Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/359/227 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-20
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/A+A/359/227 Lindroos binary systems X-ray emission (Huelamo+, 2000)
*================================================================================
*X-ray emission from Lindroos binary systems.
* Huelamo N., Neuhaeuser R., Stelzer B., Supper R., Zinnecker H.
* <Astron. Astrophys. 359, 227 (2000)>
* =2000A&A...359..227H
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Stellar Data of the binary sample
integer*4 nr__
parameter (nr__=50) ! Number of records
character*90 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)
integer*4 HD (nr__) ! HD (Cat. III/135) number
character*3 m_HD (nr__) ! (A+BCX ) Multiplicity index on HD
character*12 SpType (nr__) ! MK spectral type (1)
integer*4 RAh (nr__) ! (h) Optical right ascension (J2000) (2)
integer*4 RAm (nr__) ! (min) Optical right ascension (J2000) (2)
real*4 RAs (nr__) ! (s) Optical right ascension (J2000) (2)
character*1 DE_ (nr__) ! Optical declination sign (J2000) (2)
integer*4 DEd (nr__) ! (deg) Optical declination (J2000) (2)
integer*4 DEm (nr__) ! (arcmin) Optical declination (J2000) (2)
real*4 DEs (nr__) ! (arcsec) Optical declination (J2000) (2)
real*4 Sep (nr__) ! (arcsec) Separation angle (1)
real*4 Dist (nr__) ! (pc) Distance (3)
character*1 u_Dist (nr__) ! Uncertainty flag on Dist
character*1 r_Dist (nr__) ! [+] +: data from Lindroos, 1986A&A...156..223L
real*4 e_Dist (nr__) ! (pc) ? rms uncertainty on Dist
character*1 u_e_Dist (nr__) ! Uncertainty flag on e_Dist
real*4 VmagA (nr__) ! (mag) V magnitude of the primary
character*1 n_VmagA (nr__) ! [*] Note on VmagA (4)
real*4 VmagB (nr__) ! (mag) ? V magnitude of the secondary
character*1 n_VmagB (nr__) ! [*7] Note on VmagB (4), (7)
real*4 AV (nr__) ! (mag) ? Absorption in V band
character*2 Class (nr__) ! Classification (6)
*Note (1): Taken from Pallavicini et al. (1992A&A...261..245P)
*Note (2): Coordinates of the primary star
*Note (3): Deduced from Hipparcos parallax of the primary star, except
* those marked with + taken from Lindroos, 1986A&A...156..223L
*Note (4): Adopted from Pallavicini et al. (1992A&A...261..245P) except
* those marked with an asterisk obtained from the SIMBAD database
*Note (6): Classification taken by Pallavicini et al. (1992A&A...261..245P)
* with respect to the presence of the Lithium absorption line and CaII
* (H and K) chromospheric lines in the spectrum of the secondary:
* CP (certainly physical);
* PP (probably physical);
* LO (likely optical)
*Note (7): Unknown visual magnitude for the secondary star.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! RASS observations: Detections and upper limits
integer*4 nr__1
parameter (nr__1=37) ! Number of records
character*99 ar__1 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 (nr__1) ! (deg) Right Ascension J2000
real*8 DEdeg_1 (nr__1) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 HD_1 (nr__1) ! HD (Cat. III/135) number
integer*4 RAh_1 (nr__1) ! (h) ? X-ray right ascension (J2000)
integer*4 RAm_1 (nr__1) ! (min) ? X-ray right ascension (J2000)
real*4 RAs_1 (nr__1) ! (s) ? X-ray right ascension (J2000)
character*1 DE__1 (nr__1) ! X-ray declination sign (J2000)
integer*4 DEd_1 (nr__1) ! (deg) ? X-ray declination sign (J2000)
integer*4 DEm_1 (nr__1) ! (arcmin) ? X-ray declination sign (J2000)
real*4 DEs_1 (nr__1) ! (arcsec) ? X-ray declination sign (J2000)
real*4 DeltaA (nr__1) ! (arcsec) ? Displacement between the detected X-ray
* source and the optical position of the
* primary component (1)
real*4 DeltaB (nr__1) ! (arcsec) ? Displacement between the detected X-ray
* source and the optical position of the
* secondary component (1)
character*1 l_Count (nr__1) ! Limit flag on Count
real*4 Count (nr__1) ! (ct) Count of the primary component or
* of the both is upper limit (2)
real*4 e_Count (nr__1) ! (ct) ? rms uncertainty on Counts
real*4 Bcnt (nr__1) ! (ct) ? Counts of the secondary component
real*4 ExpTime (nr__1) ! (s) Exposition time
character*1 l_HR1 (nr__1) ! Limit flag on HR1
real*4 HR1 (nr__1) ! ? Hardness ratio 1 (G1)
real*4 e_HR1 (nr__1) ! ? rms uncertainty on HR1
character*1 l_HR2 (nr__1) ! Limit flag on HR2
real*4 HR2 (nr__1) ! ? Hardness ratio 2 (G1)
real*4 e_HR2 (nr__1) ! ? rms uncertainty on HR2
real*4 ML (nr__1) ! ? Maximum likelihood
*Note (1): Given the low spatial resolution of the PSPC, we cannot resolve
* the two components of the binary system. As a consequence, the
* displacement {delta} between the detected X-ray source and the
* optical positions of the two components of the system are given.
