Conversion of standardized ReadMe file for
file /./ftp/cats/II/203A/ 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. II/203A Second Extreme Ultra-Violet Explorer Catalog (2EUVE, 1997)
*================================================================================
*Second EUVE Source Catalog
* Bowyer S., Lampton M., Lewis J., Wu X., Jelinsky P., Malina R.F.
* <Astrophys. J. Suppl. Ser. 102, 129 (1996)>
* =1996ApJS..102..129B
*An all-sky catalog of faint extreme ultraviolet sources.
* Lampton M., Lieu R., Schmitt J.H.M.M., Bowyer S., Voges W., Lewis J.,
* Wu X.
* <Astrophys. J. Suppl. Ser. 108, 545 (1997)>
* =1997ApJS..108..545L
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! All-sky survey
integer*4 nr__
parameter (nr__=514) ! Number of records
character*72 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm
real*8 RAdeg (nr__) ! (deg) Right Ascension J2000
real*8 DEdeg (nr__) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*14 EUVE (nr__) ! Catalog designation based on J2000 position
integer*4 RAh (nr__) ! (h) Best fit Right Ascension J2000 (hours) for
* detected EUVE source
integer*4 RAm (nr__) ! (min) Best fit Right Ascension J2000 (minutes)
integer*4 RAs (nr__) ! (s) [0,60] Best fit Right Ascension J2000 (seconds)
character*1 DE_ (nr__) ! Best fit Declination J2000 (sign) for
* detected EUVE source
integer*4 DEd (nr__) ! (deg) Best fit Declination J2000 (degrees)
real*4 DEm (nr__) ! (arcmin) Best fit Declination J2000 (minutes)
integer*4 c100A (nr__) ! (ct/ks) ? 100A (10nm, 125eV) Lexan/boron band observed
* mean countrate
character*1 u_c100A (nr__) ! [)] indicates detections < 3 sigma
integer*4 e_c100A (nr__) ! (ct/ks) ? one sigma countrate error
integer*4 c200A (nr__) ! (ct/ks) ? 200A (20nm, 60eV) aluminium/carbon band
* observed mean countrate
character*1 u_c200A (nr__) ! [)] indicates detections < 3 sigma
integer*4 e_c200A (nr__) ! (ct/ks) ? one sigma countrate error
integer*4 c400A (nr__) ! (ct/ks) ? 400A (40nm, 30eV) multicomponent-filter band
* observed mean countrate
character*1 u_c400A (nr__) ! [)] indicates detections < 3 sigma
integer*4 e_c400A (nr__) ! (ct/ks) ? one sigma countrate error
integer*4 c600A (nr__) ! (ct/ks) ? 600A (60nm, 20eV) tin (Sn) band observed
* mean countrate
character*1 u_c600A (nr__) ! [)] indicates detections < 3 sigma
integer*4 e_c600A (nr__) ! (ct/ks) ? one sigma countrate error
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Deep Survey of half the ecliptic plane
integer*4 nr__1
parameter (nr__1=35) ! Number of records
character*52 ar__1 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm
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)
character*14 EUVE_1 (nr__1) ! Catalog designation based on J2000 position
integer*4 RAh_1 (nr__1) ! (h) Best fit Right Ascension J2000 (hours) for
* detected EUVE source
integer*4 RAm_1 (nr__1) ! (min) Best fit Right Ascension J2000 (minutes)
integer*4 RAs_1 (nr__1) ! (s) Best fit Right Ascension J2000 (seconds)
character*1 DE__1 (nr__1) ! Best fit Declination J2000 (sign) for
* detected EUVE source
integer*4 DEd_1 (nr__1) ! (deg) Best fit Declination J2000 (degrees)
real*4 DEm_1 (nr__1) ! (arcmin) Best fit Declination J2000 (minutes)
real*4 c100A_1 (nr__1) ! (ct/ks) ? 100A (10nm, 125eV) Lexan/boron band
* observed mean countrate
character*1 u_c100A_1 (nr__1) ! [)] ')' indicates detections < 3 sigma
real*4 e_c100A_1 (nr__1) ! (ct/ks) ? one sigma countrate error
real*4 c200A_1 (nr__1) ! (ct/ks) ? 200A (20nm, 60eV) aluminium/carbon band
* observed mean countrate
character*1 u_c200A_1 (nr__1) ! [)] ')' indicates detections < 3 sigma
real*4 e_c200A_1 (nr__1) ! (ct/ks) ? one sigma countrate error
