Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/720/555 into FORTRAN code for reading data files line by line.
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-16
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/720/555 COLA. III. AGN in compact IR galaxies (Parra+, 2010)
*================================================================================
*COLA.
*III. Radio detection of active galactic nucleus in compact moderate luminosity
*infrared galaxies.
* Parra R., Conway J.E., Aalto S., Appleton P.N., Norris R.P.,
* Pihlstrom Y.M., Kewley L.J.
* <Astrophys. J., 720, 555-568 (2010)>
* =2010ApJ...720..555P
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! COLA North sample
integer*4 nr__
parameter (nr__=110) ! Number of records
character*79 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg ! (deg) Right Ascension J2000
real*8 DEdeg ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*11 IRAS ! IRAS name (G1)
character*6 OName ! Other name
integer*4 RAh ! (h) VLA Hour of Right Ascension (J2000)
integer*4 RAm ! (min) VLA Minute of Right Ascension (J2000)
real*4 RAs ! (s) VLA Second of Right Ascension (J2000)
character*1 DE_ ! VLA Sign of declination (J2000)
integer*4 DEd ! (deg) VLA Degree of Declination (J2000)
integer*4 DEm ! (arcmin) VLA Arcminute of Declination (J2000)
real*4 DEs ! (arcsec) VLA Arcsecond of Declination (J2000)
character*1 IR ! [I] I: indicates an IRAS position;
* not detected by VLA
integer*4 VHel ! (km/s) NED Heliocentric velocity
real*4 DL ! (Mpc) Luminosity distance (1)
real*4 logLIR ! ([Lsun]) Log of IR luminosity
real*4 logL1_4 ! ([W/Hz]) Log of 1.4GHz luminosity (2)
real*4 logLFIR ! ([W/Hz]) Log of far IR spectral luminosity
real*4 q1_4 ! ([-]) Log ratio of far IR to 1.4GHz luminosities (3)
*Note (1): The luminosity distance D_L_ for each source was calculated in NED
* assuming the three attractor model of Mould et al. (2000ApJ...529..786M)
* and the cosmological parameters derived from 5 year WMAP data
* (Hinshaw et al. 2009ApJS..180..225H), i.e., {Omega}_m_=0.276,
* {Omega}_{nu}_=0.726, and H_0_=70.5km/s.
*Note (2): Calculated from the NVSS catalog (Condon et al. 1998, Cat. VIII/65).
*Note (3): Infrared total flux densities were taken from the IRAS Point Source
* Catalog (Beichman et al., Cat. II/125). In order to calculate
* source infrared to radio (1.4GHz) ratios (q1.4) as defined by Helou et
* al. (1985ApJ...298L...7H) we calculated for each source an equivalent
* FIR flux density from
* S_FIR_=1.26x10^-14^(2.58f_60_+f_100_)/3.75x10^12^W/m^2^/Hz, where
* f_60_ and f_100_ are the cataloged 60 and 100um IRAS flux densities.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Radio and optical observations and results
integer*4 nr__1
parameter (nr__1=110) ! Number of records
character*65 ar__1 ! Full-size record
character*11 IRAS_1 ! IRAS name (G1)
character*5 Array ! VLA array used
character*3 Morph ! VLA morphology class of 4.8GHz image (4)
real*8 S4_8t ! (mJy) ? Recovered 4.8GHz flux density
real*4 q4_8 ! ([-]) ? Log ratio of S4.8t to FIR flux densities
real*4 S4_8c ! (mJy) ? Total gaussian fitted 4.8GHz flux density (5)
real*4 amaj ! (arcsec) ? Fitted gaussian major axis (6)
real*4 bmin ! (arcsec) ? Fitted gaussian minor axis (6)
real*4 logTb ! ([K]) ? Log Peak 4.8GHz brightness temperature (7)
character*3 Epoch ! VLBI epoch(s) observed
character*1 V ! [*] *: VLBI detection
character*2 Cl ! Optical class (G2)
*Note (4): VLA morphology class (as defined by Neff & Hutchings,
* 1992AJ....103.1746N) as follows:
* C = Compact;
* E = Extended;
* CE = Compact plus Extended;
* CER = Compact plus extended with ring;
* U = Undetected.
*Note (5): Fitted to brightest feature in VLA image (after removing VLBI
* component, hence zero indicates that brightest feature was dominated
* by the VLBI component).
*Note (6): To peak VLA feature (FWHM), Note for IRAS15327+2340 (Arp 220) these
* are for the western nucleus as taken from the literature (see Section 4.5).
*Note (7): Of gaussian component (see Section 4.5).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! VLBI results
integer*4 nr__2
parameter (nr__2=21) ! Number of records
character*71 ar__2 ! Full-size record
character*11 IRAS_2 ! IRAS name (G1)
character*7 OName_1 ! Other name
character*1 l_Eb_Wb ! Limit flag on Eb-Wb (1)
real*4 Eb_Wb ! (mJy) ? VLBI 4.8GHz flux obtained from the peak in the
* Delay-Rate map (Effelsberg telescope)
real*4 e_Eb_Wb ! (mJy) ? 1{sigma} uncertainty on Eb-Wb
character*1 l_Eb_Jb1 ! Limit flag on Eb-Jb1 (1)
real*4 Eb_Jb1 ! (mJy) ? VLBI 4.8GHz flux obtained from the peak in the
* Delay-Rate map (Jodrell Bank, Lovell telescope)
real*4 e_Eb_Jb1 ! (mJy) ? 1{sigma} uncertainty on Eb-Jb1
character*1 l_Eb_Ar ! Limit flag on Eb-Ar (1)
real*8 Eb_Ar ! (mJy) ? VLBI 4.8GHz flux obtained from the peak in the
* Delay-Rate map (Arecibo)
real*4 e_Eb_Ar ! (mJy) ? 1{sigma} uncertainty on Eb-Ar
character*1 f_Eb_Ar ! [n] Flag on Arp 220 (2)
character*1 l_ASize ! Limit flag on ASize
real*4 ASize ! (mas) ? Angular size (3)
character*1 l_LSize ! Limit flag on LSize
real*4 LSize ! (pc) ? Corresponding fitted Gaussian FWHM linear size
character*1 Cl_1 ! Optical class (G2)
*Note (1): Upper limits for the non-detections are indicated at 5{sigma}.
