Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/149/5 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/149/5 Solar neighborhood. XXXV. Distances to M dwarfs (Winters+, 2015)
*================================================================================
*The solar neighborhood.
*XXXV. Distances to 1404 M dwarf systems within 25 pc in the southern sky.
* Winters J.G., Hambly N.C., Jao W.-C., Dieterich S.B., Lurie J.C.,
* Henry T.J., Hosey A.D., Slatten K.J., Boyd M.R., Ianna P.A., Riedel A.R.,
* Subasavage J.P., Finch C.T., Bartlett J.L.
* <Astron. J., 149, 5 (2015)>
* =2015AJ....149....5W
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Observed data for southern red dwarf systems
integer*4 nr__
parameter (nr__=1748) ! Number of records
character*160 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*14 Name (nr__) ! Name of the M dwarf primary (G1)
integer*4 Nc (nr__) ! Number of known components in the system
integer*4 Np (nr__) ! ? Indicates how many of the components are
* included in the photometry
integer*4 RAh (nr__) ! (h) Hour of Right Ascension (J2000)
integer*4 RAm (nr__) ! (min) Minute of Right Ascension (J2000)
real*4 RAs (nr__) ! (s) Second of Right Ascension (J2000)
character*1 DE_ (nr__) ! Sign of the Declination (J2000)
integer*4 DEd (nr__) ! (deg) Degree of Declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Arcminute of Declination (J2000)
integer*4 DEs (nr__) ! (arcsec) Arcsecond of Declination (J2000)
real*4 pm (nr__) ! (arcsec/yr) Total proper motion magnitude
real*4 pmPA (nr__) ! (deg) Proper motion position angle
integer*4 r_pm (nr__) ! Reference for pm (in refs.dat file) (1)
real*8 plx (nr__) ! (mas) ? Weighted mean of published trigonometric
* parallaxes (see Section 3.4)
character*2 f_plx (nr__) ! Note on plx (2)
real*4 e_plx (nr__) ! (mas) ? Error in plx
integer*4 o_plx (nr__) ! ? Number of measurements for plx
character*13 r_plx (nr__) ! Reference for plx (in ref.dat file)
real*4 Bmag (nr__) ! (mag) ? SuperCOSMOS B_J_ plate magnitude (3)
character*1 f_Bmag (nr__) ! [J] Magnitude blended due to a close companion
real*4 Fmag (nr__) ! (mag) ? SuperCOSMOS R_59F_ plate magnitude (3)
character*1 f_Fmag (nr__) ! [J] Magnitude blended due to a close companion
real*4 Nmag (nr__) ! (mag) ? SuperCOSMOS I_IVN_ plate magnitude (3)
character*1 f_Nmag (nr__) ! [J] Magnitude blended due to a close companion
real*4 Vmag (nr__) ! (mag) ? The Johnson V band magnitude (4)
character*1 f_Vmag (nr__) ! [J] Magnitude blended due to a close companion
real*4 Rmag (nr__) ! (mag) ? The Kron-Cousins R band magnitude (4)
character*1 f_Rmag (nr__) ! [J] Magnitude blended due to a close companion
real*4 Imag (nr__) ! (mag) ? The Kron-Cousins I band magnitude (4)
character*1 f_Imag (nr__) ! [J] Magnitude blended due to a close companion
integer*4 o_Imag (nr__) ! ? Number of VRI nights from REsearch
* Consortium On Nearby Stars (RECONS;
* http://www.recons.org/)
integer*4 r_Imag (nr__) ! ? Reference for RECONS VRI magnitudes
character*1 New (nr__) ! [U] Indicates updated RECONS VRI values (5)
real*4 Jmag (nr__) ! (mag) 2MASS J band magnitude
character*2 f_Jmag (nr__) ! Blended or inaccurate Jmag (6)
real*4 Hmag (nr__) ! (mag) 2MASS H band magnitude
character*2 f_Hmag (nr__) ! Blended or inaccurate Hmag (6)
real*4 Kmag (nr__) ! (mag) 2MASS Ks band magnitude
character*2 f_Kmag (nr__) ! Blended or inaccurate Kmag (6)
*Note (1): All proper motions are from SuperCOSMOS, except where noted. Some of
* the proper motion values from the SuperCOSMOS Sky Survey for SCR objects
* presented here differ slightly from those in the original discovery papers.
* For the new values, a more comprehensive method has been used that provides
* multiple measurements of proper motion between various plate pairs, while
* before only a single value was available that incorporated all plates into
* the solution simultaneously. The proper motions provided here are those
* that yield consistent values among multiple determinations and are
* preferred.
*Note (2): Flag on parallax defined as follows:
* a = The weighted mean parallax includes the parallax of both the primary and
* the secondary components;
* b = The HIP parallax is markedly different from that published in the Yale
* Parallax Catalog (YPC; Also called The General Catalogue of Trigonometric
* Stellar Parallaxes, Fourth Edition, van Altena 1995, cat. I/174) and has
* an error of ~45mas.
