Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/153/214 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-20
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/153/214 Star-forming potential in the Perseus complex (Mercimek+, 2017)
*================================================================================
*An estimation of the star formation rate in the Perseus complex.
* Mercimek S., Myers P.C., Lee K.I., Sadavoy S.I.
* <Astron. J., 153, 214-214 (2017)>
* =2017AJ....153..214M (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! Starless Cores in Each Clump
integer*4 nr__
parameter (nr__=69) ! Number of records
character*61 ar__ ! Full-size record
C J2000 position composed of: RAdeg DEdeg
character*8 Clump (nr__) ! Clump name
integer*4 Field (nr__) ! [1/26] Field identifier
character*16 Name (nr__) ! Core name (JHHMMSS.s+DDMMSS)
real*8 RAdeg (nr__) ! (deg) Right Ascension in decimal degrees (J2000)
real*8 DEdeg (nr__) ! (deg) Declination in decimal degrees (J2000)
real*4 Mass (nr__) ! (Msun) [0.051/24.529] Mass
real*4 Reff (nr__) ! (pc) [0.0082/76] Effective radius
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! Protostellar Cores in Each Clump
integer*4 nr__1
parameter (nr__1=42) ! Number of records
character*61 ar__1 ! Full-size record
C J2000 position composed of: RAdeg DEdeg
character*8 Clump_1 (nr__1) ! Clump name
integer*4 Field_1 (nr__1) ! [1/26] Field identifier
character*16 Name_1 (nr__1) ! Core name (JHHMMSS.s+DDMMSS)
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 Mass_1 (nr__1) ! (Msun) [0.051/24.529] Mass
real*4 Reff_1 (nr__1) ! (pc) [0.0082/76] Effective radius
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6.dat' ! Class 0 in Each Clump
integer*4 nr__2
parameter (nr__2=28) ! Number of records
character*38 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)
character*8 Clump_2 (nr__2) ! Clump name
integer*4 Field_2 (nr__2) ! [1/12] Field identifier
character*7 Name_2 (nr__2) ! Source name
integer*4 RAh (nr__2) ! (h) Hour of Right Ascension (J2000)
integer*4 RAm (nr__2) ! (min) Minute of Right Ascension (J2000)
real*4 RAs (nr__2) ! (s) Second of Right Ascension (J2000)
character*1 DE_ (nr__2) ! Sign of the Declination (J2000)
integer*4 DEd (nr__2) ! (deg) Degree of Declination (J2000)
integer*4 DEm (nr__2) ! (arcmin) Arcminute of Declination (J2000)
integer*4 DEs (nr__2) ! (arcsec) Arcsecond of Declination (J2000)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table7.dat' ! Class I in Each Clump
integer*4 nr__3
parameter (nr__3=57) ! Number of records
character*69 ar__3 ! Full-size record
C J2000 position composed of: RAdeg DEdeg
character*8 Clump_3 (nr__3) ! Clump name
integer*4 Field_3 (nr__3) ! [1/53] Field identifier
character*19 Name_3 (nr__3) ! Spitzer source name (JHHMMSS.ss+DDMMSS.s)
character*19 Class (nr__3) ! Spitzer c2d (Evans et al. 2009, J/ApJS/181/321)
* classification (1)
real*8 RAdeg_3 (nr__3) ! (deg) Right Ascension in decimal degrees (J2000)
real*8 DEdeg_3 (nr__3) ! (deg) Declination in decimal degrees (J2000)
*Note (1): Classification from Evans et al. (2009, J/ApJS/181/321) as follows:
* YSOc = Candidates for YSOs. Detections in all four IRAC bands and MIPS-1;
* see selection criteria in section 3.1;
* red = Flux densities at 24 {mu}m that are at least 3 times the flux
* density from the nearest available IRAC band;
* PAH_em = Have colors indicative of a peak in the 8 {mu}m band;
* star+dust = The SED is consistent with that of a stellar photosphere for
* wavelengths shorter than a particular band but an excess in that
* band of at least 3{sigma}. This band was appended to make a full
* name such as "YSOc_star+dust(MP1)" where MP1 implies the first
* MIPS band, at 24 {mu}m or "YSOc_star+dust(IR4)" where IR4 implies
* the fourth IRAC band, at 8.0 {mu}m;
* rising = Lack photometry at enough wavelengths to be classified as YSOc,
* but were later added as YSOs based on other information. The
* available flux densities rise significantly to longer wavelengths.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table8.dat' ! Class Flat in Each Clump
integer*4 nr__4
parameter (nr__4=26) ! Number of records
character*69 ar__4 ! Full-size record
C J2000 position composed of: RAdeg DEdeg
character*8 Clump_4 (nr__4) ! Clump name
integer*4 Field_4 (nr__4) ! [1/53] Field identifier
character*19 Name_4 (nr__4) ! Spitzer source name (JHHMMSS.ss+DDMMSS.s)