*Note (2): In the case of non-detection, upper limits are computed at
* the positions of both components, A and B, respectively.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! PSPC pointed observations
integer*4 nr__2
parameter (nr__2=5) ! Number of records
character*112 ar__2 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_2 (nr__2) ! (deg) Right Ascension J2000
real*8 DEdeg_2 (nr__2) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 HD_2 (nr__2) ! HD (Cat. III/135) number
integer*4 n_HD (nr__2) ! [1/2]? Individual note (1)
integer*4 ROR (nr__2) ! ROSAT Observation request number
character*1 m_ROR (nr__2) ! Multiplicity index on ROR
integer*4 RAh_2 (nr__2) ! (h) ? X-ray right ascension (J2000)
integer*4 RAm_2 (nr__2) ! (min) ? X-ray right ascension (J2000)
real*4 RAs_2 (nr__2) ! (s) ? X-ray right ascension (J2000)
character*1 DE__2 (nr__2) ! X-ray declination sign (J2000)
integer*4 DEd_2 (nr__2) ! (deg) ? X-ray declination sign (J2000)
integer*4 DEm_2 (nr__2) ! (arcmin) ? X-ray declination sign (J2000)
real*4 DEs_2 (nr__2) ! (arcsec) ? X-ray declination sign (J2000)
real*4 DeltaA_1 (nr__2) ! (arcsec) ? Displacement between the detected X-ray
* source and the optical position of the
* primary component
real*4 DeltaB_1 (nr__2) ! (arcsec) ? Displacement between the detected X-ray
* source and the optical position of the
* secondary component
real*4 Offaxis (nr__2) ! (arcmin) ? Offaxis
character*1 l_Count_1 (nr__2) ! Limit flag on Count
real*4 Count_1 (nr__2) ! (ct) Count of the primary component or
* of the both is upper limit (2)
real*4 e_Count_1 (nr__2) ! (ct) ? rms uncertainty on Counts
real*4 Bcnt_1 (nr__2) ! (ct) ? Counts of the secondary component
real*8 ExpTime_1 (nr__2) ! (s) Exposition time
real*4 HR1_1 (nr__2) ! ? Hardness ratio 1 (G1)
real*4 e_HR1_1 (nr__2) ! ? rms uncertainty on HR1
real*4 HR2_1 (nr__2) ! ? Hardness ratio 2 (G1)
real*4 e_HR2_1 (nr__2) ! ? rms uncertainty on HR2
real*8 ML_1 (nr__2) ! ? Maximum likelihood
*Note (1): Individual notes as follows:
* 1 = The source is very close to the support structure of the
* telescope, so we are not sure about the reliability of the
* upper limit
* 2 = This source has two PSPC observations: 201271p and 201271 p-1.
* There are no detections in the individual observations, so we
* have added up both files to improve the S/N ratio.
