Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/126/1023 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-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/126/1023 White Dwarfs in the SDSS (Harris+, 2003)
*================================================================================
*An initial survey of white dwarfs in the Sloan Digital Sky Survey.
* Harris H.C., Liebert J., Kleinman S.J., Nitta A., Anderson S.F., Knapp G.R.,
* Krzesinski J., Schmidt G., STrauss M.A., Vanden Berk D., Eisenstein D.,
* Hawley S., Margon B., Munn J.A., Silvestri N.M., Smith J.A., Szkody P.,
* Collinge M.J., Dahn C.C., Fan X., Hall P.B., Schneider D.P., Brinkmann J.,
* Burles S., Gunn J.E., Hennessy G.S., Hindsley R., Ivezic Z., Kent S.,
* Lamb D.Q., Lupton R.H., Nichol R.C., Pier J.R., Schlegel D.J., Subbarao M.,
* Uomoto A., Yanny B., York D.G.
* <Astron. J. 126, 1023 (2003)>
* =2003AJ....126.1023H
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! DA and DB white dwarfs
integer*4 nr__
parameter (nr__=249) ! Number of records
character*84 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)
integer*4 RAh ! (h) Hour of right ascension (J2000) (1)
integer*4 RAm ! (min) Minute of right ascension (J2000) (1)
real*4 RAs ! (s) Second of right ascension (J2000) (1)
character*1 DE_ ! Sign of the declination (J2000) (1)
integer*4 DEd ! (deg) Degree of declination (J2000) (1)
integer*4 DEm ! (arcmin) Arcminute of declination (J2000) (1)
real*4 DEs ! (arcsec) Arcsecond of declination (J2000) (1)
real*4 gmag ! (mag) SDSS g-band magnitude
real*4 u_g ! (mag) ? The SDSS (u-g) color
real*4 g_r ! (mag) The SDSS (g-r) color
real*4 r_i ! (mag) The SDSS (r-i) color
real*4 i_z ! (mag) The SDSS (i-z) color
real*4 Au ! (mag) Full SDSS u-band interstellar absorption (2)
character*1 l_pm ! [<~] Limit or approximate flag on PM
integer*4 pm ! (mas/yr) Total proper motion (3)
integer*4 pmPA ! (deg) ? Position angle of the proper motion
character*7 SpType ! Spectral type (4)
character*5 Note ! Individual notes, detailed in file notes.dat
*Note (1): Object name is "SDSS J+" plus the coordinates.
*Note (2): From Schlegel et al. (1998ApJ...500..525S).
* Reddening can be calculated using E(u-g)=0.264Au, E(g-r)=0.202Au,
* E(r-i)=0.129Au, and E(i-z)=0.119Au. For most stars at these high
* latitudes, the reddening is small whether or not the full absorption
*Note (3): Calculated using the USNO-A2.0 catalog (Monet et al., Cat. <I/252>)
* for the first-epoch position. For a few stars not in the USNO-A
* catalog, usually because they are too faint to be detected on both the
* POSS-I blue and red plates, the first-epoch position is taken from the
* USNO-B1.0 catalog (Monet et al., 2003, Cat. <I/284>). The proper
* motions typically have errors of 6-8mas/yr rms. Where the motion is
* less than 20mas/yr, it may not be real, and the position angle of the
* motion is omitted.
*Note (4): From our classification of the SDSS spectra.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Unusual white dwarfs
integer*4 nr__1
parameter (nr__1=69) ! Number of records
character*84 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)
integer*4 RAh_1 ! (h) Hour of right ascension (J2000) (1)
integer*4 RAm_1 ! (min) Minute of right ascension (J2000) (1)
real*4 RAs_1 ! (s) Second of right ascension (J2000) (1)
character*1 DE__1 ! Sign of the declination (J2000) (1)
integer*4 DEd_1 ! (deg) Degree of declination (J2000) (1)
integer*4 DEm_1 ! (arcmin) Arcminute of declination (J2000) (1)
real*4 DEs_1 ! (arcsec) Arcsecond of declination (J2000) (1)
real*4 gmag_1 ! (mag) SDSS g-band magnitude
real*4 u_g_1 ! (mag) ? The SDSS (u-g) color
real*4 g_r_1 ! (mag) The SDSS (g-r) color
real*4 r_i_1 ! (mag) The SDSS (r-i) color
real*4 i_z_1 ! (mag) The SDSS (i-z) color
real*4 Au_1 ! (mag) Full SDSS u-band interstellar absorption (2)
character*1 l_pm_1 ! [<~] Limit or approximate flag on PM
integer*4 pm_1 ! (mas/yr) Total proper motion (3)
integer*4 pmPA_1 ! (deg) ? Position angle of the proper motion
character*7 SpType_1 ! Spectral type (4)
character*5 Note_1 ! Individual notes, detailed in file notes.dat
*Note (1): Object name is "SDSS J+" plus the coordinates.
