Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/150/107 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-Aug-15
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/150/107 Variable stars from TNTS. I. 2012-2014 (Yao+, 2015)
*================================================================================
*Photometry of variable stars from the THU-NAOC transient survey.
*I. The first two years.
* Yao X., Wang L., Wang X., Zhang T., Chen J., Yuan W., Mo J., Li W., Jin Z.,
* Wu X., Nie J., Zhou X.
* <Astron. J., 150, 107 (2015)>
* =2015AJ....150..107Y (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Variable stars
integer*4 nr__
parameter (nr__=1237) ! Number of records
character*107 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs 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*4 Field (nr__) ! Survey field identifier
integer*4 Star (nr__) ! Identifier within the field
integer*4 RAh (nr__) ! (h) Hour of Right Ascension (J2000) (1)
integer*4 RAm (nr__) ! (min) Minute of Right Ascension (J2000) (1)
real*4 RAs (nr__) ! (s) Second of Right Ascension (J2000) (1)
integer*4 DEd (nr__) ! (deg) Degree of Declination (J2000) (1)
integer*4 DEm (nr__) ! (arcmin) Arcminute of Declination (J2000) (1)
real*4 DEs (nr__) ! (arcsec) Arcsecond of Declination (J2000) (1)
real*4 v_mag_ (nr__) ! (mag) [9.3/141.2] Mean unfiltered magnitude (2)
real*4 Av (nr__) ! (mag) [0.01/1.2] Line-of-sight extinction (3)
real*4 Amp (nr__) ! (mag) [0/3.8] Amplitude of variation (4)
real*4 Js (nr__) ! [0.31/30] Welch-Stetson variability index J_s_
* (Stetson, 1996PASP..108..851S)
real*8 Per1 (nr__) ! (d) [0.1/730]? Period from our measurement (Tsinghua
* University-NAOC Transient Survey; TNTS)
character*3 Meth (nr__) ! Period calculate method (LS, PDM, or VSX) (5)
real*8 Per2 (nr__) ! (d) [0.2/730]? Period from International Variable
* Star Index (VSX; cat. B/vsx)
real*8 T0 (nr__) ! [121/882]? Epoch when primary eclipse or minimum
* light occurs
character*7 Type (nr__) ! Tentative classification about the variable star
* whenever possible (6)
character*1 VSX (nr__) ! [V] Indicates a VSX variable (7)
character*1 CSS (nr__) ! [C] Indicates a CSS variable (7)
character*1 New (nr__) ! [N] Indicates a new variable
character*1 LIN (nr__) ! [L] Indicates a LINEAR variable (7)
*Note (1): Based on reference images from Tsinghua University-NAOC Transient
* Survey (TNTS).
*Note (2): Calibrated with the R-band magnitudes of the Position and Proper
* Motions eXtended (PPMX; cat. I/312) catalog.
*Note (3): Based on Schlafly & Finkbeiner (2011ApJ...737..103S).
*Note (4): Magnitude from maximum to minimum.
*Note (5): The methods are defined as below:
* LS = Lomb-Scargle method;
* PDM = Phase Dispersion Minimization method;
* VSX = From International Variable Star Index (VSX; cat. B/vsx) catalogs.
*Note (6): Including previous identification of variables from VSX (cat. B/vsx)
* database and GCVS (cat. B/gcvs), defined as follows:
* ACEP = Anomalous Cepheids;
* RS = RS Canum Venaticorum;
* EC = Contact binary;
* ES = Semi-detached binary;
* ED = Detached binary;
* CWA = W Virginis;
* RR = RR Lyrae variable;
* BL = "Blazhko effect";
* CEP = Cepheids;
* GDOR = Gamma Doradus star;
* DSCT = Delta Scuti star;
* SR = Semiregular pulsator;
* M = Mira variable;
* LPV = Long Period Variable;
* L = Slow irregular variable.
*Note (7): Information flag defined as below:
* V = Variable in International Variable Star Index (VSX; cat. B/vsx) of the
* Association of Variable Star Observers (AAVSO);
* C = Variable in Catalina Sky Survey (CSS) sample (Drake et al. 2014,
* cat. J/ApJS/213/9);
* L = Variable in Lincoln Near-Earth Asteroid Research (LINEAR) survey sample
* (Palaversa et al. 2013, cat. J/AJ/146/101);
* N = New variable.
C=============================================================================
C Loading file 'table1.dat' ! Variable stars
C Format for file interpretation
1 format(
+ A4,1X,I5,1X,I2,1X,I2,1X,F5.2,1X,I3,1X,I2,1X,F5.2,1X,F6.2,1X,
+ F4.2,1X,F4.2,1X,F5.2,1X,F12.8,1X,A3,1X,F10.6,1X,F7.3,1X,A7,1X,
+ A1,A1,A1,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,1237
read(1,'(A107)')ar__
read(ar__,1)
+ Field(i__),Star(i__),RAh(i__),RAm(i__),RAs(i__),DEd(i__),
+ DEm(i__),DEs(i__),v_mag_(i__),Av(i__),Amp(i__),Js(i__),
+ Per1(i__),Meth(i__),Per2(i__),T0(i__),Type(i__),VSX(i__),
+ CSS(i__),New(i__),LIN(i__)
if(ar__(60:71) .EQ. '') Per1(i__) = rNULL__
if(ar__(77:86) .EQ. '') Per2(i__) = rNULL__
if(ar__(88:94) .EQ. '') T0(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.
c ..............Just test output...........
write(6,1)
+ Field(i__),Star(i__),RAh(i__),RAm(i__),RAs(i__),DEd(i__),
+ DEm(i__),DEs(i__),v_mag_(i__),Av(i__),Amp(i__),Js(i__),
+ Per1(i__),Meth(i__),Per2(i__),T0(i__),Type(i__),VSX(i__),
+ CSS(i__),New(i__),LIN(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end