Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/507/655 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-19
C=============================================================================
* This code was generated from the ReadMe file documenting a catalogue
* according to the "Standard for Documentation of Astronomical Catalogues"
* currently in use by the Astronomical Data Centers (CDS, ADC, A&A)
* (see full documentation at URL http://vizier.u-strasbg.fr/doc/catstd.htx)
* Please report problems or questions to
C=============================================================================
implicit none
* Unspecified or NULL values, generally corresponding to blank columns,
* are assigned one of the following special values:
* rNULL__ for unknown or NULL floating-point values
* iNULL__ for unknown or NULL integer values
real*4 rNULL__
integer*4 iNULL__
parameter (rNULL__=--2147483648.) ! NULL real number
parameter (iNULL__=(-2147483647-1)) ! NULL int number
integer idig ! testing NULL number
C=============================================================================
Cat. J/ApJ/507/655 VI photometry of new Cepheids in NGC 2541 (Ferrarese+, 1998)
*================================================================================
*The Hubble Space Telescope Key Project on the extragalactic distance scale.
*XII. The discovery of cepheids and a new distance to NGC 2541.
* Ferrarese L., Bresolin F., Kennicutt R.C.Jr, Saha A., Stetson P.B.,
* Freedman W.L., Mould J.R., Madore B.F., Sakai S., Ford H.C., Gibson B.K.,
* Graham J.A., Han M., Hoessel J.G., Huchra J., Hughes S.M.,
* Illingworth G.D., Phelps R., Prosser C.F., Silbermann N.A.
* <Astrophys. J. 507, 655 (1998)>
* =1998ApJ...507..655F (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! Astrometry for the NGC 2541 Cepheids
integer*4 nr__
parameter (nr__=34) ! Number of records
character*46 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)
character*3 v_FBK98_ (nr__) ! Identification (CNN or VNN) (1)
real*4 Xpos (nr__) ! (pix) X position (2)
real*4 Ypos (nr__) ! (pix) Y position (2)
integer*4 RAh (nr__) ! (h) Right ascension (J2000) (3)
integer*4 RAm (nr__) ! (min) Right ascension (J2000) (3)
real*4 RAs (nr__) ! (s) Right ascension (J2000) (3)
character*1 DE_ (nr__) ! Declination sign (J2000)
integer*4 DEd (nr__) ! (deg) Declination (J2000) (3)
integer*4 DEm (nr__) ! (arcmin) Declination (J2000) (3)
real*4 DEs (nr__) ! (arcsec) Declination (J2000) (3)
character*4 Chip (nr__) ! Chip (PC, WF 2, WF 3, WF 4)
*Note (1): CNN for Cepheids stars, VNN for other variable stars
*Note (2): The X- and Y-coordinates are relative to the 1995 October 30 epoch.
* For each 800 x 800 pixels chip, pixel [1, 1] is located at the edge
* of the pyramid.
*Note (3): RA and DE are calculated using the IRAF task
* STSDAS.HST CALIB.WFPC.METRIC, version 1.3.5 (1996 July).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6.dat' ! V (F555W) photometry for NGC 2541 Cepheids
integer*4 nr__1
parameter (nr__1=437) ! Number of records
character*26 ar__1 ! Full-size record
character*3 v_FBK98__1 (nr__1) ! Identification (CNN or VNN)
real*8 HJD (nr__1) ! (d) Heliocentric Julian date
real*4 mag (nr__1) ! (mag) V or I magnitude
real*4 e_mag (nr__1) ! (mag) rms uncertainty on mag
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table7.dat' ! I (F814W) photometry for NGC 2541 Cepheids
integer*4 nr__2
parameter (nr__2=159) ! Number of records
character*26 ar__2 ! Full-size record
character*3 v_FBK98__2 (nr__2) ! Identification (CNN or VNN)
real*8 HJD_1 (nr__2) ! (d) Heliocentric Julian date
real*4 mag_1 (nr__2) ! (mag) V or I magnitude
real*4 e_mag_1 (nr__2) ! (mag) rms uncertainty on mag
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table8.dat' ! DOPHOT mean photometry of the NGC 2541 Cepheids
integer*4 nr__3
parameter (nr__3=34) ! Number of records
character*79 ar__3 ! Full-size record
character*3 v_FBK98__3 (nr__3) ! Identification (CNN or VNN)
character*1 l_Per (nr__3) ! Limit flag on Per
real*4 Per (nr__3) ! (d) Period
character*1 l_Per2 (nr__3) ! Limit flag on Per2
integer*4 Per2 (nr__3) ! (d) ? Upper limit for period interval
real*4 F555Wph (nr__3) ! (mag) Phase-weighted mean F555W magnitude
real*4 F555Wav (nr__3) ! (mag) Intensity-averaged mean F555W magnitude
