Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/651/L49 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/ApJ/651/L49 Upper Sco OB association IRAC observations (Carpenter+, 2006)
*================================================================================
*Evidence for mass-dependent circumstellar disk evolution in the 5Myr
*old upper Scorpius OB association.
* Carpenter J.M., Mamajek E.E., Hillenbrand L.A., Meyer M.R.
* <Astrophys. J., 651, L49-L52 (2006)>
* =2006ApJ...651L..49C
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Observed IRAC and IRS Fluxes Source
integer*4 nr__
parameter (nr__=218) ! Number of records
character*120 ar__ ! Full-size record
character*1 Flag ! [ab] a: from this study, b: from FEPS (Meyer
* et al., 2006, Cat. <J/PASP/118/1690>
character*31 Source ! Source name
character*8 SpType ! MK spectral type
character*3 r_SpType ! Reference for spectral type (1)
integer*4 Obs4_5um ! Spitzer observation number for 4.5um
real*8 S4_5um ! (mJy) IRAC 4.5um flux (2)
real*4 e_S4_5um ! (mJy) rms uncertainty on S4.5um
integer*4 Obs8um ! Spitzer observation number for 8um
real*8 S8um ! (mJy) IRAC 8um flux (3)
real*4 e_S8um ! (mJy) rms uncertainty on S8um
character*1 f_S8um ! [s] s for saturated
integer*4 Obs16um ! ? Spitzer observation number for 16um
real*4 S16um ! (mJy) ? IRAC 16um flux (4)
character*1 n_S16um ! [e] Note on S16um (5)
real*4 e_S16um ! (mJy) ? rms uncertainty on S16um
character*1 E8 ! [Y/N] 8um excess?
character*1 E16 ! [Y/N?] 16um excess?
character*1 n_E16 ! [f] Note on E16um (5)
*Note (1): References as follows:
* H82 = Houk, 1982, Cat. <III/80>
* H88 = Houk, 1988, Cat. <III/133>
* K99 = Kunkel, 1999, Ph.D. thesis, Julius-Maximilians-Univ., Wuerzburg
* K00 = Koehler et al., 2000, Cat. <J/A+A/356/541>
* MML = Mamajek, Meyer & Liebert, unpublished
* P98 = Preibisch et al, 1998, Cat. <J/A+A/333/619>
* P01 = Preibisch et al., 2001, Cat. <J/AJ/121/1040>
* P02 = Preibisch et al., 2002, Cat. <J/AJ/124/404>
* W94 = Walter et al., 1994AJ....107..692W
*Note (2): IRAC 4.5um photometry measured using a flux calibration factor of
* 0.1388MJy/sr/(DN/s).
*Note (3): IRAC 8um photometry measured using a flux calibration factor of
* 0.2021MJy/sr/(DN/s).
*Note (4): IRS 16um PUI photometry measured using a flux calibration factor
* of 0.01375MJy/sr/(e^-^/s). Saturated sources are listed as sat.
*Note (5): Note as follows:
* e = Aperture curve of growth deviates from a point source by
* more than 4%
* f = ScoPMS 17 is not considered an excess source for this study
* since the apparent 16 excess is likely from a nearby source
* that falls partially within the measurement aperture.
C=============================================================================
C Loading file 'table1.dat' ! Observed IRAC and IRS Fluxes Source
C Format for file interpretation
1 format(
+ A1,1X,A31,1X,A8,1X,A3,1X,I8,1X,F8.2,F6.2,1X,I8,1X,F7.2,1X,
+ F5.2,A1,I8,1X,F6.2,A1,1X,F4.2,1X,A1,1X,A1,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,218
read(1,'(A120)')ar__
read(ar__,1)
+ Flag,Source,SpType,r_SpType,Obs4_5um,S4_5um,e_S4_5um,Obs8um,
+ S8um,e_S8um,f_S8um,Obs16um,S16um,n_S16um,e_S16um,E8,E16,n_E16
if(ar__(95:102) .EQ. '') Obs16um = iNULL__
if(ar__(104:109) .EQ. '') S16um = rNULL__
if(ar__(112:115) .EQ. '') e_S16um = rNULL__
c ..............Just test output...........
write(6,1)
+ Flag,Source,SpType,r_SpType,Obs4_5um,S4_5um,e_S4_5um,Obs8um,
+ S8um,e_S8um,f_S8um,Obs16um,S16um,n_S16um,e_S16um,E8,E16,n_E16
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end