Conversion of standardized ReadMe file for
file /./ftp/cats/J/MNRAS/411/705 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-Oct-13
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/411/705 Spectrophotometric distances of HII regions (Moises+, 2011)
*================================================================================
*Spectrophotometric distances to Galactic H II regions.
* Moises A.P., Damineli A., Figueredo E., Blum R.D., Conti P.S., Barbosa C.L.
* <Mon. Not. R. Astron. Soc., 411, 705-760 (2011)>
* =2011MNRAS.411..705M
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Massive YSOs identified using the color-color
and color-magnitude diagrams and with a
counterpart in their respective Spitzer images
integer*4 nr__
parameter (nr__=65) ! Number of records
character*93 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*10 v_MDF2011_ ! Region designation, GLLL.ll+B.bb
character*1 r__MDF2011_ ! [abcde] Reference for the region (1)
character*10 Name ! Other name of the region, or [MDF2011]
integer*4 Cand ! Candidate number,
* [MDF2011] GLLL.ll+B.bb NNNN in Simbad
integer*4 RAh ! (h) Right ascension (J2000)
integer*4 RAm ! (min) Right ascension (J2000)
real*4 RAs ! (s) Right ascension (J2000)
character*1 DE_ ! Declination sign (J2000)
integer*4 DEd ! (deg) Declination (J2000)
integer*4 DEm ! (arcmin) Declination (J2000)
real*4 DEs ! (arcsec) Declination (J2000)
real*4 Ksmag ! (mag) MYSO Ks-band magnitude
real*4 v_3_6_ ! (mag) ? IRAC 3.6um magnitude
integer*4 n__3_6_ ! [1/3]? reason of non-detection in [3.6] (2)
real*4 v_4_5_ ! (mag) ? IRAC 4.5um magnitude
integer*4 n__4_5_ ! [1/3]? reason of non-detection in [4.5] (2)
real*4 v_5_8_ ! (mag) ? IRAC 5.8um magnitude
integer*4 n__5_8_ ! [1/3]? reason of non-detection in [5.8] (2)
real*4 v_8_0_ ! (mag) ? IRAC 8.0um magnitude
integer*4 n__8_0_ ! [1/4]? reason of non-detection in [8.0] (2)
character*4 Class ! Classificiation of the MYSO, when possible
*Note (1): References as follows:
* a = Blum et al. (2001AJ....121.3149B)
* b = Blum et al. (2000AJ....119.1860B
* c = Blum et al. (1999AJ....117.1392B)
* d = Figueredo et al. (2008AJ....136..221F)
* e = Figueredo et al. (2005AJ....129.1523F)
*Note (2): Identification of non-detected objects code as follows:
* 1 = undetected object
* 2 = saturated object
* 3 = strong nebulosity obscurating the object
* 4 = crowded cluster
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Regions with distances derived from the
trigonometric parallax
integer*4 nr__1
parameter (nr__1=19) ! Number of records
character*48 ar__1 ! Full-size record
C Position composed of: GLON GLAT
real*4 GLON ! (deg) Galactic longitude
real*4 GLAT ! (deg) Galactic latitude
character*10 Name_1 ! Name of the HII region
real*4 Dkin ! (kpc) Kinematic distance (1)
real*4 Dplx ! (kpc) Distance derived from the trigonometric parallax
real*4 E_Dplx ! (kpc) Error on Dplx (upper value)
real*4 e_Dplx_1 ! (kpc) Error on Dplx (lower value)
integer*4 r_Dplx ! References for Dplx (2)
*Note (1): Kinematic distance from From Reid et al. (2009ApJ...700..137R)
*Note (2): References for the adopted distance moduli as follows:
* 1 = Reid et al. (2009ApJ...693..397R)
* 2 = Moscadelli et al. (2009ApJ...693..406M)
* 3 = Xu et al. (2009ApJ...693..413X)
* 4 = Zhang et al. (2009ApJ...693..419Z)
* 5 = Brunthaler et al. (2009ApJ...693..424B)
* 6 = Bartkiewicz et al. (2008A&A...490..787B)
* 7 = Moellenbrock, Claussen & Goss (2009ApJ...694..192M)
* 8 = Sato et al. (2008PASJ...60..975S)
* 9 = Xu et al. (2006Sci...311...54X),
* Hachisuka et al. (2006ApJ...645..337H)
* 10 = Hachisuka et al. (2009ApJ...696.1981H)
* 11 = Honma et al. (2007PASJ...59..889H)
* 12 = Hirota et al. (2007PASJ...59..897H),
* Menten et al. (2007A&A...474..515M)
* 13 = Choi et al. (2008PASJ...60.1007C)