*Note (2):
* n = For IRAS15327+2340 (Arp 220) on the longer baselines the two rows give
* results for the west and east nuclei, respectively.
*Note (3): FWHM of a circular Gaussian source fitting the flux ratio between the
* Eb-Wb and Eb-Ar baselines (see Section 4.3). Sources with flux upper
* limits on the Eb-Ar have consequently size lower limits.
C=============================================================================
C Loading file 'table1.dat' ! COLA North sample
C Format for file interpretation
1 format(
+ A11,1X,A6,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,A1,1X,
+ I4,1X,F5.1,1X,F5.2,1X,F5.2,1X,F5.2,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,110
read(1,'(A79)')ar__
read(ar__,1)
+ IRAS,OName,RAh,RAm,RAs,DE_,DEd,DEm,DEs,IR,VHel,DL,logLIR,
+ logL1_4,logLFIR,q1_4
RAdeg = rNULL__
DEdeg = rNULL__
c Derive coordinates RAdeg and DEdeg from input data
c (RAdeg and DEdeg are set to rNULL__ when unknown)
if(RAh .GT. -180) RAdeg=RAh*15.
if(RAm .GT. -180) RAdeg=RAdeg+RAm/4.
if(RAs .GT. -180) RAdeg=RAdeg+RAs/240.
if(DEd .GE. 0) DEdeg=DEd
if(DEm .GE. 0) DEdeg=DEdeg+DEm/60.
if(DEs .GE. 0) DEdeg=DEdeg+DEs/3600.
if(DE_.EQ.'-'.AND.DEdeg.GE.0) DEdeg=-DEdeg
c ..............Just test output...........
write(6,1)
+ IRAS,OName,RAh,RAm,RAs,DE_,DEd,DEm,DEs,IR,VHel,DL,logLIR,
+ logL1_4,logLFIR,q1_4
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Radio and optical observations and results
C Format for file interpretation
2 format(
+ A11,1X,A5,1X,A3,1X,F8.2,1X,F5.2,1X,F5.2,1X,F4.2,1X,F4.2,1X,
+ F4.2,1X,A3,A1,1X,A2)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,110
read(1,'(A65)')ar__1
read(ar__1,2)
+ IRAS_1,Array,Morph,S4_8t,q4_8,S4_8c,amaj,bmin,logTb,Epoch,V,Cl
if(ar__1(23:30) .EQ. '') S4_8t = rNULL__
if(ar__1(32:36) .EQ. '') q4_8 = rNULL__
if(ar__1(38:42) .EQ. '') S4_8c = rNULL__
if(ar__1(44:47) .EQ. '') amaj = rNULL__
if(ar__1(49:52) .EQ. '') bmin = rNULL__
if(ar__1(54:57) .EQ. '') logTb = rNULL__
c ..............Just test output...........
write(6,2)
+ IRAS_1,Array,Morph,S4_8t,q4_8,S4_8c,amaj,bmin,logTb,Epoch,V,Cl
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4.dat' ! VLBI results
C Format for file interpretation
3 format(
+ A11,1X,A7,1X,A1,F4.2,1X,F4.2,1X,A1,F4.2,1X,F4.2,1X,A1,F8.2,1X,
+ F4.2,A1,1X,A1,F4.2,1X,A1,F4.2,1X,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,21
read(1,'(A71)')ar__2
read(ar__2,3)
+ IRAS_2,OName_1,l_Eb_Wb,Eb_Wb,e_Eb_Wb,l_Eb_Jb1,Eb_Jb1,e_Eb_Jb1,
+ l_Eb_Ar,Eb_Ar,e_Eb_Ar,f_Eb_Ar,l_ASize,ASize,l_LSize,LSize,Cl_1
if(ar__2(22:25) .EQ. '') Eb_Wb = rNULL__
if(ar__2(27:30) .EQ. '') e_Eb_Wb = rNULL__
if(ar__2(33:36) .EQ. '') Eb_Jb1 = rNULL__
if(ar__2(38:41) .EQ. '') e_Eb_Jb1 = rNULL__
if(ar__2(44:51) .EQ. '') Eb_Ar = rNULL__
if(ar__2(53:56) .EQ. '') e_Eb_Ar = rNULL__
if(ar__2(60:63) .EQ. '') ASize = rNULL__
if(ar__2(66:69) .EQ. '') LSize = rNULL__
c ..............Just test output...........
write(6,3)
+ IRAS_2,OName_1,l_Eb_Wb,Eb_Wb,e_Eb_Wb,l_Eb_Jb1,Eb_Jb1,e_Eb_Jb1,
+ l_Eb_Ar,Eb_Ar,e_Eb_Ar,f_Eb_Ar,l_ASize,ASize,l_LSize,LSize,Cl_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end