Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/719/9 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-10
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/719/9 IRAC point-source catalog of Vela-D cloud (Strafella+, 2010)
*================================================================================
*The Spitzer-IRAC point-source catalog of the Vela-D cloud.
* Strafella F., Elia D., Campeggio L., Giannini T., Lorenzetti D.,
* Marengo M., Smith H.A., Fazio G., De Luca M., Massi F.
* <Astrophys. J., 719, 9-27 (2010)>
* =2010ApJ...719....9S
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! VMR-D MIPS catalog
integer*4 nr__
parameter (nr__=1363) ! Number of records
character*102 ar__ ! Full-size record
C J2000 position composed of: RAdeg DEdeg
integer*4 MIPS (nr__) ! MIPS catalog number
* (<[SEC2010] MIPS NNNN> in Simbad)
real*8 RAdeg (nr__) ! (deg) Right Ascension in decimal degrees (J2000)
real*8 DEdeg (nr__) ! (deg) Declination in decimal degrees (J2000)
real*8 GLON (nr__) ! (deg) Galactic longitude
real*8 GLAT (nr__) ! (deg) Galactic latitude
real*4 F24 (nr__) ! (Jy) Spitzer/MIPS 24 micron band flux density
real*4 e_F24 (nr__) ! (Jy) Uncertainty in F24 (1)
real*4 F70 (nr__) ! (Jy) Spitzer/MIPS 70 micron band flux density
real*4 e_F70 (nr__) ! (Jy) Uncertainty in F70 (1)
real*4 Dist (nr__) ! (arcsec) Distance between centroids at 24 and 70 microns
character*1 IRAC (nr__) ! [IN] Source inside(I) / outside(N) IRAC observed
* region
character*1 v12CO (nr__) ! [CAON] Association with ^12^CO(1-0) (G1)
character*1 v13CO (nr__) ! [CAON] Association with ^13^CO(2-1) (G1)
character*6 Dust (nr__) ! Name of 1.2mm dust core (G2)
*Note (1): When the flux reported is an upper limit, the uncertainty has
* been put to zero.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! VMR-D IRAC point source catalog
integer*4 nr__1
parameter (nr__1=170299) ! Number of records
character*233 ar__1 ! Full-size record
C J2000 position composed of: RAdeg DEdeg
integer*4 IRAC_1 (nr__1) ! IRAC catalog number
* (<[SEC2010] IRAC NNNNNN> in Simbad)
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*8 GLON_1 (nr__1) ! (deg) Galactic longitude
real*8 GLAT_1 (nr__1) ! (deg) Galactic latitude
real*4 F3_6 (nr__1) ! (Jy) ? Spitzer/IRAC 3.6 micron band flux density
real*4 e_F3_6 (nr__1) ! (Jy) ?=0 Uncertainty in F3.6
character*2 q_F3_6 (nr__1) ! Quality flag on F3.6 (1)
real*4 F4_5 (nr__1) ! (Jy) ? Spitzer/IRAC 4.5 micron band flux density
real*4 e_F4_5 (nr__1) ! (Jy) ?=0 Uncertainty in F4.5
character*2 q_F4_5 (nr__1) ! Quality flag on F4.5 (1)
real*4 F5_8 (nr__1) ! (Jy) ? Spitzer/IRAC 5.8 micron band flux density
real*4 e_F5_8 (nr__1) ! (Jy) ?=0 Uncertainty in F5.8
character*2 q_F5_8 (nr__1) ! Quality flag on F5.8 (1)
real*4 F8_0 (nr__1) ! (Jy) ? Spitzer/IRAC 8.0 micron band flux density
real*4 e_F8_0 (nr__1) ! (Jy) ?=0 Uncertainty in F8.0
character*2 q_F8_0 (nr__1) ! Quality flag on F8.0 (1)
integer*4 MIPS_1 (nr__1) ! ?=- Associated MIPS catalog number
* (<[SEC2010] MIPS NNNN> in Simbad) (2)
real*4 Dist_1 (nr__1) ! (arcsec) Distance of associated MIPS source centroid
