Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/675/1319 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-Jul-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/ApJ/675/1319 Infrared photometry of NGC 3603 (Harayama+, 2008)
*================================================================================
*The initial mass function of the massive star-forming region NGC 3603 from
*near-infrared adaptive optics observations.
* Harayama Y., Eisenhauer F., Martins F.
* <Astrophys. J., 675, 1319-1342 (2008)>
* =2008ApJ...675.1319H
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6.dat' ! Photometry list
integer*4 nr__
parameter (nr__=256) ! Number of records
character*88 ar__ ! Full-size record
integer*4 No ! [1/256] Running identification number
* <[HEM2008] NNN> in Simbad
real*4 oRA ! (arcsec) Offset in Right Ascension (1)
real*4 oDE ! (arcsec) Offset in Declination (1)
real*4 Jmag ! (mag) J band magnitude
real*4 Hmag ! (mag) H band magnitude
real*4 Ksmag ! (mag) K_S_ band magnitude
real*4 L_mag ! (mag) ? L' band magnitude (2)
character*11 SpType ! MK spectral type (3)
character*1 f_MDS94 ! [H] H indicates that source is found to have a
* X-ray counterpart by Moffat et al.
* (2002ApJ...573..191M)
integer*4 MDS94 ! ? Identification in Moffat et al.
* (1994ApJ...436..183M) (4)
character*9 OName ! Other names (5)
character*6 Rem ! Remarks on Moffat names (6)
character*2 NS03 ! Identification in Nurnberger & Stanke
* (2003A&A...400..223N) (7)
character*2 n_NS03 ! Note on NS03 (8)
integer*4 SB04 ! ? Identification in Sung & Bessel
* (2004, Cat. <J/AJ/127/1014>) (9)
character*2 n_SB04 ! "e1" indicates that Stars 21 and 52 together
* would correspond to 10207
*Note (1): Source location is shown in an offset from the center of the
* cluster (J2000): 11:15:07.337-61:15:38.19
* (instead of 11:15:05.90-61:15:28.4 as indicated in the paper)
*Note (2): Note that, since the photometric calibration of the L' band
* photometry was done by merely one data set of a standard star,
* the presented L' band magnitude has to be considered as a
* roughly-calibrated photometry.
*Note (3): Adopted from a list in Crowther & Dessart (1998MNRAS.296..622C)
* (Tab. 8 therein) which consists of spectra types in their study
* combined with those in Moffat (1983A&A...124..273M) and Drissen et al.
* (1995AJ....110.2235D).
*Note (4): Designated IDs of potential counterparts in HST optical
* detections by Moffat et al. (1994ApJ...436..183M), named
* <Cl* NGC 3603 MDS NN> in Simbad.
*Note (5): IDs originated in previous works such as Melnick et al.
* (1989A&A...213...89M); letters were adopted from tables in Moffat
* et al. (1994ApJ...436..183M). The letters A-F were originated in
* van den Bos (1928BAN.....4..261V) (G in Walborn 1973ApJ...182L..21W),
* and the source A was resolved into A1-3 by Hofmann & Weigelt
* (1986A&A...167L..15H).
*Note (6): Notes as follows:
* c1 = Star 19 and 45 together would correspond to MDS-61 (G/MTT-10)
* c2 = Star 55 and 57 together would correspond to MDS-67 (MTT-36)
* c3 = Multiple detections. MDS-58 and 62 correspond to MTT-15
* c4 = MDS-8 and 9 correspond to MTT-21
* c5 = MDS-49, 50, 52, and 53 correspond to D
* c6 = MDS-68 and 69 correspond to MTT-44
* c7 = MDS-10 and 11 correspond to MTT-22
* c8 = MDS-12 and 13 correspond to MTT-30
* c9 = A1, A2, and A3 together consist of a X-ray source within the
* match of smoothed PSF in Moffat et al. (2002ApJ...573..191M)
* c10 = MDS-49 and 50 together consist of a X-ray source
*Note (7): Designated IDs of potential counterparts in a mid-infrared
* detections by Nurnberger & Stanke (2003A&A...400..223N, [NS2003] NNA
* in Simbad). The 11.9 micron sources 6A-F are in the concentrated
* cluster core.
*Note (8): Notes as follows:
* d1 = Star 19, 33 and 51 together would correspond to 6G
* d2 = Star 18 and 43 together would correspond to 6K
* d3 = Star 17 and 22 together would correspond to 6N
*Note (9): IDs in Sung & Bessell (2004, Cat. <J/AJ/127/1014>, [SB2004] NNNNN
* in Simbad) (Tab. 2 therein). Sources brighter than V=14mag detected in
* their analysis of the HST/PC1 archival data set.
C=============================================================================
C Loading file 'table6.dat' ! Photometry list
C Format for file interpretation
1 format(
+ I3,1X,F6.2,1X,F6.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,A11,1X,
+ A1,I2,A9,1X,A6,1X,A2,1X,A2,1X,I5,1X,A2)
C Effective file loading
open(unit=1,status='old',file=
+'table6.dat')
write(6,*) '....Loading file: table6.dat'
do i__=1,256
read(1,'(A88)')ar__
read(ar__,1)
+ No,oRA,oDE,Jmag,Hmag,Ksmag,L_mag,SpType,f_MDS94,MDS94,OName,
+ Rem,NS03,n_NS03,SB04,n_SB04
if(ar__(37:41) .EQ. '') L_mag = rNULL__
if(ar__(56:57) .EQ. '') MDS94 = iNULL__
if(ar__(81:85) .EQ. '') SB04 = iNULL__
c ..............Just test output...........
write(6,1)
+ No,oRA,oDE,Jmag,Hmag,Ksmag,L_mag,SpType,f_MDS94,MDS94,OName,
+ Rem,NS03,n_NS03,SB04,n_SB04
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end