*Note (3): The wavelength ranges for the B_J_, R_59F_, and I_IVN_ filters are
* 3950-5400{AA}, 5900-6900{AA}, and 7150-9000{AA}, respectively (Morgan,
* 1995ASPC...84..137M, p137). See Section 3.1 for more details about the
* B_J_R_59F_I_IVN_ plate photometry. The plate R_59F_ magnitude is the
* second, more recent R epoch measurement of the two available in the
* SuperCOSMOS Sky Survey.
*Note (4): Primarily the V_J_, R_KC_, I_KC_ magnitudes measured by REsearch
* Consortium On Nearby Stars (RECONS; http://www.recons.org/) group at Cerro
* Tololo Inter-American Observatory (CTIO) and the number of observations,
* or VRI from a trusted source. The central wavelengths for the V_J_(old),
* V_J_(new), R_KC_, and I_KC_ filters are 5438, 5475, 6425, and 8075{AA},
* respectively. See Jao et al., 2011AJ....141..117J, for a discussion of the
* nearly identical V_J_(old) and V_J_(new) filters. See Section 3.2 for more
* details about the V_J_R_KC_I_KC_ CCD photometry.
*Note (5):
* u = We have previously published photometry for this object, but have since
* then acquired more data and updated the value.
*Note (6): Flag on 2MASS magnitude defined as follows:
* J = Indicates that light from a close companion has resulted in blended
* photometry;
* c = 2MASS magnitude error greater than 0.05mag.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Derived data for southern red dwarf systems
integer*4 nr__1
parameter (nr__1=1748) ! Number of records
character*98 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*14 Name2 (nr__1) ! Name of the M dwarf primary (G1)
integer*4 RAh_1 (nr__1) ! (h) Hour of Right Ascension (J2000)
integer*4 RAm_1 (nr__1) ! (min) Minute of Right Ascension (J2000)
real*4 RAs_1 (nr__1) ! (s) Second of Right Ascension (J2000)
character*1 DE__1 (nr__1) ! Sign of the Declination (J2000)
integer*4 DEd_1 (nr__1) ! (deg) Degree of Declination (J2000)
integer*4 DEm_1 (nr__1) ! (arcmin) Arcminute of Declination (J2000)
integer*4 DEs_1 (nr__1) ! (arcsec) Arcsecond of Declination (J2000)
real*4 dplt (nr__1) ! (pc) ? The plate derived distance (7)
character*3 f_dplt (nr__1) ! Distance closer or further than estimated (8)
real*4 e_dplt (nr__1) ! (pc) ? Total error in dplt
integer*4 o_dplt (nr__1) ! Number of relations used in dplt
real*4 dccd (nr__1) ! (pc) ? The CCD derived distance (9)
character*3 f_dccd (nr__1) ! Distance closer or further than estimated (8)
real*4 e_dccd (nr__1) ! (pc) ? Total error in dccd
integer*4 o_dccd (nr__1) ! ? Number of relations used in dccd
real*4 dtrig (nr__1) ! (pc) ? Distance from weighted mean of published
* parallaxes (see Section 3.4 for details)
character*1 f_dtrig (nr__1) ! [a] Indicates the weighted mean distance
* includes that of both the primary and the
* secondary components
real*4 e_dtrig (nr__1) ! (pc) ? Weighted mean error in dtrig
integer*4 o_dtrig (nr__1) ! ? Number of parallaxes used in dtrig
real*4 dbest (nr__1) ! (pc) [2.7/214] Most reliable distance
character*1 f_dbest (nr__1) ! Distance closer or further than estimated (8)
character*3 n_dbest (nr__1) ! Most reliable distance type (ccd, plt, trg)
*Note (7): Calculated by combining SuperCOSMOS BRI photometry with 2MASS infrared
* photometry via a suite of 15 color-M_K_ relations using BRIJHK, as
* described in Hambly et al. (2004AJ....128..437H). See Secion 4.1 for
* additional details.
*Note (8): The flags on distance are defined as follows:
* c = Confirmed or candidate subdwarf (distance typically closer than estimated);
* f = Distance based on blended photometry (distance typically further than
* estimated).
*Note (9): Determined using a method similar to that used for the plate derived
* distances and as described by Henry et al. (2004AJ....128..437H). The
* difference is that we use more accurate CCD VRI magnitudes obtained at
* Cerro Tololo Inter-American Observatory (CTIO) instead of plate magnitudes
* from SuperCOSMOS to determine the suite of color-M_K_ relations.
