Conversion of standardized ReadMe file for
file /./ftp/cats/II/197 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-Oct-14
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/197 ISM towards IC 348 and Per OB2 (Cernis, 1993)
*================================================================================
*Interstellar extinction in the direction of the open cluster IC 348 and the
*Per OB2 association
* Cernis K.
* <Baltic Astron. 2, 214 (1993)>
* =1993BaltA...2..214C
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1' ! The results of photometry (all stars)
integer*4 nr__
parameter (nr__=189) ! Number of records
character*81 ar__ ! Full-size record
C B1950 position composed of: RAh RAm RAs DE- DEd DEm
real*8 RAdeg (nr__) ! (deg) Right Ascension B1950
real*8 DEdeg (nr__) ! (deg) Declination B1950
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 Seq (nr__) ! Sequential number
character*1 n_Seq (nr__) ! [*] Note (1)
character*6 BD (nr__) ! BD designation
integer*4 HD (nr__) ! []? HD designation
integer*4 RAh (nr__) ! (h) Right ascension B1950
integer*4 RAm (nr__) ! (min) Right ascension B1950
integer*4 RAs (nr__) ! (s) Right ascension B1950
character*1 DE_ (nr__) ! Declination sign B1950
integer*4 DEd (nr__) ! (deg) Declination B1950
real*4 DEm (nr__) ! (arcmin) Declination B1950
character*8 Sp (nr__) ! spectral type
real*4 Vmag (nr__) ! (mag) V magnitude (Vilnius system)
real*4 U_P (nr__) ! (mag) U-P colour index (Vilnius system)
real*4 P_X (nr__) ! (mag) P-X colour index (Vilnius system)
real*4 X_Y (nr__) ! (mag) X-Y colour index (Vilnius system)
real*4 Y_Z (nr__) ! (mag) Y-Z colour index (Vilnius system)
real*4 Z_V (nr__) ! (mag) Z-V colour index (Vilnius system)
real*4 V_S (nr__) ! (mag) V-S colour index (Vilnius system)
integer*4 n (nr__) ! Number of independent observations
*Note (1):
* 6. IDS 90-59 AB, {DELTA}m = 1.6, D = 2.4" . Measured together.
* 22. Photometric classification is uncertain. Possible photometric binary star
* as B3III+F5I.
* 36. ADS 2696A, {DELTA}m = 0.2, D = 6", measured separately.
* 37. ADS 2696B.
* 42. V magnitude from BSC4, Hoffleit (1982).
* 63. ADS 2723, {DELTA}m = 0.0, D = 11.4", measured separately.
* 67. o Per. V magnitude from BSC4, Hoffleit (1982).
* 69. The star has considerably lower Q_XZS_ values due to possible emission in
* the H{alpha} line.
* 71. ADS 2729 AB, {DELTA}m = 0.2, D =1". Measured together.
* 77. ADS 2730, {DELTA}m = 0.2, D = 0.45" . Measured together.
* 97. LkH{alpha} 329 (Herbig and Rao 1972). The star has considerably lower
* Q_XZS_ values.
* 102. LKH{alpha} 330 (Herbig and Rao 1972).
* 106. ADS 2723, {DELTA}m = 0.0, D = 11". Measured together.
* 117. ADS 2771A.
* 118. ADS 2772AB, {DELTA}m = 2.5, D = 3".
* 121. ADS 2784 AB, {DELTA}m = 2.0, D = 2".
* 123. SB, Var V467 Per, eclipsing binary system.
* 127. ADS 2804 AB, {DELTA}m = 4.7 , D = 1". Measured together.
* 147. ADS 2834 A, {DELTA}m = 5.7, D = 7". Measured together.
* 149. V magnitude from BSC4, Hoffleit (1982).
* 152. ADS 2857, {DELTA}m = 2.3, D = 3". Measured together.
* 153. ADS 2859, {DELTA}m = 5.8, D = 22". Var X Per, ({gamma} Cas type).
* Spectrum from BSC4, Hoffleit (1982).
* 155. ADS 2866 AB, {DELTA}m = 3.4, D = 1". Measured together.
* 159. Var, NSV 1418, {beta} Cep- type.
* 163. V magnitude and spectrum from BSC4, Hoffleit (1982).
* 186. ADS 2975 AB, {DELTA}m = 0.2, D = 2". Measured together.
* 188. Var, NSV 1459, V = 6.98 -- 7.27 (BSC4, Hoffleit, 1982).
* 189. Var, AG Per, Eclipsing binary system. {DELTA}m = 0.8, D = 0.8".
