Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJS/129/435 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-Aug-15
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/ApJS/129/435 NORAS galaxy cluster survey. I. (Bohringer+, 2000)
*================================================================================
*The northern ROSAT all-sky (NORAS) galaxy cluster survey. I.
*X-ray properties of clusters detected as extended X-ray sources.
* Bohringer H., Voges W., Huchra J.P., McLean B., Giacconi R., Rosati P.,
* Burg R., Mader J., Schuecker P., Simic D., Komossa S., Reiprich T.H.,
* Retzlaff J., Trumper J.
* <Astrophys. J. Suppl. Ser. 129, 435 (2000)>
* =2000ApJS..129..435B
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! The NORAS Cluster X-Ray Source Catalog
integer*4 nr__
parameter (nr__=378) ! Number of records
character*110 ar__ ! Full-size record
C J2000.0 position composed of: RAdeg DEdeg
character*16 RXC (nr__) ! RXC designation (based on J2000 position)
character*15 Name (nr__) ! Alternative name
character*2 n_Name (nr__) ! Note on Name (1)
real*8 RAdeg (nr__) ! (deg) Right ascension (J2000.0)
real*8 DEdeg (nr__) ! (deg) Declination (J2000.0)
real*4 z (nr__) ! Redshift
real*4 CR (nr__) ! (ct/s) Count rate
real*4 FX (nr__) ! (10-15W/m2) X-ray flux
real*4 FX_ (nr__) ! (10-15W/m2) Corrrected X-ray flux
real*4 Error (nr__) ! (%) Factional uncertainty for the count rate,
* the fluxes, and the luminosity
real*4 LX (nr__) ! (10+37W) Rest-frame X-ray luminosity of the clusters
* in the 0.1-2.4keV energy band (10+44erg/s)
real*4 NH (nr__) ! (10+20cm-2) Absorbing column density in the line of
* sight to the source
character*3 ID (nr__) ! Identification flag (2)
character*9 r_z (nr__) ! Redshift reference (separated by commas)
* in refs.dat file
*Note (1): Individual notes are the following:
* a = See also Bade et al., 1998A&AS..127..145B
* b = See also Ebeling et al., 1998MNRAS.301..881E
* c = Barton et al., 1996AJ....112..871B
* d = Crawford et al., 1995MNRAS.274...75C
* e = Cooray et al., 1998AJ....115.1388C
* f = Struble & Rood, 1991ApJ...374..395S
* g = See also Tucker et al., 1995ApJ...444..532T
* h = Appenzeller et al., 1998ApJS..117..319A
* i = Wegner et al., 1996ApJS..106....1W
*Note (2): Identification flag:
* ?: if the identification as a cluster leaves some residual doubts
* B: sources that have been deblended
* L: sources that have been analyzed in extra large fields
* C: sources that may be contaminated
* For the position we have used the coordinates determined by the
* moment method with a 3' aperture radius. As an exception, in the
* case of 12 cluster sources we have either chosen to redetermine the
* center position by a moment method with a larger aperture of 5' or
* 7.5' or determined a center position by hand. In these sources the
* automatic detection has selected a maximum that is significantly
* offset from the global center of symmetry of the clusters.