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Sources detected in other ways
integer*4 nr__2
parameter (nr__2=188) ! Number of records
character*74 ar__2 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm
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)
character*14 EUVE_2 (nr__2) ! Catalog designation based on J2000 position
integer*4 RAh_2 (nr__2) ! (h) Best fit Right Ascension J2000 (hours) for
* detected EUVE source
integer*4 RAm_2 (nr__2) ! (min) Best fit Right Ascension J2000 (minutes)
integer*4 RAs_2 (nr__2) ! (s) [0,60] Best fit Right Ascension J2000 (seconds)
character*1 DE__2 (nr__2) ! Best fit Declination J2000 (sign) for
* detected EUVE source
integer*4 DEd_2 (nr__2) ! (deg) Best fit Declination J2000 (degrees)
real*4 DEm_2 (nr__2) ! (arcmin) [0,60] Best fit Declination J2000 (minutes)
real*4 c100A_2 (nr__2) ! (ct/ks) ? 100A (10nm, 125eV) Lexan/boron band
* observed mean countrate
character*1 n_c100A (nr__2) ! [U] indicates possible UV leak
real*4 c200A_2 (nr__2) ! (ct/ks) ? 200A (20nm, 60eV) aluminium/carbon band
* observed mean countrate
character*1 u_c200A_2 (nr__2) ! [U] indicates possible UV leak
real*4 c400A_1 (nr__2) ! (ct/ks) ? 400A (40nm, 30eV) multicomponent-filter
* band observed mean countrate
character*1 n_c400A (nr__2) ! [U] indicates possible UV leak
real*4 c600A_1 (nr__2) ! (ct/ks) ? 600A (60nm, 20eV) tin (Sn) band observed
* mean countrate
character*1 n_c600A (nr__2) ! [U] indicates possible UV leak
real*4 c100DS (nr__2) ! (ct/ks) ? DS100A (10nm, 125eV) Lexan/boron band
* observed mean countrate
character*1 n_c100DS (nr__2) ! [U] indicates possible UV leak
real*4 c200DS (nr__2) ! (ct/ks) ? DS200A (20nm, 60eV) aluminium/carbon band
* observed mean countrate
character*1 n_c200DS (nr__2) ! [U] indicates possible UV leak
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'id1.dat' ! Identifications of table1
integer*4 nr__3
parameter (nr__3=551) ! Number of records
character*91 ar__3 ! Full-size record
character*14 EUVE_3 (nr__3) ! Catalog designation based on J2000 position
character*1 Q (nr__3) ! [12UH] Identification characterisation (1)
character*17 Name1 (nr__3) ! ID name 1
character*17 Name2 (nr__3) ! ID name 2
character*11 Type (nr__3) ! ID spectral type or description
real*4 MAG (nr__3) ! (mag) ? magnitude of ID object
integer*4 Sep (nr__3) ! (arcsec) ? angle separating EUVE & ID in arcsec
character*16 Comments (nr__3) ! See note (2)
*Note (1): the `Q' column indicates our level of confidence in each
* source detection:
* Q=1 denotes likely identification on basis of known EUV emitter from
* previous work or from membership in a class of known EUV emitters.
* Q=2 denotes acceptable positional coincidence but little or no
* other supporting evidence.
* Q=U denotes some of the detected source counts originate from the
* known UV leak of one or more of the EUVE filters
* Q=H means no counterpart has been found, but the detection is
* statistically secure found, the detection is statistically
* secure in the sense of its satisfying the more stringent
* selection criteria.
* Q= (a blank) indicates that the detection lies in the less stringent
* group, and no other supporting evidence is available.
*Note (2): the following catalogue abbreviations are used:
* 1E =1979ApJ...234L...1G First Einstein survey (Giacconi et al.)
* 4U =1978ApJS...38..357F Fourth Uhuru catalog (Forman et al.)
* AF =1995ApJ...441..726F High Galactic Latitude Planetary Nebulae
* (Fruscione et al.),
* AF2 = X-Ray Selected EUV Galaxies (Fruscione A. 1995, ApJ, submitted)
* DK = D. Kilkenny M. Mathioudakis (1995 private communication)
* HM =1995ApJ...455..574D All-sky Survey (Marshall et al.)
