Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJS/247/7 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 2026-Jun-15
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/247/7 Narrowband Ca photometry for dwarf spheroidal galaxies (Han+, 2020)
*================================================================================
*Narrowband Ca photometry for dwarf spheroidal galaxies.
*I. Chemostructural study on Draco, Sextans, and Canes Venatici I.
* Han S.-I., Kim H.-S., Yoon S.-J., Lee Y.-W., Arimoto N., Okamoto S.,
* Ree C.H.
* <Astrophys. J. Suppl. Ser., 247, 7 (2020)>
* =2020ApJS..247....7H
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Photometric measurements for the point sources
in Draco
integer*4 nr__
parameter (nr__=139435) ! Number of records
character*73 ar__ ! Full-size record
C J2000 position composed of: RAdeg DEdeg
real*8 RAdeg (nr__) ! (deg) Right Ascension in decimal degrees (J2000)
real*8 DEdeg (nr__) ! (deg) Declination in decimal degrees (J2000)
real*4 Ca (nr__) ! (mag) [14.1/28.1] The Subaru/Sprime-Cam Ca narrow
* filter magnitude (1)
real*4 e_Ca (nr__) ! (mag) [0.001/1.6] Uncertainty in Ca
real*4 b (nr__) ! (mag) [12.5/27.7] The Subaru/Sprime-Cam b narrow
* filter magnitude (1)
real*4 e_b (nr__) ! (mag) [0.001/1.6] Uncertainty in b
real*4 y (nr__) ! (mag) [12.3/27.4] The Subaru/Sprime-Cam y narrow
* filter magnitude (1)
real*4 e_y (nr__) ! (mag) [0.001/1.7] Uncertainty in y
real*4 CHI (nr__) ! [0.2/23.2] DAOPHOT CHI parameter
real*4 SHARP (nr__) ! [-5.51/11.2] DAOPHOT SHARP parameter
*Note (1): The instrumental Ca, b, and y magnitudes were converted to the
* standard system using the Milky Way globular clusters M5 and M15
* because the standard stars are too bright for the Suprime-Cam. These
* GCs were observed with the du Pont 2.5m telescope using the same new
* Ca-by filter set and transformed to the standard Ca-by photometric
* system. See section 2 for further explanations.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Photometric measurements for the point sources
in Sextans
integer*4 nr__1
parameter (nr__1=69962) ! Number of records
character*73 ar__1 ! Full-size record
C J2000 position composed of: RAdeg DEdeg
real*8 RAdeg_1 (nr__1) ! (deg) Right Ascension in decimal degrees (J2000)
real*8 DEdeg_1 (nr__1) ! (deg) Declination in decimal degrees (J2000)
real*4 Ca_1 (nr__1) ! (mag) [14.1/28.1] The Subaru/Sprime-Cam Ca narrow
* filter magnitude (1)
real*4 e_Ca_1 (nr__1) ! (mag) [0.001/1.6] Uncertainty in Ca
real*4 b_1 (nr__1) ! (mag) [12.5/27.7] The Subaru/Sprime-Cam b narrow
* filter magnitude (1)
real*4 e_b_1 (nr__1) ! (mag) [0.001/1.6] Uncertainty in b
real*4 y_1 (nr__1) ! (mag) [12.3/27.4] The Subaru/Sprime-Cam y narrow
* filter magnitude (1)
real*4 e_y_1 (nr__1) ! (mag) [0.001/1.7] Uncertainty in y
real*4 CHI_1 (nr__1) ! [0.2/23.2] DAOPHOT CHI parameter
real*4 SHARP_1 (nr__1) ! [-5.51/11.2] DAOPHOT SHARP parameter
*Note (1): The instrumental Ca, b, and y magnitudes were converted to the
* standard system using the Milky Way globular clusters M5 and M15
* because the standard stars are too bright for the Suprime-Cam. These
* GCs were observed with the du Pont 2.5m telescope using the same new
* Ca-by filter set and transformed to the standard Ca-by photometric
