Conversion of standardized ReadMe file for
catalog 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-May-02
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. III/197 IRAS Low Resolution Spectra (IRAS team, 1987)
*================================================================================
*IRAS Low Resolution Spectra (LRS)
* Joint IRAS Science Working Group
* <NASA RP-1190 (1987)>
* =1987yCat.3197....0J
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'assoc.dat' ! Associated sources
integer*4 nr__
parameter (nr__=10913) ! Number of records
character*58 ar__ ! Full-size record
character*11 IRAS ! IRAS source name
integer*4 RecNo ! Record number of IRAS source in lrs.dat
integer*4 CatNum ! Catalog number (1)
character*15 Source ! Source identification
character*5 Type ! Source type or spectral class (1)
integer*4 Radius ! (arcsec) Radius vector from IRAS source to association
integer*4 Pos ! (deg) Position angle (E of N), IRAS source to object
integer*4 Field1 ! Object data field 1, catalog dependent (1)
integer*4 Field2 ! Object data field 2, catalog dependent (1)
integer*4 Field3 ! Object data field 3, catalog dependent (1)
*Note (1): Table X.B.4 in the "IRAS Catalogs and Atlases Explanatory:
* Meaning of the Source Association Fields.
* ------------------------------------------------------------------------------
* CatNum Field and Meaning
* ------------------------------------------------------------------------------
* 1 GCVS Type Blank
* Field1 = Code gives meaning for Fields 2-3
* if Field1 = 1 Field2 and Field3 are B mag [decimag] at
* max,min
* = 2 Field2 and Field3 are V mag [decimag] at
* max,min
* = 3 Field2 and Field3 are photographic mag
* [decimag] at max,min
* = 4 Field2 and Field3 are estimated V mag
* [decimag] at max,min
* = 5 Field2 is 999 and Field3 is 0
* ------------------------------------------------------------------------------
* 2 Dearborn Type Blank
* Obs. Field1 Code for Field2 (1,2)
* Field2 if Field1 is 1, Field2 is red magnitude
* [decimag]*
* if Field1 is 2, Field2 is 999
* Field3 0
* ------------------------------------------------------------------------------
* 3 Revised Type Blank
* AFGL Field1 Magnitude at 4.2 microns [decimag]
* Field2 Magnitude at 11 microns [decimag]
* Field3 Magnitude at 27 microns [decimag]
* ------------------------------------------------------------------------------
* 4 2-Micron Type Blank
* Sky Survey Field1 K magnitude [decimag]
* Field2 I magnitude [decimag]
* Field3 0
* ------------------------------------------------------------------------------
* 5 Globules Type Blank
* (Wesselius) Field1 999
* Field2 Minimum diameter [arcsec]
* Field3 Maximum diameter [arcsec]
* ------------------------------------------------------------------------------
* 6 RC2 Type Blank
* Field1 Harvard V magnitude [decimag]
* Field2 B(T) [decimag]
* Field3 D(0) [arcsec]
* ------------------------------------------------------------------------------
* 7 Stars with Type Blank
* em. lines Field1 V magnitude [decimag]
* Field2 999
* Field3 0
* ------------------------------------------------------------------------------
* 8 Equatorial Type Blank
* IR Cat. Field1 Flux density [1.0E-16 W/cm**2/um]
* at 2.7 microns
* Field2 999
* Field3 0
* ------------------------------------------------------------------------------
* 9 UGC Type Blank
* Field1 Zwicky magnitude [decimag]
* Field2 Minimum diameter [arcsec] in B
* Field3 Maximum diameter [arcsec] in B
* ------------------------------------------------------------------------------
* 10 MCG Type Blank
* Field1 999
* Field2 Minimum diameter [arcsec] in B
* Field3 Maximum diameter [arcsec] in B
* ------------------------------------------------------------------------------
* 11 Strasbourg Type Blank
* Planetary Nebulae Field1 V magnitude of Nebula [decimag]
* Field2 B magnitude of Center Star [decimag]
* Field3 Minimum diameter of Nebula [arcsec]
* ------------------------------------------------------------------------------
* 12 Zwicky Type Blank
* Field1 Zwicky magnitude [decimag]
* Field2 999
* Field3 0
* ------------------------------------------------------------------------------
* 13 SAO Type Spectral Type
* Field1 V magnitude [decimag]
* Field2 p(g) magnitude [decimag]
* Field3 0
* ------------------------------------------------------------------------------
* 14 ESO/ Type First 3 characters of object type
* Uppsala Field1 B magnitude [decimag]
* Field2 Maximum diameter [arcsec]
* Field3 Minimum diameter [arcsec]
* ------------------------------------------------------------------------------
* 15 Bright Type Spectral Type
* Stars Field1 V magnitude [decimag]
* Field2 B-V [centimag]
* Field3 U-B [centimag]
* ------------------------------------------------------------------------------
