Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/785/159 into FORTRAN code for loading all data files into arrays.
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-09
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/785/159 SONYC census of substellar objects in Lupus 3 (Muzic+, 2014)
*================================================================================
*Substellar objects in nearby young clusters (SONYC).
*VIII. Substellar population in Lupus 3.
* Muzic K., Scholz A., Geers V.C., Jayawardhana R., Lopez Marti B.
* <Astrophys. J., 785, 159 (2014)>
* =2014ApJ...785..159M (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Photometry and Spectral Types for the Objects
of Spectral Type M, or Slightly Earlier,
Identified Toward Lupus 3
integer*4 nr__
parameter (nr__=27) ! Number of records
character*128 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg (nr__) ! (deg) Right Ascension J2000
real*8 DEdeg (nr__) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*4 ID (nr__) ! SONYC candidate identifier (S-NN) (G1)
integer*4 RAh (nr__) ! (h) Hour of Right Ascension (J2000)
integer*4 RAm (nr__) ! (min) Minute of Right Ascension (J2000)
real*4 RAs (nr__) ! (s) Second of Right Ascension (J2000)
character*1 DE_ (nr__) ! Sign of the Declination (J2000)
integer*4 DEd (nr__) ! (deg) Degree of Declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Arcminute of Declination (J2000)
real*4 DEs (nr__) ! (arcsec) Arcsecond of Declination (J2000)
real*4 imag (nr__) ! (mag) MOSAIC-II i-band magnitude
real*4 Jmag (nr__) ! (mag) NEWFIRM J-band magnitude
real*4 Ksmag (nr__) ! (mag) NEWFIRM K_S_-band magnitude
real*4 Av (nr__) ! (mag) Absorption in V band from photometry
character*1 l_SpType (nr__) ! [<] Limit flag on SpType
character*6 SpType (nr__) ! Spectral type
real*4 AvSp (nr__) ! (mag) ? Absorption in V band from spectral type
real*4 pmRA (nr__) ! (mas/yr) ? Proper motion along RA (pmRA*cosDE)
real*4 e_pmRA (nr__) ! (mas/yr) ? Error on pmRA
real*4 pmDE (nr__) ! (mas/yr) ? Proper motion along DE
real*4 e_pmDE (nr__) ! (mas/yr) ? Error on pmDE
character*1 Cand (nr__) ! [yn-] Proper motion candidate (y=yes, n=no)
real*4 EW (nr__) ! (0.1nm) ? Equivalent width of the H{alpha} line
character*9 Memb (nr__) ! Cluster membership
character*1 n_Memb (nr__) ! [2/3] Note on Memb (1)
character*22 Com (nr__) ! Comment (2)
character*3 r_Com (nr__) ! [abcd, ] Comment reference(s) (3)
*Note (1): Note as follows:
* 2 = Background giant;
* 3 = Field dwarf.
*Note (2): Comment as follows:
* C09 = Candidate member in Comeron et al. (2009, J/A+A/500/1045), Table 9;
* M08 = IRAC YSO candidate from Merin et al. (2008, J/ApJS/177/551);
* G06 = X-ray source from Gondoin (2006, J/A+A/454/595).
*Note (3): Reference as follows:
* a = Comeron et al. 2003A&A...406.1001C;
* b = Mortier et al. 2011MNRAS.418.1194M;
* c = Allen et al. 2007ApJ...655.1095A;
* d = Comeron et al. 2013A&A...554A..86C.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Effective Temperature and Extinction Derived
from Models, for the Objects of Spectral Type M
(or Slightly Earlier) Toward Lupus 3
integer*4 nr__1
parameter (nr__1=27) ! Number of records
character*34 ar__1 ! Full-size record
character*4 ID_1 (nr__1) ! SONYC candidate identifier (S-NN) (G1)
character*1 l_TeffAD (nr__1) ! [>] Limit flag on TeffAD
integer*4 TeffAD (nr__1) ! (K) ? Effective temperature derived using
* AMES-Dusty models (Allard et al.
* 2001ApJ...556..357A)
real*4 AvAD (nr__1) ! (mag) ? Absorption in V band corresponding to TeffAD
integer*4 TeffBTS (nr__1) ! (K) Effective temperature derived using
* BT-Settl models (Allard et al.
