Conversion of standardized ReadMe file for
file /./ftp/cats/II/223/ 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. II/223 First Byurakan Survey (FBS), 2nd Program (Abrahamian et al., 1990-1996)
*================================================================================
*First Byurakan Survey (FBS), 2nd Program
* Abrahamian et al.
* <Astrophysics 32, 14 (1990); 33, 418 (1990); 33, 493 (1990);
* 34, 7 (1991); 36, 62 (1993); 36, 306 (1993); 37, 27 (1994);
* 37, 117 (1994); 37, 224 (1994); 38, 108 (1995); 39, 315 (1996) >
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'fbs2.dat' ! The second part of the First Byurakan Survey
integer*4 nr__
parameter (nr__=1103) ! Number of records
character*68 ar__ ! Full-size record
C B1950 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg ! (deg) Right Ascension B1950
real*8 DEdeg ! (deg) Declination B1950
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 Seq ! [1,1103]+ Sequential number (FBS B NNNN)
character*9 FBS ! FBS named based on B1950 position
integer*4 RAh ! (h) Right Ascension B1950 (hours)
integer*4 RAm ! (min) Right Ascension B1950 (minutes)
real*4 RAs ! (s) Right Ascension B1950 (seconds)
character*1 DE_ ! Declination B1950 (sign)
integer*4 DEd ! (deg) Declination B1950 (degrees)
integer*4 DEm ! (arcmin) Declination B1950 (minutes)
integer*4 DEs ! (arcsec) ? Declination B1950 (seconds)
real*4 Bmag ! (mag) Photographic magnitude
character*1 aType ! [QG*] abbreviation for QSO, Galaxy or Star
character*4 Type ! *Type of the object
character*5 SpType ! Spectral type for stars
character*3 survey ! *Existence in other survey
real*4 Mag2 ! (mag) ? Magnitude from survey
real*4 z ! ? Redshift, when known
character*8 Name ! Other name of the source
*Note on Type: this Type is made of two parameters:
* 1. The first parameter (related to B-V index) describes the ratio of
* the intensities of the red and blue regions of the spectrum:
* 'B' means that the blue part is stronger than the red part
* 'N' means that the intensities of the two parts are equal
* 2. The second parameter (related to U-B index) characterizes the
* intensity of the ultraviolet region of the spectrum:
* '1' means that the blue-violet part is approximately 1.5 times
* longer than the red-yellow part
* '3' means that the blue-violet part is approximately as long as
* the red-yellow part
* '2' describes the intermediate situation.
* In addition, the existence of emission details is noted by 'e' or 'e:',
* and absorption details by 'a' or 'a:'
*Note on survey: the other surveys are
* PG = Palomar Green survey (see Cat. <II/207>)
* CBS = Case Blue Stars (Pesch and Sanduleak, 1983-95)
* CSO = Case Stellar Objects (Pesch and Sanduleak, 1983-95)
* KUV = Kiso UV excess objects (Nogushi et al., 1980AnTok..18...55N)
C=============================================================================
C Loading file 'fbs2.dat' ! The second part of the First Byurakan Survey
C Format for file interpretation
1 format(
+ I4,1X,A9,1X,I2,I2,F4.1,A1,I2,I2,I2,1X,F4.1,A1,A4,1X,A5,A3,
+ F5.2,F5.3,1X,A8)
C Effective file loading
open(unit=1,status='old',file=
+'fbs2.dat')
write(6,*) '....Loading file: fbs2.dat'
do i__=1,1103
read(1,'(A68)')ar__
read(ar__,1)
+ Seq,FBS,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Bmag,aType,Type,SpType,
+ survey,Mag2,z,Name
if(ar__(29:30) .EQ. '') DEs = iNULL__
if(ar__(50:54) .EQ. '') Mag2 = rNULL__
if(ar__(55:59) .EQ. '') 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)
+ Seq,FBS,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Bmag,aType,Type,SpType,
+ survey,Mag2,z,Name
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end