Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/121/3048 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/AJ/121/3048 Multicolor photometry in NGC 1512 and NGC 5248 (Maoz+, 2001)
*================================================================================
*An ultraviolet through infrared look at star formation and super star clusters
*in two circumnuclear starburst rings.
* Maoz D., Barth A.J., Ho L.C., Sternberg A., Filippenko A.V.
* <Astron. J. 121, 3048 (2001)>
* =2001AJ....121.3048M
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Emission-Line Complexes
integer*4 nr__
parameter (nr__=32) ! Number of records
character*62 ar__ ! Full-size record
character*8 Cluster (nr__) ! Cluster name
integer*4 ELC (nr__) ! Emission-Line Complexe number in the
* cluster
* ([MBH2001 NGC NNNN ELC NN in Simbad)
integer*4 Xpos (nr__) ! (pix) X position
integer*4 Ypos (nr__) ! (pix) Y position
real*4 DRA (nr__) ! (arcsec) Offset in right ascension
* from the galaxy nucleus (1)
real*4 DDE (nr__) ! (arcsec) Offset in declination
* from the galaxy nucleus (1)
real*4 Rad (nr__) ! (arcsec) Angular radius of circular aperture
* used for flux measurements (2)
real*4 FHa (nr__) ! (10-19W/m2) Line flux in H{alpha}+[NII]
* (in F658N filter) (3)
real*4 FPaa (nr__) ! (10-19W/m2) Line flux in Pa{alpha} (3)
real*4 F1_6um (nr__) ! (10-19W/m2) Line flux in 1.6{mu}m (3)
real*4 FHa_FPaa (nr__) ! Ratio of H{alpha}+[NII] to Pa{alpha} lines
integer*4 FPaa_F1_6um(nr__) ! Ratio of Pa{alpha} to 1.6{mu}m lines
*Note (1): Cluster center coordinates:
* NGC 1512: 04:03:54.29 (J2000) -43:20:56.7 (419.6, 390.7)
* NGC 5248: 13:37:32.0 (J2000) +08:53:08 (422.16, 396.02)
*Note (2): At a distance of 10 Mpc, 0.1" corresponds to 5pc
*Note (3): At a distance of 10 Mpc this unit corresponds to a luminosity
* of 1.2x10^36^erg/s.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Compact sources brightest in V - NGC 1512
integer*4 nr__1
parameter (nr__1=475) ! Number of records
character*110 ar__1 ! Full-size record
integer*4 CS (nr__1) ! Compact source number
* ([MBH2001 NGC NNNN CS NN in Simbad)
real*4 Xpix (nr__1) ! (pix) X pixel PC coordinate in the F547M frame
real*4 Ypix (nr__1) ! (pix) Y pixel PC coordinate in the F547M frame
real*4 oRA (nr__1) ! (arcsec) Right Ascension offset from
* galaxy nucleus (1)
real*4 oDE (nr__1) ! (arcsec) Declination offset from
* galaxy nucleus (1)
real*4 Vmag (nr__1) ! (mag) ? The V band magnitude
real*4 Del1_3 (nr__1) ! (mag) ? Magnitude difference between F547M
* photometry (about Stroemgren y) in
* 3-pixel and 1-pixel radius aperture
character*1 l_F2300 (nr__1) ! Limit flag on F2300 (2)
real*8 F2300 (nr__1) ! (10-21W/m2/nm) ? The f_{lambda}_ flux at 2300{AA} (3)
real*4 e_F2300 (nr__1) ! (10-21W/m2/nm) ? The one {sigma} error in F2300 (4)
character*1 l_F3350 (nr__1) ! Limit flag on F3350 (2)
real*4 F3350 (nr__1) ! (10-21W/m2/nm) ? The f_{lambda}_ flux at 3350{AA} (3)
real*4 e_F3350 (nr__1) ! (10-21W/m2/nm) ? The one {sigma} error in F3350 (U) (4)
character*1 l_F5490 (nr__1) ! Limit flag on F5490 (2)
real*4 F5490 (nr__1) ! (10-21W/m2/nm) The f_{lambda}_ flux at 5490{AA} (V) (3)
real*4 e_F5490 (nr__1) ! (10-21W/m2/nm) ? The one {sigma} error in F5490 (4)
character*1 l_F8040 (nr__1) ! Limit flag on F8040 (2)
real*4 F8040 (nr__1) ! (10-21W/m2/nm) The f_{lambda}_ flux at 8040{AA} (I) (3)
real*4 e_F8040 (nr__1) ! (10-21W/m2/nm) ? The one {sigma} error in F8040 (4)
character*1 l_F1_6 (nr__1) ! Limit flag on F1.6 (2)
real*4 F1_6 (nr__1) ! (10-21W/m2/nm) ? The f_{lambda}_ flux at 1.6{mu}m (H)
* (3)(4)
real*4 e_F1_6 (nr__1) ! (10-21W/m2/nm) ? The one {sigma} error in F1.6 (4)
*Note (1): Galaxy nucleus of NGC 1512 (table3.dat) is at pixel coordinates
* 419.6, 390.7.