* b: 5' moment method
* c: 7.5' moment method
* o: determination by eye
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! The Noncluster X-Ray Sources among the Extended
RASS 1 Sources
integer*4 nr__1
parameter (nr__1=99) ! Number of records
character*101 ar__1 ! Full-size record
C J2000.0 position composed of: RAdeg DEdeg
character*15 RXJ (nr__1) ! RXJ designation (based on J2000 position)
character*7 Name_1 (nr__1) ! Alternative name
real*8 RAdeg_1 (nr__1) ! (deg) Right ascension (J2000.0)
real*8 DEdeg_1 (nr__1) ! (deg) Declination (J2000.0)
real*4 CR_1 (nr__1) ! (ct/s) Count rate
real*4 FX_1 (nr__1) ! (10-15W/m2) X-ray flux (in 10^-12^erg/s/cm^2^)
real*4 FX__1 (nr__1) ! (10-15W/m2) Corrected X-ray flux
real*4 Error_1 (nr__1) ! (%) Factional uncertainty for the count rate,
* the fluxes, and the luminosity
real*4 Pext (nr__1) ! (%) Extent parameter from the K-S test (1)
real*4 Rc (nr__1) ! (arcmin) Best -fitting core radius
real*4 Rmin (nr__1) ! (arcmin) Minimal radius value consistent with
* the 2{sigma} uncertainty limit
real*4 HR (nr__1) ! Hardness ratio
real*4 e_HR (nr__1) ! rms uncertainty on HR
real*4 DHR (nr__1) ! Deviation from the expected value of HR
* in units of {sigma}
real*4 NH_1 (nr__1) ! (10+20cm-2) Interstellar H I column density
character*1 ID_1 (nr__1) ! [cob] Alternative center determination flag (2)
*Note (1): Probability result of the Kolmogorov-Smirnov test for the source
* to be a point source. For very low probabilities for the consistency
* with a point source the parameter Pext was limited to a value of 30
* for the entry in the table. A source is considered very likely to be
* extended if this parameter has at least a value of 2 (point source
* excluded with 99% probability).
*Note (2): Alternative center determination:
* b: 5' moment method
* c: 7.5' moment method
* o: determination by eye
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! The AGNs in Clusters and Noncluster Sources in the
Line of Sight with Probable Clusters
integer*4 nr__2
parameter (nr__2=18) ! Number of records
character*101 ar__2 ! Full-size record
C J2000.0 position composed of: RAdeg DEdeg
character*15 RXJ_1 (nr__2) ! RXJ designation (based on J2000 position)
character*7 Name_2 (nr__2) ! Alternative name
real*8 RAdeg_2 (nr__2) ! (deg) Right ascension (J2000.0)
real*8 DEdeg_2 (nr__2) ! (deg) Declination (J2000.0)
real*4 CR_2 (nr__2) ! (ct/s) Count rate
real*4 FX_2 (nr__2) ! (10-15W/m2) X-ray flux (in 10^-12^erg/s/cm^2^)
real*4 FX__2 (nr__2) ! (10-15W/m2) Corrected X-ray flux
real*4 Error_2 (nr__2) ! (%) Factional uncertainty for the count rate,
* the fluxes, and the luminosity
real*4 Pext_1 (nr__2) ! (%) Extent parameter from the K-S test (1)
real*4 Rc_1 (nr__2) ! (arcmin) Best -fitting core radius
real*4 Rmin_1 (nr__2) ! (arcmin) Minimal radius value consistent with
* the 2{sigma} uncertainty limit
real*4 HR_1 (nr__2) ! Hardness ratio
real*4 e_HR_1 (nr__2) ! rms uncertainty on HR
real*4 DHR_1 (nr__2) ! Deviation from the expected value of HR
* in units of {sigma}
real*4 NH_2 (nr__2) ! (10+20cm-2) Interstellar H I column density
character*1 ID_2 (nr__2) ! [cob] Alternative center determination flag (2)
*Note (1): Probability result of the Kolmogorov-Smirnov test for the source
* to be a point source. For very low probabilities for the consistency
* with a point source the parameter Pext was limited to a value of 30
* for the entry in the table. A source is considered very likely to be
* extended if this parameter has at least a value of 2 (point source
* excluded with 99% probability).