*Note (2): In the case of non-detection, upper limits are computed at the
* positions of both components, A and B, respectively.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! HRI observations
integer*4 nr__3
parameter (nr__3=46) ! Number of records
character*112 ar__3 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_3 (nr__3) ! (deg) Right Ascension J2000
real*8 DEdeg_3 (nr__3) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 HD_3 (nr__3) ! ? HD (Cat. III/135) number)
character*3 n_HD_1 (nr__3) ! Note on HD (1)
integer*4 ROR_1 (nr__3) ! ROSAT Observation request number
character*5 m_ROR_1 (nr__3) ! Multiplicity index on ROR
character*2 n_Comp (nr__3) ! Note on elongation (2)
character*6 Comp (nr__3) ! Composant designation
integer*4 RAh_3 (nr__3) ! (h) ? X-ray right ascension (J2000)
integer*4 RAm_3 (nr__3) ! (min) ? X-ray right ascension (J2000)
real*4 RAs_3 (nr__3) ! (s) ? X-ray right ascension (J2000)
character*1 DE__3 (nr__3) ! X-ray declination sign (J2000)
integer*4 DEd_3 (nr__3) ! (deg) ? X-ray declination (J2000)
integer*4 DEm_3 (nr__3) ! (arcmin) ? X-ray declination (J2000)
real*4 DEs_3 (nr__3) ! (arcsec) ? X-ray declination (J2000)
real*4 DeltaA_2 (nr__3) ! (arcsec) ? Displacement between the detected X-ray
* source and the optical position of the
* binary system or of the primary component
* if DeltaB exist (3)
real*4 DeltaB_2 (nr__3) ! (arcsec) ? Displacement between the detected X-ray
* source and the optical position of the
* secondary component (3)
real*4 OffAxis_1 (nr__3) ! (arcmin) ? Displacement of the sources with respect to
* the axis of the telescope
character*1 l_Count_2 (nr__3) ! Limit flag on Count
real*8 Count_2 (nr__3) ! (ct) Total counts in the broad band
real*4 e_Count_2 (nr__3) ! (ct) ? rms uncertainty on Counts
real*8 ExpTime_2 (nr__3) ! (s) Exposition time (4)
character*1 l_HR (nr__3) ! Limit flag in HR
real*4 HR (nr__3) ! ? Hardness ratio
real*4 e_HR (nr__3) ! ? rms uncertainty on HR
real*4 ML_2 (nr__3) ! ? Maximum of likelihood coefficient
*Note (1): Notes as follows:
* 1 = If both components are detected, coordinates of both X-ray
* sources are given. The displacement of the secondary with
* respect to the detected X-ray source is computed comparing with
* its optical coordinates.
* 2 = The two stars of the system are not completely resolved so each
* star is contributing to the count rate of the companion.
* 3 = The undetected component is so close to the X-ray source that no
* reliable upper limit can be computed.
* 4 = HD74146 has another observation, 200186h, but with very low
* exposure time (t_exp_=357.5s).
* s = stars previously studied by Schmitt et al. (1993ApJ...402L..13S).
*Note (2): Elongation information as follows:
* e = for elongated sources;
* * = The elongated shape is due to attitude problems in the
* processed data
*Note (3): When we cannot resolve the two components of the binary system,
* the displacement {delta} between the detected X-ray source and the
* optical positions of the two components of the system are given.
*Note (4): For ROR 201685h B, the printed value is "4535.3.8", modified
* in 45353.8 in the present table.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! X-ray luminosities
integer*4 nr__4
parameter (nr__4=51) ! Number of records
character*43 ar__4 ! Full-size record
integer*4 HD_4 (nr__4) ! HD (Cat. III/135) number
character*3 Comp_1 (nr__4) ! Component designation
character*1 l_logNH (nr__4) ! Limit flag on logNH
real*4 logNH (nr__4) ! ([cm-2]) Computed hydrogen column density
integer*4 r_logNH (nr__4) ! ? Source of logNH (1)
character*1 Obs (nr__4) ! [HRP] Type of observations (2)
character*1 l_logLX (nr__4) ! Limit flag on logLX
real*4 logLX (nr__4) ! ([10-7W]) X-ray luminosity (3)
real*4 e_logLX (nr__4) ! ([10-7W]) ? rms uncertainty on logLX
character*1 n_logLX (nr__4) ! [*] *: Mean X-ray luminosity computed from
* several observations
character*1 l_logLX2 (nr__4) ! Limit flag on logLX2
real*4 logLX2 (nr__4) ! ([10-7W]) ? X-ray luminosity of the secondary
*Note (1): Source of logNH as follows:
* 1 = Adopted from Berghofer et al. (1996, Cat. J/A+AS/118/481)
* 2 = Adopted from Fruscione et al. (1994, Cat. J/ApJS/94/127)
*Note (2): Type of observation as follows:
* R = RASS (ROSAT All-Sky Survey, Cat. IX/10)
* P = PSPC (Position-Sensitive Proportional Counter, Cat. IX/30)
* H = HRI (High Resolution Imager, Cat. IX/28)
*Note (3): If the binary system is observed and resolved by the HRI, we
* provide the fluxes and luminosities for both members of the pair.