* JD =1995ApJ...455..574D Hot White Dwarfs in the LISM (Dupuis et al.)
* JE =1995ApJ...454..442E Millisecond Pulsar J0437-4715 (Edelstein et al.)
* JF =1994BAAS...26..870F Middle Aged Pulsar PSR 0656+14 (Finley et al.)
* JL = Transient/Flaring EUV Sources (Lewis et al. 1995,
* Proc. EUV Colloq. 152, Berkeley CA)
* KM =1994AJ....108.1843M First Year of EUVE RAP (McDonald et al. 1994)
* LTT = Luyten 1957, "Catalogue of 9867 stars in the Southern
* Hemisphere with Proper Motion Exceeding 0.2" (Univ. Minnesota)
* Luyten 1961, "Catalogue of 7127 Stars in the Northern
* Hemisphere with Proper Motion Exceeding 0.2" (Univ. Minnesota)
* MM =1995A&A...300..775M Activity Versus Rotation (Mathioudakis et al.)
* NC = Optical ID of EUV Sources (Craig et al. 1995, ApJ, submitted)
* NC2 = N. Craig (1995 private communication)
* RE =1993MNRAS.260...77P Rosat WFC Catalog (Pounds et al.)
* RF = EUV Emission from Neutron Stars (Foster et al. 1995,
* Proc. EUV Colloq 152, UC Berkeley)
* RG =1995AJ....110..788G Field of EUVE J1027+323 (Genova et al. 1995)
* RL = EUV Emission of Active Galactic Nuclei (Lieu et al. 1995,
* Adv. Space Res., 16(3), 81)
* SV =1995ApJ...448L...9V EUV from Seyfert Ton S180 (Vennes et al.)
* TD1 =1983MNRAS.202..317C TD1 UV survey (Carnochan Wilson 1983;
* catalog <II/59>)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'id2.dat' ! Identifications of table2
integer*4 nr__4
parameter (nr__4=37) ! Number of records
character*91 ar__4 ! Full-size record
character*14 EUVE_4 (nr__4) ! Catalog designation based on J2000 position
character*1 Q_1 (nr__4) ! [12UH] Identification characterisation (1)
character*17 Name1_1 (nr__4) ! ID name 1
character*17 Name2_1 (nr__4) ! ID name 2
character*11 Type_1 (nr__4) ! ID spectral type or description
real*4 MAG_1 (nr__4) ! (mag) ? magnitude of ID object
integer*4 Sep_1 (nr__4) ! (arcsec) ? angle separating EUVE & ID in arcsec
character*16 Comments_1 (nr__4) ! See note (2)
*Note (1): the `Q' column indicates our level of confidence in each
* source detection:
* Q=1 denotes likely identification on basis of known EUV emitter from
* previous work or from membership in a class of known EUV emitters.
* Q=2 denotes acceptable positional coincidence but little or no
* other supporting evidence.
* Q=U denotes some of the detected source counts originate from the
* known UV leak of one or more of the EUVE filters
* Q=H means no counterpart has been found, but the detection is
* statistically secure found, the detection is statistically
* secure in the sense of its satisfying the more stringent
* selection criteria.
* Q= (a blank) indicates that the detection lies in the less stringent
* group, and no other supporting evidence is available.
*Note (2): the following catalogue abbreviations are used:
* 1E =1979ApJ...234L...1G First Einstein survey (Giacconi et al.)
* 4U =1978ApJS...38..357F Fourth Uhuru catalog (Forman et al.)
* AF =1995ApJ...441..726F High Galactic Latitude Planetary Nebulae
* (Fruscione et al.),
* AF2 = X-Ray Selected EUV Galaxies (Fruscione A. 1995, ApJ, submitted)
* DK = D. Kilkenny M. Mathioudakis (1995 private communication)
* HM =1995ApJ...455..574D All-sky Survey (Marshall et al.)
* JD =1995ApJ...455..574D Hot White Dwarfs in the LISM (Dupuis et al.)
* JE =1995ApJ...454..442E Millisecond Pulsar J0437-4715 (Edelstein et al.)
* JF =1994BAAS...26..870F Middle Aged Pulsar PSR 0656+14 (Finley et al.)