*Note (2): Alternative center determination:
* b: 5' moment method
* c: 7.5' moment method
* o: determination by eye
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! X-Ray Properties of the Noncluster X-Ray Source
Cluster Combinations
integer*4 nr__3
parameter (nr__3=18) ! Number of records
character*64 ar__3 ! Full-size record
character*15 RXJ_2 (nr__3) ! RXJ designation (based on J2000 position)
real*4 z_1 (nr__3) ! ? Redshift of AGN
character*41 Com (nr__3) ! Comments
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! X-Ray Properties of the NORAS Cluster X-Ray Source
integer*4 nr__4
parameter (nr__4=378) ! Number of records
character*62 ar__4 ! Full-size record
character*16 RXC_1 (nr__4) ! RXC designation (based on J2000 position)
real*4 LX_1 (nr__4) ! (10+37W) Rest-frame ROSAT-band X-ray luminosity
real*4 RXang (nr__4) ! (arcmin) Radius out to which the source count rate has
* been integrated, in arcmin
real*4 RXMpc (nr__4) ! (Mpc) Radius out to which the source count rate has
* been integrated, in Mpc
real*4 Pext_2 (nr__4) ! (%) Extent parameter from the K-S test (1)
real*4 Rc_2 (nr__4) ! (arcmin) Best -fitting core radius
real*4 Rmin_2 (nr__4) ! (arcmin) Minimal radius value consistent with
* the 2{sigma} uncertainty limit
real*4 HR_2 (nr__4) ! Hardness ratio
real*4 e_HR_2 (nr__4) ! rms uncertainty on HR
real*4 DHR_2 (nr__4) ! Deviation from the expected value of HR
* in units of {sigma}
*Note (1): Probability result of the Kolmogorov-Smirnov test for the source
* to be a point source. For very low probabilities for the consistency
* with a point source the parameter Pext was limited to a value of 30
* for the entry in the table. A source is considered very likely to be
* extended if this parameter has at least a value of 2 (point source
* excluded with 99% probability).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6.dat' ! Additional ACO89 (Cat. <VII/110>) Clusters
Detected as X-Ray Sources in the 9h-14h Region
integer*4 nr__5
parameter (nr__5=85) ! Number of records
character*110 ar__5 ! Full-size record
C J2000.0 position composed of: RAdeg DEdeg
character*16 RXC_2 (nr__5) ! RXC designation (based on J2000 position)
character*15 Name_3 (nr__5) ! Alternative name
character*2 n_Name_1 (nr__5) ! Note on Name (1)
real*8 RAdeg_3 (nr__5) ! (deg) Right ascension (J2000.0)
real*8 DEdeg_3 (nr__5) ! (deg) Declination (J2000.0)
real*4 z_2 (nr__5) ! Redshift
real*4 CR_3 (nr__5) ! (ct/s) Count rate
real*4 FX_3 (nr__5) ! (10-15W/m2) X-ray flux
real*4 FX__3 (nr__5) ! (10-15W/m2) Corrrected X-ray flux
real*4 Error_3 (nr__5) ! (%) Factional uncertainty for the count rate,
* the fluxes, and the luminosity
real*4 LX_2 (nr__5) ! (10+37W) Rest-frame X-ray luminosity of the clusters
* in the 0.1-2.4keV energy band (10+44erg/s)
real*4 NH_3 (nr__5) ! (10+20cm-2) Absorbing column density in the line of
* sight to the source
character*3 ID_3 (nr__5) ! Identification flag (2)
character*9 r_z_1 (nr__5) ! Redshift reference (separated by commas)
* in refs.dat file
*Note (1): Individual notes are the following:
* a = See also Bade et al., 1998A&AS..127..145B
* b = See also Ebeling et al., 1998MNRAS.301..881E
* c = Barton et al., 1996AJ....112..871B
* d = Crawford et al., 1995MNRAS.274...75C
* e = Cooray et al., 1998AJ....115.1388C
* f = Struble & Rood, 1991ApJ...374..395S
* g = See also Tucker et al., 1995ApJ...444..532T
* h = Appenzeller et al., 1998ApJS..117..319A
* i = Wegner et al., 1996ApJS..106....1W
*Note (2): Identification flag:
* ?: if the identification as a cluster leaves some residual doubts
* B: sources that have been deblended
* L: sources that have been analyzed in extra large fields
* C: sources that may be contaminated
* For the position we have used the coordinates determined by the
* moment method with a 3' aperture radius. As an exception, in the
* case of 12 cluster sources we have either chosen to redetermine the
* center position by a moment method with a larger aperture of 5' or
* 7.5' or determined a center position by hand. In these sources the
* automatic detection has selected a maximum that is significantly
* offset from the global center of symmetry of the clusters.