* If unresolved, we just can provide one X-ray luminosity associated
* with the pair. In hese cases we have adopted a temperature of 1keV
* to compute the ECF's although, in principle, both stars could be
* contributing to the total emission. he last method has also been
* applied to those systems with only RASS or PSPC pointed observations,
* given that they are always unresolved. In the case of RASS or PSPC
* non-detections, we have estimated two upper limit luminosities,
* corresponding to the count rates computed at the optical positions
* of the primary and the secondary star, respectively (see Table 2).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6.dat' ! HRI soft-band rate and UV-rate for detected
early-type stars
integer*4 nr__5
parameter (nr__5=10) ! Number of records
character*37 ar__5 ! Full-size record
integer*4 HD_5 (nr__5) ! HD (Cat. III/135) number
character*1 n_Umag (nr__5) ! Note on U-magnitudes (1)
real*4 Umag (nr__5) ! (mag) U magnitude (from HR catalogue V/50)
real*4 Srate (nr__5) ! (ct/ks) S-band count rate (2)
real*4 UVrate (nr__5) ! (ct/ks) UV count rate (2)
real*8 S_UV (nr__5) ! S to UV rates ratio
real*4 log_LX_Lbol(nr__5) ! Bolometric to X-ray Luminosity ratio
*Note (1): *: No U-magnitudes available. We derived them from their spectral
* types and their V-magnitudes, according to Kenyon & Hartmann (1995,
* Cat. J/ApJS/101/117).
*Note (2): The S-band rate and the UV rate have been both computed in
* channels 1-8 of the detector.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table7.dat' ! Stellar properties of the post-TTau (PTTS) candidates
integer*4 nr__6
parameter (nr__6=20) ! Number of records
character*67 ar__6 ! Full-size record
integer*4 HD_6 (nr__6) ! HD (Cat. III/135) number
character*1 Comp_2 (nr__6) ! Component designation
character*1 u_Comp (nr__6) ! [?] Uncertainty flag on Comp
character*1 n_HD_2 (nr__6) ! [t] Note on HD (1)
character*4 SpType_1 (nr__6) ! MK Spectral type
character*1 l_logLX_1 (nr__6) ! Limit flag on logLX
real*4 logLX_1 (nr__6) ! ([10-7W]) X-ray luminosity
character*1 l_EWLi (nr__6) ! Limit flag on EWLi
real*4 EWLi (nr__6) ! (0.1nm) Li I absorption line equivalent width
real*4 e_EWLi (nr__6) ! (0.1nm) ? rms uncertainty on EWLi
character*1 n_EWLi (nr__6) ! [1-3] Note on EWLi (2)
real*4 F12um (nr__6) ! (Jy) ? 12{mu}m flux density (3)
character*1 u_F12um (nr__6) ! [?] ?: unknown value
real*4 F100um (nr__6) ! (Jy) ? 100{mu}m flux density (3)
character*1 u_F100um (nr__6) ! [?] ?: unknown value
character*2 f_RV (nr__6) ! [Ee :] Radial velocity comment (4)
character*1 Xray (nr__6) ! [+-] X-ray emission ? (5)
character*1 LiI (nr__6) ! [+-] Li I equivalent width ? (5)
character*1 IR_ex (nr__6) ! [+-?] Measured IR excess ? (5)
character*3 RV (nr__6) ! [+-? ()] Measured radial velocity of pair ? (5)
*Note (1): The two sources marked with a t are located close to the Galactic
* plane and this seems to be the reason of not being detected by IRAS
*Note (2): Most of the Li I EW values have been adopted Pallavicini et al.
