Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/125/1711 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-17
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/AJ/125/1711 Broad Absorption Line Quasars from SDSS (Reichard+, 2003)
*================================================================================
*A catalog of Broad Absorption Line Quasars from the
*Sloan Digital Sky Survey Early Data Release.
* Reichard T.A., Richards G.T., Schneider D.P., Hall P.B., Tolea A.,
* Krolik J.H., Tsvetanov Z., Vanden Berk D.E., York D.G., Knapp G.R.,
* Gunn J.E., Brinkmann J.
* <Astron. J. 125, 1711 (2003)>
* =2003AJ....125.1711R
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! SDSS EDR BALQSO Catalog: Objects with 1.7<=z<=4.2
integer*4 nr__
parameter (nr__=185) ! Number of records
character*100 ar__ ! Full-size record
character*18 SDSS (nr__) ! SDSS object name (1)
integer*4 PNum (nr__) ! Plate number
integer*4 FNum (nr__) ! Fiber number
integer*4 MJD (nr__) ! (d) Modified Julian Date of observation
integer*4 Final (nr__) ! [0/1] Final quasar target candidate (2)
integer*4 EDR (nr__) ! [0/1] Early Data Release quasar target
* candidate (2)
integer*4 Ser (nr__) ! [0/1] Early Data Release serendipity target
* candidate (2)
real*4 v20cm (nr__) ! (mJy) ? FIRST peak flux density at 20cm (3)
real*4 z (nr__) ! Redshift
real*4 i_mag (nr__) ! (mag) Apparent i*-band magnitude (4)
real*4 i_Mag_1 (nr__) ! (mag) Resulting absolute i*-band magnitude
integer*4 CIV1 (nr__) ! (km/s) ? C IV balnicity index (5)
integer*4 CIV2 (nr__) ! (km/s) ? C IV balnicity index from Tolea et al.,
* 2002ApJ...578L..31T (6)
integer*4 MgII (nr__) ! (km/s) ? Mg II balnicity index (5)
character*1 C1 (nr__) ! [HN] Fitted composite algorithm
* classification (7)
character*1 C2 (nr__) ! [HN] The Tolea et al., 2002ApJ...578L..31T
* classification (7)
character*6 C3 (nr__) ! Visual classification (8)
character*4 C4 (nr__) ! Overall classification (9)
character*2 Notes (nr__) ! Additional notes (10)
*Note (1): Using the SDSS format of J2000 right ascension (hhmmss.ss) and
* declination ({+/-}ddmmss.s). The "J" prefix should be added.
*Note (2): Final quasar target candidate:
* 1 = Selected;
* 0 = Not selected.
*Note (3): Null value indicates that the object is undetected in the FIRST
* survey at the ~1mJy limit.
*Note (4): Corrected for Galactic reddening using Schlegel, Finkbeiner,
* & Davis, 1998ApJ...500..525S.
*Note (5): Computed using a fitted EDR composite spectrum as the continuum.
*Note (6): Computed using a power law with Gaussian C IV emission line as
* the continuum.
*Note (7): Classification:
* H = HiBAL;
* N = Non-BALQSO.
*Note (8): A question mark means uncertainty in the previous code;
* e.g., ``HiLo?'' means a tentative LoBAL through in a definite HiBAL.
* HiZ = HiBAL at z>=3.90, where LoBALs could be missed because
* {lambda}_AlIII_>9150{AA};
* Hiz/Loz = Hi/LoBAL at z>=2.26, where LoBALs could be missed because
* {lambda}_MgII_>9150{AA};
* Hi = Only high-ionization lines are present;
* Lo = Both high- and low-ionization lines are present;
* LoZ = LoBAL at z>=3.90, where LoBALs could be missed because
* {lambda}_AlIII_>9150{AA};
* FeLo = High-, low-, and metastable Fe II/Fe III lines (~2600{AA},
* or otherwise) or atypical absorption that more readily
* classifies the object as an unusual or extreme BALQSO,
* usually with strong iron absorption;
* no = No broad absorption lines are present (non-BAL).
*Note (9): Overall classification:
* Lo = LoBAL if visual inspection classified the object as a LoBAL;
* FeLo = Visual inspection also revealed a few unusual LoBALs with
* iron absorption (FeLoBALs);
* Hi = The remaining objects are those classified as HiBALs by at
* least one of the three classification methods.
