Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/701/508 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 2024-Apr-16
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/701/508 5000 AGNs behind the Magellanic clouds (Kozlowski+, 2009)
*================================================================================
*Discovery of 5000 active galactic nuclei behind the Magellanic Clouds.
* Kozlowski S., Kochanek C.S.
* <Astrophys. J., 701, 508-513 (2009)>
* =2009ApJ...701..508K
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! AGN candidates behind the Large Magellanic Cloud
integer*4 nr__
parameter (nr__=4699) ! Number of records
character*176 ar__ ! Full-size record
C J2000 position composed of: RAdeg DEdeg
character*20 ID (nr__) ! Source identification (JHHMMSS.ss+DDMMSS.s)
* (see Nomenclature notes)
real*8 RAdeg (nr__) ! (deg) Right Ascension in decimal degrees (J2000)
real*8 DEdeg (nr__) ! (deg) Declination in decimal degrees (J2000)
real*4 v_3_6_ (nr__) ! (mag) ?=99.999 Spitzer/IRAC 3.6 micron band magnitude
real*4 e__3_6_ (nr__) ! (mag) ?=9.999 The 1{sigma} error in 3.6mag
real*4 v_4_5_ (nr__) ! (mag) ?=99.999 Spitzer/IRAC 4.5 micron band magnitude
real*4 e__4_5_ (nr__) ! (mag) ?=9.999 The 1{sigma} error in 4.5mag
real*4 v_5_8_ (nr__) ! (mag) ?=99.999 Spitzer/IRAC 5.8 micron band magnitude
real*4 e__5_8_ (nr__) ! (mag) ?=9.999 The 1{sigma} error in 5.8mag
real*4 v_8_0_ (nr__) ! (mag) ?=99.999 Spitzer/IRAC 8.0 micron band magnitude
real*4 e__8_0_ (nr__) ! (mag) ?=9.999 The 1{sigma} error in 8.0mag
real*4 Vmag (nr__) ! (mag) ?=99.999 V band magnitude
real*4 e_Vmag (nr__) ! (mag) ?=9.999 The 1{sigma} error in Vmag
real*4 Imag (nr__) ! (mag) ?=99.999 I band magnitude
real*4 e_Imag (nr__) ! (mag) ?=9.999 The 1{sigma} error in Imag
character*15 OGLE (nr__) ! OGLE-III identification (smc/lmcFFF.F.NNNNNN;
* <OGLE {L/S}MCFFF.F NNNNNN> in Simbad)
character*6 Type (nr__) ! Source type, from color-magnitude diagrams (1)
real*4 z (nr__) ! ?=-1 Redshift
character*27 r_z (nr__) ! Reference of z (2)
*Note (1): The classification scheme is QSO-[AB][0ab] or YSO-[AB][0ab]
* according to the location in color-magnitude diagrams: A and B for
* IRAC colors/magnitudes, a and b with the I color from OGLE-III;
* 0 means that the source had no optical match (outside the OGLE-III
* regions or too faint). See section 2 of the paper for details.
*Note (2): In table 1, we indicate if the source is a known quasar if it is
* flagged as a "YSO" by Whitney et al. (2008, Cat. J/AJ/136/18), and if
* it is within the 90% confidence radius of a ROSAT source ("HP99",
* Haberl & Pietsch 1999, Cat. J/A+AS/139/277; <[HP99] NNNN> in Simbad).
* We estimate that 30% of the ROSAT identifications will be false
* positives. For the ROSAT sources we indicate the ROSAT catalog number
* using the format HP99_number. In table 2, if it is flagged as a "YSO"
* by Bolatto et al. (2007, Cat. J/ApJ/655/212) and if it is within the
* 90% confidence radius of a ROSAT source (H00, Haberl et al. 2000, Cat.