real*4 F814Wph (nr__3) ! (mag) ? Phase-weighted mean F814W magnitude
real*4 F814WphCor (nr__3) ! (mag) ? Correction adopted for F814Wph (1)
real*4 F814Wav (nr__3) ! (mag) ? Intensity-average mean F814W magnitude
real*4 F814WavCor (nr__3) ! (mag) ? Correction adopted for F814Wav (1)
real*4 Vmagph (nr__3) ! (mag) ? Phase-weighted mean V magnitude
real*4 Vmagav (nr__3) ! (mag) ? Intensity-averaged mean V magnitude
real*4 Imagph (nr__3) ! (mag) ? Phase-weighted mean I magnitude
real*4 Imagav (nr__3) ! (mag) ? Intensity-averaged mean I magnitude
real*4 chi2_sigma (nr__3) ! ? Reduced {xi}^2^_r_ value for DoPHOT or
* {sigma} for ALLFRAME
*Note (1): Value of the magnitude correction applied to the F814W magnitudes,
* defined as in section 4.4 of the paper.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table9.dat' ! Allframe mean photometry of the NGC 2541 Cepheids
integer*4 nr__4
parameter (nr__4=34) ! Number of records
character*79 ar__4 ! Full-size record
character*3 v_FBK98__4 (nr__4) ! Identification (CNN or VNN)
character*1 l_Per_1 (nr__4) ! Limit flag on Per
real*4 Per_1 (nr__4) ! (d) Period
character*1 l_Per2_1 (nr__4) ! Limit flag on Per2
integer*4 Per2_1 (nr__4) ! (d) ? Upper limit for period interval
real*4 F555Wph_1 (nr__4) ! (mag) Phase-weighted mean F555W magnitude
real*4 F555Wav_1 (nr__4) ! (mag) Intensity-averaged mean F555W magnitude
real*4 F814Wph_1 (nr__4) ! (mag) ? Phase-weighted mean F814W magnitude
real*4 F814WphCor_1(nr__4) ! (mag) ? Correction adopted for F814Wph (1)
real*4 F814Wav_1 (nr__4) ! (mag) ? Intensity-average mean F814W magnitude
real*4 F814WavCor_1(nr__4) ! (mag) ? Correction adopted for F814Wav (1)
real*4 Vmagph_1 (nr__4) ! (mag) ? Phase-weighted mean V magnitude
real*4 Vmagav_1 (nr__4) ! (mag) ? Intensity-averaged mean V magnitude
real*4 Imagph_1 (nr__4) ! (mag) ? Phase-weighted mean I magnitude
real*4 Imagav_1 (nr__4) ! (mag) ? Intensity-averaged mean I magnitude
real*4 chi2_sigma_1(nr__4) ! ? Reduced {xi}^2^_r_ value for DoPHOT or
* {sigma} for ALLFRAME
*Note (1): Value of the magnitude correction applied to the F814W magnitudes,
* defined as in section 4.4 of the paper.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table12.dat' ! Astrometry for other NGC 2541 variable candidates
integer*4 nr__5
parameter (nr__5=23) ! Number of records
character*46 ar__5 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 (nr__5) ! (deg) Right Ascension J2000
real*8 DEdeg_1 (nr__5) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*3 v_FBK98__5 (nr__5) ! Identification (CNN or VNN) (1)
real*4 Xpos_1 (nr__5) ! (pix) X position (2)
real*4 Ypos_1 (nr__5) ! (pix) Y position (2)
integer*4 RAh_1 (nr__5) ! (h) Right ascension (J2000) (3)
integer*4 RAm_1 (nr__5) ! (min) Right ascension (J2000) (3)
real*4 RAs_1 (nr__5) ! (s) Right ascension (J2000) (3)
character*1 DE__1 (nr__5) ! Declination sign (J2000)
integer*4 DEd_1 (nr__5) ! (deg) Declination (J2000) (3)
integer*4 DEm_1 (nr__5) ! (arcmin) Declination (J2000) (3)
real*4 DEs_1 (nr__5) ! (arcsec) Declination (J2000) (3)
character*4 Chip_1 (nr__5) ! Chip (PC, WF 2, WF 3, WF 4)
*Note (1): CNN for Cepheids stars, VNN for other variable stars
*Note (2): The X- and Y-coordinates are relative to the 1995 October 30 epoch.
* For each 800 x 800 pixels chip, pixel [1, 1] is located at the edge
* of the pyramid.
*Note (3): RA and DE are calculated using the IRAF task
* STSDAS.HST CALIB.WFPC.METRIC, version 1.3.5 (1996 July).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table13.dat' ! V photometry for other NGC 2541 variable candidates
integer*4 nr__6
parameter (nr__6=297) ! Number of records
character*26 ar__6 ! Full-size record
character*3 v_FBK98__6 (nr__6) ! Identification (CNN or VNN)
real*8 HJD_2 (nr__6) ! (d) Heliocentric Julian date
real*4 mag_2 (nr__6) ! (mag) V or I magnitude
real*4 e_mag_2 (nr__6) ! (mag) rms uncertainty on mag
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table14.dat' ! I photometry for other NGC 2541 variable candidates
integer*4 nr__7
parameter (nr__7=106) ! Number of records
character*26 ar__7 ! Full-size record
character*3 v_FBK98__7 (nr__7) ! Identification (CNN or VNN)
real*8 HJD_3 (nr__7) ! (d) Heliocentric Julian date
real*4 mag_3 (nr__7) ! (mag) V or I magnitude
real*4 e_mag_3 (nr__7) ! (mag) rms uncertainty on mag