*Note (2): From Schlegel et al. (1998ApJ...500..525S).
* Reddening can be calculated using E(u-g)=0.264Au, E(g-r)=0.202Au,
* E(r-i)=0.129Au, and E(i-z)=0.119Au. For most stars at these high
* latitudes, the reddening is small whether or not the full absorption
*Note (3): Calculated using the USNO-A2.0 catalog (Monet et al., Cat. <I/252>)
* for the first-epoch position. For a few stars not in the USNO-A
* catalog, usually because they are too faint to be detected on both the
* POSS-I blue and red plates, the first-epoch position is taken from the
* USNO-B1.0 catalog (Monet et al., 2003, Cat. <I/284>). The proper
* motions typically have errors of 6-8mas/yr rms. Where the motion is
* less than 20mas/yr, it may not be real, and the position angle of the
* motion is omitted.
*Note (4): From our classification of the SDSS spectra.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Hot subdwarfs
integer*4 nr__2
parameter (nr__2=56) ! Number of records
character*84 ar__2 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_2 ! (deg) Right Ascension J2000
real*8 DEdeg_2 ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 RAh_2 ! (h) Hour of right ascension (J2000) (1)
integer*4 RAm_2 ! (min) Minute of right ascension (J2000) (1)
real*4 RAs_2 ! (s) Second of right ascension (J2000) (1)
character*1 DE__2 ! Sign of the declination (J2000) (1)
integer*4 DEd_2 ! (deg) Degree of declination (J2000) (1)
integer*4 DEm_2 ! (arcmin) Arcminute of declination (J2000) (1)
real*4 DEs_2 ! (arcsec) Arcsecond of declination (J2000) (1)
real*4 gmag_2 ! (mag) SDSS g-band magnitude
real*4 u_g_2 ! (mag) ? The SDSS (u-g) color
real*4 g_r_2 ! (mag) The SDSS (g-r) color
real*4 r_i_2 ! (mag) The SDSS (r-i) color
real*4 i_z_2 ! (mag) The SDSS (i-z) color
real*4 Au_2 ! (mag) Full SDSS u-band interstellar absorption (2)
character*1 l_pm_2 ! [<~] Limit or approximate flag on PM
integer*4 pm_2 ! (mas/yr) Total proper motion (3)
integer*4 pmPA_2 ! (deg) ? Position angle of the proper motion
character*7 SpType_2 ! Spectral type (4)
character*5 Note_2 ! Individual notes, detailed in file notes.dat
*Note (1): Object name is "SDSS J+" plus the coordinates.
*Note (2): From Schlegel et al. (1998ApJ...500..525S).
* Reddening can be calculated using E(u-g)=0.264Au, E(g-r)=0.202Au,
* E(r-i)=0.129Au, and E(i-z)=0.119Au. For most stars at these high
* latitudes, the reddening is small whether or not the full absorption
*Note (3): Calculated using the USNO-A2.0 catalog (Monet et al., Cat. <I/252>)
* for the first-epoch position. For a few stars not in the USNO-A
* catalog, usually because they are too faint to be detected on both the
* POSS-I blue and red plates, the first-epoch position is taken from the
* USNO-B1.0 catalog (Monet et al., 2003, Cat. <I/284>). The proper
* motions typically have errors of 6-8mas/yr rms. Where the motion is
* less than 20mas/yr, it may not be real, and the position angle of the
* motion is omitted.