real*4 F24_1 (nr__1) ! (Jy) ? Spitzer/MIPS 24 micron band flux density (3)
real*4 e_F24_1 (nr__1) ! (Jy) Uncertainty in F24
character*1 q_F24 (nr__1) ! [Gbu] Quality flag on F24 (4)
real*4 F70_1 (nr__1) ! (Jy) ? Spitzer/MIPS 70 micron band flux density
real*4 e_F70_1 (nr__1) ! (Jy) Uncertainty in F70
character*1 q_F70 (nr__1) ! [Gbu] Quality flag on F70 (4)
real*4 alpha (nr__1) ! ? Spectral slope; 2um<{lambda}<20um (for
* table 9 only)
character*1 v12CO_1 (nr__1) ! [CAON] Association with ^12^CO(1-0) (G1)
character*1 v13CO_1 (nr__1) ! [CAON] Association with ^13^CO(2-1) (G1)
character*6 Dust_1 (nr__1) ! Name of 1.2mm dust core (G2)
*Note (1): Photometry quality code as follows:
* H1 = (High): "good photometry", refer to a more than 10{sigma} detection;
* "1" indicates that the source lies in the sky area covered only in
* one observing epoch
* H2 = (High): "good photometry", refer to a more than 10{sigma} detection;
* "2" indicates that the source lies in the sky area covered in both
* observing epochs
* L1 = (Low): source is revealed between 5 and 10{sigma} and lies in the
* sky area covered only in one observing epoch
* L2 = (Low): source is revealed between 5 and 10{sigma} and lies in the
* sky area covered in both observing epochs
* b = "bad photometry"
* u = upper limit
*Note (2): This is reported if its centroid is within a distance of 6" from
* the IRAC source. MIPS sources detected only at 70 micron are reported
* when the centroid is within 20". Notice that, due to the different
* beam sizes, the association of more than one IRAC source with the same
* MIPS source is allowed.
*Note (3): A blank value denotes a position falling outside the MIPS mosaic.
*Note (4): The quality flag is similar to that used for IRAC flux densities
* but with good photometry simply flagged "G".
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table9.dat' ! VMR-D IRAC YSO catalog
integer*4 nr__2
parameter (nr__2=637) ! Number of records
character*233 ar__2 ! Full-size record
C J2000 position composed of: RAdeg DEdeg
integer*4 IRAC_2 (nr__2) ! IRAC catalog number
* (<[SEC2010] IRAC NNNNNN> in Simbad)
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*8 GLON_2 (nr__2) ! (deg) Galactic longitude
real*8 GLAT_2 (nr__2) ! (deg) Galactic latitude
real*4 F3_6_1 (nr__2) ! (Jy) ? Spitzer/IRAC 3.6 micron band flux density
real*4 e_F3_6_1 (nr__2) ! (Jy) ?=0 Uncertainty in F3.6
character*2 q_F3_6_1 (nr__2) ! Quality flag on F3.6 (1)
real*4 F4_5_1 (nr__2) ! (Jy) ? Spitzer/IRAC 4.5 micron band flux density
real*4 e_F4_5_1 (nr__2) ! (Jy) ?=0 Uncertainty in F4.5
character*2 q_F4_5_1 (nr__2) ! Quality flag on F4.5 (1)
real*4 F5_8_1 (nr__2) ! (Jy) ? Spitzer/IRAC 5.8 micron band flux density
real*4 e_F5_8_1 (nr__2) ! (Jy) ?=0 Uncertainty in F5.8
character*2 q_F5_8_1 (nr__2) ! Quality flag on F5.8 (1)
real*4 F8_0_1 (nr__2) ! (Jy) ? Spitzer/IRAC 8.0 micron band flux density
real*4 e_F8_0_1 (nr__2) ! (Jy) ?=0 Uncertainty in F8.0
character*2 q_F8_0_1 (nr__2) ! Quality flag on F8.0 (1)
integer*4 MIPS_2 (nr__2) ! ?=- Associated MIPS catalog number
* (<[SEC2010] MIPS NNNN> in Simbad) (2)
real*4 Dist_2 (nr__2) ! (arcsec) Distance of associated MIPS source centroid
