Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJS/160/450 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 2026-Oct-11
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/ApJS/160/450 X-ray emission in Orion Nebula young stars (Flaccomio+, 2005)
*================================================================================
*Rotational modulation of X-ray emission in Orion Nebula young stars.
* Flaccomio E., Micela G., Sciortino S., Feigelson E.D., Herbst W.,
* Favata F., Harnden F.R.JR, Vrtilek S.D.
* <Astrophys. J. Suppl. Ser., 160, 450-468 (2005)>
* =2005ApJS..160..450F
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! COUP sources with assigned rotational period.
integer*4 nr__
parameter (nr__=295) ! Number of records
character*60 ar__ ! Full-size record
integer*4 COUP ! The COUP source number
integer*4 Cts ! (ct) Net (background subtracted) ACIS counts
integer*4 OptId ! ? Optical identification (1)
character*1 m_OptId ! [ab] Multiplicity indicator (1)
real*4 Per ! (d) Optically determined rotation period
character*1 n_Per ! Note on Per (2)
character*4 r_Per ! Reference for Per (3)
real*4 Mass ! (solMass) ? Stellar mass
real*4 LogAge ! ([yr]) ? Log of the stellar age
real*4 LogLx ! ([10-7W]) ? Log of the X-ray luminosity in erg/s
real*4 Log_Lx_Lb ! ([-]) ? Log of the X-ray to bolometric
* luminosity ratio
real*4 WCaII ! (0.1nm) ? Ca II line equivalent width in Angstroms
character*3 Mod ! The X-ray modulation flag (4)
*Note (1): Identification number from Hillenbrand (1997, Cat. J/AJ/113/1733),
* Herbst+ (2002, Cat. J/A+A/396/513).
*Note (2): Indicates other periods reported in the literature when differing by
* more than 10% from Per. References (note 3) are given in parentheses.
* Note on Per, defined as follows:
* a = 2.99 (Carpenter et al. 2001, Cat. J/AJ/121/3160);
* b = 1.40 (Herbst et al. 2000AJ....119..261H);
* c = 2.85 (Carpenter et al. 2001, Cat. J/AJ/121/3160);
* d = 20.10 (Herbst et al. 2000AJ....119..261H);
* e = 1.57 (Herbst et al. 2000AJ....119..261H);
* f = 7.78 (Stassun et al. 1999, Cat. J/AJ/117/2941);
* g = 13.43 (Carpenter et al. 2001, Cat. J/AJ/121/3160);
* h = 5.59 (Herbst et al. 2000AJ....119..261H);
* i = 2.13 (Stassun et al. 1999, Cat. J/AJ/117/2941);
* j = 11.19 (Carpenter et al. 2001, Cat. J/AJ/121/3160);
* k = 4.00 (Herbst et al. 2000AJ....119..261H);
* l = 2.40 (Carpenter et al. 2001, Cat. J/AJ/121/3160);
* m = 9.04 (Carpenter et al. 2001, Cat. J/AJ/121/3160);
* n = 1.55 (Herbst et al. 2000AJ....119..261H);
* o = 5.76 (Herbst et al. 2000AJ....119..261H);
* p = 8.69 (Stassun et al. 1999, Cat. J/AJ/117/2941);
* q = 0.84 (Stassun et al. 1999, Cat. J/AJ/117/2941 ;
* Herbst et al. 2002, Cat. J/A+A/396/513);
* r = 0.66 (Herbst et al. 2002, Cat. J/A+A/396/513);
* s = 3.51 (Herbst et al. 2000AJ....119..261H);
* t = 0.85 (Stassun et al. 1999, Cat. J/AJ/117/2941 ;
* Herbst et al. 2002, Cat. J/A+A/396/513);
* u = 8.44 (Herbst et al. 2000AJ....119..261H);
*Note (3): Reference for Per, defined as follows:
* H = Herbst et al. (2002, Cat. J/A+A/396/513);
* h = Herbst et al. (2000AJ....119..261H);
* s = Stassun et al. (1999, Cat. J/AJ/117/2941);
* c = Carpenter et al. (2001, Cat. J/AJ/121/3160);
* U = W. Herbst (unpublished).
*Note (4): Indicates filtered light curves (N,L or H) for which the LNP analysis
* yielded FAP<0.1%. A '+' indicates that the periodogram analysis
* was not performed because either Per<2.0d or Cts<100.
C=============================================================================
C Loading file 'table1.dat' ! COUP sources with assigned rotational period.
C Format for file interpretation
1 format(
+ I4,1X,I5,1X,I5,A1,1X,F5.2,1X,A1,1X,A4,1X,F5.2,1X,F3.1,1X,F4.1,
+ 1X,F4.1,1X,F5.1,1X,A3)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,295
read(1,'(A60)')ar__
read(ar__,1)
+ COUP,Cts,OptId,m_OptId,Per,n_Per,r_Per,Mass,LogAge,LogLx,
+ Log_Lx_Lb,WCaII,Mod
if(ar__(12:16) .EQ. '') OptId = iNULL__
if(ar__(32:36) .EQ. '') Mass = rNULL__
if(ar__(38:40) .EQ. '') LogAge = rNULL__
if(ar__(42:45) .EQ. '') LogLx = rNULL__
if(ar__(47:50) .EQ. '') Log_Lx_Lb = rNULL__
if(ar__(52:56) .EQ. '') WCaII = rNULL__
c ..............Just test output...........
write(6,1)
+ COUP,Cts,OptId,m_OptId,Per,n_Per,r_Per,Mass,LogAge,LogLx,
+ Log_Lx_Lb,WCaII,Mod
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end