* (1992A&A...261..245P). These measurements were derived from
* high-resolution spectra (resolution of 0.1{AA}), except those
* with a note (1, 2 or 3):
* 1 = obtained from low-resolution spectra (resolution of 2{AA})
* 2 = taken from Martin et al., 1992A&A...257..186M
* (disp. of 0.22{AA}/pix)
* 3 = adopted from Webb et al. (1999ApJ...512L..63W);
*Note (3): The IR data are taken from Ray et al. (1995ApJ...440L..89R)
*Note (4): If similar radial velocities have been measured for both members
* of the pair it is indicated by an 'e' (if taken from Gahm, 1982,
* Stockholm Obs. Rep. No.20 ) and by an 'E' (if taken from Martin et
* al., 1992A&A...257..186M). If the measurements are doubtful, it is
* indicated by a ":" (see Gahm, 1982, Stockholm Obs. Rep. No.20, and
* Martin et al., 1992A&A...257..186M, for more details)
*Note (5): We have summarized the data of the table in these columns using
* the symbols +,- and ? for positive, negative and unknown properties
* respectively. The (+) symbols indicate doubtful properties.
C=============================================================================
C Loading file 'table1.dat' ! Stellar Data of the binary sample
C Format for file interpretation
1 format(
+ I6,1X,A3,1X,A12,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,
+ F5.1,1X,F6.1,A1,A1,F5.1,A1,1X,F4.2,A1,1X,F5.2,A1,1X,F4.2,1X,A2)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,50
read(1,'(A90)')ar__
read(ar__,1)
+ HD(i__),m_HD(i__),SpType(i__),RAh(i__),RAm(i__),RAs(i__),
+ DE_(i__),DEd(i__),DEm(i__),DEs(i__),Sep(i__),Dist(i__),
+ u_Dist(i__),r_Dist(i__),e_Dist(i__),u_e_Dist(i__),VmagA(i__),
+ n_VmagA(i__),VmagB(i__),n_VmagB(i__),AV(i__),Class(i__)
if(ar__(64:68) .EQ. '') e_Dist(i__) = rNULL__
if(ar__(77:81) .EQ. '') VmagB(i__) = rNULL__
if(ar__(84:87) .EQ. '') AV(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)
+ HD(i__),m_HD(i__),SpType(i__),RAh(i__),RAm(i__),RAs(i__),
+ DE_(i__),DEd(i__),DEm(i__),DEs(i__),Sep(i__),Dist(i__),
+ u_Dist(i__),r_Dist(i__),e_Dist(i__),u_e_Dist(i__),VmagA(i__),
+ n_VmagA(i__),VmagB(i__),n_VmagB(i__),AV(i__),Class(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 'table2.dat' ! RASS observations: Detections and upper limits
C Format for file interpretation
2 format(
+ I6,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,F5.1,1X,F5.2,A1,
+ F6.2,1X,F4.1,2X,F4.2,2X,F6.1,1X,A1,F5.2,1X,F4.2,1X,A1,F5.2,1X,
+ F4.2,1X,F6.1)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,37
read(1,'(A99)')ar__1
read(ar__1,2)
+ HD_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),DeltaA(i__),DeltaB(i__),
+ l_Count(i__),Count(i__),e_Count(i__),Bcnt(i__),ExpTime(i__),
+ l_HR1(i__),HR1(i__),e_HR1(i__),l_HR2(i__),HR2(i__),e_HR2(i__),
+ ML(i__)
if(ar__1(8:9) .EQ. '') RAh_1(i__) = iNULL__
if(ar__1(11:12) .EQ. '') RAm_1(i__) = iNULL__
if(ar__1(14:18) .EQ. '') RAs_1(i__) = rNULL__
if(ar__1(21:22) .EQ. '') DEd_1(i__) = iNULL__
if(ar__1(24:25) .EQ. '') DEm_1(i__) = iNULL__
