Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/592/A120 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-20
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/592/A120 Variable stars in NGC 6715 (Figuera Jaimes+, 2016)
*================================================================================
*Many new variable stars discovered in the core of globular cluster NGC 6715
*(M54) with EMCCD observations.
* Figuera Jaimes R., Bramich D.M., Kains N., Skottfelt J., Jorgensen U.G.,
* Horne K., Dominik M., Alsubai K.A., Bozza V., Burgdorf M.J.,
* Calchi Novati S., Ciceri S., D'Ago G., Evans D.F., Galianni P., Gu S.H.,
* Harpsoe K.B.W, Haugbolle T., Hinse T.C., Hundertmark M., Juncher D.,
* Kerins E., Korhonen H., Kuffmeier M., Mancini L., Peixinho N., Popovas A.,
* Rabus M., Rahvar S., Scarpetta G., Schmidt R.W., Snodgrass C.,
* Southworth J., Starkey D., Street R.A., Surdej J., Tronsgaard R.,
* Unda-Sanzana E., von Essen C., Wang X. B., Wertz O.,
* (The MiNDSTEp Consortium)
* <Astron. Astrophys. 592, A120 (2016)>
* =2016A&A...592A.120F (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Ephemerides and main characteristics of the variable
stars in the field of globular cluster NGC 6715
integer*4 nr__
parameter (nr__=85) ! Number of records
character*121 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*4 VName ! Variable star ID (VNNN)
character*1 Note ! [a] a: Epochs, periods, mean magnitudes,
* amplitudes, and classifications taken from
* OGLE database
character*30 OName ! Previously known ID assigned to the stars (1)
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)
real*4 DEs ! (arcsec) Declination (J2000)
real*8 Epoch ! (d) ?=- Epoch used (HJD)
real*8 Per ! (d) ?=- Period measured in this work unless the
* variable is an OGLE star, in which case
* we use their period
real*8 e_Per ! (d) ? rms uncertainty on Per
real*4 Imag ! (mag) ?=- Median I magnitude
character*1 n_Imag ! [d] d: Peak magnitude
real*4 Amp_i_z ! (mag) ?=- Peak-to-peak amplitude in the
* light curve (i'+z')
integer*4 N ! Number of epochs
character*4 Type ! Classification of the variable
*Note (1): Other names as follows:
* NNNNN = OGLE identifications of the form OGLE-BLG-RRLYR-NNNNN
* (Soszynski et al, 2014, Cat. J/AcA/64/177)
* O16 = variable star was discovered independently by Hamanowicz et al.
* (2016AcA....66..197H, [arXiv:1605.04906])
* VCNN = from Montiel & Mighell, 2010, Cat. J/AJ/140/1500
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Time series I photometry for all the variables
studied in this work
integer*4 nr__1
parameter (nr__1=3651) ! Number of records
character*93 ar__1 ! Full-size record
character*4 VName_1 ! Variable star ID (VNNN)
character*1 Filt ! [I] Observation filter
real*8 HJD ! (d) Heliocentric Julian date at mid-exposure
real*4 mag_s ! (mag) ?=0 Standard magnitude (I band)
real*4 mag_i ! (mag) ?=0 Instrumental magnitude (I band)
real*4 e_mag_i ! (mag) ?=0 Magnitude uncertainty (standard or
* instrumental)
real*8 Fref ! (s-1) ?=0 Reference flux (I band) (in ADU/s unit) (1)
real*8 e_Fref ! (s-1) ?=0 Reference flux uncertainty (in ADU/s unit)
real*8 DFlux ! (s-1) Difference flux (I band) (in ADU/s unit) (1)
real*8 e_DFlux ! (s-1) Difference flux uncertainty (in ADU/s unit)
real*4 p ! Photometric scale factor (1)
*Note (1): Light curves for each star were constructed by calculating the total
* flux ftot(t) in adu/s at each epoch t from
*
* ftot(t)=fref+fdiff(t)/p(t)
*
* where fref is the reference flux (adu/s), fdiff(t) is the
* differential flux (adu/s) and p(t) is the photometric scalefactor (the
* integral of the kernel solution)
*
* Conversion to instrumental magnitudes was achieved using
*
* mins(t)=17.5-2.5log(ftot(t))
*
* where mins(t) is the instrumental magnitude of the star at time t.