real*4 F24_2 (nr__2) ! (Jy) ? Spitzer/MIPS 24 micron band flux density (3)
real*4 e_F24_2 (nr__2) ! (Jy) Uncertainty in F24
character*1 q_F24_1 (nr__2) ! [Gbu] Quality flag on F24 (4)
real*4 F70_2 (nr__2) ! (Jy) ? Spitzer/MIPS 70 micron band flux density
real*4 e_F70_2 (nr__2) ! (Jy) Uncertainty in F70
character*1 q_F70_1 (nr__2) ! [Gbu] Quality flag on F70 (4)
real*4 alpha_1 (nr__2) ! ? Spectral slope; 2um<{lambda}<20um (for
* table 9 only)
character*1 v12CO_2 (nr__2) ! [CAON] Association with ^12^CO(1-0) (G1)
character*1 v13CO_2 (nr__2) ! [CAON] Association with ^13^CO(2-1) (G1)
character*6 Dust_2 (nr__2) ! Name of 1.2mm dust core (G2)
*Note (1): Photometry quality code as follows:
* H1 = (High): "good photometry", refer to a more than 10{sigma} detection;
* "1" indicates that the source lies in the sky area covered only in
* one observing epoch
* H2 = (High): "good photometry", refer to a more than 10{sigma} detection;
* "2" indicates that the source lies in the sky area covered in both
* observing epochs
* L1 = (Low): source is revealed between 5 and 10{sigma} and lies in the
* sky area covered only in one observing epoch
* L2 = (Low): source is revealed between 5 and 10{sigma} and lies in the
* sky area covered in both observing epochs
* b = "bad photometry"
* u = upper limit
*Note (2): This is reported if its centroid is within a distance of 6" from
* the IRAC source. MIPS sources detected only at 70 micron are reported
* when the centroid is within 20". Notice that, due to the different
* beam sizes, the association of more than one IRAC source with the same
* MIPS source is allowed.
*Note (3): A blank value denotes a position falling outside the MIPS mosaic.
*Note (4): The quality flag is similar to that used for IRAC flux densities
* but with good photometry simply flagged "G".
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table10.dat' ! VMR-D MIPS YSO catalog
integer*4 nr__3
parameter (nr__3=276) ! Number of records
character*113 ar__3 ! Full-size record
C J2000 position composed of: RAdeg DEdeg
integer*4 MIPS_3 (nr__3) ! MIPS catalog number
* (<[SEC2010] MIPS NNNN> in Simbad)
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)
real*8 GLON_3 (nr__3) ! (deg) Galactic longitude
real*8 GLAT_3 (nr__3) ! (deg) Galactic latitude
real*4 F24_3 (nr__3) ! (Jy) Spitzer/MIPS 24 micron band flux density
real*4 e_F24_3 (nr__3) ! (Jy) Uncertainty in F24 (zero for upper limit) (1)
real*4 F70_3 (nr__3) ! (Jy) Spitzer/MIPS 70 micron band flux density
real*4 e_F70_3 (nr__3) ! (Jy) Uncertainty in F70 (zero for upper limit) (1)
real*4 Dist_3 (nr__3) ! (arcsec) Distance between centroids at 24 and 70 microns
real*4 alpha_2 (nr__3) ! Spectral slope; 2um<{lambda}<20um
integer*4 IRAC_3 (nr__3) ! ?=- IRAC catalog number
* (<[SEC2010] IRAC NNNN> in Simbad)
character*1 v12CO_3 (nr__3) ! [CAON] Association with ^12^CO(1-0) (G1)
character*1 v13CO_3 (nr__3) ! [CAON] Association with ^13^CO(2-1) (G1)
character*6 Dust_3 (nr__3) ! Name of 1.2mm dust core (G2)
*Note (1): When the flux reported is an upper limit, the uncertainty has
* been put to zero.