if(ar__1(27:31) .EQ. '') DEs_1(i__) = rNULL__
if(ar__1(32:36) .EQ. '') DeltaA(i__) = rNULL__
if(ar__1(38:42) .EQ. '') DeltaB(i__) = rNULL__
if(ar__1(51:54) .EQ. '') e_Count(i__) = rNULL__
if(ar__1(57:60) .EQ. '') Bcnt(i__) = rNULL__
if(ar__1(71:75) .EQ. '') HR1(i__) = rNULL__
if(ar__1(77:80) .EQ. '') e_HR1(i__) = rNULL__
if(ar__1(83:87) .EQ. '') HR2(i__) = rNULL__
if(ar__1(89:92) .EQ. '') e_HR2(i__) = rNULL__
if(ar__1(94:99) .EQ. '') ML(i__) = rNULL__
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(6,2)
+ HD_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),DeltaA(i__),DeltaB(i__),
+ l_Count(i__),Count(i__),e_Count(i__),Bcnt(i__),ExpTime(i__),
+ l_HR1(i__),HR1(i__),e_HR1(i__),l_HR2(i__),HR2(i__),e_HR2(i__),
+ ML(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! PSPC pointed observations
C Format for file interpretation
3 format(
+ I6,1X,I1,1X,I6,A1,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,
+ F4.1,1X,F4.1,1X,F5.2,1X,A1,F6.1,1X,F4.1,1X,F5.2,1X,F7.1,1X,
+ F5.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,F7.1)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,5
read(1,'(A112)')ar__2
read(ar__2,3)
+ HD_2(i__),n_HD(i__),ROR(i__),m_ROR(i__),RAh_2(i__),RAm_2(i__),
+ RAs_2(i__),DE__2(i__),DEd_2(i__),DEm_2(i__),DEs_2(i__),
+ DeltaA_1(i__),DeltaB_1(i__),Offaxis(i__),l_Count_1(i__),
+ Count_1(i__),e_Count_1(i__),Bcnt_1(i__),ExpTime_1(i__),
+ HR1_1(i__),e_HR1_1(i__),HR2_1(i__),e_HR2_1(i__),ML_1(i__)
if(ar__2(8:8) .EQ. '') n_HD(i__) = iNULL__
if(ar__2(18:19) .EQ. '') RAh_2(i__) = iNULL__
if(ar__2(21:22) .EQ. '') RAm_2(i__) = iNULL__
if(ar__2(24:28) .EQ. '') RAs_2(i__) = rNULL__
if(ar__2(31:32) .EQ. '') DEd_2(i__) = iNULL__
if(ar__2(34:35) .EQ. '') DEm_2(i__) = iNULL__
if(ar__2(37:41) .EQ. '') DEs_2(i__) = rNULL__
if(ar__2(42:45) .EQ. '') DeltaA_1(i__) = rNULL__
if(ar__2(47:50) .EQ. '') DeltaB_1(i__) = rNULL__
if(ar__2(52:56) .EQ. '') Offaxis(i__) = rNULL__
if(ar__2(66:69) .EQ. '') e_Count_1(i__) = rNULL__
if(ar__2(71:75) .EQ. '') Bcnt_1(i__) = rNULL__
if(ar__2(85:89) .EQ. '') HR1_1(i__) = rNULL__
if(ar__2(91:94) .EQ. '') e_HR1_1(i__) = rNULL__
if(ar__2(96:99) .EQ. '') HR2_1(i__) = rNULL__
if(ar__2(101:104) .EQ. '') e_HR2_1(i__) = rNULL__
if(ar__2(106:112) .EQ. '') ML_1(i__) = rNULL__
RAdeg_2(i__) = rNULL__
DEdeg_2(i__) = rNULL__
c Derive coordinates RAdeg_2 and DEdeg_2 from input data
c (RAdeg_2 and DEdeg_2 are set to rNULL__ when unknown)
if(RAh_2(i__) .GT. -180) RAdeg_2(i__)=RAh_2(i__)*15.
if(RAm_2(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAm_2(i__)/4.
if(RAs_2(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAs_2(i__)/240.
if(DEd_2(i__) .GE. 0) DEdeg_2(i__)=DEd_2(i__)
if(DEm_2(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEm_2(i__)/60.
if(DEs_2(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEs_2(i__)/3600.
if(DE__2(i__).EQ.'-'.AND.DEdeg_2(i__).GE.0) DEdeg_2(i__)=-DEdeg_2(i__)
c ..............Just test output...........