*Note (4): From our classification of the SDSS spectra.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'notes.dat' ! Notes on tables 1, 2, 3
integer*4 nr__3
parameter (nr__3=46) ! Number of records
character*81 ar__3 ! Full-size record
integer*4 Note_3 ! Note number (1-24 in table 1, 30-47 in table2,
* 46- 51 in table3)
character*76 Text ! Text of the note
C=============================================================================
C Loading file 'table1.dat' ! DA and DB white dwarfs
C Format for file interpretation
1 format(
+ I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F5.2,1X,F5.2,1X,
+ F5.2,1X,F5.2,1X,F5.2,1X,F4.2,1X,A1,3X,I3,1X,I3,1X,A7,1X,A5)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,249
read(1,'(A84)')ar__
read(ar__,1)
+ RAh,RAm,RAs,DE_,DEd,DEm,DEs,gmag,u_g,g_r,r_i,i_z,Au,l_pm,pm,
+ pmPA,SpType,Note
if(ar__(31:35) .EQ. '') u_g = rNULL__
if(ar__(68:70) .EQ. '') pmPA = iNULL__
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)
+ RAh,RAm,RAs,DE_,DEd,DEm,DEs,gmag,u_g,g_r,r_i,i_z,Au,l_pm,pm,
+ pmPA,SpType,Note
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Unusual white dwarfs
C Format for file interpretation
2 format(
+ I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F5.2,1X,F5.2,1X,
+ F5.2,1X,F5.2,1X,F5.2,1X,F4.2,1X,A1,3X,I3,1X,I3,1X,A7,1X,A5)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,69
read(1,'(A84)')ar__1
read(ar__1,2)
+ RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,gmag_1,u_g_1,g_r_1,
+ r_i_1,i_z_1,Au_1,l_pm_1,pm_1,pmPA_1,SpType_1,Note_1
if(ar__1(31:35) .EQ. '') u_g_1 = rNULL__
if(ar__1(68:70) .EQ. '') pmPA_1 = iNULL__
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)
+ RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,gmag_1,u_g_1,g_r_1,
+ r_i_1,i_z_1,Au_1,l_pm_1,pm_1,pmPA_1,SpType_1,Note_1
write(6,'(6H Pos: 2F8.4)') RAdeg_1,DEdeg_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Hot subdwarfs
C Format for file interpretation
3 format(
+ I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F5.2,1X,F5.2,1X,
+ F5.2,1X,F5.2,1X,F5.2,1X,F4.2,1X,A1,3X,I3,1X,I3,1X,A7,1X,A5)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,56
read(1,'(A84)')ar__2
read(ar__2,3)
+ RAh_2,RAm_2,RAs_2,DE__2,DEd_2,DEm_2,DEs_2,gmag_2,u_g_2,g_r_2,
+ r_i_2,i_z_2,Au_2,l_pm_2,pm_2,pmPA_2,SpType_2,Note_2
if(ar__2(31:35) .EQ. '') u_g_2 = rNULL__
if(ar__2(68:70) .EQ. '') pmPA_2 = iNULL__
RAdeg_2 = rNULL__
DEdeg_2 = rNULL__
c Derive coordinates RAdeg_2 and DEdeg_2 from input data
c (RAdeg_2 and DEdeg_2 are set to rNULL__ when unknown)
if(RAh_2 .GT. -180) RAdeg_2=RAh_2*15.
if(RAm_2 .GT. -180) RAdeg_2=RAdeg_2+RAm_2/4.
if(RAs_2 .GT. -180) RAdeg_2=RAdeg_2+RAs_2/240.
if(DEd_2 .GE. 0) DEdeg_2=DEd_2
if(DEm_2 .GE. 0) DEdeg_2=DEdeg_2+DEm_2/60.
if(DEs_2 .GE. 0) DEdeg_2=DEdeg_2+DEs_2/3600.
if(DE__2.EQ.'-'.AND.DEdeg_2.GE.0) DEdeg_2=-DEdeg_2
c ..............Just test output...........
write(6,3)
+ RAh_2,RAm_2,RAs_2,DE__2,DEd_2,DEm_2,DEs_2,gmag_2,u_g_2,g_r_2,
+ r_i_2,i_z_2,Au_2,l_pm_2,pm_2,pmPA_2,SpType_2,Note_2
write(6,'(6H Pos: 2F8.4)') RAdeg_2,DEdeg_2
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'notes.dat' ! Notes on tables 1, 2, 3
C Format for file interpretation
4 format(I2,3X,A76)
C Effective file loading
open(unit=1,status='old',file=
+'notes.dat')
write(6,*) '....Loading file: notes.dat'
do i__=1,46
read(1,'(A81)')ar__3
read(ar__3,4)Note_3,Text
c ..............Just test output...........
write(6,4)Note_3,Text
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end