* 14 = Reid et al. (2009ApJ...705.1548R)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! Spectrophotometric distances
integer*4 nr__2
parameter (nr__2=27) ! Number of records
character*63 ar__2 ! Full-size record
C Position composed of: GLON GLAT
real*4 GLON_1 ! (deg) Galactic longitude
real*4 GLAT_1 ! (deg) Galactic latitude
character*10 Name_2 ! Name of the HII region
integer*4 r_Dist ! Reference for adopted distance moduli (1)
integer*4 Nstar ! Number of stars used in each region
real*4 Dkin_1 ! (kpc) Kinematic distance (2)
real*4 e_Dkin ! (kpc) rms uncertainty on Dkin
real*4 DM ! (kpc) Spectrophotometric distance using the Mathis
* (1990ARA&A..28...37M) interstellar
* extinction law
real*4 e_DM ! (kpc) rms uncertainty on DM
real*4 DS ! (kpc) Spectrophotometric distance using the
* Stead & Hoare (2009MNRAS.400..731S)
* interstellar extinction law
real*4 e_DS ! (kpc) rms uncertainty on DS
real*4 v_Dspec_ ! (kpc) Average of both spectrophotometric distances
*Note (1): References for the adopted distance moduli as follows:
* 1 = Bik et al. (2005A&A...440..121B)
* 2 = Blum et al. (2001AJ....121.3149B)
* 3 = Hanson et al. (1996, Cat. J/ApJS/107/281)
* 4 = Blum et al. (2000AJ....119.1860B)
* 5 = Blum et al. (1999AJ....117.1392B)
* 6 = Figueredo et al. (2008AJ....136..221F)
* 7 = Navarete et al. (in preparation)
* 8 = Figueredo et al. (2005AJ....129.1523F)
*Note (2): All kinematic distances are from Russeil (2003, Cat. J/A+A/397/133)
* except for W31-South and W31-North with distances from
* Corbel & Eikenberry (2004A&A...419..191C).
C=============================================================================
C Loading file 'table2.dat' ! Massive YSOs identified using the color-color
* and color-magnitude diagrams and with a
* counterpart in their respective Spitzer images
C Format for file interpretation
1 format(
+ A10,A1,1X,A10,I4,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,
+ 1X,F5.2,1X,F5.2,1X,I1,1X,F5.2,1X,I1,1X,F5.2,1X,I1,1X,F4.2,1X,
+ I1,1X,A4)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,65
read(1,'(A93)')ar__
read(ar__,1)
+ v_MDF2011_,r__MDF2011_,Name,Cand,RAh,RAm,RAs,DE_,DEd,DEm,DEs,
+ Ksmag,v_3_6_,n__3_6_,v_4_5_,n__4_5_,v_5_8_,n__5_8_,v_8_0_,
+ n__8_0_,Class
if(ar__(59:63) .EQ. '') v_3_6_ = rNULL__
if(ar__(65:65) .EQ. '') n__3_6_ = iNULL__
if(ar__(67:71) .EQ. '') v_4_5_ = rNULL__
if(ar__(73:73) .EQ. '') n__4_5_ = iNULL__
if(ar__(75:79) .EQ. '') v_5_8_ = rNULL__
if(ar__(81:81) .EQ. '') n__5_8_ = iNULL__
if(ar__(83:86) .EQ. '') v_8_0_ = rNULL__
if(ar__(88:88) .EQ. '') n__8_0_ = 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)
+ v_MDF2011_,r__MDF2011_,Name,Cand,RAh,RAm,RAs,DE_,DEd,DEm,DEs,
+ Ksmag,v_3_6_,n__3_6_,v_4_5_,n__4_5_,v_5_8_,n__5_8_,v_8_0_,
+ n__8_0_,Class
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Regions with distances derived from the
* trigonometric parallax
C Format for file interpretation
2 format(
+ F6.2,1X,F6.2,1X,A10,2X,F4.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,I2)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,19
read(1,'(A48)')ar__1
read(ar__1,2)GLON,GLAT,Name_1,Dkin,Dplx,E_Dplx,e_Dplx_1,r_Dplx
c ..............Just test output...........
write(6,2)GLON,GLAT,Name_1,Dkin,Dplx,E_Dplx,e_Dplx_1,r_Dplx
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4.dat' ! Spectrophotometric distances
C Format for file interpretation
3 format(
+ F5.1,1X,F4.1,1X,A10,1X,I1,1X,I1,1X,F5.2,1X,F3.1,1X,F5.2,1X,
+ F4.2,1X,F5.2,1X,F4.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,27
read(1,'(A63)')ar__2
read(ar__2,3)
+ GLON_1,GLAT_1,Name_2,r_Dist,Nstar,Dkin_1,e_Dkin,DM,e_DM,DS,
+ e_DS,v_Dspec_
c ..............Just test output...........
write(6,3)
+ GLON_1,GLAT_1,Name_2,r_Dist,Nstar,Dkin_1,e_Dkin,DM,e_DM,DS,
+ e_DS,v_Dspec_
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end