* JL = Transient/Flaring EUV Sources (Lewis et al. 1995,
* Proc. EUV Colloq. 152, Berkeley CA)
* KM =1994AJ....108.1843M First Year of EUVE RAP (McDonald et al. 1994)
* LTT = Luyten 1957, "Catalogue of 9867 stars in the Southern
* Hemisphere with Proper Motion Exceeding 0.2" (Univ. Minnesota)
* Luyten 1961, "Catalogue of 7127 Stars in the Northern
* Hemisphere with Proper Motion Exceeding 0.2" (Univ. Minnesota)
* MM =1995A&A...300..775M Activity Versus Rotation (Mathioudakis et al.)
* NC = Optical ID of EUV Sources (Craig et al. 1995, ApJ, submitted)
* NC2 = N. Craig (1995 private communication)
* RE =1993MNRAS.260...77P Rosat WFC Catalog (Pounds et al.)
* RF = EUV Emission from Neutron Stars (Foster et al. 1995,
* Proc. EUV Colloq 152, UC Berkeley)
* RG =1995AJ....110..788G Field of EUVE J1027+323 (Genova et al. 1995)
* RL = EUV Emission of Active Galactic Nuclei (Lieu et al. 1995,
* Adv. Space Res., 16(3), 81)
* SV =1995ApJ...448L...9V EUV from Seyfert Ton S180 (Vennes et al.)
* TD1 =1983MNRAS.202..317C TD1 UV survey (Carnochan Wilson 1983;
* catalog <II/59>)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'id3.dat' ! Identifications of table3
integer*4 nr__5
parameter (nr__5=213) ! Number of records
character*91 ar__5 ! Full-size record
character*14 EUVE_5 (nr__5) ! Catalog designation based on J2000 position
character*1 Q_2 (nr__5) ! [12UH] Identification characterisation (1)
character*17 Name1_2 (nr__5) ! ID name 1
character*17 Name2_2 (nr__5) ! ID name 2
character*11 Type_2 (nr__5) ! ID spectral type or description
real*4 MAG_2 (nr__5) ! (mag) ? magnitude of ID object
integer*4 Sep_2 (nr__5) ! (arcsec) ? angle separating EUVE & ID in arcsec
character*16 Comments_2 (nr__5) ! See note (2)
*Note (1): the `Q' column indicates our level of confidence in each
* source detection:
* Q=1 denotes likely identification on basis of known EUV emitter from
* previous work or from membership in a class of known EUV emitters.
* Q=2 denotes acceptable positional coincidence but little or no
* other supporting evidence.
* Q=U denotes some of the detected source counts originate from the
* known UV leak of one or more of the EUVE filters
* Q=H means no counterpart has been found, but the detection is
* statistically secure found, the detection is statistically
* secure in the sense of its satisfying the more stringent
* selection criteria.
* Q= (a blank) indicates that the detection lies in the less stringent
* group, and no other supporting evidence is available.
*Note (2): the following catalogue abbreviations are used:
* 1E =1979ApJ...234L...1G First Einstein survey (Giacconi et al.)
* 4U =1978ApJS...38..357F Fourth Uhuru catalog (Forman et al.)
* AF =1995ApJ...441..726F High Galactic Latitude Planetary Nebulae
* (Fruscione et al.),
* AF2 = X-Ray Selected EUV Galaxies (Fruscione A. 1995, ApJ, submitted)
* DK = D. Kilkenny M. Mathioudakis (1995 private communication)
* HM =1995ApJ...455..574D All-sky Survey (Marshall et al.)
* JD =1995ApJ...455..574D Hot White Dwarfs in the LISM (Dupuis et al.)
* JE =1995ApJ...454..442E Millisecond Pulsar J0437-4715 (Edelstein et al.)
* JF =1994BAAS...26..870F Middle Aged Pulsar PSR 0656+14 (Finley et al.)
* JL = Transient/Flaring EUV Sources (Lewis et al. 1995,
* Proc. EUV Colloq. 152, Berkeley CA)
* KM =1994AJ....108.1843M First Year of EUVE RAP (McDonald et al. 1994)
* LTT = Luyten 1957, "Catalogue of 9867 stars in the Southern
* Hemisphere with Proper Motion Exceeding 0.2" (Univ. Minnesota)
* Luyten 1961, "Catalogue of 7127 Stars in the Northern
* Hemisphere with Proper Motion Exceeding 0.2" (Univ. Minnesota)
* MM =1995A&A...300..775M Activity Versus Rotation (Mathioudakis et al.)
