Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/683/822 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-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/ApJ/683/822 Star formation in Ophiuchus and Perseus II. (Jorgensen+, 2008)
*================================================================================
*Current star formation in the Ophiuchus and Perseus molecular clouds:
*constraints and comparisons from unbiased submillimeter and mid-infrared
*surveys. II.
* Jorgensen J.K., Johnstone D., Kirk H., Myers P.C., Allen L.E., Shirley Y.L.
* <Astrophys. J., 683, 822-843 (2008)>
* =2008ApJ...683..822J
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! List of candidate embedded YSOs in Ophiuchus
integer*4 nr__
parameter (nr__=27) ! Number of records
character*103 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 RAh (nr__) ! (h) c2d Hour of right ascension (J2000) (1)
integer*4 RAm (nr__) ! (min) c2d Minute of right ascension (J2000) (1)
real*4 RAs (nr__) ! (s) c2d Second of right ascension (J2000) (1)
character*1 DE_ (nr__) ! c2d Declination sign (J2000) (1)
integer*4 DEd (nr__) ! (deg) c2d Degree of declination (J2000) (1)
integer*4 DEm (nr__) ! (arcmin) c2d Arcminute of declination (J2000) (1)
real*4 DEs (nr__) ! (arcsec) c2d Arcsecond of declination (J2000) (1)
real*4 Conc (nr__) ! Concentration of the nearest SCUBA core
real*4 v3_6_4_5 (nr__) ! ? Spitzer [3.6]-[4.5] color index
real*4 v8_0_24 (nr__) ! ? Spitzer [8.0]-[24.0] color index
real*4 Sep (nr__) ! (arcsec) Separation between the Spitzer source and
* SCUBA core
real*4 Flux (nr__) ! (Jy) SCUBA Flux at 850um in Jy/beam
character*3 n_Flux (nr__) ! [ABC- ] Code for type of sources (2)
character*44 XID (nr__) ! Common identifiers from Simbad
character*2 Rem (nr__) ! [*g ] Remarks on source (3)
*Note (1): Position of Spitzer source from c2d catalog.
*Note (2): Code indicating whether the given source obeys:
* A = MIPS 24um source with [3.6]-[4.5]>1 and [8.0]-[24]>4.5;
* B = separation between Spitzer source and nearest SCUBA core less than 15";
* C = Associated submillimeter core has concentration higher than 0.6.
* A- = SCUBA flux refers to flux density at the exact position in the maps;
* for the remaining sources to the peak flux from the Clumpfind algorithm.
* Note that only A and B are used to construct this sample.
*Note (3): Flag as follows:
* * = Sources are included in the list of embedded YSOs by Wilking et al.
* (2008hsf2.book..351W).
* g = A complex system of at least three protostellar candidates: in addition
* to GSS 30-IRS1 a nearby source is seen at 16:26:22.38-24:22:52.9
* at a distance of 10.4" from the SCUBA core:
* [AMD2002] J162622-242254/ VSSG 12/ISO-Oph 34/GSS 30-IRS2.