* Galaxy nucleus of NGC 5248 (table4.dat) is at pixel coordinates
* 422.16, 396.02
*Note (2): For null detections, the flux limits actually depend on the local
* background and crowding, and the limits quoted are just those
* typical for the band.
*Note (3): Fluxes are in units of 10^-19^ergs/s/cm^2^/{AA}
*Note (4): Missing entries are for sources outside the field of view of the
* FOC or NICMOS.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! Compact sources brightest in V - NGC 5248
integer*4 nr__2
parameter (nr__2=507) ! Number of records
character*110 ar__2 ! Full-size record
integer*4 CS_1 (nr__2) ! Compact source number
* ([MBH2001 NGC NNNN CS NN in Simbad)
real*4 Xpix_1 (nr__2) ! (pix) X pixel PC coordinate in the F547M frame
real*4 Ypix_1 (nr__2) ! (pix) Y pixel PC coordinate in the F547M frame
real*4 oRA_1 (nr__2) ! (arcsec) Right Ascension offset from
* galaxy nucleus (1)
real*4 oDE_1 (nr__2) ! (arcsec) Declination offset from
* galaxy nucleus (1)
real*4 Vmag_1 (nr__2) ! (mag) ? The V band magnitude
real*4 Del1_3_1 (nr__2) ! (mag) ? Magnitude difference between F547M
* photometry (about Stroemgren y) in
* 3-pixel and 1-pixel radius aperture
character*1 l_F2300_1 (nr__2) ! Limit flag on F2300 (2)
real*8 F2300_1 (nr__2) ! (10-21W/m2/nm) ? The f_{lambda}_ flux at 2300{AA} (3)
real*4 e_F2300_1 (nr__2) ! (10-21W/m2/nm) ? The one {sigma} error in F2300 (4)
character*1 l_F3350_1 (nr__2) ! Limit flag on F3350 (2)
real*4 F3350_1 (nr__2) ! (10-21W/m2/nm) ? The f_{lambda}_ flux at 3350{AA} (3)
real*4 e_F3350_1 (nr__2) ! (10-21W/m2/nm) ? The one {sigma} error in F3350 (U) (4)
character*1 l_F5490_1 (nr__2) ! Limit flag on F5490 (2)
real*4 F5490_1 (nr__2) ! (10-21W/m2/nm) The f_{lambda}_ flux at 5490{AA} (V) (3)
real*4 e_F5490_1 (nr__2) ! (10-21W/m2/nm) ? The one {sigma} error in F5490 (4)
character*1 l_F8040_1 (nr__2) ! Limit flag on F8040 (2)
real*4 F8040_1 (nr__2) ! (10-21W/m2/nm) The f_{lambda}_ flux at 8040{AA} (I) (3)
real*4 e_F8040_1 (nr__2) ! (10-21W/m2/nm) ? The one {sigma} error in F8040 (4)
character*1 l_F1_6_1 (nr__2) ! Limit flag on F1.6 (2)
real*4 F1_6_1 (nr__2) ! (10-21W/m2/nm) ? The f_{lambda}_ flux at 1.6{mu}m (H)
* (3)(4)
real*4 e_F1_6_1 (nr__2) ! (10-21W/m2/nm) ? The one {sigma} error in F1.6 (4)
*Note (1): Galaxy nucleus of NGC 1512 (table3.dat) is at pixel coordinates
* 419.6, 390.7.
* Galaxy nucleus of NGC 5248 (table4.dat) is at pixel coordinates
* 422.16, 396.02
*Note (2): For null detections, the flux limits actually depend on the local
* background and crowding, and the limits quoted are just those
* typical for the band.