* Measured together.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2' ! The results of photometric quantification of
stars in the vicinity of the dark cloud L1470
integer*4 nr__1
parameter (nr__1=40) ! Number of records
character*53 ar__1 ! Full-size record
integer*4 No (nr__1) ! Sequential number
character*6 BD_1 (nr__1) ! BD number
character*2 Sp_1 (nr__1) ! Spectral type
integer*4 n_Sp (nr__1) ! [1-2]? Note on Sp (1)
character*7 Sp_Viln (nr__1) ! Spectral type from Vilnius system
real*4 Vmag_1 (nr__1) ! (mag) V magnitude
real*4 Mv (nr__1) ! (mag) Absolute magnitude
character*1 u_Mv (nr__1) ! uncertainty flag on Mv
real*4 E_B_V (nr__1) ! (mag) Reddening
real*4 Av (nr__1) ! (mag) Visual extinction
integer*4 Dist (nr__1) ! (pc) Distance
character*1 u_Dist (nr__1) ! [)] uncertainty flag on Dist
*Note (1): References for the spectra:
* 1: Cannon and Mayall (1949), 2: AGK 3 catalog.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4' ! The results of photometric quantification of
IC 348 stars
integer*4 nr__2
parameter (nr__2=46) ! Number of records
character*70 ar__2 ! Full-size record
integer*4 Seq_1 (nr__2) ! Sequential number
character*1 n_Seq_1 (nr__2) ! [*] Note (1)
character*6 BD_2 (nr__2) ! BD denomination
integer*4 G (nr__2) ! []? Number in the Gingrich (1922) list
character*2 F (nr__2) ! Number in the Fredrick (1956) list
character*7 Sp_2 (nr__2) ! Spectral type
character*1 n_Sp_1 (nr__2) ! [3-6] Note for Sp (2)
character*8 Sp_Viln_1 (nr__2) ! Spectral type from Vilnius system
real*4 Vmag_2 (nr__2) ! (mag) V magnitude (Vilnius system)
real*4 Mv_1 (nr__2) ! (mag) Absolute magnitude
character*1 u_Mv_1 (nr__2) ! Uncertainty flag on Mv
real*4 E_B_V_1 (nr__2) ! (mag) Redenning
real*4 Av_1 (nr__2) ! (mag) Visual extinction
integer*4 Dist_1 (nr__2) ! (pc) Distance
character*1 u_Dist_1 (nr__2) ! [)] uncertainty flag on Dist
character*4 Mem (nr__2) ! Membership (3)
*Note (1): Numbers of the most reliable cluster members, estimated by Fredrick
* (1956), are marked by asterisks.
*Note (2): References for spectra:
* 3: Harris et al. (1954), 4: Strom et al. (1974),
* 5: Vyssotsky and Williams (1948), 6: Herbig and Rao (1972).
*Note (3): nm: no member, m: member
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6' ! The results of photometric quantification of
stars in the region of the association Per OB2
integer*4 nr__3
parameter (nr__3=100) ! Number of records
character*69 ar__3 ! Full-size record
integer*4 Seq_2 (nr__3) ! Sequential number
character*6 BD_3 (nr__3) ! BD denomination
character*7 Sp_3 (nr__3) ! Spectral type
character*1 n_Sp_2 (nr__3) ! [7-9] Note for Sp (1)
character*8 Sp_Viln_1 (nr__3) ! Spectral type from Vilnius system
real*4 Vmag_3 (nr__3) ! (mag) V magnitude (Vilnius system)
real*4 Mv_2 (nr__3) ! (mag) Absolute magnitude
character*1 u_Mv_2 (nr__3) ! uncertainty flag on Mv
real*4 E_B_V_1 (nr__3) ! (mag) Redenning
real*4 Av_2 (nr__3) ! (mag) Visual extinction
integer*4 Dist_2 (nr__3) ! (pc) Distance
character*1 u_Dist_2 (nr__3) ! [)] uncertainty flag on Dist
character*4 Mem_1 (nr__3) ! Membership (2)
*Note (1): References for spectra:
* 7: Guetter (1977), 8: Klochkova & Kopylov (1985)
* 9: Seyfert et al. (1960)
*Note (2): nm: no member, m: member
C=============================================================================
C Loading file 'table1' ! The results of photometry (all stars)
C Format for file interpretation
1 format(
+ I3,A1,1X,A6,1X,I5,1X,I2,1X,I2,1X,I2,A1,I2,1X,F4.1,1X,A8,1X,
+ F5.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,I1)
C Effective file loading
open(unit=1,status='old',file=
+'table1')
write(6,*) '....Loading file: table1'
do i__=1,189
read(1,'(A81)')ar__
read(ar__,1)
+ Seq(i__),n_Seq(i__),BD(i__),HD(i__),RAh(i__),RAm(i__),
+ RAs(i__),DE_(i__),DEd(i__),DEm(i__),Sp(i__),Vmag(i__),
+ U_P(i__),P_X(i__),X_Y(i__),Y_Z(i__),Z_V(i__),V_S(i__),n(i__)
if(ar__(13:17) .EQ. '') HD(i__) = iNULL__
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(DE_(i__).EQ.'-'.AND.DEdeg(i__).GE.0) DEdeg(i__)=-DEdeg(i__)
c ..............Just test output...........