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table15.dat' ! DOPHOT mean photometry of other NGC 2541 variables
integer*4 nr__8
parameter (nr__8=22) ! Number of records
character*79 ar__8 ! Full-size record
character*3 v_FBK98__8 (nr__8) ! Identification (CNN or VNN)
character*1 l_Per_2 (nr__8) ! Limit flag on Per
real*4 Per_2 (nr__8) ! (d) Period
character*1 l_Per2_2 (nr__8) ! Limit flag on Per2
integer*4 Per2_2 (nr__8) ! (d) ? Upper limit for period interval
real*4 F555Wph_2 (nr__8) ! (mag) Phase-weighted mean F555W magnitude
real*4 F555Wav_2 (nr__8) ! (mag) Intensity-averaged mean F555W magnitude
real*4 F814Wph_2 (nr__8) ! (mag) ? Phase-weighted mean F814W magnitude
real*4 F814WphCor_2(nr__8) ! (mag) ? Correction adopted for F814Wph (1)
real*4 F814Wav_2 (nr__8) ! (mag) ? Intensity-average mean F814W magnitude
real*4 F814WavCor_2(nr__8) ! (mag) ? Correction adopted for F814Wav (1)
real*4 Vmagph_2 (nr__8) ! (mag) ? Phase-weighted mean V magnitude
real*4 Vmagav_2 (nr__8) ! (mag) ? Intensity-averaged mean V magnitude
real*4 Imagph_2 (nr__8) ! (mag) ? Phase-weighted mean I magnitude
real*4 Imagav_2 (nr__8) ! (mag) ? Intensity-averaged mean I magnitude
real*4 chi2_sigma_2(nr__8) ! ? Reduced {xi}^2^_r_ value for DoPHOT or
* {sigma} for ALLFRAME
*Note (1): Value of the magnitude correction applied to the F814W magnitudes,
* defined as in section 4.4 of the paper.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table16.dat' ! Allframe mean photometry of other NGC 2541 variables
integer*4 nr__9
parameter (nr__9=11) ! Number of records
character*79 ar__9 ! Full-size record
character*3 v_FBK98__9 (nr__9) ! Identification (CNN or VNN)
character*1 l_Per_3 (nr__9) ! Limit flag on Per
real*4 Per_3 (nr__9) ! (d) Period
character*1 l_Per2_3 (nr__9) ! Limit flag on Per2
integer*4 Per2_3 (nr__9) ! (d) ? Upper limit for period interval
real*4 F555Wph_3 (nr__9) ! (mag) Phase-weighted mean F555W magnitude
real*4 F555Wav_3 (nr__9) ! (mag) Intensity-averaged mean F555W magnitude
real*4 F814Wph_3 (nr__9) ! (mag) ? Phase-weighted mean F814W magnitude
real*4 F814WphCor_3(nr__9) ! (mag) ? Correction adopted for F814Wph (1)
real*4 F814Wav_3 (nr__9) ! (mag) ? Intensity-average mean F814W magnitude
real*4 F814WavCor_3(nr__9) ! (mag) ? Correction adopted for F814Wav (1)
real*4 Vmagph_3 (nr__9) ! (mag) ? Phase-weighted mean V magnitude
real*4 Vmagav_3 (nr__9) ! (mag) ? Intensity-averaged mean V magnitude
real*4 Imagph_3 (nr__9) ! (mag) ? Phase-weighted mean I magnitude
real*4 Imagav_3 (nr__9) ! (mag) ? Intensity-averaged mean I magnitude
real*4 chi2_sigma_3(nr__9) ! ? Reduced {xi}^2^_r_ value for DoPHOT or
* {sigma} for ALLFRAME
*Note (1): Value of the magnitude correction applied to the F814W magnitudes,
* defined as in section 4.4 of the paper.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table17.dat' ! Photometry for the PC secondary standards
integer*4 nr__10
parameter (nr__10=24) ! Number of records
character*71 ar__10 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_2 (nr__10) ! (deg) Right Ascension J2000
real*8 DEdeg_2 (nr__10) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*4 Xpos_2 (nr__10) ! (pix) X position (1)
real*4 Ypos_2 (nr__10) ! (pix) Y position (1)
integer*4 RAh_2 (nr__10) ! (h) Right ascension (J2000) (2)
integer*4 RAm_2 (nr__10) ! (min) Right ascension (J2000) (2)
real*4 RAs_2 (nr__10) ! (s) Right ascension (J2000) (2)
character*1 DE__2 (nr__10) ! Declination sign (J2000) (2)
integer*4 DEd_2 (nr__10) ! (deg) Declination (J2000) (2)
integer*4 DEm_2 (nr__10) ! (arcmin) Declination (J2000) (2)
real*4 DEs_2 (nr__10) ! (arcsec) Declination (J2000) (2)
real*4 F555W (nr__10) ! (mag) F555W magnitude(3)
real*4 e_F555W (nr__10) ! (mag) rms uncertainty on F555W
real*4 F814W (nr__10) ! (mag) F814W magnitude (3)
real*4 e_F814W (nr__10) ! (mag) rms uncertainty on F814W
real*4 Vmag (nr__10) ! (mag) V magnitude (4)
real*4 Imag (nr__10) ! (mag) I magnitude (4)
*Note (1): The X and Y coordinate are relative to the 1995 October 30 epoch.
* For each 800x800 pixels chip, pixel [1,1] is located at the edge
* of the WFPC2 pyramid
*Note (2): RA and DE are calculated using the IRAF task
* STSDAS.HST_CALIB.WFPC.METRIC, version 1.3.5 (July 1996)
*Note (3): F555W and F814W instrumental magnitudes are intensity averaged
* over 13 and 5 epochs respectively.