character*19 Class_1 (nr__4) ! Spitzer c2d (Evans et al. 2009, J/ApJS/181/321)
* classification (1)
real*8 RAdeg_4 (nr__4) ! (deg) Right Ascension in decimal degrees (J2000)
real*8 DEdeg_4 (nr__4) ! (deg) Declination in decimal degrees (J2000)
*Note (1): Classification from Evans et al. (2009, J/ApJS/181/321) as follows:
* YSOc = Candidates for YSOs. Detections in all four IRAC bands and MIPS-1;
* see selection criteria in section 3.1;
* red = Flux densities at 24 {mu}m that are at least 3 times the flux
* density from the nearest available IRAC band;
* PAH_em = Have colors indicative of a peak in the 8 {mu}m band;
* star+dust = The SED is consistent with that of a stellar photosphere for
* wavelengths shorter than a particular band but an excess in that
* band of at least 3{sigma}. This band was appended to make a full
* name such as "YSOc_star+dust(MP1)" where MP1 implies the first
* MIPS band, at 24 {mu}m or "YSOc_star+dust(IR4)" where IR4 implies
* the fourth IRAC band, at 8.0 {mu}m;
* rising = Lack photometry at enough wavelengths to be classified as YSOc,
* but were later added as YSOs based on other information. The
* available flux densities rise significantly to longer wavelengths.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table9.dat' ! Class II in Each Clump
integer*4 nr__5
parameter (nr__5=102) ! Number of records
character*69 ar__5 ! Full-size record
C J2000 position composed of: RAdeg DEdeg
character*8 Clump_5 (nr__5) ! Clump name
integer*4 Field_5 (nr__5) ! [1/53] Field identifier
character*19 Name_5 (nr__5) ! Spitzer source name (JHHMMSS.ss+DDMMSS.s)
character*19 Class_2 (nr__5) ! Spitzer c2d (Evans et al. 2009, J/ApJS/181/321)
* classification (1)
real*8 RAdeg_5 (nr__5) ! (deg) Right Ascension in decimal degrees (J2000)
real*8 DEdeg_5 (nr__5) ! (deg) Declination in decimal degrees (J2000)
*Note (1): Classification from Evans et al. (2009, J/ApJS/181/321) as follows:
* YSOc = Candidates for YSOs. Detections in all four IRAC bands and MIPS-1;
* see selection criteria in section 3.1;
* red = Flux densities at 24 {mu}m that are at least 3 times the flux
* density from the nearest available IRAC band;
* PAH_em = Have colors indicative of a peak in the 8 {mu}m band;
* star+dust = The SED is consistent with that of a stellar photosphere for
* wavelengths shorter than a particular band but an excess in that
* band of at least 3{sigma}. This band was appended to make a full
* name such as "YSOc_star+dust(MP1)" where MP1 implies the first
* MIPS band, at 24 {mu}m or "YSOc_star+dust(IR4)" where IR4 implies
* the fourth IRAC band, at 8.0 {mu}m;
* rising = Lack photometry at enough wavelengths to be classified as YSOc,
* but were later added as YSOs based on other information. The
* available flux densities rise significantly to longer wavelengths.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table10.dat' ! Class III in Each Clump
integer*4 nr__6
parameter (nr__6=9) ! Number of records
character*69 ar__6 ! Full-size record
C J2000 position composed of: RAdeg DEdeg
character*8 Clump_6 (nr__6) ! Clump name
integer*4 Field_6 (nr__6) ! [1/53] Field identifier
character*19 Name_6 (nr__6) ! Spitzer source name (JHHMMSS.ss+DDMMSS.s)
character*19 Class_3 (nr__6) ! Spitzer c2d (Evans et al. 2009, J/ApJS/181/321)
* classification (1)
real*8 RAdeg_6 (nr__6) ! (deg) Right Ascension in decimal degrees (J2000)
real*8 DEdeg_6 (nr__6) ! (deg) Declination in decimal degrees (J2000)
*Note (1): Classification from Evans et al. (2009, J/ApJS/181/321) as follows:
* YSOc = Candidates for YSOs. Detections in all four IRAC bands and MIPS-1;
* see selection criteria in section 3.1;
* red = Flux densities at 24 {mu}m that are at least 3 times the flux
* density from the nearest available IRAC band;
* PAH_em = Have colors indicative of a peak in the 8 {mu}m band;
* star+dust = The SED is consistent with that of a stellar photosphere for
* wavelengths shorter than a particular band but an excess in that
* band of at least 3{sigma}. This band was appended to make a full
* name such as "YSOc_star+dust(MP1)" where MP1 implies the first
* MIPS band, at 24 {mu}m or "YSOc_star+dust(IR4)" where IR4 implies
* the fourth IRAC band, at 8.0 {mu}m;
* rising = Lack photometry at enough wavelengths to be classified as YSOc,
* but were later added as YSOs based on other information. The
* available flux densities rise significantly to longer wavelengths.