* Uncertainties were propagated in the correct analytical fashion.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'tableb1.dat' ! Cross-identification between the RR Lyrae variables
listed by the CVSGGC, the variable star candidates
from Montiel & Mighell and the OGLE RR Lyrae stars
integer*4 nr__2
parameter (nr__2=129) ! Number of records
character*22 ar__2 ! Full-size record
character*4 CVSGGC ! CVSGGC designation (VNNN),
* Clement et al., 2001AJ....122.2587C,
* Cl* NGC 6715 SAW VNNN in Simbad
character*11 OGLE ! OGLE designation (RRLYR-NNNNN),
* Soszynski et al., 2014, Cat. J/AcA/64/177,
* OGLE BLG-RRLYR-NNNNN in Simbad
character*4 VC ! Montiel designation (VCNN),
* Montiel & Mighell, 2010, Cat. J/AJ/140/1500
* [MM2010] VCNN in Simbad
C=============================================================================
C Loading file 'table3.dat' ! Ephemerides and main characteristics of the variable
* stars in the field of globular cluster NGC 6715
C Format for file interpretation
1 format(
+ A4,A1,1X,A30,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F5.2,1X,
+ F12.4,1X,F12.8,3X,F10.8,1X,F5.2,A1,1X,F4.2,1X,I2,1X,A4)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,85
read(1,'(A121)')ar__
read(ar__,1)
+ VName,Note,OName,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Epoch,Per,e_Per,
+ Imag,n_Imag,Amp_i_z,N,Type
if (idig(ar__(64:75)).EQ.0) Epoch = rNULL__
if (idig(ar__(77:88)).EQ.0) Per = rNULL__
if(ar__(92:101) .EQ. '') e_Per = rNULL__
if (idig(ar__(103:107)).EQ.0) Imag = rNULL__
if (idig(ar__(110:113)).EQ.0) Amp_i_z = rNULL__
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)
+ VName,Note,OName,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Epoch,Per,e_Per,
+ Imag,n_Imag,Amp_i_z,N,Type
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table1.dat' ! Time series I photometry for all the variables
* studied in this work
C Format for file interpretation
2 format(
+ A4,1X,A1,1X,F13.5,1X,F6.3,1X,F6.3,1X,F5.3,1X,F11.3,1X,F11.3,
+ 1X,F12.3,1X,F8.3,1X,F6.4)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,3651
read(1,'(A93)')ar__1
read(ar__1,2)
+ VName_1,Filt,HJD,mag_s,mag_i,e_mag_i,Fref,e_Fref,DFlux,
+ e_DFlux,p
c ..............Just test output...........
write(6,2)
+ VName_1,Filt,HJD,mag_s,mag_i,e_mag_i,Fref,e_Fref,DFlux,
+ e_DFlux,p
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'tableb1.dat' ! Cross-identification between the RR Lyrae variables
* listed by the CVSGGC, the variable star candidates
* from Montiel & Mighell and the OGLE RR Lyrae stars
C Format for file interpretation
3 format(A4,1X,A11,2X,A4)
C Effective file loading
open(unit=1,status='old',file=
+'tableb1.dat')
write(6,*) '....Loading file: tableb1.dat'
do i__=1,129
read(1,'(A22)')ar__2
read(ar__2,3)CVSGGC,OGLE,VC
c ..............Just test output...........
write(6,3)CVSGGC,OGLE,VC
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end
C Locate position of first digit in string; or return 0
integer function idig(c)
character*(*) c
character*1 c1
integer lc,i
lc=len(c)
idig=0
do i=1,lc
if(c(i:i).ne.' ') go to 1
end do
1 if(i.gt.lc) return
c1=c(i:i)
if(c1.eq.'.'.or.c1.eq.'-'.or.c1.eq.'+') i=i+1
if(i.gt.lc) return
c1=c(i:i)
if(c1.ge.'0'.and.c1.le.'9') idig=i
return
end