*Note (4): V and I magnitudes are calculated from the instrumental
* F555W and F814W magnitudes as described in section 3 of the paper.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table18.dat' ! Photometry for the WF2 secondary standards
integer*4 nr__11
parameter (nr__11=29) ! Number of records
character*71 ar__11 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_3 (nr__11) ! (deg) Right Ascension J2000
real*8 DEdeg_3 (nr__11) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*4 Xpos_3 (nr__11) ! (pix) X position (1)
real*4 Ypos_3 (nr__11) ! (pix) Y position (1)
integer*4 RAh_3 (nr__11) ! (h) Right ascension (J2000) (2)
integer*4 RAm_3 (nr__11) ! (min) Right ascension (J2000) (2)
real*4 RAs_3 (nr__11) ! (s) Right ascension (J2000) (2)
character*1 DE__3 (nr__11) ! Declination sign (J2000) (2)
integer*4 DEd_3 (nr__11) ! (deg) Declination (J2000) (2)
integer*4 DEm_3 (nr__11) ! (arcmin) Declination (J2000) (2)
real*4 DEs_3 (nr__11) ! (arcsec) Declination (J2000) (2)
real*4 F555W_1 (nr__11) ! (mag) F555W magnitude(3)
real*4 e_F555W_1 (nr__11) ! (mag) rms uncertainty on F555W
real*4 F814W_1 (nr__11) ! (mag) F814W magnitude (3)
real*4 e_F814W_1 (nr__11) ! (mag) rms uncertainty on F814W
real*4 Vmag_1 (nr__11) ! (mag) V magnitude (4)
real*4 Imag_1 (nr__11) ! (mag) I magnitude (4)
*Note (1): The X and Y coordinate are relative to the 1995 October 30 epoch.
* For each 800x800 pixels chip, pixel [1,1] is located at the edge
* of the WFPC2 pyramid
*Note (2): RA and DE are calculated using the IRAF task
* STSDAS.HST_CALIB.WFPC.METRIC, version 1.3.5 (July 1996)
*Note (3): F555W and F814W instrumental magnitudes are intensity averaged
* over 13 and 5 epochs respectively.
*Note (4): V and I magnitudes are calculated from the instrumental
* F555W and F814W magnitudes as described in section 3 of the paper.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table19.dat' ! Photometry for the WF3 secondary standards
integer*4 nr__12
parameter (nr__12=32) ! Number of records
character*71 ar__12 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_4 (nr__12) ! (deg) Right Ascension J2000
real*8 DEdeg_4 (nr__12) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*4 Xpos_4 (nr__12) ! (pix) X position (1)
real*4 Ypos_4 (nr__12) ! (pix) Y position (1)
integer*4 RAh_4 (nr__12) ! (h) Right ascension (J2000) (2)
integer*4 RAm_4 (nr__12) ! (min) Right ascension (J2000) (2)
real*4 RAs_4 (nr__12) ! (s) Right ascension (J2000) (2)
character*1 DE__4 (nr__12) ! Declination sign (J2000) (2)
integer*4 DEd_4 (nr__12) ! (deg) Declination (J2000) (2)
integer*4 DEm_4 (nr__12) ! (arcmin) Declination (J2000) (2)
real*4 DEs_4 (nr__12) ! (arcsec) Declination (J2000) (2)
real*4 F555W_2 (nr__12) ! (mag) F555W magnitude(3)
real*4 e_F555W_2 (nr__12) ! (mag) rms uncertainty on F555W
real*4 F814W_2 (nr__12) ! (mag) F814W magnitude (3)
real*4 e_F814W_2 (nr__12) ! (mag) rms uncertainty on F814W
real*4 Vmag_2 (nr__12) ! (mag) V magnitude (4)
real*4 Imag_2 (nr__12) ! (mag) I magnitude (4)
*Note (1): The X and Y coordinate are relative to the 1995 October 30 epoch.
* For each 800x800 pixels chip, pixel [1,1] is located at the edge
* of the WFPC2 pyramid
*Note (2): RA and DE are calculated using the IRAF task
* STSDAS.HST_CALIB.WFPC.METRIC, version 1.3.5 (July 1996)
*Note (3): F555W and F814W instrumental magnitudes are intensity averaged
* over 13 and 5 epochs respectively.
*Note (4): V and I magnitudes are calculated from the instrumental
* F555W and F814W magnitudes as described in section 3 of the paper.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table20.dat' ! Photometry for the WF4 secondary standards
integer*4 nr__13
parameter (nr__13=29) ! Number of records
character*71 ar__13 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_5 (nr__13) ! (deg) Right Ascension J2000
real*8 DEdeg_5 (nr__13) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
real*4 Xpos_5 (nr__13) ! (pix) X position (1)
real*4 Ypos_5 (nr__13) ! (pix) Y position (1)
integer*4 RAh_5 (nr__13) ! (h) Right ascension (J2000) (2)
integer*4 RAm_5 (nr__13) ! (min) Right ascension (J2000) (2)
real*4 RAs_5 (nr__13) ! (s) Right ascension (J2000) (2)
character*1 DE__5 (nr__13) ! Declination sign (J2000) (2)
integer*4 DEd_5 (nr__13) ! (deg) Declination (J2000) (2)
integer*4 DEm_5 (nr__13) ! (arcmin) Declination (J2000) (2)
real*4 DEs_5 (nr__13) ! (arcsec) Declination (J2000) (2)
real*4 F555W_3 (nr__13) ! (mag) F555W magnitude(3)
real*4 e_F555W_3 (nr__13) ! (mag) rms uncertainty on F555W
real*4 F814W_3 (nr__13) ! (mag) F814W magnitude (3)
real*4 e_F814W_3 (nr__13) ! (mag) rms uncertainty on F814W
real*4 Vmag_3 (nr__13) ! (mag) V magnitude (4)
real*4 Imag_3 (nr__13) ! (mag) I magnitude (4)
*Note (1): The X and Y coordinate are relative to the 1995 October 30 epoch.