* NC = Optical ID of EUV Sources (Craig et al. 1995, ApJ, submitted)
* NC2 = N. Craig (1995 private communication)
* RE =1993MNRAS.260...77P Rosat WFC Catalog (Pounds et al.)
* RF = EUV Emission from Neutron Stars (Foster et al. 1995,
* Proc. EUV Colloq 152, UC Berkeley)
* RG =1995AJ....110..788G Field of EUVE J1027+323 (Genova et al. 1995)
* RL = EUV Emission of Active Galactic Nuclei (Lieu et al. 1995,
* Adv. Space Res., 16(3), 81)
* SV =1995ApJ...448L...9V EUV from Seyfert Ton S180 (Vennes et al.)
* TD1 =1983MNRAS.202..317C TD1 UV survey (Carnochan Wilson 1983;
* catalog <II/59>)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'faint.dat' ! Faint sources detected jointly in EUVE and ROSAT WF
(table 1 of Lampton et al., 1997ApJS..108..545L)
integer*4 nr__6
parameter (nr__6=534) ! Number of records
character*76 ar__6 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_3 (nr__6) ! (deg) Right Ascension J2000
real*8 DEdeg_3 (nr__6) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*14 EUVE_6 (nr__6) ! EUVE name
character*1 f_EUVE (nr__6) ! [*] indicates a name which differs from 2EUVE (1)
integer*4 RAh_3 (nr__6) ! (h) Right Ascension J2000 (hours) of X-ray centroid
integer*4 RAm_3 (nr__6) ! (min) Right Ascension J2000 (minutes) of X-ray centroid
integer*4 RAs_3 (nr__6) ! (s) Right Ascension J2000 (seconds) of X-ray centroid
character*1 DE__3 (nr__6) ! Declination J2000 (sign) of X-ray centroid
integer*4 DEd_3 (nr__6) ! (deg) Declination J2000 (degrees) of X-ray centroid
integer*4 DEm_3 (nr__6) ! (arcmin) Declination J2000 (minutes) of X-ray centroid
integer*4 DEs (nr__6) ! (arcsec) Declination J2000 (seconds) of X-ray centroid
real*4 EUVct (nr__6) ! (ct/s) EUVE (100{AA}, 125eV) count rate
real*4 XRT (nr__6) ! (ct/s) X-ray (50{AA}, 250eV) ROSAT WFC count rate
real*4 Sep_3 (nr__6) ! (arcmin) separation between EUVE and X-ray positions
character*16 ID (nr__6) ! Designation of source
character*3 n_EUVE (nr__6) ! [UN2W, ] EUV Status (2)
*Note (1): this flag is set when the source is also present in tables 1 to 3,
* but with a slightly different name, like the first source
* EUVE J0003+436 which is named
* EUVE J0003+435 in table1.dat
*Note (2): the statuses are:
* N = newly reported object (not in tables 1-3)
* 2 = object in 2EUVE (in tables 1-3)
* W = object in ROSAT Wide Field Camera (J/MNRAS/274/1165)
* U = a bright early-type star s closer than 1.5' of the EUV position,
* some or all of the EUVE count rate could be due to UV radiation.
C=============================================================================
C Loading file 'table1.dat' ! All-sky survey
C Format for file interpretation
1 format(
+ A14,1X,I2,1X,I2,1X,I2,1X,A1,I2,1X,F4.1,1X,I5,A1,I3,1X,I5,A1,
+ I3,1X,I5,A1,I3,1X,I5,A1,I3)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,514
read(1,'(A72)')ar__
read(ar__,1)
+ EUVE(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),c100A(i__),u_c100A(i__),e_c100A(i__),c200A(i__),
+ u_c200A(i__),e_c200A(i__),c400A(i__),u_c400A(i__),
+ e_c400A(i__),c600A(i__),u_c600A(i__),e_c600A(i__)
if(ar__(34:38) .EQ. '') c100A(i__) = iNULL__
if(ar__(40:42) .EQ. '') e_c100A(i__) = iNULL__
if(ar__(44:48) .EQ. '') c200A(i__) = iNULL__
if(ar__(50:52) .EQ. '') e_c200A(i__) = iNULL__
if(ar__(54:58) .EQ. '') c400A(i__) = iNULL__
if(ar__(60:62) .EQ. '') e_c400A(i__) = iNULL__
if(ar__(64:68) .EQ. '') c600A(i__) = iNULL__
if(ar__(70:72) .EQ. '') e_c600A(i__) = iNULL__
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(DE_(i__).EQ.'-'.AND.DEdeg(i__).GE.0) DEdeg(i__)=-DEdeg(i__)
c ..............Just test output...........