C=============================================================================
C Loading file 'table4.dat' ! Starless Cores in Each Clump
C Format for file interpretation
1 format(A8,1X,I2,1X,A16,1X,F8.4,1X,F8.4,1X,F6.3,1X,E7.2)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,69
read(1,'(A61)')ar__
read(ar__,1)
+ Clump(i__),Field(i__),Name(i__),RAdeg(i__),DEdeg(i__),
+ Mass(i__),Reff(i__)
c ..............Just test output...........
write(6,1)
+ Clump(i__),Field(i__),Name(i__),RAdeg(i__),DEdeg(i__),
+ Mass(i__),Reff(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table5.dat' ! Protostellar Cores in Each Clump
C Format for file interpretation
2 format(A8,1X,I2,1X,A16,1X,F8.4,1X,F8.4,1X,F6.3,1X,E7.2)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,42
read(1,'(A61)')ar__1
read(ar__1,2)
+ Clump_1(i__),Field_1(i__),Name_1(i__),RAdeg_1(i__),
+ DEdeg_1(i__),Mass_1(i__),Reff_1(i__)
c ..............Just test output...........
write(6,2)
+ Clump_1(i__),Field_1(i__),Name_1(i__),RAdeg_1(i__),
+ DEdeg_1(i__),Mass_1(i__),Reff_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table6.dat' ! Class 0 in Each Clump
C Format for file interpretation
3 format(A8,1X,I2,1X,A7,1X,I1,1X,I2,1X,F4.1,A1,I2,1X,I2,1X,I2)
C Effective file loading
open(unit=1,status='old',file=
+'table6.dat')
write(6,*) '....Loading file: table6.dat'
do i__=1,28
read(1,'(A38)')ar__2
read(ar__2,3)
+ Clump_2(i__),Field_2(i__),Name_2(i__),RAh(i__),RAm(i__),
+ RAs(i__),DE_(i__),DEd(i__),DEm(i__),DEs(i__)
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(i__) .GT. -180) RAdeg_2(i__)=RAh(i__)*15.
if(RAm(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAm(i__)/4.
if(RAs(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAs(i__)/240.
if(DEd(i__) .GE. 0) DEdeg_2(i__)=DEd(i__)
if(DEm(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEm(i__)/60.
if(DEs(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEs(i__)/3600.
if(DE_(i__).EQ.'-'.AND.DEdeg_2(i__).GE.0) DEdeg_2(i__)=-DEdeg_2(i__)
c ..............Just test output...........
write(6,3)
+ Clump_2(i__),Field_2(i__),Name_2(i__),RAh(i__),RAm(i__),
+ RAs(i__),DE_(i__),DEd(i__),DEm(i__),DEs(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' ! Class I in Each Clump
C Format for file interpretation
4 format(A8,1X,I2,1X,A19,1X,A19,1X,F8.5,1X,F8.5)
C Effective file loading
open(unit=1,status='old',file=
+'table7.dat')
write(6,*) '....Loading file: table7.dat'
do i__=1,57
read(1,'(A69)')ar__3
read(ar__3,4)
+ Clump_3(i__),Field_3(i__),Name_3(i__),Class(i__),RAdeg_3(i__),
+ DEdeg_3(i__)
c ..............Just test output...........
write(6,4)
+ Clump_3(i__),Field_3(i__),Name_3(i__),Class(i__),RAdeg_3(i__),
+ DEdeg_3(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table8.dat' ! Class Flat in Each Clump
C Format for file interpretation
5 format(A8,1X,I2,1X,A19,1X,A19,1X,F8.5,1X,F8.5)
C Effective file loading
open(unit=1,status='old',file=
+'table8.dat')
write(6,*) '....Loading file: table8.dat'
do i__=1,26
read(1,'(A69)')ar__4
read(ar__4,5)
+ Clump_4(i__),Field_4(i__),Name_4(i__),Class_1(i__),
+ RAdeg_4(i__),DEdeg_4(i__)
c ..............Just test output...........
write(6,5)
+ Clump_4(i__),Field_4(i__),Name_4(i__),Class_1(i__),
+ RAdeg_4(i__),DEdeg_4(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table9.dat' ! Class II in Each Clump
C Format for file interpretation
6 format(A8,1X,I2,1X,A19,1X,A19,1X,F8.5,1X,F8.5)
C Effective file loading
open(unit=1,status='old',file=
+'table9.dat')
write(6,*) '....Loading file: table9.dat'
do i__=1,102
read(1,'(A69)')ar__5
read(ar__5,6)
+ Clump_5(i__),Field_5(i__),Name_5(i__),Class_2(i__),
+ RAdeg_5(i__),DEdeg_5(i__)
c ..............Just test output...........
write(6,6)
+ Clump_5(i__),Field_5(i__),Name_5(i__),Class_2(i__),
+ RAdeg_5(i__),DEdeg_5(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table10.dat' ! Class III in Each Clump
C Format for file interpretation
7 format(A8,1X,I2,1X,A19,1X,A19,1X,F8.5,1X,F8.5)
C Effective file loading
open(unit=1,status='old',file=
+'table10.dat')
write(6,*) '....Loading file: table10.dat'
do i__=1,9
read(1,'(A69)')ar__6
read(ar__6,7)
+ Clump_6(i__),Field_6(i__),Name_6(i__),Class_3(i__),
+ RAdeg_6(i__),DEdeg_6(i__)
c ..............Just test output...........
write(6,7)
+ Clump_6(i__),Field_6(i__),Name_6(i__),Class_3(i__),
+ RAdeg_6(i__),DEdeg_6(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end