* 16 Suspected Type Spectral Information
* Var. Field1 V magnitude at maximum [decimag]
* Field2 999
* Field3 0
* ------------------------------------------------------------------------------
* 17 Carbon Type Spectral Type (May be truncated)
* Stars Field1 p(g) magnitude [decimag]
* Field2 V magnitude [decimag]
* Field3 I magnitude [decimag]
* ------------------------------------------------------------------------------
* 18 Gliese Type Spectral Type (May be truncated)
* Field1 V magnitude [decimag]
* Field2 B-V magnitude [millimag]
* Field3 U-B magnitude [millimag]
* ------------------------------------------------------------------------------
* 19 S Stars Type Blank
* Field1 p(g) magnitude [millimag]
* Field2 V magnitude [decimag]
* Field3 I magnitude [decimag]
* ------------------------------------------------------------------------------
* 20 Parkes HII Type Blank
* Survey Field1 999
* Field2 Minimum diameter [arcsec]
* Field3 Maximum diameter [arcsec]
* ------------------------------------------------------------------------------
* 21 Bonn HII Type Blank
* Survey Field1 Flux density at 4.875 GHz (Jy)
* Field2 Diameter [arcsec]
* Field3 0
* ------------------------------------------------------------------------------
* 22 Blitz Type Blank
* Field1 Diameter [arcsec]
* Field2 V(CO) [Km/s]
* Field3 Peak T(A) [degrees K]
* ------------------------------------------------------------------------------
* 23 OSU Type Blank
* Field1 999
* Field2 999
* Field3 Diameter [arcsec]
* ------------------------------------------------------------------------------
* 24 IRC Type C if 2.2 micron sources are possibly
* confused, w/good pos. blank otherwise
* Field1 Right ascension difference (IRC-IRAS)
* [deciseconds of time]
* Field2 Declination difference (IRC-IRAS)
* [seconds of arc]
* Field3 0
* ------------------------------------------------------------------------------
* 25 DDO Type Blank
* Field1 999
* Field2 999
* Field3 0
* ------------------------------------------------------------------------------
* 26 Arp Type Blank
* Field1 999
* Field2 999
* Field 0
* ------------------------------------------------------------------------------
* 27 Markarian Type Blank
* Field1 999
* Field2 999
* Field3 0
* ------------------------------------------------------------------------------
* 28 Strong Type Object type (GAL or QSO)
* 5 GHz Field1 V magnitude [decimag]
* Field2 5 GHz flux density [deciJy]
* Field3 0
* ------------------------------------------------------------------------------
* 29 Veron- Type Object classification
* Veron Field1 V magnitude [decimag]
* Field2 Redshift x 1000
* Field3 0
* ------------------------------------------------------------------------------
* 30 Zwicky Type Blank
* 8 Lists Field1 999
* Field2 999
* Field3 0
* ------------------------------------------------------------------------------
* 31 VV Type Blank
* Field1 Special flag, (see below) 999 otherwise
* Field2 999
* Field3 0
* ------------------------------------------------------------------------------
* VV Catalog Special Flags (Catalog 31)
* ------------------------------------------------------------------------------
* Field1 Explanation
* 10 VV 10 has the same coordinates as VV 29 in the VV Atlas. The
* UGC was used to confirm that the coordinate is correct for VV
* 29 and erroneous for VV 10. The UGC position for VV 10 = UGC
* 10814 was adopted.
* 11 The VV position is substantially different (>400") from
* positions for the object in other catalogs. The VV position
* has been assumed to be in error because two or more other
* catalogs agree on a different position. The UGC position has
* been adopted.
* 12 Same as for 11, but the OSU position has been adopted.
* 13 The position in the VV Atlas, and the position listed for the
* VV object in the OSU are in disagreement. The true position
* has been established to be close to that of the OSU by the use
* of overlay transparencies on the POSS. The OSU position has
* been adopted.
* 14 Same as for 13, but the OSU position is not very good either,
* so a new position has been measured (accurate to about 1').
* ------------------------------------------------------------------------------
C=============================================================================
C Loading file 'assoc.dat' ! Associated sources
C Format for file interpretation
1 format(A11,I6,1X,I2,A15,A5,I3,I3,I4,I4,I4)
C Effective file loading
open(unit=1,status='old',file=
+'III/197/assoc.dat')
write(6,*) '....Loading file: assoc.dat'
do i__=1,10913
read(1,'(A58)')ar__
read(ar__,1)
+ IRAS,RecNo,CatNum,Source,Type,Radius,Pos,Field1,Field2,Field3
c ..............Just test output...........
write(6,1)
+ IRAS,RecNo,CatNum,Source,Type,Radius,Pos,Field1,Field2,Field3
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end