*Note (3): Fluxes are in units of 10^-19^ergs/s/cm^2^/{AA}
*Note (4): Missing entries are for sources outside the field of view of the
* FOC or NICMOS.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! Cluster ages, extinctions and masses - NGC 1512
integer*4 nr__3
parameter (nr__3=248) ! Number of records
character*64 ar__3 ! Full-size record
integer*4 CS_2 (nr__3) ! Compact source number
* ([MBH2001] NGC NNNN CS NNN in Simbad)
integer*4 o_CS (nr__3) ! Number of bands source observed in (1)
integer*4 B_Age (nr__3) ! (Myr) Best fitting model age
real*4 B_AV (nr__3) ! (mag) Best fitting model V band extinction
real*4 B_Mass (nr__3) ! (10+4solMass) Best fitting model mass
real*4 B_chi2 (nr__3) ! Reduced {chi}^2^ of best fitting model
integer*4 Y_Age (nr__3) ! (Myr) ? Youngest acceptable model age
real*4 Y_AV (nr__3) ! (mag) ? Youngest acceptable model V band
* extinction
real*4 Y_Mass (nr__3) ! (10+4solMass) ? Youngest acceptable model mass
real*4 Y_chi2 (nr__3) ! ? Reduced {chi}^2^ of youngest acceptable
* model
integer*4 O_Age (nr__3) ! (Myr) ? Oldest acceptable model age
real*4 O_AV (nr__3) ! (mag) ? Oldest acceptable model V band extinction
real*4 O_Mass (nr__3) ! (10+4solMass) ? Oldest acceptable model mass
real*4 O_chi2 (nr__3) ! ? Reduced {chi}^2^ of oldest acceptable
* model
*Note (1): Objects with detections in fewer than 4 bands not fitted. Formally
* ``acceptable'' models have {chi}^2^ per degree of freedom <2.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6.dat' ! Cluster ages, extinctions and masses - NGC 5248
integer*4 nr__4
parameter (nr__4=308) ! Number of records
character*64 ar__4 ! Full-size record
integer*4 CS_3 (nr__4) ! Compact source number
* ([MBH2001] NGC NNNN CS NNN in Simbad)
integer*4 o_CS_1 (nr__4) ! Number of bands source observed in (1)
integer*4 B_Age_1 (nr__4) ! (Myr) Best fitting model age
real*4 B_AV_1 (nr__4) ! (mag) Best fitting model V band extinction
real*4 B_Mass_1 (nr__4) ! (10+4solMass) Best fitting model mass
real*4 B_chi2_1 (nr__4) ! Reduced {chi}^2^ of best fitting model
integer*4 Y_Age_1 (nr__4) ! (Myr) ? Youngest acceptable model age
real*4 Y_AV_1 (nr__4) ! (mag) ? Youngest acceptable model V band
* extinction
real*4 Y_Mass_1 (nr__4) ! (10+4solMass) ? Youngest acceptable model mass
real*4 Y_chi2_1 (nr__4) ! ? Reduced {chi}^2^ of youngest acceptable
* model
integer*4 O_Age_1 (nr__4) ! (Myr) ? Oldest acceptable model age
real*4 O_AV_1 (nr__4) ! (mag) ? Oldest acceptable model V band extinction
real*4 O_Mass_1 (nr__4) ! (10+4solMass) ? Oldest acceptable model mass
real*4 O_chi2_1 (nr__4) ! ? Reduced {chi}^2^ of oldest acceptable
* model
*Note (1): Objects with detections in fewer than 4 bands not fitted. Formally
* ``acceptable'' models have {chi}^2^ per degree of freedom <2.
C=============================================================================
C Loading file 'table2.dat' ! Emission-Line Complexes
C Format for file interpretation
1 format(
+ A8,1X,I2,1X,I3,1X,I3,1X,F5.2,2X,F5.2,1X,F4.2,1X,F5.1,1X,F4.1,
+ 1X,F5.1,1X,F3.1,1X,I3)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,32
read(1,'(A62)')ar__
read(ar__,1)
+ Cluster(i__),ELC(i__),Xpos(i__),Ypos(i__),DRA(i__),DDE(i__),
+ Rad(i__),FHa(i__),FPaa(i__),F1_6um(i__),FHa_FPaa(i__),
+ FPaa_F1_6um(i__)
c ..............Just test output...........