* A third source, GSS 30-IRS3/LFAM 1*, is at 16:26:21.72-24:22:50.5,
* separated by 4.5" and with [3.6]-[4.5]=0.9 and [8.0]-[24]=5.3
* (although with low S/N in MIPS1 due to confusion with GSS 30-IRS1).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! List of candidate embedded YSOs for sources with
separations of 15"-30" of a MIPS source
integer*4 nr__1
parameter (nr__1=11) ! Number of records
character*103 ar__1 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 (nr__1) ! (deg) Right Ascension J2000
real*8 DEdeg_1 (nr__1) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 RAh_1 (nr__1) ! (h) c2d Hour of right ascension (J2000) (1)
integer*4 RAm_1 (nr__1) ! (min) c2d Minute of right ascension (J2000) (1)
real*4 RAs_1 (nr__1) ! (s) c2d Second of right ascension (J2000) (1)
character*1 DE__1 (nr__1) ! c2d Declination sign (J2000) (1)
integer*4 DEd_1 (nr__1) ! (deg) c2d Degree of declination (J2000) (1)
integer*4 DEm_1 (nr__1) ! (arcmin) c2d Arcminute of declination (J2000) (1)
real*4 DEs_1 (nr__1) ! (arcsec) c2d Arcsecond of declination (J2000) (1)
real*4 Conc_1 (nr__1) ! Concentration of the nearest SCUBA core
real*4 v3_6_4_5_1 (nr__1) ! ? Spitzer [3.6]-[4.5] color index
real*4 v8_0_24_1 (nr__1) ! ? Spitzer [8.0]-[24.0] color index
real*4 Sep_1 (nr__1) ! (arcsec) Separation between the Spitzer source and
* SCUBA core
real*4 Flux_1 (nr__1) ! (Jy) SCUBA Flux at 850um in Jy/beam
character*3 n_Flux_1 (nr__1) ! [ABC- ] Code for type of sources (2)
character*44 XID_1 (nr__1) ! Common identifiers from Simbad
character*2 Rem_1 (nr__1) ! [*g ] Remarks on source (3)
*Note (1): Position of Spitzer source from c2d catalog.
*Note (2): Code indicating whether the given source obeys:
* A = MIPS 24um source with [3.6]-[4.5]>1 and [8.0]-[24]>4.5;
* B = separation between Spitzer source and nearest SCUBA core less than 15";
* C = Associated submillimeter core has concentration higher than 0.6.
* A- = SCUBA flux refers to flux density at the exact position in the maps;
* for the remaining sources to the peak flux from the Clumpfind algorithm.
* Note that only A and B are used to construct this sample.
*Note (3): Flag as follows:
* * = Sources are included in the list of embedded YSOs by Wilking et al.
* (2008hsf2.book..351W).
* g = A complex system of at least three protostellar candidates: in addition
* to GSS 30-IRS1 a nearby source is seen at 16:26:22.38-24:22:52.9
* at a distance of 10.4" from the SCUBA core:
* [AMD2002] J162622-242254/ VSSG 12/ISO-Oph 34/GSS 30-IRS2.
* A third source, GSS 30-IRS3/LFAM 1*, is at 16:26:21.72-24:22:50.5,
* separated by 4.5" and with [3.6]-[4.5]=0.9 and [8.0]-[24]=5.3
* (although with low S/N in MIPS1 due to confusion with GSS 30-IRS1).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! List of candidate embedded YSOs for interesting MIPS
sources with very red colors, but no associated
SCUBA flux (e.g., candidate edge-on disks)
integer*4 nr__2
parameter (nr__2=6) ! Number of records
character*103 ar__2 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_2 (nr__2) ! (deg) Right Ascension J2000
real*8 DEdeg_2 (nr__2) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 RAh_2 (nr__2) ! (h) c2d Hour of right ascension (J2000) (1)
integer*4 RAm_2 (nr__2) ! (min) c2d Minute of right ascension (J2000) (1)
real*4 RAs_2 (nr__2) ! (s) c2d Second of right ascension (J2000) (1)
character*1 DE__2 (nr__2) ! c2d Declination sign (J2000) (1)
integer*4 DEd_2 (nr__2) ! (deg) c2d Degree of declination (J2000) (1)
integer*4 DEm_2 (nr__2) ! (arcmin) c2d Arcminute of declination (J2000) (1)
real*4 DEs_2 (nr__2) ! (arcsec) c2d Arcsecond of declination (J2000) (1)
real*4 Conc_2 (nr__2) ! Concentration of the nearest SCUBA core
real*4 v3_6_4_5_2 (nr__2) ! ? Spitzer [3.6]-[4.5] color index
real*4 v8_0_24_2 (nr__2) ! ? Spitzer [8.0]-[24.0] color index
real*4 Sep_2 (nr__2) ! (arcsec) Separation between the Spitzer source and
* SCUBA core
real*4 Flux_2 (nr__2) ! (Jy) SCUBA Flux at 850um in Jy/beam
character*3 n_Flux_2 (nr__2) ! [ABC- ] Code for type of sources (2)
character*44 XID_2 (nr__2) ! Common identifiers from Simbad
character*2 Rem_2 (nr__2) ! [*g ] Remarks on source (3)
*Note (1): Position of Spitzer source from c2d catalog.