*Note (10): Additional notes:
* e: The balnicity indexes of these objects are formally zero (or
* unmeasured), but visual inspection suggests that the objects
* belong in this table.
* For SDSS 0149-0114 and SDSS 1132+0104 a small change in redshift
* would yield a positive BI.
* In the case of SDSS 1730+5850, Hall et al., 2002ApJS..141..267H
* found a BI greater than 10,900.
* f: See also Hall et al., 2002ApJS..141..267H;
* g: See also Menou et al., 2001ApJ...561..645M;
* h: This quasar was selected for spectroscopic follow-up as a star;
* i: This quasar was selected for spectroscopic follow-up as a galaxy.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Supplementary SDSS EDR BALQSO Catalog
integer*4 nr__1
parameter (nr__1=39) ! Number of records
character*99 ar__1 ! Full-size record
character*18 SDSS_1 (nr__1) ! SDSS object name (1)
integer*4 PNum_1 (nr__1) ! Plate number
integer*4 FNum_1 (nr__1) ! Fiber number
integer*4 MJD_1 (nr__1) ! (d) Modified Julian Date of observation
integer*4 Final_1 (nr__1) ! [0/1] Final quasar target candidate (2)
integer*4 EDR_1 (nr__1) ! [0/1] Early Data Release quasar target
* candidate (2)
integer*4 Ser_1 (nr__1) ! [0/1] Early Data Release serendipity target
* candidate (2)
real*4 v20cm_1 (nr__1) ! (mJy) ? FIRST peak flux density at 20cm (3)
real*4 z_1 (nr__1) ! Redshift
real*4 i_mag_2 (nr__1) ! (mag) Apparent i*-band magnitude (4)
real*4 i_Mag_3 (nr__1) ! (mag) Resulting absolute i*-band magnitude
integer*4 CIV1_1 (nr__1) ! (km/s) ? C IV balnicity index (5)
integer*4 CIV2_1 (nr__1) ! (km/s) ? C IV balnicity index from Tolea et al.,
* 2002ApJ...578L..31T (6)
integer*4 MgII_1 (nr__1) ! (km/s) ? Mg II balnicity index (5)
character*1 C1_1 (nr__1) ! [HN] Fitted composite algorithm
* classification (7)
character*1 C2_1 (nr__1) ! [HN] The Tolea et al., 2002ApJ...578L..31T
* classification (7)
character*6 C3_1 (nr__1) ! Visual classification (8)
character*4 C4_1 (nr__1) ! Overall classification (9)
character*2 Notes_1 (nr__1) ! Additional notes (10)
*Note (1): Using the SDSS format of J2000 right ascension (hhmmss.ss) and
* declination ({+/-}ddmmss.s). The "J" prefix should be added.
*Note (2): Final quasar target candidate:
* 1 = Selected;
* 0 = Not selected.
*Note (3): Null value indicates that the object is undetected in the FIRST
* survey at the ~1mJy limit.
*Note (4): Corrected for Galactic reddening using Schlegel, Finkbeiner,
* & Davis, 1998ApJ...500..525S.
*Note (5): Computed using a fitted EDR composite spectrum as the continuum.
*Note (6): Computed using a power law with Gaussian C IV emission line as
* the continuum.
*Note (7): Classification:
* H = HiBAL;
* N = Non-BALQSO.
*Note (8): A question mark means uncertainty in the previous code;
* e.g., ``HiLo?'' means a tentative LoBAL through in a definite HiBAL.
* HiZ = HiBAL at z>=3.90, where LoBALs could be missed because
* {lambda}_AlIII_>9150{AA};
* Hiz/Loz = Hi/LoBAL at z>=2.26, where LoBALs could be missed because
* {lambda}_MgII_>9150{AA};
* Hi = Only high-ionization lines are present;
* Lo = Both high- and low-ionization lines are present;
* LoZ = LoBAL at z>=3.90, where LoBALs could be missed because
* {lambda}_AlIII_>9150{AA};
* FeLo = High-, low-, and metastable Fe II/Fe III lines (~2600{AA},
* or otherwise) or atypical absorption that more readily
* classifies the object as an unusual or extreme BALQSO,
* usually with strong iron absorption;
* no = No broad absorption lines are present (non-BAL).