write(6,1)
+ Cluster(i__),ELC(i__),Xpos(i__),Ypos(i__),DRA(i__),DDE(i__),
+ Rad(i__),FHa(i__),FPaa(i__),F1_6um(i__),FHa_FPaa(i__),
+ FPaa_F1_6um(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Compact sources brightest in V - NGC 1512
C Format for file interpretation
2 format(
+ I3,1X,F6.2,1X,F6.2,1X,F6.2,1X,F6.2,1X,F5.2,1X,F4.2,1X,A1,F7.1,
+ 1X,F6.1,1X,A1,F6.1,1X,F5.1,1X,A1,F6.1,1X,F4.1,1X,A1,F5.1,1X,
+ F4.1,1X,A1,F5.1,1X,F4.1)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,475
read(1,'(A110)')ar__1
read(ar__1,2)
+ CS(i__),Xpix(i__),Ypix(i__),oRA(i__),oDE(i__),Vmag(i__),
+ Del1_3(i__),l_F2300(i__),F2300(i__),e_F2300(i__),l_F3350(i__),
+ F3350(i__),e_F3350(i__),l_F5490(i__),F5490(i__),e_F5490(i__),
+ l_F8040(i__),F8040(i__),e_F8040(i__),l_F1_6(i__),F1_6(i__),
+ e_F1_6(i__)
if(ar__1(33:37) .EQ. '') Vmag(i__) = rNULL__
if(ar__1(39:42) .EQ. '') Del1_3(i__) = rNULL__
if(ar__1(45:51) .EQ. '') F2300(i__) = rNULL__
if(ar__1(53:58) .EQ. '') e_F2300(i__) = rNULL__
if(ar__1(61:66) .EQ. '') F3350(i__) = rNULL__
if(ar__1(68:72) .EQ. '') e_F3350(i__) = rNULL__
if(ar__1(82:85) .EQ. '') e_F5490(i__) = rNULL__
if(ar__1(94:97) .EQ. '') e_F8040(i__) = rNULL__
if(ar__1(100:104) .EQ. '') F1_6(i__) = rNULL__
if(ar__1(106:109) .EQ. '') e_F1_6(i__) = rNULL__
c ..............Just test output...........
write(6,2)
+ CS(i__),Xpix(i__),Ypix(i__),oRA(i__),oDE(i__),Vmag(i__),
+ Del1_3(i__),l_F2300(i__),F2300(i__),e_F2300(i__),l_F3350(i__),
+ F3350(i__),e_F3350(i__),l_F5490(i__),F5490(i__),e_F5490(i__),
+ l_F8040(i__),F8040(i__),e_F8040(i__),l_F1_6(i__),F1_6(i__),
+ e_F1_6(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4.dat' ! Compact sources brightest in V - NGC 5248
C Format for file interpretation
3 format(
+ I3,1X,F6.2,1X,F6.2,1X,F6.2,1X,F6.2,1X,F5.2,1X,F4.2,1X,A1,F7.1,
+ 1X,F6.1,1X,A1,F6.1,1X,F5.1,1X,A1,F6.1,1X,F4.1,1X,A1,F5.1,1X,
+ F4.1,1X,A1,F5.1,1X,F4.1)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,507
read(1,'(A110)')ar__2
read(ar__2,3)
+ CS_1(i__),Xpix_1(i__),Ypix_1(i__),oRA_1(i__),oDE_1(i__),
+ Vmag_1(i__),Del1_3_1(i__),l_F2300_1(i__),F2300_1(i__),
+ e_F2300_1(i__),l_F3350_1(i__),F3350_1(i__),e_F3350_1(i__),
+ l_F5490_1(i__),F5490_1(i__),e_F5490_1(i__),l_F8040_1(i__),
+ F8040_1(i__),e_F8040_1(i__),l_F1_6_1(i__),F1_6_1(i__),
+ e_F1_6_1(i__)
if(ar__2(33:37) .EQ. '') Vmag_1(i__) = rNULL__
if(ar__2(39:42) .EQ. '') Del1_3_1(i__) = rNULL__
if(ar__2(45:51) .EQ. '') F2300_1(i__) = rNULL__
if(ar__2(53:58) .EQ. '') e_F2300_1(i__) = rNULL__
if(ar__2(61:66) .EQ. '') F3350_1(i__) = rNULL__
if(ar__2(68:72) .EQ. '') e_F3350_1(i__) = rNULL__
if(ar__2(82:85) .EQ. '') e_F5490_1(i__) = rNULL__
if(ar__2(94:97) .EQ. '') e_F8040_1(i__) = rNULL__
if(ar__2(100:104) .EQ. '') F1_6_1(i__) = rNULL__
if(ar__2(106:109) .EQ. '') e_F1_6_1(i__) = rNULL__
c ..............Just test output...........
