Conversion of standardized ReadMe file for
file /./ftp/cats/J/PASJ/52/631 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-20
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/PASJ/52/631 Galactic plane VERA survey (Honma+, 2000)
*================================================================================
*J-net galactic-plane survey of VLBI radio sources for
*VLBI Exploration of Radio Astrometry (VERA)
* Honma M., Oyama T., Hachisuka K., Sawada-Satoh S., Sebata K., Miyoshi M.,
* Kameya O., Manabe S., Kawaguchi N., Sasao T., Kameno S., Fujisawa K.,
* Shibata K.M., Bushimata T., Miyaji T., Kobayashi H., Inoue M., Imai H.,
* Araki H., Hanada H., Iwadate K., Kaneko Y., Kuji S., Sato K., Tsuruta S.,
* Sakai S., Tamura Y., Horiai K., Hara T., Yokoyama K., Nakajima J.,
* Kawai E., Okubo H., Osaki H., Koyama Y., Sekido M., Suzuyama T.,
* Ichikawa R., Kondo T., Sakai K., Wada K., Harada N., Tougou N.,
* Fujishita M., Shimizu R., Kawaguchi S., Yoshimura A., Nakamura M.,
* Hasegawa W., Morisaki S., Kamohara R., Funaki T., Yamashita N.,
* Watanabe T., Shimoikura T., Nishio M., Omodaka T., Okudaira A.
* <Publ. Astron. Soc. Jap., 52, 631 (2000)>
* =2000PASJ...52..631H
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! List of 284 VLBI source candidates.
integer*4 nr__
parameter (nr__=284) ! Number of records
character*69 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*12 TXS ! Texas source name (TXS HHMM+DDd)
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*4 DEs ! (arcsec) Declination (J2000)
real*4 GLON ! (deg) Galactic longitude
real*4 GLAT ! (deg) Galactic latitude
real*4 S_N ! ? Signal-to-noise ratio with Nobeyama-Kashima
* baseline
integer*4 S22GHz ! (mJy) ? Correlated flux density at 22GHz for
* Nobeyania-Kashinia baseline (1)
character*3 Note ! [IVM ] Note (2)
*Note (1): The correlated flux density was calculated using
* S=[2k{rho}/{eta}_c_]*[(T_sys1_*Tsys2_)/{eta}_e1_{eta}_e2_A1A2)]^1/2^
* where {rho} is the correlation coefficient,
* T_sys_ the system noise temperature,
* A the antenna temperature, {eta}_e_ the antenna efficiency,
* k the Boltzmann constant and {eta}_c_ the sampling efficiency.
*Note (2): Note as follows:
* I = source listed in ICRF catalog (Ma et al., 1998, Cat. <I/251>)
* V = source listed in VLBA calibrator source (Peck & Beasley, 1998,
* in Radio emission from Galactic and Extragalactic Compact
* Sources, IAU Colloquium 646, ASP Conf. Ser. 144, p. 155)
* M = source listed in 2 GHz VLBI survey (Morabito et al.,
* 1986AJ.....91.1038M)
C=============================================================================
C Loading file 'table1.dat' ! List of 284 VLBI source candidates.
C Format for file interpretation
1 format(
+ A12,1X,I2,1X,I2,1X,F7.4,1X,A1,I2,1X,I2,1X,F6.3,1X,F6.2,1X,
+ F6.2,1X,F5.1,1X,I4,1X,A3)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,284
read(1,'(A69)')ar__
read(ar__,1)
+ TXS,RAh,RAm,RAs,DE_,DEd,DEm,DEs,GLON,GLAT,S_N,S22GHz,Note
if(ar__(56:60) .EQ. '') S_N = rNULL__
if(ar__(62:65) .EQ. '') S22GHz = 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)
+ TXS,RAh,RAm,RAs,DE_,DEd,DEm,DEs,GLON,GLAT,S_N,S22GHz,Note
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end