*Note (9): Overall classification:
* Lo = LoBAL if visual inspection classified the object as a LoBAL;
* FeLo = Visual inspection also revealed a few unusual LoBALs with
* iron absorption (FeLoBALs);
* Hi = The remaining objects are those classified as HiBALs by at
* least one of the three classification methods.
*Note (10): Additional notes:
* e: The balnicity indexes of these objects are formally zero (or
* unmeasured), but visual inspection suggests that the objects
* belong in this table.
* For SDSS 0149-0114 and SDSS 1132+0104 a small change in redshift
* would yield a positive BI.
* In the case of SDSS 1730+5850, Hall et al., 2002ApJS..141..267H
* found a BI greater than 10,900.
* f: See also Hall et al., 2002ApJS..141..267H;
* g: See also Menou et al., 2001ApJ...561..645M;
* h: This quasar was selected for spectroscopic follow-up as a star;
* i: This quasar was selected for spectroscopic follow-up as a galaxy.
C=============================================================================
C Loading file 'table1.dat' ! SDSS EDR BALQSO Catalog: Objects with 1.7<=z<=4.2
C Format for file interpretation
1 format(
+ A18,1X,I3,1X,I3,1X,I5,1X,I1,1X,I1,1X,I1,1X,F5.2,1X,F5.3,1X,
+ F5.2,1X,F6.2,1X,I5,1X,I5,1X,I4,1X,A1,1X,A1,1X,A6,1X,A4,1X,A2)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,185
read(1,'(A100)')ar__
read(ar__,1)
+ SDSS(i__),PNum(i__),FNum(i__),MJD(i__),Final(i__),EDR(i__),
+ Ser(i__),v20cm(i__),z(i__),i_mag(i__),i_Mag_1(i__),CIV1(i__),
+ CIV2(i__),MgII(i__),C1(i__),C2(i__),C3(i__),C4(i__),Notes(i__)
if(ar__(40:44) .EQ. '') v20cm(i__) = rNULL__
if(ar__(65:69) .EQ. '') CIV1(i__) = iNULL__
if(ar__(71:75) .EQ. '') CIV2(i__) = iNULL__
if(ar__(77:80) .EQ. '') MgII(i__) = iNULL__
c ..............Just test output...........
write(6,1)
+ SDSS(i__),PNum(i__),FNum(i__),MJD(i__),Final(i__),EDR(i__),
+ Ser(i__),v20cm(i__),z(i__),i_mag(i__),i_Mag_1(i__),CIV1(i__),
+ CIV2(i__),MgII(i__),C1(i__),C2(i__),C3(i__),C4(i__),Notes(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Supplementary SDSS EDR BALQSO Catalog
C Format for file interpretation
2 format(
+ A18,1X,I3,1X,I3,1X,I5,1X,I1,1X,I1,1X,I1,1X,F5.2,1X,F5.3,1X,
+ F5.2,1X,F6.2,1X,I5,1X,I5,1X,I4,1X,A1,1X,A1,1X,A6,1X,A4,1X,A2)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,39
read(1,'(A99)')ar__1
read(ar__1,2)
+ SDSS_1(i__),PNum_1(i__),FNum_1(i__),MJD_1(i__),Final_1(i__),
+ EDR_1(i__),Ser_1(i__),v20cm_1(i__),z_1(i__),i_mag_2(i__),
+ i_Mag_3(i__),CIV1_1(i__),CIV2_1(i__),MgII_1(i__),C1_1(i__),
+ C2_1(i__),C3_1(i__),C4_1(i__),Notes_1(i__)
if(ar__1(40:44) .EQ. '') v20cm_1(i__) = rNULL__
if(ar__1(65:69) .EQ. '') CIV1_1(i__) = iNULL__
if(ar__1(71:75) .EQ. '') CIV2_1(i__) = iNULL__
if(ar__1(77:80) .EQ. '') MgII_1(i__) = iNULL__
c ..............Just test output...........
write(6,2)
+ SDSS_1(i__),PNum_1(i__),FNum_1(i__),MJD_1(i__),Final_1(i__),
+ EDR_1(i__),Ser_1(i__),v20cm_1(i__),z_1(i__),i_mag_2(i__),
+ i_Mag_3(i__),CIV1_1(i__),CIV2_1(i__),MgII_1(i__),C1_1(i__),
+ C2_1(i__),C3_1(i__),C4_1(i__),Notes_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end