Conversion of standardized ReadMe file for
file /./ftp/cats/J/MNRAS/459/220 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/MNRAS/459/220 Optical redshifts of OH- and HI-emitting galaxies (Suess+, 2016)
*================================================================================
*Identifying OH imposters in the ALFALFA Neutral Hydrogen Survey.
* Suess K.A., Darling J., Haynes M.P., Giovanelli R.
* <Mon. Not. R. Astron. Soc., 459, 220-231 (2016)>
* =2016MNRAS.459..220S (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Optical counterpart redshifts of HI-emitting
galaxies
integer*4 nr__
parameter (nr__=130) ! Number of records
character*60 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg (nr__) ! (deg) Right Ascension J2000
real*8 DEdeg (nr__) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*17 Name (nr__) ! Object name
character*1 n_Name (nr__) ! [2-6] Note on Name (1)
integer*4 RAh (nr__) ! (h) Optical counterpart right ascension (J2000)
integer*4 RAm (nr__) ! (min) Optical counterpart right ascension (J2000)
real*4 RAs (nr__) ! (s) Optical counterpart right ascension (J2000)
character*1 DE_ (nr__) ! Optical counterpart declination sign (J2000)
integer*4 DEd (nr__) ! (deg) Optical counterpart declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Optical counterpart declination (J2000)
real*4 DEs (nr__) ! (arcsec) Optical counterpart declination (J2000)
character*6 n_Pos (nr__) ! Note on Pos (2)
integer*4 Vopt (nr__) ! (km/s) Optical velocity (uncertainty is 130km/s)
integer*4 VHI (nr__) ! (km/s) ? HI velocity from Haynes et al.
* (2011, Cat. J/AJ/142/170)
integer*4 e_VHI (nr__) ! (km/s) ? rms uncertainty on VHI
*Note (1): 2 Notes as follows:
* 2 = This spectrum showed both emission and absorption lines. The emission
* lines were more prevalent, but the offset absorption lines clearly
* showed in the blue half of the spectrum. Absorption was especially
* evident in H{beta} and blueward Balmer series lines, where broad emission
* lines were nearly divided in two by the offset absorption. The emission
* velocity occurred at 5035km/s, a match for the ALFALFA HI line; the
* absorption lines were offset to 5770km/s. The velocity listed in Table 3
* is the emission velocity, which matches the ALFALFA HI velocity. The
* galaxy exhibits disturbed morphology in SDSS, and the absorption and
* emission lines may be offset because they come from different nuclei.
* 3 = This object was identified as a clear HI detection; in SDSS it appears
* to be a blue compact dwarf galaxy.
* 4 = The optical counterpart for this object was confirmed to be the blue
* extended object to the west of the central ALFALFA coordinates.
* 5 = Two objects were observed within the ALFALFA beam radius. One observed
* galaxy was to the east of the ALFALFA target coordinates, and one to the
* south. Both galaxies matched the HI velocity, so the coordinates and
* measured velocities for both are included in this table.
* 6 = Most observed objects have at least five identifying spectral lines. For
* this object, only H{alpha} was identified. Despite the scarcity of
* observable optical lines in this spectra, we are confident of the HI
* confirmation. The singular line is bright, shows extension along the
* spatial axis of the spectrum, and it is very close to the expected HI
* redshift. In visible light, the object appears to be a low surface
* brightness galaxy.
*Note (2): For 249263, East and North optical counterparts.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! Ambiguous optical counterparts
integer*4 nr__1
parameter (nr__1=62) ! Number of records
character*87 ar__1 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 (nr__1) ! (deg) Right Ascension J2000
real*8 DEdeg_1 (nr__1) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*17 Name_1 (nr__1) ! Object name
character*2 m_Name (nr__1) ! [AB: ] Multiplicity index on Name
character*1 n_Name_1 (nr__1) ! [2-9] Note on Name (1)
integer*4 RAh_1 (nr__1) ! (h) Observed right ascension (J2000)
integer*4 RAm_1 (nr__1) ! (min) Observed right ascension (J2000)
real*4 RAs_1 (nr__1) ! (s) Observed right ascension (J2000)
character*1 DE__1 (nr__1) ! Observed declination sign (J2000)
integer*4 DEd_1 (nr__1) ! (deg) Observed declination (J2000)
integer*4 DEm_1 (nr__1) ! (arcmin) Observed declination (J2000)
real*4 DEs_1 (nr__1) ! (arcsec) Observed declination (J2000)
character*2 n_Pos_1 (nr__1) ! Note on Pos (2)
integer*4 Vopt_1 (nr__1) ! (km/s) ? Optical velocity (uncertainty is 130km/s)
integer*4 VHI_1 (nr__1) ! (km/s) ? HI velocity from Haynes et al.
* (2011, Cat. J/AJ/142/170)
integer*4 e_VHI_1 (nr__1) ! (km/s) ? rms uncertainty on VHI
integer*4 VOH (nr__1) ! (km/s) ? OH velocity
integer*4 e_VOH (nr__1) ! (km/s) ? rms uncertainty on VOH
character*17 Com (nr__1) ! Comments (3)
*Note (1): Notes as follows:
* 2 = Possible pointing error during observations; this object may not be the
* WISE bright source or the ALFALFA detection.