write(6,1)
+ EUVE(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),c100A(i__),u_c100A(i__),e_c100A(i__),c200A(i__),
+ u_c200A(i__),e_c200A(i__),c400A(i__),u_c400A(i__),
+ e_c400A(i__),c600A(i__),u_c600A(i__),e_c600A(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' ! Deep Survey of half the ecliptic plane
C Format for file interpretation
2 format(
+ A14,1X,I2,1X,I2,1X,I2,1X,A1,I2,1X,F4.1,1X,F5.1,A1,F3.1,1X,
+ F5.1,A1,F3.1)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,35
read(1,'(A52)')ar__1
read(ar__1,2)
+ EUVE_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),c100A_1(i__),u_c100A_1(i__),
+ e_c100A_1(i__),c200A_1(i__),u_c200A_1(i__),e_c200A_1(i__)
if(ar__1(34:38) .EQ. '') c100A_1(i__) = rNULL__
if(ar__1(40:42) .EQ. '') e_c100A_1(i__) = rNULL__
if(ar__1(44:48) .EQ. '') c200A_1(i__) = rNULL__
if(ar__1(50:52) .EQ. '') e_c200A_1(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(DE__1(i__).EQ.'-'.AND.DEdeg_1(i__).GE.0) DEdeg_1(i__)=-DEdeg_1(i__)
c ..............Just test output...........
write(6,2)
+ EUVE_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),c100A_1(i__),u_c100A_1(i__),
+ e_c100A_1(i__),c200A_1(i__),u_c200A_1(i__),e_c200A_1(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' ! Sources detected in other ways
C Format for file interpretation
3 format(
+ A14,1X,I2,1X,I2,1X,I2,1X,A1,I2,1X,F4.1,1X,F5.1,A1,1X,F5.1,A1,
+ 1X,F5.1,A1,1X,F5.1,A1,F6.1,A1,1X,F5.1,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,188
read(1,'(A74)')ar__2
read(ar__2,3)
+ EUVE_2(i__),RAh_2(i__),RAm_2(i__),RAs_2(i__),DE__2(i__),
+ DEd_2(i__),DEm_2(i__),c100A_2(i__),n_c100A(i__),c200A_2(i__),
+ u_c200A_2(i__),c400A_1(i__),n_c400A(i__),c600A_1(i__),
+ n_c600A(i__),c100DS(i__),n_c100DS(i__),c200DS(i__),
+ n_c200DS(i__)
if(ar__2(34:38) .EQ. '') c100A_2(i__) = rNULL__
if(ar__2(41:45) .EQ. '') c200A_2(i__) = rNULL__
if(ar__2(48:52) .EQ. '') c400A_1(i__) = rNULL__
if(ar__2(55:59) .EQ. '') c600A_1(i__) = rNULL__
if(ar__2(61:66) .EQ. '') c100DS(i__) = rNULL__
if(ar__2(69:73) .EQ. '') c200DS(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(DE__2(i__).EQ.'-'.AND.DEdeg_2(i__).GE.0) DEdeg_2(i__)=-DEdeg_2(i__)
c ..............Just test output...........
write(6,3)
+ EUVE_2(i__),RAh_2(i__),RAm_2(i__),RAs_2(i__),DE__2(i__),
+ DEd_2(i__),DEm_2(i__),c100A_2(i__),n_c100A(i__),c200A_2(i__),
+ u_c200A_2(i__),c400A_1(i__),n_c400A(i__),c600A_1(i__),
+ n_c600A(i__),c100DS(i__),n_c100DS(i__),c200DS(i__),
+ n_c200DS(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 'id1.dat' ! Identifications of table1
C Format for file interpretation
4 format(A14,1X,A1,1X,A17,1X,A17,1X,A11,1X,F5.2,1X,I3,1X,A16)
C Effective file loading
open(unit=1,status='old',file=
+'id1.dat')
write(6,*) '....Loading file: id1.dat'
do i__=1,551
read(1,'(A91)')ar__3
read(ar__3,4)
+ EUVE_3(i__),Q(i__),Name1(i__),Name2(i__),Type(i__),MAG(i__),
+ Sep(i__),Comments(i__)
if(ar__3(66:70) .EQ. '') MAG(i__) = rNULL__
if(ar__3(72:74) .EQ. '') Sep(i__) = iNULL__
c ..............Just test output...........