* b: 5' moment method
* c: 7.5' moment method
* o: determination by eye
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table7.dat' ! X-Ray Properties of the Additionally Found ACO89
Clusters
integer*4 nr__6
parameter (nr__6=84) ! Number of records
character*62 ar__6 ! Full-size record
character*16 RXC_3 (nr__6) ! RXC designation (based on J2000 position)
real*4 LX_3 (nr__6) ! (10+37W) Rest-frame ROSAT-band X-ray luminosity
real*4 RXang_1 (nr__6) ! (arcmin) Radius out to which the source count rate has
* been integrated, in arcmin
real*4 RXMpc_1 (nr__6) ! (Mpc) Radius out to which the source count rate has
* been integrated, in Mpc
real*4 Pext_3 (nr__6) ! (%) Extent parameter from the K-S test (1)
real*4 Rc_3 (nr__6) ! (arcmin) Best -fitting core radius
real*4 Rmin_3 (nr__6) ! (arcmin) Minimal radius value consistent with
* the 2{sigma} uncertainty limit
real*4 HR_3 (nr__6) ! Hardness ratio
real*4 e_HR_3 (nr__6) ! rms uncertainty on HR
real*4 DHR_3 (nr__6) ! Deviation from the expected value of HR
* in units of {sigma}
*Note (1): Probability result of the Kolmogorov-Smirnov test for the source
* to be a point source. For very low probabilities for the consistency
* with a point source the parameter Pext was limited to a value of 30
* for the entry in the table. A source is considered very likely to be
* extended if this parameter has at least a value of 2 (point source
* excluded with 99% probability).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table8.dat' ! Additional Clusters Detected as Extended X-Ray
Sources in the 9h-14h Region
integer*4 nr__7
parameter (nr__7=21) ! Number of records
character*110 ar__7 ! Full-size record
C J2000.0 position composed of: RAdeg DEdeg
character*16 RXC_4 (nr__7) ! RXC designation (based on J2000 position)
character*15 Name_4 (nr__7) ! Alternative name
character*2 n_Name_2 (nr__7) ! Note on Name (1)
real*8 RAdeg_4 (nr__7) ! (deg) Right ascension (J2000.0)
real*8 DEdeg_4 (nr__7) ! (deg) Declination (J2000.0)
real*4 z_3 (nr__7) ! Redshift
real*4 CR_4 (nr__7) ! (ct/s) Count rate
real*4 FX_4 (nr__7) ! (10-15W/m2) X-ray flux
real*4 FX__4 (nr__7) ! (10-15W/m2) Corrrected X-ray flux
real*4 Error_4 (nr__7) ! (%) Factional uncertainty for the count rate,
* the fluxes, and the luminosity
real*4 LX_4 (nr__7) ! (10+37W) Rest-frame X-ray luminosity of the clusters
* in the 0.1-2.4keV energy band (10+44erg/s)
real*4 NH_4 (nr__7) ! (10+20cm-2) Absorbing column density in the line of
* sight to the source
character*3 ID_4 (nr__7) ! Identification flag (2)
character*9 r_z_2 (nr__7) ! Redshift reference (separated by commas)
* in refs.dat file
*Note (1): Individual notes are the following:
* a = See also Bade et al., 1998A&AS..127..145B
* b = See also Ebeling et al., 1998MNRAS.301..881E
* c = Barton et al., 1996AJ....112..871B
* d = Crawford et al., 1995MNRAS.274...75C
* e = Cooray et al., 1998AJ....115.1388C
* f = Struble & Rood, 1991ApJ...374..395S
* g = See also Tucker et al., 1995ApJ...444..532T
* h = Appenzeller et al., 1998ApJS..117..319A
* i = Wegner et al., 1996ApJS..106....1W
*Note (2): Identification flag:
* ?: if the identification as a cluster leaves some residual doubts
* B: sources that have been deblended
* L: sources that have been analyzed in extra large fields
* C: sources that may be contaminated
* For the position we have used the coordinates determined by the
* moment method with a 3' aperture radius. As an exception, in the
* case of 12 cluster sources we have either chosen to redetermine the
* center position by a moment method with a larger aperture of 5' or
* 7.5' or determined a center position by hand. In these sources the
* automatic detection has selected a maximum that is significantly
* offset from the global center of symmetry of the clusters.