* 2011ASPC..448...91A)
real*4 AvBTS (nr__1) ! (mag) Absorption in V band corresponding to TeffBTS
integer*4 Teff (nr__1) ! (K) ? Effective temperature
character*1 n_Teff (nr__1) ! [ab] Note on Teff (1)
real*4 Avmean (nr__1) ! (mag) ? Absorption in V band
*Note (1): Note as follows:
* a = Parameters derived by Comeron et al. (2009, J/A+A/500/1045);
* b = Parameters derived by Comeron et al. (2013A&A...554A..86C).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! Spectroscopically Confirmed Very Low Mass
Members of Lupus 3
integer*4 nr__2
parameter (nr__2=82) ! Number of records
character*122 ar__2 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 (nr__2) ! (deg) Right Ascension J2000
real*8 DEdeg_1 (nr__2) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*17 ID_2 (nr__2) ! Member of Lupus 3 identifier (1)
integer*4 RAh_1 (nr__2) ! (h) Hour of Right Ascension (J2000)
integer*4 RAm_1 (nr__2) ! (min) Minute of Right Ascension (J2000)
real*4 RAs_1 (nr__2) ! (s) Second of Right Ascension (J2000)
character*1 DE__1 (nr__2) ! Sign of the Declination (J2000)
integer*4 DEd_1 (nr__2) ! (deg) Degree of Declination (J2000)
integer*4 DEm_1 (nr__2) ! (arcmin) Arcminute of Declination (J2000)
real*4 DEs_1 (nr__2) ! (arcsec) Arcsecond of Declination (J2000)
real*4 Jmag_1 (nr__2) ! (mag) ? J-band magnitude
real*4 Ksmag_1 (nr__2) ! (mag) ? K_S_-band magnitude
character*1 l_SpType1 (nr__2) ! [<] Limit flag on SpType1
character*6 SpType1 (nr__2) ! Spectral type 1
character*3 r_SpType1 (nr__2) ! [acdefgh, ] Spectral type 1 reference(s) (2)
character*4 SpType2 (nr__2) ! Spectral type 2
character*3 r_SpType2 (nr__2) ! [cdfgh, ] Spectral type 2 reference(s) (2)
character*4 SpType3 (nr__2) ! Spectral type 3
character*1 r_SpType3 (nr__2) ! [fgh] Spectral type 3 reference (2)
character*4 SpType4 (nr__2) ! Spectral type 4
character*1 r_SpType4 (nr__2) ! [h] Spectral type 4 reference (2)
integer*4 Teff1 (nr__2) ! (K) ? Effective temperature 1
character*3 r_Teff1 (nr__2) ! [acgh, ] Effective temperature 1 reference(s)
* (2)
integer*4 Teff2 (nr__2) ! (K) ? Effective temperature 2
character*3 r_Teff2 (nr__2) ! [bh, ] Effective temperature 2 reference(s) (2)
integer*4 Teff3 (nr__2) ! (K) ? Effective temperature 3
character*1 r_Teff3 (nr__2) ! [c] Effective temperature 3 reference (2)
character*17 Other (nr__2) ! Other name
character*1 r_Other (nr__2) ! [c] Other name reference (2)
*Note (1): Identifiers are from:
* Schwartz (1977ApJS...35..161S, Sz);
* Comeron et al. (2003A&A...406.1001C, Par-Lup3);
* Lopez Marti et al. (2005A&A...440..139L, Lup);
* Mortier et al. (2011MNRAS.418.1194M, M);
* 2MASS (Cat. II/246, J16)
* this paper (SONYC-Lup3).
*Note (2): Reference as follows:
* a = This work;
* b = Comeron et al. 2009, J/A+A/500/1045;
* c = Comeron et al. 2013A&A...554A..86C;
* d = Comeron et al. 2003A&A...406.1001C;
* e = Allen et al. 2007ApJ...655.1095A;
* f = Hughes et al. 1994AJ....108.1071H;
* g = Mortier et al. 2011MNRAS.418.1194M;
* h = Alcala et al. 2014, J/A+A/561/A2.
C=============================================================================
C Loading file 'table2.dat' ! Photometry and Spectral Types for the Objects
* of Spectral Type M, or Slightly Earlier,
* Identified Toward Lupus 3
C Format for file interpretation
1 format(
+ A4,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F4.1,1X,F4.1,
+ 1X,F4.1,1X,F4.1,1X,A1,A6,1X,F3.1,1X,F5.1,1X,F3.1,1X,F5.1,1X,
+ F3.1,1X,A1,1X,F6.1,1X,A9,1X,A1,1X,A22,1X,A3)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,27
read(1,'(A128)')ar__
read(ar__,1)
+ ID(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),
+ DEs(i__),imag(i__),Jmag(i__),Ksmag(i__),Av(i__),l_SpType(i__),
+ SpType(i__),AvSp(i__),pmRA(i__),e_pmRA(i__),pmDE(i__),
+ e_pmDE(i__),Cand(i__),EW(i__),Memb(i__),n_Memb(i__),Com(i__),
+ r_Com(i__)
if(ar__(58:60) .EQ. '') AvSp(i__) = rNULL__
if(ar__(62:66) .EQ. '') pmRA(i__) = rNULL__
if(ar__(68:70) .EQ. '') e_pmRA(i__) = rNULL__
if(ar__(72:76) .EQ. '') pmDE(i__) = rNULL__
if(ar__(78:80) .EQ. '') e_pmDE(i__) = rNULL__
if(ar__(84:89) .EQ. '') EW(i__) = rNULL__
RAdeg(i__) = rNULL__
DEdeg(i__) = rNULL__
c Derive coordinates RAdeg and DEdeg from input data
c (RAdeg and DEdeg are set to rNULL__ when unknown)
if(RAh(i__) .GT. -180) RAdeg(i__)=RAh(i__)*15.