* 3 = The {alpha}.40 data release of the ALFALFA catalogue incorrectly states
* that this object is an OHM (Haynes et al., 2011, Cat. J/AJ/142/170).
* While the measured optical velocity is much higher than the ALFALFA
* velocity, it does not match the OH velocity and the object's identity
* remains unknown.
* 4 = The velocity determination for this object was measured from only one
* line, presumed to be H{alpha}.
* 5 = Bleed-in from a nearby star obscured optical lines for this object.
* 6 = Two objects were observed within beam uncertainty of the ALFALFA
* detection. The first had no visible optical lines, and the second (the
* velocity listed in Table 4) showed broad line emission that matched
* neither the OH nor the HI velocity.
* 7 = Due to high redshift, this object is likely an AGN.
* 8 = Guiding errors during observing rendered these frames unusable; no
* further observations were made.
* 9 = Two possible optical counterparts were observed. One matched neither OH
* nor HI velocities, and the other had no clear optical lines.
*Note (2): A: or B: for HI011145+290458
*Note (3): Comments as follows:
* neither = observed velocity matches neither HI nor OH
* no lines = objects for which no optical lines were observable and no velocity
* determination could be made
* ML = ALFALFA HI detection is a marginal line, likely not a real detections
* UL = ALFALFA line is uncertain, and could be HI or another line
C=============================================================================
C Loading file 'table3.dat' ! Optical counterpart redshifts of HI-emitting
* galaxies
C Format for file interpretation
1 format(
+ A17,A1,1X,I2,I2,F5.2,A1,I2,I2,F4.1,1X,A6,1X,I5,1X,I5,1X,I3)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,130
read(1,'(A60)')ar__
read(ar__,1)
+ Name(i__),n_Name(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
+ DEd(i__),DEm(i__),DEs(i__),n_Pos(i__),Vopt(i__),VHI(i__),
+ e_VHI(i__)
if(ar__(52:56) .EQ. '') VHI(i__) = iNULL__
if(ar__(58:60) .EQ. '') e_VHI(i__) = iNULL__
RAdeg(i__) = rNULL__
DEdeg(i__) = rNULL__
c Derive coordinates RAdeg and DEdeg from input data
c (RAdeg and DEdeg are set to rNULL__ when unknown)
if(RAh(i__) .GT. -180) RAdeg(i__)=RAh(i__)*15.
if(RAm(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAm(i__)/4.
if(RAs(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAs(i__)/240.
if(DEd(i__) .GE. 0) DEdeg(i__)=DEd(i__)
if(DEm(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEm(i__)/60.
if(DEs(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEs(i__)/3600.
if(DE_(i__).EQ.'-'.AND.DEdeg(i__).GE.0) DEdeg(i__)=-DEdeg(i__)
c ..............Just test output...........
write(6,1)
+ Name(i__),n_Name(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
+ DEd(i__),DEm(i__),DEs(i__),n_Pos(i__),Vopt(i__),VHI(i__),
+ e_VHI(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4.dat' ! Ambiguous optical counterparts
C Format for file interpretation
2 format(
+ A17,A2,A1,1X,I2,I2,F5.2,A1,I2,I2,F4.1,1X,A2,1X,I6,2X,I5,1X,I2,
+ 1X,I6,1X,I2,1X,A17)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,62
read(1,'(A87)')ar__1
read(ar__1,2)
+ Name_1(i__),m_Name(i__),n_Name_1(i__),RAh_1(i__),RAm_1(i__),
+ RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),
+ n_Pos_1(i__),Vopt_1(i__),VHI_1(i__),e_VHI_1(i__),VOH(i__),
+ e_VOH(i__),Com(i__)
if(ar__1(44:49) .EQ. '') Vopt_1(i__) = iNULL__
if(ar__1(52:56) .EQ. '') VHI_1(i__) = iNULL__
if(ar__1(58:59) .EQ. '') e_VHI_1(i__) = iNULL__
if(ar__1(61:66) .EQ. '') VOH(i__) = iNULL__
if(ar__1(68:69) .EQ. '') e_VOH(i__) = iNULL__
RAdeg_1(i__) = rNULL__
DEdeg_1(i__) = 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(i__) .GT. -180) RAdeg_1(i__)=RAh_1(i__)*15.
if(RAm_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAm_1(i__)/4.
if(RAs_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAs_1(i__)/240.
if(DEd_1(i__) .GE. 0) DEdeg_1(i__)=DEd_1(i__)
if(DEm_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEm_1(i__)/60.
if(DEs_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEs_1(i__)/3600.
if(DE__1(i__).EQ.'-'.AND.DEdeg_1(i__).GE.0) DEdeg_1(i__)=-DEdeg_1(i__)
c ..............Just test output...........
write(6,2)
+ Name_1(i__),m_Name(i__),n_Name_1(i__),RAh_1(i__),RAm_1(i__),
+ RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),
+ n_Pos_1(i__),Vopt_1(i__),VHI_1(i__),e_VHI_1(i__),VOH(i__),
+ e_VOH(i__),Com(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end