* b: 5' moment method
* c: 7.5' moment method
* o: determination by eye
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table9.dat' ! X-Ray Properties of the Additional Extended
Cluster Sources
integer*4 nr__8
parameter (nr__8=21) ! Number of records
character*62 ar__8 ! Full-size record
character*16 RXC_5 (nr__8) ! RXC designation (based on J2000 position)
real*4 LX_5 (nr__8) ! (10+37W) Rest-frame ROSAT-band X-ray luminosity
real*4 RXang_2 (nr__8) ! (arcmin) Radius out to which the source count rate has
* been integrated, in arcmin
real*4 RXMpc_2 (nr__8) ! (Mpc) Radius out to which the source count rate has
* been integrated, in Mpc
real*4 Pext_4 (nr__8) ! (%) Extent parameter from the K-S test (1)
real*4 Rc_4 (nr__8) ! (arcmin) Best -fitting core radius
real*4 Rmin_4 (nr__8) ! (arcmin) Minimal radius value consistent with
* the 2{sigma} uncertainty limit
real*4 HR_4 (nr__8) ! Hardness ratio
real*4 e_HR_4 (nr__8) ! rms uncertainty on HR
real*4 DHR_4 (nr__8) ! Deviation from the expected value of HR
* in units of {sigma}
*Note (1): Probability result of the Kolmogorov-Smirnov test for the source
* to be a point source. For very low probabilities for the consistency
* with a point source the parameter Pext was limited to a value of 30
* for the entry in the table. A source is considered very likely to be
* extended if this parameter has at least a value of 2 (point source
* excluded with 99% probability).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'refs.dat' ! Redshift references
integer*4 nr__9
parameter (nr__9=81) ! Number of records
character*151 ar__9 ! Full-size record
integer*4 Ref (nr__9) ! Reference code
character*19 BibCode (nr__9) ! Bibcode
character*33 Aut (nr__9) ! Author's name
character*94 Com_1 (nr__9) ! Comments
C=============================================================================
C Loading file 'table1.dat' ! The NORAS Cluster X-Ray Source Catalog
C Format for file interpretation
1 format(
+ A16,1X,A15,A2,1X,F8.4,1X,F8.4,1X,F6.4,1X,F5.2,1X,F6.2,1X,F6.2,
+ 1X,F5.1,1X,F5.2,1X,F4.1,1X,A3,1X,A9)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,378
read(1,'(A110)')ar__
read(ar__,1)
+ RXC(i__),Name(i__),n_Name(i__),RAdeg(i__),DEdeg(i__),z(i__),
+ CR(i__),FX(i__),FX_(i__),Error(i__),LX(i__),NH(i__),ID(i__),
+ r_z(i__)
c ..............Just test output...........
write(6,1)
+ RXC(i__),Name(i__),n_Name(i__),RAdeg(i__),DEdeg(i__),z(i__),
+ CR(i__),FX(i__),FX_(i__),Error(i__),LX(i__),NH(i__),ID(i__),
+ r_z(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! The Noncluster X-Ray Sources among the Extended
* RASS 1 Sources
C Format for file interpretation
2 format(
+ A15,1X,A7,1X,F8.4,1X,F8.4,1X,F4.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,
+ F4.1,1X,F3.1,1X,F3.1,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.1,1X,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,99
read(1,'(A101)')ar__1
read(ar__1,2)
+ RXJ(i__),Name_1(i__),RAdeg_1(i__),DEdeg_1(i__),CR_1(i__),
+ FX_1(i__),FX__1(i__),Error_1(i__),Pext(i__),Rc(i__),Rmin(i__),
+ HR(i__),e_HR(i__),DHR(i__),NH_1(i__),ID_1(i__)
c ..............Just test output...........