if(RAm(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAm(i__)/4.
if(RAs(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAs(i__)/240.
if(DEd(i__) .GE. 0) DEdeg(i__)=DEd(i__)
if(DEm(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEm(i__)/60.
if(DEs(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEs(i__)/3600.
if(DE_(i__).EQ.'-'.AND.DEdeg(i__).GE.0) DEdeg(i__)=-DEdeg(i__)
c ..............Just test output...........
write(6,1)
+ ID(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),
+ DEs(i__),imag(i__),Jmag(i__),Ksmag(i__),Av(i__),l_SpType(i__),
+ SpType(i__),AvSp(i__),pmRA(i__),e_pmRA(i__),pmDE(i__),
+ e_pmDE(i__),Cand(i__),EW(i__),Memb(i__),n_Memb(i__),Com(i__),
+ r_Com(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Effective Temperature and Extinction Derived
* from Models, for the Objects of Spectral Type M
* (or Slightly Earlier) Toward Lupus 3
C Format for file interpretation
2 format(A4,1X,A1,I4,1X,F3.1,1X,I4,1X,F3.1,1X,I4,1X,A1,1X,F3.1)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,27
read(1,'(A34)')ar__1
read(ar__1,2)
+ ID_1(i__),l_TeffAD(i__),TeffAD(i__),AvAD(i__),TeffBTS(i__),
+ AvBTS(i__),Teff(i__),n_Teff(i__),Avmean(i__)
if(ar__1(7:10) .EQ. '') TeffAD(i__) = iNULL__
if(ar__1(12:14) .EQ. '') AvAD(i__) = rNULL__
if(ar__1(25:28) .EQ. '') Teff(i__) = iNULL__
if(ar__1(32:34) .EQ. '') Avmean(i__) = rNULL__
c ..............Just test output...........
write(6,2)
+ ID_1(i__),l_TeffAD(i__),TeffAD(i__),AvAD(i__),TeffBTS(i__),
+ AvBTS(i__),Teff(i__),n_Teff(i__),Avmean(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4.dat' ! Spectroscopically Confirmed Very Low Mass
* Members of Lupus 3
C Format for file interpretation
3 format(
+ A17,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F4.1,1X,
+ F4.1,1X,A1,A6,A3,1X,A4,A3,1X,A4,A1,1X,A4,A1,1X,I4,A3,1X,I4,A3,
+ I4,A1,1X,A17,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,82
read(1,'(A122)')ar__2
read(ar__2,3)
+ ID_2(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),Jmag_1(i__),Ksmag_1(i__),
+ l_SpType1(i__),SpType1(i__),r_SpType1(i__),SpType2(i__),
+ r_SpType2(i__),SpType3(i__),r_SpType3(i__),SpType4(i__),
+ r_SpType4(i__),Teff1(i__),r_Teff1(i__),Teff2(i__),
+ r_Teff2(i__),Teff3(i__),r_Teff3(i__),Other(i__),r_Other(i__)
if(ar__2(43:46) .EQ. '') Jmag_1(i__) = rNULL__
if(ar__2(48:51) .EQ. '') Ksmag_1(i__) = rNULL__
if(ar__2(84:87) .EQ. '') Teff1(i__) = iNULL__
if(ar__2(92:95) .EQ. '') Teff2(i__) = iNULL__
if(ar__2(99:102) .EQ. '') Teff3(i__) = iNULL__
RAdeg_1(i__) = rNULL__
DEdeg_1(i__) = 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(i__) .GT. -180) RAdeg_1(i__)=RAh_1(i__)*15.
if(RAm_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAm_1(i__)/4.
if(RAs_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAs_1(i__)/240.
if(DEd_1(i__) .GE. 0) DEdeg_1(i__)=DEd_1(i__)
if(DEm_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEm_1(i__)/60.
if(DEs_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEs_1(i__)/3600.
if(DE__1(i__).EQ.'-'.AND.DEdeg_1(i__).GE.0) DEdeg_1(i__)=-DEdeg_1(i__)
c ..............Just test output...........
write(6,3)
+ ID_2(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),Jmag_1(i__),Ksmag_1(i__),
+ l_SpType1(i__),SpType1(i__),r_SpType1(i__),SpType2(i__),
+ r_SpType2(i__),SpType3(i__),r_SpType3(i__),SpType4(i__),
+ r_SpType4(i__),Teff1(i__),r_Teff1(i__),Teff2(i__),
+ r_Teff2(i__),Teff3(i__),r_Teff3(i__),Other(i__),r_Other(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end