C=============================================================================
C Loading file 'table2.dat' ! VMR-D MIPS catalog
C Format for file interpretation
1 format(
+ I4,1X,F9.5,1X,F9.5,1X,F9.5,1X,F8.5,1X,E10.3,1X,E9.3,1X,E9.3,
+ 1X,E9.3,1X,F4.1,1X,A1,1X,A1,1X,A1,1X,A6)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,1363
read(1,'(A102)')ar__
read(ar__,1)
+ MIPS(i__),RAdeg(i__),DEdeg(i__),GLON(i__),GLAT(i__),F24(i__),
+ e_F24(i__),F70(i__),e_F70(i__),Dist(i__),IRAC(i__),v12CO(i__),
+ v13CO(i__),Dust(i__)
c ..............Just test output...........
write(6,1)
+ MIPS(i__),RAdeg(i__),DEdeg(i__),GLON(i__),GLAT(i__),F24(i__),
+ e_F24(i__),F70(i__),e_F70(i__),Dist(i__),IRAC(i__),v12CO(i__),
+ v13CO(i__),Dust(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table5.dat' ! VMR-D IRAC point source catalog
C Format for file interpretation
2 format(
+ I6,1X,F10.6,1X,F10.6,1X,F10.6,1X,F9.6,1X,E12.5,1X,E11.5,1X,A2,
+ 1X,E12.5,1X,E11.5,1X,A2,1X,E12.5,1X,E11.5,1X,A2,1X,E12.5,1X,
+ E11.5,1X,A2,1X,I4,1X,F4.1,1X,E10.3,1X,E9.3,1X,A1,1X,E9.3,1X,
+ E9.3,1X,A1,1X,F5.2,1X,A1,1X,A1,1X,A6)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,170299
read(1,'(A233)')ar__1
read(ar__1,2)
+ IRAC_1(i__),RAdeg_1(i__),DEdeg_1(i__),GLON_1(i__),GLAT_1(i__),
+ F3_6(i__),e_F3_6(i__),q_F3_6(i__),F4_5(i__),e_F4_5(i__),
+ q_F4_5(i__),F5_8(i__),e_F5_8(i__),q_F5_8(i__),F8_0(i__),
+ e_F8_0(i__),q_F8_0(i__),MIPS_1(i__),Dist_1(i__),F24_1(i__),
+ e_F24_1(i__),q_F24(i__),F70_1(i__),e_F70_1(i__),q_F70(i__),
+ alpha(i__),v12CO_1(i__),v13CO_1(i__),Dust_1(i__)
if(ar__1(51:62) .EQ. '') F3_6(i__) = rNULL__
if(ar__1(79:90) .EQ. '') F4_5(i__) = rNULL__
if(ar__1(107:118) .EQ. '') F5_8(i__) = rNULL__
if(ar__1(135:146) .EQ. '') F8_0(i__) = rNULL__
if (MIPS_1(i__) .EQ. 45) MIPS_1(i__) = iNULL__
if(ar__1(173:182) .EQ. '') F24_1(i__) = rNULL__
if(ar__1(196:204) .EQ. '') F70_1(i__) = rNULL__
if(ar__1(218:222) .EQ. '') alpha(i__) = rNULL__
c ..............Just test output...........
write(6,2)
+ IRAC_1(i__),RAdeg_1(i__),DEdeg_1(i__),GLON_1(i__),GLAT_1(i__),
+ F3_6(i__),e_F3_6(i__),q_F3_6(i__),F4_5(i__),e_F4_5(i__),
+ q_F4_5(i__),F5_8(i__),e_F5_8(i__),q_F5_8(i__),F8_0(i__),
+ e_F8_0(i__),q_F8_0(i__),MIPS_1(i__),Dist_1(i__),F24_1(i__),
+ e_F24_1(i__),q_F24(i__),F70_1(i__),e_F70_1(i__),q_F70(i__),
+ alpha(i__),v12CO_1(i__),v13CO_1(i__),Dust_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table9.dat' ! VMR-D IRAC YSO catalog
C Format for file interpretation
3 format(
+ I6,1X,F10.6,1X,F10.6,1X,F10.6,1X,F9.6,1X,E12.5,1X,E11.5,1X,A2,
