Conversion of standardized ReadMe file for
file /./ftp/cats/J/MNRAS/446/2330 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-May-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/MNRAS/446/2330 Overmassive black holes (Savorgnan+, 2015)
*================================================================================
*Overmassive black holes in the MBH-{sigma} diagram do not belong to over
*(dry) merged galaxies.
* Savorgnan G.A.D., Graham A.W.
* <Mon. Not. R. Astron. Soc., 446, 2330-2336 (2015)>
* =2015MNRAS.446.2330S (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Galaxy sample
integer*4 nr__
parameter (nr__=89) ! Number of records
character*105 ar__ ! Full-size record
character*9 Galaxy (nr__) ! Galaxy name
character*1 n_Galaxy (nr__) ! [*] Note on Galaxy (1)
real*8 Dist (nr__) ! (Mpc) Distance
real*8 MBH (nr__) ! (10+8Msun) Black hole mass
real*8 E_MBH (nr__) ! (10+8Msun) Error on MBH (upper value)
real*8 e_MBH_1 (nr__) ! (10+8Msun) Error on MBH (lower value)
real*4 MBHR (nr__) ! (10+8Msun) ? For the 10 measurements taken from Rusli et
* al. (2013, Cat. J/AJ/146/45), measurement
* obtained without including in the modelling
* the effects of dark matter
integer*4 sigma (nr__) ! (km/s) Stellar velocity dispersions
integer*4 e_sigma (nr__) ! (km/s) ? rms uncertainty on sigma
integer*4 sigmaU (nr__) ! (km/s) ? Upper value of sigma when interval
character*4 Ref (nr__) ! References of black hole mass and velocity
* dispersion measurements reported here (2)
character*4 Core (nr__) ! [yes/no? ] Presence of a partially depleted
* core (3)
character*4 Bar (nr__) ! [yes/no ?] Presence of a bar
real*4 Mdef1 (nr__) ! (10+8Msun) ? Central stellar mass deficits as measured by
* Rusli et al. (2013, Cat. J/AJ/146/45).
real*4 e_Mdef1 (nr__) ! (10+8Msun) ? rms uncertainty on Mdef1
integer*4 Mdef2 (nr__) ! (10+8Msun) ? For seven galaxies we reconstructed the
* 'no-dark-matter' values (see Section 3.1)
integer*4 Mdef3 (nr__) ! (10+8Msun) ? Central stellar mass deficits as measured by
* Dullo & Graham (2014MNRAS.444.2700D)
integer*4 e_Mdef3 (nr__) ! (10+8Msun) ? rms uncertainty on Mdef3
character*4 Class (nr__) ! Kinematical classification (fast/slow rotator)
*Note (1): for the 18 galaxies marked with a *, the black hole masses were
* estimated including in the modelling the effects of dark matter.
*Note (2): References as follows:
* G+03 = Greenhill et al., 2003ApJ...590..162G
* R+13 = Rusli et al., 2013AJ....146...45R, Cat. J/AJ/146/45
* GS13 = Graham & Scott, 2013ApJ...764..151G
*Note (3): The question mark is used when the classification has come from the
* velocity dispersion criteria mentioned in Section 3.
C=============================================================================
C Loading file 'table1.dat' ! Galaxy sample
C Format for file interpretation
1 format(
+ A9,A1,1X,F7.3,1X,F7.3,1X,F7.3,1X,F7.3,2X,F5.2,1X,I3,1X,I2,1X,
+ I3,1X,A4,1X,A4,1X,A4,F5.1,1X,F5.1,2X,I3,2X,I3,1X,I3,1X,A4)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,89
read(1,'(A105)')ar__
read(ar__,1)
+ Galaxy(i__),n_Galaxy(i__),Dist(i__),MBH(i__),E_MBH(i__),
+ e_MBH_1(i__),MBHR(i__),sigma(i__),e_sigma(i__),sigmaU(i__),
+ Ref(i__),Core(i__),Bar(i__),Mdef1(i__),e_Mdef1(i__),
+ Mdef2(i__),Mdef3(i__),e_Mdef3(i__),Class(i__)
if(ar__(45:49) .EQ. '') MBHR(i__) = rNULL__
if(ar__(55:56) .EQ. '') e_sigma(i__) = iNULL__
if(ar__(58:60) .EQ. '') sigmaU(i__) = iNULL__
if(ar__(76:80) .EQ. '') Mdef1(i__) = rNULL__
if(ar__(82:86) .EQ. '') e_Mdef1(i__) = rNULL__
if(ar__(89:91) .EQ. '') Mdef2(i__) = iNULL__
if(ar__(94:96) .EQ. '') Mdef3(i__) = iNULL__
if(ar__(98:100) .EQ. '') e_Mdef3(i__) = iNULL__
c ..............Just test output...........
write(6,1)
+ Galaxy(i__),n_Galaxy(i__),Dist(i__),MBH(i__),E_MBH(i__),
+ e_MBH_1(i__),MBHR(i__),sigma(i__),e_sigma(i__),sigmaU(i__),
+ Ref(i__),Core(i__),Bar(i__),Mdef1(i__),e_Mdef1(i__),
+ Mdef2(i__),Mdef3(i__),e_Mdef3(i__),Class(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end