write(6,3)
+ HD_2(i__),n_HD(i__),ROR(i__),m_ROR(i__),RAh_2(i__),RAm_2(i__),
+ RAs_2(i__),DE__2(i__),DEd_2(i__),DEm_2(i__),DEs_2(i__),
+ DeltaA_1(i__),DeltaB_1(i__),Offaxis(i__),l_Count_1(i__),
+ Count_1(i__),e_Count_1(i__),Bcnt_1(i__),ExpTime_1(i__),
+ HR1_1(i__),e_HR1_1(i__),HR2_1(i__),e_HR2_1(i__),ML_1(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_2(i__),DEdeg_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4.dat' ! HRI observations
C Format for file interpretation
4 format(
+ I6,1X,A3,2X,I6,A5,1X,A2,A6,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,
+ 1X,F4.1,1X,F4.1,1X,F3.1,1X,F5.2,1X,A1,F7.2,1X,F4.1,1X,F7.1,1X,
+ A1,F5.2,1X,F4.2,1X,F6.1)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,46
read(1,'(A112)')ar__3
read(ar__3,4)
+ HD_3(i__),n_HD_1(i__),ROR_1(i__),m_ROR_1(i__),n_Comp(i__),
+ Comp(i__),RAh_3(i__),RAm_3(i__),RAs_3(i__),DE__3(i__),
+ DEd_3(i__),DEm_3(i__),DEs_3(i__),DeltaA_2(i__),DeltaB_2(i__),
+ OffAxis_1(i__),l_Count_2(i__),Count_2(i__),e_Count_2(i__),
+ ExpTime_2(i__),l_HR(i__),HR(i__),e_HR(i__),ML_2(i__)
if(ar__3(1:6) .EQ. '') HD_3(i__) = iNULL__
if(ar__3(34:35) .EQ. '') RAh_3(i__) = iNULL__
if(ar__3(37:38) .EQ. '') RAm_3(i__) = iNULL__
if(ar__3(40:44) .EQ. '') RAs_3(i__) = rNULL__
if(ar__3(47:48) .EQ. '') DEd_3(i__) = iNULL__
if(ar__3(50:51) .EQ. '') DEm_3(i__) = iNULL__
if(ar__3(53:56) .EQ. '') DEs_3(i__) = rNULL__
if(ar__3(58:61) .EQ. '') DeltaA_2(i__) = rNULL__
if(ar__3(63:65) .EQ. '') DeltaB_2(i__) = rNULL__
if(ar__3(67:71) .EQ. '') OffAxis_1(i__) = rNULL__
if(ar__3(82:85) .EQ. '') e_Count_2(i__) = rNULL__
if(ar__3(96:100) .EQ. '') HR(i__) = rNULL__
if(ar__3(102:105) .EQ. '') e_HR(i__) = rNULL__
if(ar__3(107:112) .EQ. '') ML_2(i__) = rNULL__
RAdeg_3(i__) = rNULL__
DEdeg_3(i__) = rNULL__
c Derive coordinates RAdeg_3 and DEdeg_3 from input data
c (RAdeg_3 and DEdeg_3 are set to rNULL__ when unknown)
if(RAh_3(i__) .GT. -180) RAdeg_3(i__)=RAh_3(i__)*15.
if(RAm_3(i__) .GT. -180) RAdeg_3(i__)=RAdeg_3(i__)+RAm_3(i__)/4.
if(RAs_3(i__) .GT. -180) RAdeg_3(i__)=RAdeg_3(i__)+RAs_3(i__)/240.
if(DEd_3(i__) .GE. 0) DEdeg_3(i__)=DEd_3(i__)
if(DEm_3(i__) .GE. 0) DEdeg_3(i__)=DEdeg_3(i__)+DEm_3(i__)/60.
if(DEs_3(i__) .GE. 0) DEdeg_3(i__)=DEdeg_3(i__)+DEs_3(i__)/3600.
if(DE__3(i__).EQ.'-'.AND.DEdeg_3(i__).GE.0) DEdeg_3(i__)=-DEdeg_3(i__)
c ..............Just test output...........