write(6,2)
+ RXJ(i__),Name_1(i__),RAdeg_1(i__),DEdeg_1(i__),CR_1(i__),
+ FX_1(i__),FX__1(i__),Error_1(i__),Pext(i__),Rc(i__),Rmin(i__),
+ HR(i__),e_HR(i__),DHR(i__),NH_1(i__),ID_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! The AGNs in Clusters and Noncluster Sources in the
* Line of Sight with Probable Clusters
C Format for file interpretation
3 format(
+ A15,1X,A7,1X,F8.4,1X,F8.4,1X,F4.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,
+ F4.1,1X,F3.1,1X,F3.1,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.1,1X,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,18
read(1,'(A101)')ar__2
read(ar__2,3)
+ RXJ_1(i__),Name_2(i__),RAdeg_2(i__),DEdeg_2(i__),CR_2(i__),
+ FX_2(i__),FX__2(i__),Error_2(i__),Pext_1(i__),Rc_1(i__),
+ Rmin_1(i__),HR_1(i__),e_HR_1(i__),DHR_1(i__),NH_2(i__),
+ ID_2(i__)
c ..............Just test output...........
write(6,3)
+ RXJ_1(i__),Name_2(i__),RAdeg_2(i__),DEdeg_2(i__),CR_2(i__),
+ FX_2(i__),FX__2(i__),Error_2(i__),Pext_1(i__),Rc_1(i__),
+ Rmin_1(i__),HR_1(i__),e_HR_1(i__),DHR_1(i__),NH_2(i__),
+ ID_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4.dat' ! X-Ray Properties of the Noncluster X-Ray Source
* Cluster Combinations
C Format for file interpretation
4 format(A15,1X,F6.4,1X,A41)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,18
read(1,'(A64)')ar__3
read(ar__3,4)RXJ_2(i__),z_1(i__),Com(i__)
if(ar__3(17:22) .EQ. '') z_1(i__) = rNULL__
c ..............Just test output...........
write(6,4)RXJ_2(i__),z_1(i__),Com(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table5.dat' ! X-Ray Properties of the NORAS Cluster X-Ray Source
C Format for file interpretation
5 format(
+ A16,1X,F5.2,1X,F4.1,1X,F4.2,1X,F4.1,1X,F3.1,1X,F3.1,1X,F5.2,
+ 1X,F4.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,378
read(1,'(A62)')ar__4
read(ar__4,5)
+ RXC_1(i__),LX_1(i__),RXang(i__),RXMpc(i__),Pext_2(i__),
+ Rc_2(i__),Rmin_2(i__),HR_2(i__),e_HR_2(i__),DHR_2(i__)
c ..............Just test output...........
write(6,5)
+ RXC_1(i__),LX_1(i__),RXang(i__),RXMpc(i__),Pext_2(i__),
+ Rc_2(i__),Rmin_2(i__),HR_2(i__),e_HR_2(i__),DHR_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table6.dat' ! Additional ACO89 (Cat. <VII/110>) Clusters
* Detected as X-Ray Sources in the 9h-14h Region
C Format for file interpretation
6 format(
+ A16,1X,A15,A2,1X,F8.4,1X,F8.4,1X,F6.4,1X,F5.2,1X,F6.2,1X,F6.2,
+ 1X,F5.1,1X,F5.2,1X,F4.1,1X,A3,1X,A9)
C Effective file loading
open(unit=1,status='old',file=
+'table6.dat')
write(6,*) '....Loading file: table6.dat'
do i__=1,85
read(1,'(A110)')ar__5
read(ar__5,6)
+ RXC_2(i__),Name_3(i__),n_Name_1(i__),RAdeg_3(i__),
+ DEdeg_3(i__),z_2(i__),CR_3(i__),FX_3(i__),FX__3(i__),
+ Error_3(i__),LX_2(i__),NH_3(i__),ID_3(i__),r_z_1(i__)
c ..............Just test output...........