* For each 800x800 pixels chip, pixel [1,1] is located at the edge
* of the WFPC2 pyramid
*Note (2): RA and DE are calculated using the IRAF task
* STSDAS.HST_CALIB.WFPC.METRIC, version 1.3.5 (July 1996)
*Note (3): F555W and F814W instrumental magnitudes are intensity averaged
* over 13 and 5 epochs respectively.
*Note (4): V and I magnitudes are calculated from the instrumental
* F555W and F814W magnitudes as described in section 3 of the paper.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'note5.dat' ! Individual notes on Cepheids
integer*4 nr__14
parameter (nr__14=44) ! Number of records
character*80 ar__14 ! Full-size record
character*3 v_FBK98__10(nr__14) ! Identification (CNN or VNN)
character*76 Note (nr__14) ! Text of the note (1)
*Note (1): The term "isolated" is use d for stars for which no companions are
* identified within a 3 pixel radius.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'note12.dat' ! Individual notes on other variable stars
integer*4 nr__15
parameter (nr__15=46) ! Number of records
character*80 ar__15 ! Full-size record
character*3 v_FBK98__11(nr__15) ! Identification (CNN or VNN)
character*76 Note_1 (nr__15) ! Text of the note (1)
*Note (1): The term "isolated" is use d for stars for which no companions are
* identified within a 3 pixel radius.
C=============================================================================
C Loading file 'table5.dat' ! Astrometry for the NGC 2541 Cepheids
C Format for file interpretation
1 format(
+ A3,1X,F6.2,1X,F6.2,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,
+ 1X,A4)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,34
read(1,'(A46)')ar__
read(ar__,1)
+ v_FBK98_(i__),Xpos(i__),Ypos(i__),RAh(i__),RAm(i__),RAs(i__),
+ DE_(i__),DEd(i__),DEm(i__),DEs(i__),Chip(i__)
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)
+ v_FBK98_(i__),Xpos(i__),Ypos(i__),RAh(i__),RAm(i__),RAs(i__),
+ DE_(i__),DEd(i__),DEm(i__),DEs(i__),Chip(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 'table6.dat' ! V (F555W) photometry for NGC 2541 Cepheids
C Format for file interpretation
2 format(A3,1X,F11.3,1X,F5.2,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table6.dat')
write(6,*) '....Loading file: table6.dat'
do i__=1,437
read(1,'(A26)')ar__1
read(ar__1,2)v_FBK98__1(i__),HJD(i__),mag(i__),e_mag(i__)
c ..............Just test output...........
write(6,2)v_FBK98__1(i__),HJD(i__),mag(i__),e_mag(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table7.dat' ! I (F814W) photometry for NGC 2541 Cepheids
C Format for file interpretation
3 format(A3,1X,F11.3,1X,F5.2,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table7.dat')
write(6,*) '....Loading file: table7.dat'
do i__=1,159
read(1,'(A26)')ar__2
read(ar__2,3)
+ v_FBK98__2(i__),HJD_1(i__),mag_1(i__),e_mag_1(i__)
c ..............Just test output...........
write(6,3)
+ v_FBK98__2(i__),HJD_1(i__),mag_1(i__),e_mag_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table8.dat' ! DOPHOT mean photometry of the NGC 2541 Cepheids
C Format for file interpretation
4 format(
+ A3,1X,A1,F4.1,1X,A1,I2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,
+ F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table8.dat')
write(6,*) '....Loading file: table8.dat'
do i__=1,34
read(1,'(A79)')ar__3
read(ar__3,4)
+ v_FBK98__3(i__),l_Per(i__),Per(i__),l_Per2(i__),Per2(i__),
+ F555Wph(i__),F555Wav(i__),F814Wph(i__),F814WphCor(i__),
+ F814Wav(i__),F814WavCor(i__),Vmagph(i__),Vmagav(i__),
+ Imagph(i__),Imagav(i__),chi2_sigma(i__)
if(ar__3(12:13) .EQ. '') Per2(i__) = iNULL__
if(ar__3(27:31) .EQ. '') F814Wph(i__) = rNULL__
if(ar__3(33:37) .EQ. '') F814WphCor(i__) = rNULL__
if(ar__3(39:43) .EQ. '') F814Wav(i__) = rNULL__
if(ar__3(45:49) .EQ. '') F814WavCor(i__) = rNULL__
if(ar__3(51:55) .EQ. '') Vmagph(i__) = rNULL__
if(ar__3(57:61) .EQ. '') Vmagav(i__) = rNULL__
if(ar__3(63:67) .EQ. '') Imagph(i__) = rNULL__
if(ar__3(69:73) .EQ. '') Imagav(i__) = rNULL__
if(ar__3(75:79) .EQ. '') chi2_sigma(i__) = rNULL__
c ..............Just test output...........