*Note (2): Code indicating whether the given source obeys:
* A = MIPS 24um source with [3.6]-[4.5]>1 and [8.0]-[24]>4.5;
* B = separation between Spitzer source and nearest SCUBA core less than 15";
* C = Associated submillimeter core has concentration higher than 0.6.
* A- = SCUBA flux refers to flux density at the exact position in the maps;
* for the remaining sources to the peak flux from the Clumpfind algorithm.
* Note that only A and B are used to construct this sample.
*Note (3): Flag as follows:
* * = Sources are included in the list of embedded YSOs by Wilking et al.
* (2008hsf2.book..351W).
* g = A complex system of at least three protostellar candidates: in addition
* to GSS 30-IRS1 a nearby source is seen at 16:26:22.38-24:22:52.9
* at a distance of 10.4" from the SCUBA core:
* [AMD2002] J162622-242254/ VSSG 12/ISO-Oph 34/GSS 30-IRS2.
* A third source, GSS 30-IRS3/LFAM 1*, is at 16:26:21.72-24:22:50.5,
* separated by 4.5" and with [3.6]-[4.5]=0.9 and [8.0]-[24]=5.3
* (although with low S/N in MIPS1 due to confusion with GSS 30-IRS1).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table7.dat' ! Properties of submillimeter cores in Ophiuchus
integer*4 nr__3
parameter (nr__3=66) ! Number of records
character*77 ar__3 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_3 (nr__3) ! (deg) Right Ascension J2000
real*8 DEdeg_3 (nr__3) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*12 Name (nr__3) ! SMM designation (HHMMSS-DDMMm, J2000)
integer*4 RAh_3 (nr__3) ! (h) Hour of right ascension (J2000) (1)
integer*4 RAm_3 (nr__3) ! (min) Minute of right ascension (J2000) (1)
real*4 RAs_3 (nr__3) ! (s) Second of right ascension (J2000) (1)
character*1 DE__3 (nr__3) ! Declination sign (J2000) (1)
integer*4 DEd_3 (nr__3) ! (deg) Degree of declination (J2000) (1)
integer*4 DEm_3 (nr__3) ! (arcmin) Arcminute of declination (J2000) (1)
real*4 DEs_3 (nr__3) ! (arcsec) Arcsecond of declination (J2000) (1)
real*4 F850 (nr__3) ! (Jy) SCUBA peak flux at 850um in Jy/beam (2)
real*4 S850 (nr__3) ! (Jy) SCUBA total flux at 850um (2)
integer*4 Reff (nr__3) ! (arcsec) Outer radius (2)
real*4 Mass (nr__3) ! (solMass) Estimated mass (3)
real*4 Conc_3 (nr__3) ! Concentration (4)
integer*4 Temp (nr__3) ! (K) Temperature (4)
real*4 MBE (nr__3) ! (solMass) BE sphere mass (4)
real*4 logn (nr__3) ! (cm-3) Central number density (4)
real*4 logP_k (nr__3) ! (cm-3/K) External pressure (4)
*Note (1): Position of peak flux within clump (accurate to 3"; the pixel size in
* the SCUBA maps and the approximate pointing accuracy of the JCMT).
*Note (2): Peak flux, total flux, and outer radius derived from Clumpfind
* (Williams, de Geus, & Blitz, 1994, Cat. J/ApJ/428/693). The peak and
* total fluxes have uncertainties of about 20%, mostly due to
* uncertainties in the absolute flux calibration. The radius has not
* been deconvolved from the telescope beam.
*Note (3): Mass derived from the total flux assuming T_d_=15K and 850cm^2^/g,
* d=125pc.
