Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/663/A12 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 2026-Aug-12
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/A+A/663/A12 Planetary nebulae in NGC3379 and NGC3384 (Hartke+, 2022)
*================================================================================
*The halo of M105 and its group environment as traced by planetary nebula
*populations. II. Using kinematics of single stars to unveil the presence of
*intragroup light around the Leo I galaxies NGC 3384 and M105.
* Hartke J., Arnaboldi M., Gerhard O., Coccato L., Merrifield M., Kuijken K.,
* Pulsoni C., Agnello A., Bhattacharya S., Spiniello C., Cortesi A.,
* Freeman K.C., Napolitano N.R., Romanowsky A.J
* <Astron. Astrophys. 663, A12 (2022)>
* =2022A&A...663A..12H (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'photom.dat' ! Planetary nebula candidates in the outer regions
of the elliptical galaxy M105 in the Leo I group
(table A1)
integer*4 nr__
parameter (nr__=226) ! Number of records
character*58 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*13 ID ! PN identifier, M105-SCAM-NNN
integer*4 RAh ! (h) Right ascension (J2000)
integer*4 RAm ! (min) Right ascension (J2000)
real*8 RAs ! (s) Right ascension (J2000)
character*1 DE_ ! Declination sign (J2000)
integer*4 DEd ! (deg) Declination (J2000)
integer*4 DEm ! (arcmin) Declination (J2000)
real*8 DEs ! (arcsec) Declination (J2000)
real*8 v_OIII_mag ! (mag) Apparent AB magnitude in the [OIII] narrow
* band (1)
real*8 Vmag ! (mag) Apparent AB magnitude in the V broad band
*Note (1): To convert AB magnitudes into 5007mag magnitudes from the [OIII] line,
* the relation by Arnaboldi et al. (2003AJ....125..514A) can be used, which is
* 5007mag = [OIII]mag + 2.49.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'kinema.dat' ! Planetary nebulae in the outer regions of the
elliptical galaxy M105 in the Leo I group
(table A2)
integer*4 nr__1
parameter (nr__1=319) ! Number of records
character*112 ar__1 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 ! (deg) Right Ascension J2000
real*8 DEdeg_1 ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*20 ID_1 ! PN identifier (1)
integer*4 RAh_1 ! (h) Right ascension (J2000)
integer*4 RAm_1 ! (min) Right ascension (J2000)
real*8 RAs_1 ! (s) Right ascension (J2000)
character*1 DE__1 ! Declination sigm (J2000)
integer*4 DEd_1 ! (deg) Declination (J2000)
integer*4 DEm_1 ! (arcmin) Declination (J2000)
real*8 DEs_1 ! (arcsec) Declination (J2000)
real*8 v_OIII_mag_1 ! (mag) Apparent AB magnitude in the [OIII] narrow
* band (2)
real*8 Vlos ! (km/s) Line-of-sight velocity
real*8 e_Vlos ! (km/s) Error on the line-of-sight velocity
real*8 fM105 ! [0/1] Membership probability to belong to the
* galaxy M105 (3)
*Note (1): Objects with IDs starting with M105-C and N3384 were observed first by
* Douglas et al. (2007ApJ...664..257D, Cat. J/ApJ/664/257, PNS-EPN NGC3379 NNN
* in Simnad) and Cortesi et al. (2013A&A...549A.115C, Cat. J/A+A/549/A115,
* PNS-EPN NGC3384-NNN in Simbad), respectively.
* Two concatenated IDs denote PNe that were observed in two fields.
*Note (2): To convert AB magnitudes into 5007mag magnitudes from the [OIII] line,
* the relation by Arnaboldi et al. (2003AJ....125..514A) can be used, which is
* 5007mag = [OIII]mag + 2.49.
*Note (3): The probability space is defined such that probabilities larger than
* f_M105>0.5 denote PNe associated with the galaxy M105 and probabilities
* smaller than f_M105<0.5 PNe associated with the companion galaxy NGC 3384.
C=============================================================================
C Loading file 'photom.dat' ! Planetary nebula candidates in the outer regions
* of the elliptical galaxy M105 in the Leo I group
* (table A1)
C Format for file interpretation
1 format(
+ A13,1X,I2,1X,I2,1X,F7.4,1X,A1,I2,1X,I2,1X,F7.4,1X,F7.4,1X,F7.4)
C Effective file loading
open(unit=1,status='old',file=
+'photom.dat')
write(6,*) '....Loading file: photom.dat'
do i__=1,226
read(1,'(A58)')ar__
read(ar__,1)ID,RAh,RAm,RAs,DE_,DEd,DEm,DEs,v_OIII_mag,Vmag
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)ID,RAh,RAm,RAs,DE_,DEd,DEm,DEs,v_OIII_mag,Vmag
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'kinema.dat' ! Planetary nebulae in the outer regions of the
* elliptical galaxy M105 in the Leo I group
* (table A2)
C Format for file interpretation
2 format(
+ A20,1X,I2,1X,I2,1X,F7.4,1X,A1,I2,1X,I2,1X,F7.4,1X,F14.10,1X,
+ F10.5,1X,F13.10,1X,F22.20)
C Effective file loading
open(unit=1,status='old',file=
+'kinema.dat')
write(6,*) '....Loading file: kinema.dat'
do i__=1,319
read(1,'(A112)')ar__1
read(ar__1,2)
+ ID_1,RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,v_OIII_mag_1,
+ Vlos,e_Vlos,fM105
RAdeg_1 = rNULL__
DEdeg_1 = rNULL__
c Derive coordinates RAdeg_1 and DEdeg_1 from input data
c (RAdeg_1 and DEdeg_1 are set to rNULL__ when unknown)
if(RAh_1 .GT. -180) RAdeg_1=RAh_1*15.
if(RAm_1 .GT. -180) RAdeg_1=RAdeg_1+RAm_1/4.
if(RAs_1 .GT. -180) RAdeg_1=RAdeg_1+RAs_1/240.
if(DEd_1 .GE. 0) DEdeg_1=DEd_1
if(DEm_1 .GE. 0) DEdeg_1=DEdeg_1+DEm_1/60.
if(DEs_1 .GE. 0) DEdeg_1=DEdeg_1+DEs_1/3600.
if(DE__1.EQ.'-'.AND.DEdeg_1.GE.0) DEdeg_1=-DEdeg_1
c ..............Just test output...........
write(6,2)
+ ID_1,RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,v_OIII_mag_1,
+ Vlos,e_Vlos,fM105
write(6,'(6H Pos: 2F8.4)') RAdeg_1,DEdeg_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end