* system. See section 2 for further explanations.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! Photometric measurements for the point sources
in Canes Venatici I (CVnI)
integer*4 nr__2
parameter (nr__2=47265) ! Number of records
character*73 ar__2 ! Full-size record
C J2000 position composed of: RAdeg DEdeg
real*8 RAdeg_2 (nr__2) ! (deg) Right Ascension in decimal degrees (J2000)
real*8 DEdeg_2 (nr__2) ! (deg) Declination in decimal degrees (J2000)
real*4 Ca_2 (nr__2) ! (mag) [14.1/28.1] The Subaru/Sprime-Cam Ca narrow
* filter magnitude (1)
real*4 e_Ca_2 (nr__2) ! (mag) [0.001/1.6] Uncertainty in Ca
real*4 b_2 (nr__2) ! (mag) [12.5/27.7] The Subaru/Sprime-Cam b narrow
* filter magnitude (1)
real*4 e_b_2 (nr__2) ! (mag) [0.001/1.6] Uncertainty in b
real*4 y_2 (nr__2) ! (mag) [12.3/27.4] The Subaru/Sprime-Cam y narrow
* filter magnitude (1)
real*4 e_y_2 (nr__2) ! (mag) [0.001/1.7] Uncertainty in y
real*4 CHI_2 (nr__2) ! [0.2/23.2] DAOPHOT CHI parameter
real*4 SHARP_2 (nr__2) ! [-5.51/11.2] DAOPHOT SHARP parameter
*Note (1): The instrumental Ca, b, and y magnitudes were converted to the
* standard system using the Milky Way globular clusters M5 and M15
* because the standard stars are too bright for the Suprime-Cam. These
* GCs were observed with the du Pont 2.5m telescope using the same new
* Ca-by filter set and transformed to the standard Ca-by photometric
* system. See section 2 for further explanations.
C=============================================================================
C Loading file 'table2.dat' ! Photometric measurements for the point sources
* in Draco
C Format for file interpretation
1 format(
+ F10.6,1X,F9.6,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3,
+ 1X,F6.3,1X,F6.3)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,139435
read(1,'(A73)')ar__
read(ar__,1)
+ RAdeg(i__),DEdeg(i__),Ca(i__),e_Ca(i__),b(i__),e_b(i__),
+ y(i__),e_y(i__),CHI(i__),SHARP(i__)
c ..............Just test output...........
write(6,1)
+ RAdeg(i__),DEdeg(i__),Ca(i__),e_Ca(i__),b(i__),e_b(i__),
+ y(i__),e_y(i__),CHI(i__),SHARP(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Photometric measurements for the point sources
* in Sextans
C Format for file interpretation
2 format(
+ F10.6,1X,F9.6,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3,
+ 1X,F6.3,1X,F6.3)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,69962
read(1,'(A73)')ar__1
read(ar__1,2)
+ RAdeg_1(i__),DEdeg_1(i__),Ca_1(i__),e_Ca_1(i__),b_1(i__),
+ e_b_1(i__),y_1(i__),e_y_1(i__),CHI_1(i__),SHARP_1(i__)
c ..............Just test output...........
write(6,2)
+ RAdeg_1(i__),DEdeg_1(i__),Ca_1(i__),e_Ca_1(i__),b_1(i__),
+ e_b_1(i__),y_1(i__),e_y_1(i__),CHI_1(i__),SHARP_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4.dat' ! Photometric measurements for the point sources
* in Canes Venatici I (CVnI)
C Format for file interpretation
3 format(
+ F10.6,1X,F9.6,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3,
+ 1X,F6.3,1X,F6.3)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,47265
read(1,'(A73)')ar__2
read(ar__2,3)
+ RAdeg_2(i__),DEdeg_2(i__),Ca_2(i__),e_Ca_2(i__),b_2(i__),
+ e_b_2(i__),y_2(i__),e_y_2(i__),CHI_2(i__),SHARP_2(i__)
c ..............Just test output...........
write(6,3)
+ RAdeg_2(i__),DEdeg_2(i__),Ca_2(i__),e_Ca_2(i__),b_2(i__),
+ e_b_2(i__),y_2(i__),e_y_2(i__),CHI_2(i__),SHARP_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end