write(6,4)
+ EUVE_3(i__),Q(i__),Name1(i__),Name2(i__),Type(i__),MAG(i__),
+ Sep(i__),Comments(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'id2.dat' ! Identifications of table2
C Format for file interpretation
5 format(A14,1X,A1,1X,A17,1X,A17,1X,A11,1X,F5.2,1X,I3,1X,A16)
C Effective file loading
open(unit=1,status='old',file=
+'id2.dat')
write(6,*) '....Loading file: id2.dat'
do i__=1,37
read(1,'(A91)')ar__4
read(ar__4,5)
+ EUVE_4(i__),Q_1(i__),Name1_1(i__),Name2_1(i__),Type_1(i__),
+ MAG_1(i__),Sep_1(i__),Comments_1(i__)
if(ar__4(66:70) .EQ. '') MAG_1(i__) = rNULL__
if(ar__4(72:74) .EQ. '') Sep_1(i__) = iNULL__
c ..............Just test output...........
write(6,5)
+ EUVE_4(i__),Q_1(i__),Name1_1(i__),Name2_1(i__),Type_1(i__),
+ MAG_1(i__),Sep_1(i__),Comments_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'id3.dat' ! Identifications of table3
C Format for file interpretation
6 format(A14,1X,A1,1X,A17,1X,A17,1X,A11,1X,F5.2,1X,I3,1X,A16)
C Effective file loading
open(unit=1,status='old',file=
+'id3.dat')
write(6,*) '....Loading file: id3.dat'
do i__=1,213
read(1,'(A91)')ar__5
read(ar__5,6)
+ EUVE_5(i__),Q_2(i__),Name1_2(i__),Name2_2(i__),Type_2(i__),
+ MAG_2(i__),Sep_2(i__),Comments_2(i__)
if(ar__5(66:70) .EQ. '') MAG_2(i__) = rNULL__
if(ar__5(72:74) .EQ. '') Sep_2(i__) = iNULL__
c ..............Just test output...........
write(6,6)
+ EUVE_5(i__),Q_2(i__),Name1_2(i__),Name2_2(i__),Type_2(i__),
+ MAG_2(i__),Sep_2(i__),Comments_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'faint.dat' ! Faint sources detected jointly in EUVE and ROSAT WF
* (table 1 of Lampton et al., 1997ApJS..108..545L)
C Format for file interpretation
7 format(
+ A14,A1,1X,I2,1X,I2,1X,I2,1X,A1,I2,1X,I2,1X,I2,1X,F6.3,1X,F5.2,
+ 1X,F4.2,1X,A16,4X,A3)
C Effective file loading
open(unit=1,status='old',file=
+'faint.dat')
write(6,*) '....Loading file: faint.dat'
do i__=1,534
read(1,'(A76)')ar__6
read(ar__6,7)
+ EUVE_6(i__),f_EUVE(i__),RAh_3(i__),RAm_3(i__),RAs_3(i__),
+ DE__3(i__),DEd_3(i__),DEm_3(i__),DEs(i__),EUVct(i__),XRT(i__),
+ Sep_3(i__),ID(i__),n_EUVE(i__)
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(i__) .GE. 0) DEdeg_3(i__)=DEdeg_3(i__)+DEs(i__)/3600.
if(DE__3(i__).EQ.'-'.AND.DEdeg_3(i__).GE.0) DEdeg_3(i__)=-DEdeg_3(i__)
c ..............Just test output...........
write(6,7)
+ EUVE_6(i__),f_EUVE(i__),RAh_3(i__),RAm_3(i__),RAs_3(i__),
+ DE__3(i__),DEd_3(i__),DEm_3(i__),DEs(i__),EUVct(i__),XRT(i__),
+ Sep_3(i__),ID(i__),n_EUVE(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_3(i__),DEdeg_3(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end