*Note (4): Concentration, temperature, mass, central number density, and external
* pressure derived from Bonnor-Ebert (BE) modeling (see text).
C=============================================================================
C Loading file 'table1.dat' ! List of candidate embedded YSOs in Ophiuchus
C Format for file interpretation
1 format(
+ I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F4.2,1X,F4.2,1X,
+ F4.2,1X,F6.1,1X,F6.3,1X,A3,1X,A44,A2)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,27
read(1,'(A103)')ar__
read(ar__,1)
+ RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),
+ DEs(i__),Conc(i__),v3_6_4_5(i__),v8_0_24(i__),Sep(i__),
+ Flux(i__),n_Flux(i__),XID(i__),Rem(i__)
if(ar__(30:33) .EQ. '') v3_6_4_5(i__) = rNULL__
if(ar__(35:38) .EQ. '') v8_0_24(i__) = rNULL__
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)
+ RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),
+ DEs(i__),Conc(i__),v3_6_4_5(i__),v8_0_24(i__),Sep(i__),
+ Flux(i__),n_Flux(i__),XID(i__),Rem(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 'table3.dat' ! List of candidate embedded YSOs for sources with
* separations of 15"-30" of a MIPS source
C Format for file interpretation
2 format(
+ I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F4.2,1X,F4.2,1X,
+ F4.2,1X,F6.1,1X,F6.3,1X,A3,1X,A44,A2)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,11
read(1,'(A103)')ar__1
read(ar__1,2)
+ RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),DEd_1(i__),
+ DEm_1(i__),DEs_1(i__),Conc_1(i__),v3_6_4_5_1(i__),
+ v8_0_24_1(i__),Sep_1(i__),Flux_1(i__),n_Flux_1(i__),
+ XID_1(i__),Rem_1(i__)
if(ar__1(30:33) .EQ. '') v3_6_4_5_1(i__) = rNULL__
if(ar__1(35:38) .EQ. '') v8_0_24_1(i__) = rNULL__
RAdeg_1(i__) = rNULL__
DEdeg_1(i__) = rNULL__
c Derive coordinates RAdeg_1 and DEdeg_1 from input data
c (RAdeg_1 and DEdeg_1 are set to rNULL__ when unknown)
if(RAh_1(i__) .GT. -180) RAdeg_1(i__)=RAh_1(i__)*15.
if(RAm_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAm_1(i__)/4.
if(RAs_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAs_1(i__)/240.
if(DEd_1(i__) .GE. 0) DEdeg_1(i__)=DEd_1(i__)
if(DEm_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEm_1(i__)/60.
if(DEs_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEs_1(i__)/3600.
if(DE__1(i__).EQ.'-'.AND.DEdeg_1(i__).GE.0) DEdeg_1(i__)=-DEdeg_1(i__)
c ..............Just test output...........
write(6,2)
+ RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),DEd_1(i__),
+ DEm_1(i__),DEs_1(i__),Conc_1(i__),v3_6_4_5_1(i__),
+ v8_0_24_1(i__),Sep_1(i__),Flux_1(i__),n_Flux_1(i__),
+ XID_1(i__),Rem_1(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4.dat' ! List of candidate embedded YSOs for interesting MIPS
* sources with very red colors, but no associated
* SCUBA flux (e.g., candidate edge-on disks)
C Format for file interpretation
3 format(
+ I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F4.2,1X,F4.2,1X,
+ F4.2,1X,F6.1,1X,F6.3,1X,A3,1X,A44,A2)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,6
read(1,'(A103)')ar__2
read(ar__2,3)
+ RAh_2(i__),RAm_2(i__),RAs_2(i__),DE__2(i__),DEd_2(i__),
+ DEm_2(i__),DEs_2(i__),Conc_2(i__),v3_6_4_5_2(i__),
+ v8_0_24_2(i__),Sep_2(i__),Flux_2(i__),n_Flux_2(i__),
+ XID_2(i__),Rem_2(i__)
if(ar__2(30:33) .EQ. '') v3_6_4_5_2(i__) = rNULL__
if(ar__2(35:38) .EQ. '') v8_0_24_2(i__) = rNULL__
RAdeg_2(i__) = rNULL__
DEdeg_2(i__) = rNULL__
c Derive coordinates RAdeg_2 and DEdeg_2 from input data
c (RAdeg_2 and DEdeg_2 are set to rNULL__ when unknown)
if(RAh_2(i__) .GT. -180) RAdeg_2(i__)=RAh_2(i__)*15.