write(6,4)
+ v_FBK98__3(i__),l_Per(i__),Per(i__),l_Per2(i__),Per2(i__),
+ F555Wph(i__),F555Wav(i__),F814Wph(i__),F814WphCor(i__),
+ F814Wav(i__),F814WavCor(i__),Vmagph(i__),Vmagav(i__),
+ Imagph(i__),Imagav(i__),chi2_sigma(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table9.dat' ! Allframe mean photometry of the NGC 2541 Cepheids
C Format for file interpretation
5 format(
+ A3,1X,A1,F4.1,1X,A1,I2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,
+ F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table9.dat')
write(6,*) '....Loading file: table9.dat'
do i__=1,34
read(1,'(A79)')ar__4
read(ar__4,5)
+ v_FBK98__4(i__),l_Per_1(i__),Per_1(i__),l_Per2_1(i__),
+ Per2_1(i__),F555Wph_1(i__),F555Wav_1(i__),F814Wph_1(i__),
+ F814WphCor_1(i__),F814Wav_1(i__),F814WavCor_1(i__),
+ Vmagph_1(i__),Vmagav_1(i__),Imagph_1(i__),Imagav_1(i__),
+ chi2_sigma_1(i__)
if(ar__4(12:13) .EQ. '') Per2_1(i__) = iNULL__
if(ar__4(27:31) .EQ. '') F814Wph_1(i__) = rNULL__
if(ar__4(33:37) .EQ. '') F814WphCor_1(i__) = rNULL__
if(ar__4(39:43) .EQ. '') F814Wav_1(i__) = rNULL__
if(ar__4(45:49) .EQ. '') F814WavCor_1(i__) = rNULL__
if(ar__4(51:55) .EQ. '') Vmagph_1(i__) = rNULL__
if(ar__4(57:61) .EQ. '') Vmagav_1(i__) = rNULL__
if(ar__4(63:67) .EQ. '') Imagph_1(i__) = rNULL__
if(ar__4(69:73) .EQ. '') Imagav_1(i__) = rNULL__
if(ar__4(75:79) .EQ. '') chi2_sigma_1(i__) = rNULL__
c ..............Just test output...........
write(6,5)
+ v_FBK98__4(i__),l_Per_1(i__),Per_1(i__),l_Per2_1(i__),
+ Per2_1(i__),F555Wph_1(i__),F555Wav_1(i__),F814Wph_1(i__),
+ F814WphCor_1(i__),F814Wav_1(i__),F814WavCor_1(i__),
+ Vmagph_1(i__),Vmagav_1(i__),Imagph_1(i__),Imagav_1(i__),
+ chi2_sigma_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table12.dat' ! Astrometry for other NGC 2541 variable candidates
C Format for file interpretation
6 format(
+ A3,1X,F6.2,1X,F6.2,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,
+ 1X,A4)
C Effective file loading
open(unit=1,status='old',file=
+'table12.dat')
write(6,*) '....Loading file: table12.dat'
do i__=1,23
read(1,'(A46)')ar__5
read(ar__5,6)
+ v_FBK98__5(i__),Xpos_1(i__),Ypos_1(i__),RAh_1(i__),RAm_1(i__),
+ RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),
+ Chip_1(i__)
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(6,6)
+ v_FBK98__5(i__),Xpos_1(i__),Ypos_1(i__),RAh_1(i__),RAm_1(i__),
+ RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),
+ Chip_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 'table13.dat' ! V photometry for other NGC 2541 variable candidates
C Format for file interpretation
7 format(A3,1X,F11.3,1X,F5.2,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table13.dat')
write(6,*) '....Loading file: table13.dat'
do i__=1,297
read(1,'(A26)')ar__6
read(ar__6,7)
+ v_FBK98__6(i__),HJD_2(i__),mag_2(i__),e_mag_2(i__)
c ..............Just test output...........
write(6,7)
+ v_FBK98__6(i__),HJD_2(i__),mag_2(i__),e_mag_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table14.dat' ! I photometry for other NGC 2541 variable candidates
C Format for file interpretation
8 format(A3,1X,F11.3,1X,F5.2,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table14.dat')
write(6,*) '....Loading file: table14.dat'
do i__=1,106
read(1,'(A26)')ar__7
read(ar__7,8)
+ v_FBK98__7(i__),HJD_3(i__),mag_3(i__),e_mag_3(i__)
c ..............Just test output...........
write(6,8)
+ v_FBK98__7(i__),HJD_3(i__),mag_3(i__),e_mag_3(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table15.dat' ! DOPHOT mean photometry of other NGC 2541 variables
C Format for file interpretation
9 format(
+ A3,1X,A1,F4.1,1X,A1,I2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,
+ F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table15.dat')
write(6,*) '....Loading file: table15.dat'
do i__=1,22
read(1,'(A79)')ar__8
read(ar__8,9)
+ v_FBK98__8(i__),l_Per_2(i__),Per_2(i__),l_Per2_2(i__),
+ Per2_2(i__),F555Wph_2(i__),F555Wav_2(i__),F814Wph_2(i__),
+ F814WphCor_2(i__),F814Wav_2(i__),F814WavCor_2(i__),
+ Vmagph_2(i__),Vmagav_2(i__),Imagph_2(i__),Imagav_2(i__),
+ chi2_sigma_2(i__)
if(ar__8(12:13) .EQ. '') Per2_2(i__) = iNULL__
if(ar__8(27:31) .EQ. '') F814Wph_2(i__) = rNULL__
if(ar__8(33:37) .EQ. '') F814WphCor_2(i__) = rNULL__
if(ar__8(39:43) .EQ. '') F814Wav_2(i__) = rNULL__
if(ar__8(45:49) .EQ. '') F814WavCor_2(i__) = rNULL__
if(ar__8(51:55) .EQ. '') Vmagph_2(i__) = rNULL__
if(ar__8(57:61) .EQ. '') Vmagav_2(i__) = rNULL__
if(ar__8(63:67) .EQ. '') Imagph_2(i__) = rNULL__
if(ar__8(69:73) .EQ. '') Imagav_2(i__) = rNULL__
if(ar__8(75:79) .EQ. '') chi2_sigma_2(i__) = rNULL__
c ..............Just test output...........