* J/A+AS/142/41; <[HFP2000] NNN> in Simbad). For the ROSAT sources we
* indicate the ROSAT catalog number using format H00_number. A "-1"
* indicates no existing reference.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! AGN candidates behind the Small Magellanic Cloud
integer*4 nr__1
parameter (nr__1=657) ! Number of records
character*176 ar__1 ! Full-size record
C J2000 position composed of: RAdeg DEdeg
character*20 ID_1 (nr__1) ! Source identification (JHHMMSS.ss+DDMMSS.s)
* (see Nomenclature notes)
real*8 RAdeg_1 (nr__1) ! (deg) Right Ascension in decimal degrees (J2000)
real*8 DEdeg_1 (nr__1) ! (deg) Declination in decimal degrees (J2000)
real*4 v_3_6__1 (nr__1) ! (mag) ?=99.999 Spitzer/IRAC 3.6 micron band magnitude
real*4 e__3_6__1 (nr__1) ! (mag) ?=9.999 The 1{sigma} error in 3.6mag
real*4 v_4_5__1 (nr__1) ! (mag) ?=99.999 Spitzer/IRAC 4.5 micron band magnitude
real*4 e__4_5__1 (nr__1) ! (mag) ?=9.999 The 1{sigma} error in 4.5mag
real*4 v_5_8__1 (nr__1) ! (mag) ?=99.999 Spitzer/IRAC 5.8 micron band magnitude
real*4 e__5_8__1 (nr__1) ! (mag) ?=9.999 The 1{sigma} error in 5.8mag
real*4 v_8_0__1 (nr__1) ! (mag) ?=99.999 Spitzer/IRAC 8.0 micron band magnitude
real*4 e__8_0__1 (nr__1) ! (mag) ?=9.999 The 1{sigma} error in 8.0mag
real*4 Vmag_1 (nr__1) ! (mag) ?=99.999 V band magnitude
real*4 e_Vmag_1 (nr__1) ! (mag) ?=9.999 The 1{sigma} error in Vmag
real*4 Imag_1 (nr__1) ! (mag) ?=99.999 I band magnitude
real*4 e_Imag_1 (nr__1) ! (mag) ?=9.999 The 1{sigma} error in Imag
character*15 OGLE_1 (nr__1) ! OGLE-III identification (smc/lmcFFF.F.NNNNNN;
* <OGLE {L/S}MCFFF.F NNNNNN> in Simbad)
character*6 Type_1 (nr__1) ! Source type, from color-magnitude diagrams (1)
real*4 z_1 (nr__1) ! ?=-1 Redshift
character*27 r_z_1 (nr__1) ! Reference of z (2)
*Note (1): The classification scheme is QSO-[AB][0ab] or YSO-[AB][0ab]
* according to the location in color-magnitude diagrams: A and B for
* IRAC colors/magnitudes, a and b with the I color from OGLE-III;
* 0 means that the source had no optical match (outside the OGLE-III
* regions or too faint). See section 2 of the paper for details.
*Note (2): In table 1, we indicate if the source is a known quasar if it is
* flagged as a "YSO" by Whitney et al. (2008, Cat. J/AJ/136/18), and if
* it is within the 90% confidence radius of a ROSAT source ("HP99",
* Haberl & Pietsch 1999, Cat. J/A+AS/139/277; <[HP99] NNNN> in Simbad).
* We estimate that 30% of the ROSAT identifications will be false
* positives. For the ROSAT sources we indicate the ROSAT catalog number
* using the format HP99_number. In table 2, if it is flagged as a "YSO"
* by Bolatto et al. (2007, Cat. J/ApJ/655/212) and if it is within the
* 90% confidence radius of a ROSAT source (H00, Haberl et al. 2000, Cat.
* J/A+AS/142/41; <[HFP2000] NNN> in Simbad). For the ROSAT sources we
* indicate the ROSAT catalog number using format H00_number. A "-1"
* indicates no existing reference.
C=============================================================================
C Loading file 'table1.dat' ! AGN candidates behind the Large Magellanic Cloud
C Format for file interpretation
1 format(
+ A20,1X,F9.6,1X,F10.6,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3,1X,F6.3,
+ 1X,F5.3,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3,1X,
+ A15,1X,A6,1X,F5.2,1X,A27)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,4699
read(1,'(A176)')ar__
read(ar__,1)
+ ID(i__),RAdeg(i__),DEdeg(i__),v_3_6_(i__),e__3_6_(i__),
+ v_4_5_(i__),e__4_5_(i__),v_5_8_(i__),e__5_8_(i__),v_8_0_(i__),
+ e__8_0_(i__),Vmag(i__),e_Vmag(i__),Imag(i__),e_Imag(i__),
+ OGLE(i__),Type(i__),z(i__),r_z(i__)
c ..............Just test output...........
write(6,1)
+ ID(i__),RAdeg(i__),DEdeg(i__),v_3_6_(i__),e__3_6_(i__),
+ v_4_5_(i__),e__4_5_(i__),v_5_8_(i__),e__5_8_(i__),v_8_0_(i__),
+ e__8_0_(i__),Vmag(i__),e_Vmag(i__),Imag(i__),e_Imag(i__),
+ OGLE(i__),Type(i__),z(i__),r_z(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! AGN candidates behind the Small Magellanic Cloud
C Format for file interpretation
2 format(
+ A20,1X,F9.6,1X,F10.6,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3,1X,F6.3,
+ 1X,F5.3,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3,1X,
+ A15,1X,A6,1X,F5.2,1X,A27)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,657
read(1,'(A176)')ar__1
read(ar__1,2)
+ ID_1(i__),RAdeg_1(i__),DEdeg_1(i__),v_3_6__1(i__),
+ e__3_6__1(i__),v_4_5__1(i__),e__4_5__1(i__),v_5_8__1(i__),
+ e__5_8__1(i__),v_8_0__1(i__),e__8_0__1(i__),Vmag_1(i__),
+ e_Vmag_1(i__),Imag_1(i__),e_Imag_1(i__),OGLE_1(i__),
+ Type_1(i__),z_1(i__),r_z_1(i__)
c ..............Just test output...........
write(6,2)
+ ID_1(i__),RAdeg_1(i__),DEdeg_1(i__),v_3_6__1(i__),
+ e__3_6__1(i__),v_4_5__1(i__),e__4_5__1(i__),v_5_8__1(i__),
+ e__5_8__1(i__),v_8_0__1(i__),e__8_0__1(i__),Vmag_1(i__),
+ e_Vmag_1(i__),Imag_1(i__),e_Imag_1(i__),OGLE_1(i__),
+ Type_1(i__),z_1(i__),r_z_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end