if(RAm_2(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAm_2(i__)/4.
if(RAs_2(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAs_2(i__)/240.
if(DEd_2(i__) .GE. 0) DEdeg_2(i__)=DEd_2(i__)
if(DEm_2(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEm_2(i__)/60.
if(DEs_2(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEs_2(i__)/3600.
if(DE__2(i__).EQ.'-'.AND.DEdeg_2(i__).GE.0) DEdeg_2(i__)=-DEdeg_2(i__)
c ..............Just test output...........
write(6,3)
+ RAh_2(i__),RAm_2(i__),RAs_2(i__),DE__2(i__),DEd_2(i__),
+ DEm_2(i__),DEs_2(i__),Conc_2(i__),v3_6_4_5_2(i__),
+ v8_0_24_2(i__),Sep_2(i__),Flux_2(i__),n_Flux_2(i__),
+ XID_2(i__),Rem_2(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_2(i__),DEdeg_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table7.dat' ! Properties of submillimeter cores in Ophiuchus
C Format for file interpretation
4 format(
+ A12,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,F4.1,1X,F5.2,1X,
+ F5.2,1X,I3,1X,F4.2,1X,F4.2,1X,I2,1X,F4.2,1X,F3.1,1X,F3.1)
C Effective file loading
open(unit=1,status='old',file=
+'table7.dat')
write(6,*) '....Loading file: table7.dat'
do i__=1,66
read(1,'(A77)')ar__3
read(ar__3,4)
+ Name(i__),RAh_3(i__),RAm_3(i__),RAs_3(i__),DE__3(i__),
+ DEd_3(i__),DEm_3(i__),DEs_3(i__),F850(i__),S850(i__),
+ Reff(i__),Mass(i__),Conc_3(i__),Temp(i__),MBE(i__),logn(i__),
+ logP_k(i__)
RAdeg_3(i__) = rNULL__
DEdeg_3(i__) = rNULL__
c Derive coordinates RAdeg_3 and DEdeg_3 from input data
c (RAdeg_3 and DEdeg_3 are set to rNULL__ when unknown)
if(RAh_3(i__) .GT. -180) RAdeg_3(i__)=RAh_3(i__)*15.
if(RAm_3(i__) .GT. -180) RAdeg_3(i__)=RAdeg_3(i__)+RAm_3(i__)/4.
if(RAs_3(i__) .GT. -180) RAdeg_3(i__)=RAdeg_3(i__)+RAs_3(i__)/240.
if(DEd_3(i__) .GE. 0) DEdeg_3(i__)=DEd_3(i__)
if(DEm_3(i__) .GE. 0) DEdeg_3(i__)=DEdeg_3(i__)+DEm_3(i__)/60.
if(DEs_3(i__) .GE. 0) DEdeg_3(i__)=DEdeg_3(i__)+DEs_3(i__)/3600.
if(DE__3(i__).EQ.'-'.AND.DEdeg_3(i__).GE.0) DEdeg_3(i__)=-DEdeg_3(i__)
c ..............Just test output...........
write(6,4)
+ Name(i__),RAh_3(i__),RAm_3(i__),RAs_3(i__),DE__3(i__),
+ DEd_3(i__),DEm_3(i__),DEs_3(i__),F850(i__),S850(i__),
+ Reff(i__),Mass(i__),Conc_3(i__),Temp(i__),MBE(i__),logn(i__),
+ logP_k(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_3(i__),DEdeg_3(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end