdeg_1(i__) = rNULL__
c Derive coordinates RAdeg_1 and DEdeg_1 from input data
c (RAdeg_1 and DEdeg_1 are set to rNULL__ when unknown)
if(RAh_1(i__) .GT. -180) RAdeg_1(i__)=RAh_1(i__)*15.
if(RAm_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAm_1(i__)/4.
if(RAs_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAs_1(i__)/240.
if(DEd_1(i__) .GE. 0) DEdeg_1(i__)=DEd_1(i__)
if(DEm_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEm_1(i__)/60.
if(DEs_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEs_1(i__)/3600.
if(DE__1(i__).EQ.'-'.AND.DEdeg_1(i__).GE.0) DEdeg_1(i__)=-DEdeg_1(i__)
c ..............Just test output...........
write(6,2)
+ Field_1(i__),BEST_1(i__),f_BEST_1(i__),v2MASS_1(i__),
+ RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),DEd_1(i__),
+ DEm_1(i__),DEs_1(i__),RBmag_1(i__),T0_1(i__),Per_1(i__),
+ e_Per_1(i__),Amp_1(i__),e_Amp_1(i__),Js_1(i__),Type_1(i__),
+ OName_1(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end