write(6,9)
+ v_FBK98__8(i__),l_Per_2(i__),Per_2(i__),l_Per2_2(i__),
+ Per2_2(i__),F555Wph_2(i__),F555Wav_2(i__),F814Wph_2(i__),
+ F814WphCor_2(i__),F814Wav_2(i__),F814WavCor_2(i__),
+ Vmagph_2(i__),Vmagav_2(i__),Imagph_2(i__),Imagav_2(i__),
+ chi2_sigma_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table16.dat' ! Allframe mean photometry of other NGC 2541 variables
C Format for file interpretation
10 format(
+ A3,1X,A1,F4.1,1X,A1,I2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,
+ F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table16.dat')
write(6,*) '....Loading file: table16.dat'
do i__=1,11
read(1,'(A79)')ar__9
read(ar__9,10)
+ v_FBK98__9(i__),l_Per_3(i__),Per_3(i__),l_Per2_3(i__),
+ Per2_3(i__),F555Wph_3(i__),F555Wav_3(i__),F814Wph_3(i__),
+ F814WphCor_3(i__),F814Wav_3(i__),F814WavCor_3(i__),
+ Vmagph_3(i__),Vmagav_3(i__),Imagph_3(i__),Imagav_3(i__),
+ chi2_sigma_3(i__)
if(ar__9(12:13) .EQ. '') Per2_3(i__) = iNULL__
if(ar__9(27:31) .EQ. '') F814Wph_3(i__) = rNULL__
if(ar__9(33:37) .EQ. '') F814WphCor_3(i__) = rNULL__
if(ar__9(39:43) .EQ. '') F814Wav_3(i__) = rNULL__
if(ar__9(45:49) .EQ. '') F814WavCor_3(i__) = rNULL__
if(ar__9(51:55) .EQ. '') Vmagph_3(i__) = rNULL__
if(ar__9(57:61) .EQ. '') Vmagav_3(i__) = rNULL__
if(ar__9(63:67) .EQ. '') Imagph_3(i__) = rNULL__
if(ar__9(69:73) .EQ. '') Imagav_3(i__) = rNULL__
if(ar__9(75:79) .EQ. '') chi2_sigma_3(i__) = rNULL__
c ..............Just test output...........
write(6,10)
+ v_FBK98__9(i__),l_Per_3(i__),Per_3(i__),l_Per2_3(i__),
+ Per2_3(i__),F555Wph_3(i__),F555Wav_3(i__),F814Wph_3(i__),
+ F814WphCor_3(i__),F814Wav_3(i__),F814WavCor_3(i__),
+ Vmagph_3(i__),Vmagav_3(i__),Imagph_3(i__),Imagav_3(i__),
+ chi2_sigma_3(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table17.dat' ! Photometry for the PC secondary standards
C Format for file interpretation
11 format(
+ F6.2,1X,F6.2,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,
+ F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table17.dat')
write(6,*) '....Loading file: table17.dat'
do i__=1,24
read(1,'(A71)')ar__10
read(ar__10,11)
+ Xpos_2(i__),Ypos_2(i__),RAh_2(i__),RAm_2(i__),RAs_2(i__),
+ DE__2(i__),DEd_2(i__),DEm_2(i__),DEs_2(i__),F555W(i__),
+ e_F555W(i__),F814W(i__),e_F814W(i__),Vmag(i__),Imag(i__)
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(6,11)
+ Xpos_2(i__),Ypos_2(i__),RAh_2(i__),RAm_2(i__),RAs_2(i__),
+ DE__2(i__),DEd_2(i__),DEm_2(i__),DEs_2(i__),F555W(i__),
+ e_F555W(i__),F814W(i__),e_F814W(i__),Vmag(i__),Imag(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 'table18.dat' ! Photometry for the WF2 secondary standards
C Format for file interpretation
12 format(
+ F6.2,1X,F6.2,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,
+ F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table18.dat')
write(6,*) '....Loading file: table18.dat'
do i__=1,29
read(1,'(A71)')ar__11
read(ar__11,12)
+ Xpos_3(i__),Ypos_3(i__),RAh_3(i__),RAm_3(i__),RAs_3(i__),
+ DE__3(i__),DEd_3(i__),DEm_3(i__),DEs_3(i__),F555W_1(i__),
+ e_F555W_1(i__),F814W_1(i__),e_F814W_1(i__),Vmag_1(i__),
+ Imag_1(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_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(6,12)
+ Xpos_3(i__),Ypos_3(i__),RAh_3(i__),RAm_3(i__),RAs_3(i__),
+ DE__3(i__),DEd_3(i__),DEm_3(i__),DEs_3(i__),F555W_1(i__),
+ e_F555W_1(i__),F814W_1(i__),e_F814W_1(i__),Vmag_1(i__),
+ Imag_1(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 'table19.dat' ! Photometry for the WF3 secondary standards
C Format for file interpretation
13 format(
+ F6.2,1X,F6.2,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,
+ F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table19.dat')
write(6,*) '....Loading file: table19.dat'
do i__=1,32
read(1,'(A71)')ar__12
read(ar__12,13)
+ Xpos_4(i__),Ypos_4(i__),RAh_4(i__),RAm_4(i__),RAs_4(i__),
+ DE__4(i__),DEd_4(i__),DEm_4(i__),DEs_4(i__),F555W_2(i__),
+ e_F555W_2(i__),F814W_2(i__),e_F814W_2(i__),Vmag_2(i__),
+ Imag_2(i__)
RAdeg_4(i__) = rNULL__
DEdeg_4(i__) = rNULL__
c Derive coordinates RAdeg_4 and DEdeg_4 from input data
c (RAdeg_4 and DEdeg_4 are set to rNULL__ when unknown)
if(RAh_4(i__) .GT. -180) RAdeg_4(i__)=RAh_4(i__)*15.