write(6,1)
+ Seq(i__),n_Seq(i__),BD(i__),HD(i__),RAh(i__),RAm(i__),
+ RAs(i__),DE_(i__),DEd(i__),DEm(i__),Sp(i__),Vmag(i__),
+ U_P(i__),P_X(i__),X_Y(i__),Y_Z(i__),Z_V(i__),V_S(i__),n(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2' ! The results of photometric quantification of
* stars in the vicinity of the dark cloud L1470
C Format for file interpretation
2 format(
+ I3,1X,A6,1X,A2,1X,I1,3X,A7,1X,F5.2,1X,F4.1,A1,1X,F4.2,1X,F4.2,
+ 1X,I4,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table2')
write(6,*) '....Loading file: table2'
do i__=1,40
read(1,'(A53)')ar__1
read(ar__1,2)
+ No(i__),BD_1(i__),Sp_1(i__),n_Sp(i__),Sp_Viln(i__),
+ Vmag_1(i__),Mv(i__),u_Mv(i__),E_B_V(i__),Av(i__),Dist(i__),
+ u_Dist(i__)
if(ar__1(15:15) .EQ. '') n_Sp(i__) = iNULL__
c ..............Just test output...........
write(6,2)
+ No(i__),BD_1(i__),Sp_1(i__),n_Sp(i__),Sp_Viln(i__),
+ Vmag_1(i__),Mv(i__),u_Mv(i__),E_B_V(i__),Av(i__),Dist(i__),
+ u_Dist(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4' ! The results of photometric quantification of
* IC 348 stars
C Format for file interpretation
3 format(
+ I3,A1,1X,A6,1X,I2,1X,A2,1X,A7,1X,A1,2X,A8,1X,F5.2,1X,F4.1,A1,
+ 1X,F4.2,1X,F4.2,1X,I4,A1,1X,A4)
C Effective file loading
open(unit=1,status='old',file=
+'table4')
write(6,*) '....Loading file: table4'
do i__=1,46
read(1,'(A70)')ar__2
read(ar__2,3)
+ Seq_1(i__),n_Seq_1(i__),BD_2(i__),G(i__),F(i__),Sp_2(i__),
+ n_Sp_1(i__),Sp_Viln_1(i__),Vmag_2(i__),Mv_1(i__),u_Mv_1(i__),
+ E_B_V_1(i__),Av_1(i__),Dist_1(i__),u_Dist_1(i__),Mem(i__)
if(ar__2(13:14) .EQ. '') G(i__) = iNULL__
c ..............Just test output...........
write(6,3)
+ Seq_1(i__),n_Seq_1(i__),BD_2(i__),G(i__),F(i__),Sp_2(i__),
+ n_Sp_1(i__),Sp_Viln_1(i__),Vmag_2(i__),Mv_1(i__),u_Mv_1(i__),
+ E_B_V_1(i__),Av_1(i__),Dist_1(i__),u_Dist_1(i__),Mem(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table6' ! The results of photometric quantification of
* stars in the region of the association Per OB2
C Format for file interpretation
4 format(
+ I3,1X,A6,1X,A7,1X,A1,2X,A8,4X,F5.2,4X,F4.1,A1,1X,F4.2,1X,F4.2,
+ 1X,I4,A1,1X,A4)
C Effective file loading
open(unit=1,status='old',file=
+'table6')
write(6,*) '....Loading file: table6'
do i__=1,100
read(1,'(A69)')ar__3
read(ar__3,4)
+ Seq_2(i__),BD_3(i__),Sp_3(i__),n_Sp_2(i__),Sp_Viln_1(i__),
+ Vmag_3(i__),Mv_2(i__),u_Mv_2(i__),E_B_V_1(i__),Av_2(i__),
+ Dist_2(i__),u_Dist_2(i__),Mem_1(i__)
c ..............Just test output...........
write(6,4)
+ Seq_2(i__),BD_3(i__),Sp_3(i__),n_Sp_2(i__),Sp_Viln_1(i__),
+ Vmag_3(i__),Mv_2(i__),u_Mv_2(i__),E_B_V_1(i__),Av_2(i__),
+ Dist_2(i__),u_Dist_2(i__),Mem_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end