+ 1X,E12.5,1X,E11.5,1X,A2,1X,E12.5,1X,E11.5,1X,A2,1X,E12.5,1X,
+ E11.5,1X,A2,1X,I4,1X,F4.1,1X,E10.3,1X,E9.3,1X,A1,1X,E9.3,1X,
+ E9.3,1X,A1,1X,F5.2,1X,A1,1X,A1,1X,A6)
C Effective file loading
open(unit=1,status='old',file=
+'table9.dat')
write(6,*) '....Loading file: table9.dat'
do i__=1,637
read(1,'(A233)')ar__2
read(ar__2,3)
+ IRAC_2(i__),RAdeg_2(i__),DEdeg_2(i__),GLON_2(i__),GLAT_2(i__),
+ F3_6_1(i__),e_F3_6_1(i__),q_F3_6_1(i__),F4_5_1(i__),
+ e_F4_5_1(i__),q_F4_5_1(i__),F5_8_1(i__),e_F5_8_1(i__),
+ q_F5_8_1(i__),F8_0_1(i__),e_F8_0_1(i__),q_F8_0_1(i__),
+ MIPS_2(i__),Dist_2(i__),F24_2(i__),e_F24_2(i__),q_F24_1(i__),
+ F70_2(i__),e_F70_2(i__),q_F70_1(i__),alpha_1(i__),
+ v12CO_2(i__),v13CO_2(i__),Dust_2(i__)
if(ar__2(51:62) .EQ. '') F3_6_1(i__) = rNULL__
if(ar__2(79:90) .EQ. '') F4_5_1(i__) = rNULL__
if(ar__2(107:118) .EQ. '') F5_8_1(i__) = rNULL__
if(ar__2(135:146) .EQ. '') F8_0_1(i__) = rNULL__
if (MIPS_2(i__) .EQ. 45) MIPS_2(i__) = iNULL__
if(ar__2(173:182) .EQ. '') F24_2(i__) = rNULL__
if(ar__2(196:204) .EQ. '') F70_2(i__) = rNULL__
if(ar__2(218:222) .EQ. '') alpha_1(i__) = rNULL__
c ..............Just test output...........
write(6,3)
+ IRAC_2(i__),RAdeg_2(i__),DEdeg_2(i__),GLON_2(i__),GLAT_2(i__),
+ F3_6_1(i__),e_F3_6_1(i__),q_F3_6_1(i__),F4_5_1(i__),
+ e_F4_5_1(i__),q_F4_5_1(i__),F5_8_1(i__),e_F5_8_1(i__),
+ q_F5_8_1(i__),F8_0_1(i__),e_F8_0_1(i__),q_F8_0_1(i__),
+ MIPS_2(i__),Dist_2(i__),F24_2(i__),e_F24_2(i__),q_F24_1(i__),
+ F70_2(i__),e_F70_2(i__),q_F70_1(i__),alpha_1(i__),
+ v12CO_2(i__),v13CO_2(i__),Dust_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table10.dat' ! VMR-D MIPS YSO catalog
C Format for file interpretation
4 format(
+ I4,1X,F9.5,1X,F9.5,1X,F9.5,1X,F8.5,1X,E10.3,1X,E9.3,1X,E9.3,
+ 1X,E9.3,1X,F4.1,1X,F5.2,1X,I6,1X,A1,1X,A1,1X,A6)
C Effective file loading
open(unit=1,status='old',file=
+'table10.dat')
write(6,*) '....Loading file: table10.dat'
do i__=1,276
read(1,'(A113)')ar__3
read(ar__3,4)
+ MIPS_3(i__),RAdeg_3(i__),DEdeg_3(i__),GLON_3(i__),GLAT_3(i__),
+ F24_3(i__),e_F24_3(i__),F70_3(i__),e_F70_3(i__),Dist_3(i__),
+ alpha_2(i__),IRAC_3(i__),v12CO_3(i__),v13CO_3(i__),Dust_3(i__)
if (IRAC_3(i__) .EQ. 45) IRAC_3(i__) = iNULL__
c ..............Just test output...........
write(6,4)
+ MIPS_3(i__),RAdeg_3(i__),DEdeg_3(i__),GLON_3(i__),GLAT_3(i__),
+ F24_3(i__),e_F24_3(i__),F70_3(i__),e_F70_3(i__),Dist_3(i__),
+ alpha_2(i__),IRAC_3(i__),v12CO_3(i__),v13CO_3(i__),Dust_3(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end