if(RAm_4(i__) .GT. -180) RAdeg_4(i__)=RAdeg_4(i__)+RAm_4(i__)/4.
if(RAs_4(i__) .GT. -180) RAdeg_4(i__)=RAdeg_4(i__)+RAs_4(i__)/240.
if(DEd_4(i__) .GE. 0) DEdeg_4(i__)=DEd_4(i__)
if(DEm_4(i__) .GE. 0) DEdeg_4(i__)=DEdeg_4(i__)+DEm_4(i__)/60.
if(DEs_4(i__) .GE. 0) DEdeg_4(i__)=DEdeg_4(i__)+DEs_4(i__)/3600.
if(DE__4(i__).EQ.'-'.AND.DEdeg_4(i__).GE.0) DEdeg_4(i__)=-DEdeg_4(i__)
c ..............Just test output...........
write(6,13)
+ Xpos_4(i__),Ypos_4(i__),RAh_4(i__),RAm_4(i__),RAs_4(i__),
+ DE__4(i__),DEd_4(i__),DEm_4(i__),DEs_4(i__),F555W_2(i__),
+ e_F555W_2(i__),F814W_2(i__),e_F814W_2(i__),Vmag_2(i__),
+ Imag_2(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_4(i__),DEdeg_4(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table20.dat' ! Photometry for the WF4 secondary standards
C Format for file interpretation
14 format(
+ F6.2,1X,F6.2,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,
+ F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table20.dat')
write(6,*) '....Loading file: table20.dat'
do i__=1,29
read(1,'(A71)')ar__13
read(ar__13,14)
+ Xpos_5(i__),Ypos_5(i__),RAh_5(i__),RAm_5(i__),RAs_5(i__),
+ DE__5(i__),DEd_5(i__),DEm_5(i__),DEs_5(i__),F555W_3(i__),
+ e_F555W_3(i__),F814W_3(i__),e_F814W_3(i__),Vmag_3(i__),
+ Imag_3(i__)
RAdeg_5(i__) = rNULL__
DEdeg_5(i__) = rNULL__
c Derive coordinates RAdeg_5 and DEdeg_5 from input data
c (RAdeg_5 and DEdeg_5 are set to rNULL__ when unknown)
if(RAh_5(i__) .GT. -180) RAdeg_5(i__)=RAh_5(i__)*15.
if(RAm_5(i__) .GT. -180) RAdeg_5(i__)=RAdeg_5(i__)+RAm_5(i__)/4.
if(RAs_5(i__) .GT. -180) RAdeg_5(i__)=RAdeg_5(i__)+RAs_5(i__)/240.
if(DEd_5(i__) .GE. 0) DEdeg_5(i__)=DEd_5(i__)
if(DEm_5(i__) .GE. 0) DEdeg_5(i__)=DEdeg_5(i__)+DEm_5(i__)/60.
if(DEs_5(i__) .GE. 0) DEdeg_5(i__)=DEdeg_5(i__)+DEs_5(i__)/3600.
if(DE__5(i__).EQ.'-'.AND.DEdeg_5(i__).GE.0) DEdeg_5(i__)=-DEdeg_5(i__)
c ..............Just test output...........
write(6,14)
+ Xpos_5(i__),Ypos_5(i__),RAh_5(i__),RAm_5(i__),RAs_5(i__),
+ DE__5(i__),DEd_5(i__),DEm_5(i__),DEs_5(i__),F555W_3(i__),
+ e_F555W_3(i__),F814W_3(i__),e_F814W_3(i__),Vmag_3(i__),
+ Imag_3(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_5(i__),DEdeg_5(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'note5.dat' ! Individual notes on Cepheids
C Format for file interpretation
15 format(A3,1X,A76)
C Effective file loading
open(unit=1,status='old',file=
+'note5.dat')
write(6,*) '....Loading file: note5.dat'
do i__=1,44
read(1,'(A80)')ar__14
read(ar__14,15)v_FBK98__10(i__),Note(i__)
c ..............Just test output...........
write(6,15)v_FBK98__10(i__),Note(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'note12.dat' ! Individual notes on other variable stars
C Format for file interpretation
16 format(A3,1X,A76)
C Effective file loading
open(unit=1,status='old',file=
+'note12.dat')
write(6,*) '....Loading file: note12.dat'
do i__=1,46
read(1,'(A80)')ar__15
read(ar__15,16)v_FBK98__11(i__),Note_1(i__)
c ..............Just test output...........
write(6,16)v_FBK98__11(i__),Note_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end