Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/108/1276 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-19
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/108/1276 Clusters in GEHRs (Mayya, 1994)
*================================================================================
*Embedded clusters in giant extragalactic HII Regions. I. BVRHalpha photometry
* Mayya Y.D.
* <Astron. J. 108, 1276 (1994)>
* =1994AJ....108.1276M (SIMBAD/NED Reference)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3' ! Photometric catalogue of H II regions
integer*4 nr__
parameter (nr__=186) ! Number of records
character*93 ar__ ! Full-size record
character*12 Gal ! Galaxies name (g for groups)
integer*4 ID ! H II region numbers (1)
integer*4 Xpos ! (pix) X pixel coordinate (2)
integer*4 Ypos ! (pix) Y coordinate (2)
character*1 dirRA ! [EW] Direction of RA position (3)
integer*4 posRA ! (arcsec) ? Approximate right ascension position (3)
character*1 dirDE ! [NS] Direction of DE position (3)
integer*4 posDE ! (arcsec) ? Approximate declination position (3)
real*4 Diam ! (arcsec) Diam. of aperture for mag. extractions
character*1 l_Vmag ! [>] Limiting character for V
real*4 Vmag ! (mag) V magnitude (4)
real*4 B_V ! (mag) []? B-V color (4)
real*4 V_R ! (mag) []? V-R color (4)
real*4 Salpha ! ([mW/m2]) Log of observed H_alpha+[N II] flux
character*1 l_W_Ha ! Limiting character for W(Ha)
integer*4 W_Ha ! (0.1nm) Emission equivalent width (5)
integer*4 Qual ! Index of photometric quality (6)
character*14 OtherID ! Id. from other authors when available (7)
*Note (1): H II region numbers as identified on the charts in the printed paper.
*Note (2): X and Y pixel coordinates on the aligned CCD images, which are the
* same as that appearing on the grid around identification charts.
* For NGC 4449 the grids contain different pixel numbers than that
* given in these columns for the reasons mentioned in the text.
*Note (3): Approximate position of the H II region, along Right Ascension and
* declination in seconds of arc, with respect to the galactic nucleus.
* These were obtained by transforming X and Y assuming that the RA-DEC
* axis is aligned with X-Y axis of the CCD. Since the alignment during
* observations is only approximate (<=5deg), RA and DEC values away
* from the center are less accurate, compared to those near the center
* of the CCD. Thus the positions should be used only for identification
* purposes. E, W, N, and S preceeding the numbers indicate respectively
* whether the H II region is to the east, west, north or south of the
* nucleus of the galaxy.
*Note (4): V Magnitude, B-V and V-R colors of H II regions after subtracting
* assumed background. The rms errors on the measured magnitudes are
* in the range 0.05-0.10, as estimated from measurements on multiple
* frames.
*Note (5): H_alpha + [N II] emission equivalent width in A with R magnitude as
* an estimate for the continuum at H_alpha, computed using the equation
* W(Ha)=1.633E-11*F_alpha/10**(-0.4(R+48.6))
* where, F_alpha is the H_alpha + [N II] flux in mW/m^2 (erg/s/cm^2).
* The measurement errors are <20A. Note that the R band magnitudes used
* in the above definition include emission from the nebular continuum
* and lines.
*Note (6): An index of photometric quality. It is an integer between 1 and 4
* and gives a measure of the background domination for BVR
* measurements. Higher the index, more sensitive are the colors to the
* background measurement. See printed paper for details.
*Note (7): Identification from other authors when available. For measurements
* with bigger apertures, individual GEHRs enclosed within the aperture
* are indicated. The notations used for identifications are:
* CM Crillon and Monnet 1969, =1969A&A.....1..449C
* HK Hodge and Kennicutt 1983, =1983AJ.....88..296H
* HP Hawley and Phillips 1980, =1980ApJ...235..783H
* AN Alloin and Nieto 1982, =1982A&AS...50..491A
* Oka Oka et. al 1974, PASJ, 26, 289
* Tpp Prabhu 1980, ApSpSci., 68, 519
* L Lindblad, P.O. see Alloin et. al, 1981A&A...101..377A
* M McCall, Rybski, and Shields 1985, =1985ApJS...57....1M
* RW Roy and Walsh: 1986MNRAS.223...39R; 1987MNRAS.228..883R;
* 1988MNRAS.234..977R
* WR Walsh and Roy: 1989MNRAS.239..297W; 1989ApJ...341..722W
C=============================================================================
C Loading file 'table3' ! Photometric catalogue of H II regions
C Format for file interpretation
1 format(
+ A12,1X,I2,2X,I3,1X,I3,2X,A1,I3,1X,A1,I3,2X,F4.1,1X,A1,F5.2,1X,
+ F5.2,1X,F5.2,2X,F6.2,1X,A1,I4,2X,I1,2X,A14)
C Effective file loading
open(unit=1,status='old',file=
+'table3')
write(6,*) '....Loading file: table3'
do i__=1,186
read(1,'(A93)')ar__
read(ar__,1)
+ Gal,ID,Xpos,Ypos,dirRA,posRA,dirDE,posDE,Diam,l_Vmag,Vmag,B_V,
+ V_R,Salpha,l_W_Ha,W_Ha,Qual,OtherID
if(ar__(28:30) .EQ. '') posRA = iNULL__
if(ar__(33:35) .EQ. '') posDE = iNULL__
if(ar__(50:54) .EQ. '') B_V = rNULL__
if(ar__(56:60) .EQ. '') V_R = rNULL__
c ..............Just test output...........
write(6,1)
+ Gal,ID,Xpos,Ypos,dirRA,posRA,dirDE,posDE,Diam,l_Vmag,Vmag,B_V,
+ V_R,Salpha,l_W_Ha,W_Ha,Qual,OtherID
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end