write(6,4)
+ HD_3(i__),n_HD_1(i__),ROR_1(i__),m_ROR_1(i__),n_Comp(i__),
+ Comp(i__),RAh_3(i__),RAm_3(i__),RAs_3(i__),DE__3(i__),
+ DEd_3(i__),DEm_3(i__),DEs_3(i__),DeltaA_2(i__),DeltaB_2(i__),
+ OffAxis_1(i__),l_Count_2(i__),Count_2(i__),e_Count_2(i__),
+ ExpTime_2(i__),l_HR(i__),HR(i__),e_HR(i__),ML_2(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_3(i__),DEdeg_3(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table5.dat' ! X-ray luminosities
C Format for file interpretation
5 format(
+ I6,1X,A3,1X,A1,F5.2,1X,I1,1X,A1,1X,A1,F5.2,2X,F5.2,A1,1X,A1,
+ F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,51
read(1,'(A43)')ar__4
read(ar__4,5)
+ HD_4(i__),Comp_1(i__),l_logNH(i__),logNH(i__),r_logNH(i__),
+ Obs(i__),l_logLX(i__),logLX(i__),e_logLX(i__),n_logLX(i__),
+ l_logLX2(i__),logLX2(i__)
if(ar__4(19:19) .EQ. '') r_logNH(i__) = iNULL__
if(ar__4(31:35) .EQ. '') e_logLX(i__) = rNULL__
if(ar__4(39:43) .EQ. '') logLX2(i__) = rNULL__
c ..............Just test output...........
write(6,5)
+ HD_4(i__),Comp_1(i__),l_logNH(i__),logNH(i__),r_logNH(i__),
+ Obs(i__),l_logLX(i__),logLX(i__),e_logLX(i__),n_logLX(i__),
+ l_logLX2(i__),logLX2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table6.dat' ! HRI soft-band rate and UV-rate for detected
* early-type stars
C Format for file interpretation
6 format(I6,A1,1X,F4.2,1X,F5.2,1X,F5.2,1X,F7.2,1X,F4.1)
C Effective file loading
open(unit=1,status='old',file=
+'table6.dat')
write(6,*) '....Loading file: table6.dat'
do i__=1,10
read(1,'(A37)')ar__5
read(ar__5,6)
+ HD_5(i__),n_Umag(i__),Umag(i__),Srate(i__),UVrate(i__),
+ S_UV(i__),log_LX_Lbol(i__)
c ..............Just test output...........
write(6,6)
+ HD_5(i__),n_Umag(i__),Umag(i__),Srate(i__),UVrate(i__),
+ S_UV(i__),log_LX_Lbol(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table7.dat' ! Stellar properties of the post-TTau (PTTS) candidates
C Format for file interpretation
7 format(
+ I6,1X,A1,A1,A1,1X,A4,1X,A1,F5.2,2X,A1,F5.3,1X,F5.3,1X,A1,1X,
+ F5.3,A1,1X,F5.3,A1,1X,A2,1X,A1,2X,A1,2X,A1,1X,A3)
C Effective file loading
open(unit=1,status='old',file=
+'table7.dat')
write(6,*) '....Loading file: table7.dat'
do i__=1,20
read(1,'(A67)')ar__6
read(ar__6,7)
+ HD_6(i__),Comp_2(i__),u_Comp(i__),n_HD_2(i__),SpType_1(i__),
+ l_logLX_1(i__),logLX_1(i__),l_EWLi(i__),EWLi(i__),e_EWLi(i__),
+ n_EWLi(i__),F12um(i__),u_F12um(i__),F100um(i__),u_F100um(i__),
+ f_RV(i__),Xray(i__),LiI(i__),IR_ex(i__),RV(i__)
if(ar__6(32:36) .EQ. '') e_EWLi(i__) = rNULL__
if(ar__6(40:44) .EQ. '') F12um(i__) = rNULL__
if(ar__6(47:51) .EQ. '') F100um(i__) = rNULL__
c ..............Just test output...........
write(6,7)
+ HD_6(i__),Comp_2(i__),u_Comp(i__),n_HD_2(i__),SpType_1(i__),
+ l_logLX_1(i__),logLX_1(i__),l_EWLi(i__),EWLi(i__),e_EWLi(i__),
+ n_EWLi(i__),F12um(i__),u_F12um(i__),F100um(i__),u_F100um(i__),
+ f_RV(i__),Xray(i__),LiI(i__),IR_ex(i__),RV(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end