Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/448/179 into FORTRAN code for loading all data files into arrays.
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-18
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/ApJ/448/179 HST photometry in R136 (Hunter+ 1995)
*================================================================================
*The intermediate stellar mass population in R136 determined from Hubble Space
*Telescope planetary camera 2 images
* Hunter D.A., Shaya E.J., Holtzman J.A., Light R.M., Earl J., Oneil Jr.
* <Astrophys. J. 448, 179 (1995)>
* =1995ApJ...448..179H
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! The photometry of stars in the R136 region
(completed with astrometry in April 2016)
integer*4 nr__
parameter (nr__=3623) ! Number of records
character*126 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg (nr__) ! (deg) Right Ascension J2000
real*8 DEdeg (nr__) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 Star (nr__) ! [1/3623] Star identification number
real*4 Xpos (nr__) ! (pix) [0/800] X pixel coordinate (1)
real*4 Ypos (nr__) ! (pix) [0/800] Yixel coordinate (1)
real*4 Umag (nr__) ! (mag) [10/22]?=100.00 HST/WFPC2 F336W magnitude
real*4 e_Umag (nr__) ! (mag) [0.01/0.6]?=100.00 F336W magnitude uncertainty
real*4 Vmag (nr__) ! (mag) [12/25]?=100.00 HST/WFPC2 F555W magnitude
real*4 e_Vmag (nr__) ! (mag) [0.01/1.4]?=100.00 F555W magnitude uncertainty
real*4 Imag (nr__) ! (mag) [11/24]?=100.00 HST/WFPC2 F814W magnitude
real*4 e_Imag (nr__) ! (mag) [0.01/0.6]?=100.00 F814W magnitude uncertainty
real*8 U_V (nr__) ! (mag) ?=100.00 F336W-F555W color
real*8 e_U_V (nr__) ! (mag) [0.02/0.6]?=100.00 F336W-F555W color uncertainty
real*8 V_I (nr__) ! (mag) ?=100.00 F555W-F814W color
real*8 e_V_I (nr__) ! (mag) [0.02/1.5]?=100.00 F555W-F814W color uncertainty
integer*4 RAh (nr__) ! (h) [5] Right Ascension J2000 (hours) (2)
integer*4 RAm (nr__) ! (min) [38] Right Ascension J2000 (minutes) (2)
real*4 RAs (nr__) ! (s) Right Ascension J2000 (seconds) (2)
character*1 DE_ (nr__) ! Declination J2000 (sign) (2)
integer*4 DEd (nr__) ! (deg) [69] Declination J2000 (degrees) (2)
integer*4 DEm (nr__) ! (arcmin) [5/6] Declination J2000 (minutes) (2)
real*4 DEs (nr__) ! (arcsec) Declination J2000 (seconds) (2)
*Note (1): the X,Y coordinates are those in the short exposure F555W image,
* and the coordinate system is indicated in Figure 2 of the printed paper.
*Note (2): accurate positions were supplied in April 2016 by B. Skiff
* (Lowell Obs.); the astrometry accuracy is estimated about +/-0.1arcsec,
* the internal error being about 0.02arcsec (0.3pix). More details about
* the reduction are given below in the "Astrometry" section below.
C=============================================================================
C Loading file 'table2.dat' ! The photometry of stars in the R136 region
* (completed with astrometry in April 2016)
C Format for file interpretation
1 format(
+ I6,1X,F6.1,1X,F6.1,1X,F6.2,1X,F6.2,1X,F6.2,1X,F6.2,1X,F6.2,1X,
+ F6.2,1X,F8.2,1X,F8.2,1X,F8.2,1X,F8.2,3X,I2,1X,I2,1X,F6.3,1X,
+ A1,I2,1X,I2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,3623
read(1,'(A126)')ar__
read(ar__,1)
+ Star(i__),Xpos(i__),Ypos(i__),Umag(i__),e_Umag(i__),Vmag(i__),
+ e_Vmag(i__),Imag(i__),e_Imag(i__),U_V(i__),e_U_V(i__),
+ V_I(i__),e_V_I(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
+ DEd(i__),DEm(i__),DEs(i__)
RAdeg(i__) = rNULL__
DEdeg(i__) = rNULL__
c Derive coordinates RAdeg and DEdeg from input data
c (RAdeg and DEdeg are set to rNULL__ when unknown)
if(RAh(i__) .GT. -180) RAdeg(i__)=RAh(i__)*15.
if(RAm(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAm(i__)/4.
if(RAs(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAs(i__)/240.
if(DEd(i__) .GE. 0) DEdeg(i__)=DEd(i__)
if(DEm(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEm(i__)/60.
if(DEs(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEs(i__)/3600.
if(DE_(i__).EQ.'-'.AND.DEdeg(i__).GE.0) DEdeg(i__)=-DEdeg(i__)
c ..............Just test output...........
write(6,1)
+ Star(i__),Xpos(i__),Ypos(i__),Umag(i__),e_Umag(i__),Vmag(i__),
+ e_Vmag(i__),Imag(i__),e_Imag(i__),U_V(i__),e_U_V(i__),
+ V_I(i__),e_V_I(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
+ DEd(i__),DEm(i__),DEs(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end