write(6,6)
+ RXC_2(i__),Name_3(i__),n_Name_1(i__),RAdeg_3(i__),
+ DEdeg_3(i__),z_2(i__),CR_3(i__),FX_3(i__),FX__3(i__),
+ Error_3(i__),LX_2(i__),NH_3(i__),ID_3(i__),r_z_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table7.dat' ! X-Ray Properties of the Additionally Found ACO89
* Clusters
C Format for file interpretation
7 format(
+ A16,1X,F5.2,1X,F4.1,1X,F4.2,1X,F4.1,1X,F3.1,1X,F3.1,1X,F5.2,
+ 1X,F4.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table7.dat')
write(6,*) '....Loading file: table7.dat'
do i__=1,84
read(1,'(A62)')ar__6
read(ar__6,7)
+ RXC_3(i__),LX_3(i__),RXang_1(i__),RXMpc_1(i__),Pext_3(i__),
+ Rc_3(i__),Rmin_3(i__),HR_3(i__),e_HR_3(i__),DHR_3(i__)
c ..............Just test output...........
write(6,7)
+ RXC_3(i__),LX_3(i__),RXang_1(i__),RXMpc_1(i__),Pext_3(i__),
+ Rc_3(i__),Rmin_3(i__),HR_3(i__),e_HR_3(i__),DHR_3(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table8.dat' ! Additional Clusters Detected as Extended X-Ray
* Sources in the 9h-14h Region
C Format for file interpretation
8 format(
+ A16,1X,A15,A2,1X,F8.4,1X,F8.4,1X,F6.4,1X,F5.2,1X,F6.2,1X,F6.2,
+ 1X,F5.1,1X,F5.2,1X,F4.1,1X,A3,1X,A9)
C Effective file loading
open(unit=1,status='old',file=
+'table8.dat')
write(6,*) '....Loading file: table8.dat'
do i__=1,21
read(1,'(A110)')ar__7
read(ar__7,8)
+ RXC_4(i__),Name_4(i__),n_Name_2(i__),RAdeg_4(i__),
+ DEdeg_4(i__),z_3(i__),CR_4(i__),FX_4(i__),FX__4(i__),
+ Error_4(i__),LX_4(i__),NH_4(i__),ID_4(i__),r_z_2(i__)
c ..............Just test output...........
write(6,8)
+ RXC_4(i__),Name_4(i__),n_Name_2(i__),RAdeg_4(i__),
+ DEdeg_4(i__),z_3(i__),CR_4(i__),FX_4(i__),FX__4(i__),
+ Error_4(i__),LX_4(i__),NH_4(i__),ID_4(i__),r_z_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table9.dat' ! X-Ray Properties of the Additional Extended
* Cluster Sources
C Format for file interpretation
9 format(
+ A16,1X,F5.2,1X,F4.1,1X,F4.2,1X,F4.1,1X,F3.1,1X,F3.1,1X,F5.2,
+ 1X,F4.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table9.dat')
write(6,*) '....Loading file: table9.dat'
do i__=1,21
read(1,'(A62)')ar__8
read(ar__8,9)
+ RXC_5(i__),LX_5(i__),RXang_2(i__),RXMpc_2(i__),Pext_4(i__),
+ Rc_4(i__),Rmin_4(i__),HR_4(i__),e_HR_4(i__),DHR_4(i__)
c ..............Just test output...........
write(6,9)
+ RXC_5(i__),LX_5(i__),RXang_2(i__),RXMpc_2(i__),Pext_4(i__),
+ Rc_4(i__),Rmin_4(i__),HR_4(i__),e_HR_4(i__),DHR_4(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'refs.dat' ! Redshift references
C Format for file interpretation
10 format(I2,1X,A19,1X,A33,1X,A94)
C Effective file loading
open(unit=1,status='old',file=
+'refs.dat')
write(6,*) '....Loading file: refs.dat'
do i__=1,81
read(1,'(A151)')ar__9
read(ar__9,10)Ref(i__),BibCode(i__),Aut(i__),Com_1(i__)
c ..............Just test output...........
write(6,10)Ref(i__),BibCode(i__),Aut(i__),Com_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end