* See Secion 4.2 for more details.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'refs.dat' ! References
integer*4 nr__2
parameter (nr__2=74) ! Number of records
character*66 ar__2 ! Full-size record
integer*4 Ref (nr__2) ! Reference identifier
character*19 BibCode (nr__2) ! Bibliographic code
character*21 Aut (nr__2) ! Author's name
character*21 Cat (nr__2) ! Catalog in VizieR database
C=============================================================================
C Loading file 'table1.dat' ! Observed data for southern red dwarf systems
C Format for file interpretation
1 format(
+ A14,1X,I1,1X,I1,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,1X,
+ F5.3,1X,F5.1,1X,I2,1X,F7.2,1X,A2,3X,F4.2,1X,I1,1X,A13,1X,F5.2,
+ A1,1X,F5.2,A1,1X,F5.2,A1,1X,F5.2,A1,1X,F5.2,A1,1X,F5.2,A1,1X,
+ I1,1X,I2,A1,1X,F5.2,A2,1X,F5.2,A2,1X,F5.2,A2)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,1748
read(1,'(A160)')ar__
read(ar__,1)
+ Name(i__),Nc(i__),Np(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
+ DEd(i__),DEm(i__),DEs(i__),pm(i__),pmPA(i__),r_pm(i__),
+ plx(i__),f_plx(i__),e_plx(i__),o_plx(i__),r_plx(i__),
+ Bmag(i__),f_Bmag(i__),Fmag(i__),f_Fmag(i__),Nmag(i__),
+ f_Nmag(i__),Vmag(i__),f_Vmag(i__),Rmag(i__),f_Rmag(i__),
+ Imag(i__),f_Imag(i__),o_Imag(i__),r_Imag(i__),New(i__),
+ Jmag(i__),f_Jmag(i__),Hmag(i__),f_Hmag(i__),Kmag(i__),
+ f_Kmag(i__)
if(ar__(18:18) .EQ. '') Np(i__) = iNULL__
if(ar__(56:62) .EQ. '') plx(i__) = rNULL__
if(ar__(69:72) .EQ. '') e_plx(i__) = rNULL__
if(ar__(74:74) .EQ. '') o_plx(i__) = iNULL__
if(ar__(90:94) .EQ. '') Bmag(i__) = rNULL__
if(ar__(97:101) .EQ. '') Fmag(i__) = rNULL__
if(ar__(104:108) .EQ. '') Nmag(i__) = rNULL__
if(ar__(111:115) .EQ. '') Vmag(i__) = rNULL__
if(ar__(118:122) .EQ. '') Rmag(i__) = rNULL__
if(ar__(125:129) .EQ. '') Imag(i__) = rNULL__
if(ar__(132:132) .EQ. '') o_Imag(i__) = iNULL__
if(ar__(134:135) .EQ. '') r_Imag(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__),Nc(i__),Np(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
+ DEd(i__),DEm(i__),DEs(i__),pm(i__),pmPA(i__),r_pm(i__),
+ plx(i__),f_plx(i__),e_plx(i__),o_plx(i__),r_plx(i__),
+ Bmag(i__),f_Bmag(i__),Fmag(i__),f_Fmag(i__),Nmag(i__),
+ f_Nmag(i__),Vmag(i__),f_Vmag(i__),Rmag(i__),f_Rmag(i__),
+ Imag(i__),f_Imag(i__),o_Imag(i__),r_Imag(i__),New(i__),
+ Jmag(i__),f_Jmag(i__),Hmag(i__),f_Hmag(i__),Kmag(i__),
+ f_Kmag(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 'table2.dat' ! Derived data for southern red dwarf systems
C Format for file interpretation
2 format(
+ A14,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,1X,F5.1,1X,A3,1X,
+ F4.1,1X,I2,1X,F5.1,1X,A3,1X,F4.1,1X,I2,1X,F5.1,1X,A1,1X,F5.1,
+ 1X,I1,1X,F5.1,A1,1X,A3)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,1748
read(1,'(A98)')ar__1
read(ar__1,2)
+ Name2(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),dplt(i__),f_dplt(i__),
+ e_dplt(i__),o_dplt(i__),dccd(i__),f_dccd(i__),e_dccd(i__),
+ o_dccd(i__),dtrig(i__),f_dtrig(i__),e_dtrig(i__),o_dtrig(i__),
+ dbest(i__),f_dbest(i__),n_dbest(i__)
if(ar__1(37:41) .EQ. '') dplt(i__) = rNULL__
if(ar__1(47:50) .EQ. '') e_dplt(i__) = rNULL__
if(ar__1(55:59) .EQ. '') dccd(i__) = rNULL__
if(ar__1(65:68) .EQ. '') e_dccd(i__) = rNULL__
if(ar__1(70:71) .EQ. '') o_dccd(i__) = iNULL__
if(ar__1(73:77) .EQ. '') dtrig(i__) = rNULL__
if(ar__1(81:85) .EQ. '') e_dtrig(i__) = rNULL__
if(ar__1(87:87) .EQ. '') o_dtrig(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)
+ Name2(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),dplt(i__),f_dplt(i__),
+ e_dplt(i__),o_dplt(i__),dccd(i__),f_dccd(i__),e_dccd(i__),
+ o_dccd(i__),dtrig(i__),f_dtrig(i__),e_dtrig(i__),o_dtrig(i__),
+ dbest(i__),f_dbest(i__),n_dbest(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'refs.dat' ! References
C Format for file interpretation
3 format(I2,1X,A19,1X,A21,1X,A21)
C Effective file loading
open(unit=1,status='old',file=
+'refs.dat')
write(6,*) '....Loading file: refs.dat'
do i__=1,74
read(1,'(A66)')ar__2
read(ar__2,3)Ref(i__),BibCode(i__),Aut(i__),Cat(i__)
c ..............Just test output...........
write(6,3)Ref(i__),BibCode(i__),Aut(i__),Cat(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end