write(6,3)
+ CS_1(i__),Xpix_1(i__),Ypix_1(i__),oRA_1(i__),oDE_1(i__),
+ Vmag_1(i__),Del1_3_1(i__),l_F2300_1(i__),F2300_1(i__),
+ e_F2300_1(i__),l_F3350_1(i__),F3350_1(i__),e_F3350_1(i__),
+ l_F5490_1(i__),F5490_1(i__),e_F5490_1(i__),l_F8040_1(i__),
+ F8040_1(i__),e_F8040_1(i__),l_F1_6_1(i__),F1_6_1(i__),
+ e_F1_6_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table5.dat' ! Cluster ages, extinctions and masses - NGC 1512
C Format for file interpretation
4 format(
+ I3,1X,I1,1X,I3,1X,F3.1,1X,F5.2,1X,F5.2,1X,I3,1X,F3.1,1X,F5.2,
+ 1X,F4.2,1X,I3,1X,F3.1,1X,F5.2,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,248
read(1,'(A64)')ar__3
read(ar__3,4)
+ CS_2(i__),o_CS(i__),B_Age(i__),B_AV(i__),B_Mass(i__),
+ B_chi2(i__),Y_Age(i__),Y_AV(i__),Y_Mass(i__),Y_chi2(i__),
+ O_Age(i__),O_AV(i__),O_Mass(i__),O_chi2(i__)
if(ar__3(27:29) .EQ. '') Y_Age(i__) = iNULL__
if(ar__3(31:33) .EQ. '') Y_AV(i__) = rNULL__
if(ar__3(35:39) .EQ. '') Y_Mass(i__) = rNULL__
if(ar__3(41:44) .EQ. '') Y_chi2(i__) = rNULL__
if(ar__3(46:48) .EQ. '') O_Age(i__) = iNULL__
if(ar__3(50:52) .EQ. '') O_AV(i__) = rNULL__
if(ar__3(54:58) .EQ. '') O_Mass(i__) = rNULL__
if(ar__3(60:63) .EQ. '') O_chi2(i__) = rNULL__
c ..............Just test output...........
write(6,4)
+ CS_2(i__),o_CS(i__),B_Age(i__),B_AV(i__),B_Mass(i__),
+ B_chi2(i__),Y_Age(i__),Y_AV(i__),Y_Mass(i__),Y_chi2(i__),
+ O_Age(i__),O_AV(i__),O_Mass(i__),O_chi2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table6.dat' ! Cluster ages, extinctions and masses - NGC 5248
C Format for file interpretation
5 format(
+ I3,1X,I1,1X,I3,1X,F3.1,1X,F5.2,1X,F5.2,1X,I3,1X,F3.1,1X,F5.2,
+ 1X,F4.2,1X,I3,1X,F3.1,1X,F5.2,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table6.dat')
write(6,*) '....Loading file: table6.dat'
do i__=1,308
read(1,'(A64)')ar__4
read(ar__4,5)
+ CS_3(i__),o_CS_1(i__),B_Age_1(i__),B_AV_1(i__),B_Mass_1(i__),
+ B_chi2_1(i__),Y_Age_1(i__),Y_AV_1(i__),Y_Mass_1(i__),
+ Y_chi2_1(i__),O_Age_1(i__),O_AV_1(i__),O_Mass_1(i__),
+ O_chi2_1(i__)
if(ar__4(27:29) .EQ. '') Y_Age_1(i__) = iNULL__
if(ar__4(31:33) .EQ. '') Y_AV_1(i__) = rNULL__
if(ar__4(35:39) .EQ. '') Y_Mass_1(i__) = rNULL__
if(ar__4(41:44) .EQ. '') Y_chi2_1(i__) = rNULL__
if(ar__4(46:48) .EQ. '') O_Age_1(i__) = iNULL__
if(ar__4(50:52) .EQ. '') O_AV_1(i__) = rNULL__
if(ar__4(54:58) .EQ. '') O_Mass_1(i__) = rNULL__
if(ar__4(60:63) .EQ. '') O_chi2_1(i__) = rNULL__
c ..............Just test output...........
write(6,5)
+ CS_3(i__),o_CS_1(i__),B_Age_1(i__),B_AV_1(i__),B_Mass_1(i__),
+ B_chi2_1(i__),Y_Age_1(i__),Y_AV_1(i__),Y_Mass_1(i__),
+ Y_chi2_1(i__),O_Age_1(i__),O_AV_1(i__),O_Mass_1(i__),
+ O_chi2_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end