Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/157/217 into FORTRAN code for reading data files line by line.
Note that special values are assigned to unknown or unspecified
numbers (also called NULL numbers);
when necessary, the coordinate components making up the right ascension
and declination are converted into floating-point numbers
representing these angles in degrees.
program load_ReadMe
C=============================================================================
C F77-compliant program generated by readme2f_1.81 (2015-09-23), on 2026-May-18
C=============================================================================
* This code was generated from the ReadMe file documenting a catalogue
* according to the "Standard for Documentation of Astronomical Catalogues"
* currently in use by the Astronomical Data Centers (CDS, ADC, A&A)
* (see full documentation at URL http://vizier.u-strasbg.fr/doc/catstd.htx)
* Please report problems or questions to
C=============================================================================
implicit none
* Unspecified or NULL values, generally corresponding to blank columns,
* are assigned one of the following special values:
* rNULL__ for unknown or NULL floating-point values
* iNULL__ for unknown or NULL integer values
real*4 rNULL__
integer*4 iNULL__
parameter (rNULL__=--2147483648.) ! NULL real number
parameter (iNULL__=(-2147483647-1)) ! NULL int number
integer idig ! testing NULL number
C=============================================================================
Cat. J/AJ/157/217 Transit times of five hot Jupiter WASP exoplanets (Bouma+, 2019)
*================================================================================
*WASP-4b arrived early for the TESS mission.
* Bouma L.G., Winn J.N., Baxter C., Bhatti W., Dai F., Daylan T.,
* Desert J.-M., Hill M.L., Kane S.R., Stassun K.G., Villasenor J.,
* Ricker G.R., Vanderspek R., Latham D.W., Seager S., Jenkins J.M.,
* Berta-Thompson Z., Colon K., Fausnaugh M., Glidden A., Guerrero N.,
* Rodriguez J.E., Twicken J.D., Wohler B.
* <Astron. J., 157, 217-217 (2019)>
* =2019AJ....157..217B (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! WASP-4b transit times, uncertainties,
and references
integer*4 nr__
parameter (nr__=59) ! Number of records
character*90 ar__ ! Full-size record
real*8 Ttra ! (d) Measured transit midtime (BJD_TDB_) (1)
real*8 e_Ttra ! (d) [5e-05/0.00184] 1{sigma} uncertainty in Ttra (2)
integer*4 Epoch ! [-4037/1925] Epoch
integer*4 H13 ! [0/1]? The midtime value was taken from
* Hoyer et al. (2013MNRAS.434...46H) (=1) or
* from Ref (=0) (only in Table 2)
character*25 Ref ! Reference describing the original observations
* (3)
character*19 Bibcode ! Bibcode of the reference
character*14 Com ! Comment on Ref
*Note (1): In Table 5: all of the literature times except for the two
* Moyano et al. (2017MNRAS.471..650M) times are from the homogeneous
* Hoyer et al. (2012ApJ...748...22H) analysis.
* In Table 7: all of the literature times are from the homogeneous
* Wilkins et al. (2017ApJ...836L..24W) analysis.
* In Table 8: all of the literature times are from the homogeneous
* Petrucci et al. (2018MNRAS.473.5126P) analysis. Fourteen of the light curves
* were acquired by ETD observers (see Petrucci et al. 2018MNRAS.473.5126P).
*Note (2): {sigma}_Ttra_ was evaluated from the sampled posteriors by taking the
* maximum of the difference between the 84th percentile minus the median, and
* the median minus the 16th percentile. The resulting error variances then
* appeared to have been overestimated, so we lowered the uncertainties as
* described in Section 2.2.
*Note (3): In Table 2, The Hoyer et al. (2013MNRAS.434...46H) BJD_TT_ times are
* equal to BJD_TDB_ for our purposes (Urban & Seidelmann 2012, Explanatory
* Supplement to the Astronomical Almanac (Mill Valley, CA: Univ. Science
* Books)). We omitted the timing measurements from Southworth et al. (2009,
* J/MNRAS/396/1023) because there were technical problems with the computer
* clock at the time of observation (Nikolov et al. 2012, J/A+A/539/A159). The
* two C. Baxter et al. (2019, in preparation) times were obtained from
* Spitzer/IRAC transit light curves in the 3.6 and 4.5 {mu}m channels.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! WASP-5b transit times, uncertainties,
and references
integer*4 nr__1
parameter (nr__1=39) ! Number of records
character*90 ar__1 ! Full-size record
real*8 Ttra_1 ! (d) Measured transit midtime (BJD_TDB_) (1)
real*8 e_Ttra_1 ! (d) [5e-05/0.00184] 1{sigma} uncertainty in Ttra (2)
integer*4 Epoch_1 ! [-4037/1925] Epoch
integer*4 H13_1 ! [0/1]? The midtime value was taken from
* Hoyer et al. (2013MNRAS.434...46H) (=1) or
* from Ref (=0) (only in Table 2)
character*25 Ref_1 ! Reference describing the original observations
* (3)
character*19 Bibcode_1 ! Bibcode of the reference
character*14 Com_1 ! Comment on Ref
*Note (1): In Table 5: all of the literature times except for the two
* Moyano et al. (2017MNRAS.471..650M) times are from the homogeneous
* Hoyer et al. (2012ApJ...748...22H) analysis.
* In Table 7: all of the literature times are from the homogeneous
* Wilkins et al. (2017ApJ...836L..24W) analysis.
* In Table 8: all of the literature times are from the homogeneous
* Petrucci et al. (2018MNRAS.473.5126P) analysis. Fourteen of the light curves
* were acquired by ETD observers (see Petrucci et al. 2018MNRAS.473.5126P).
*Note (2): {sigma}_Ttra_ was evaluated from the sampled posteriors by taking the
* maximum of the difference between the 84th percentile minus the median, and
* the median minus the 16th percentile. The resulting error variances then
* appeared to have been overestimated, so we lowered the uncertainties as
* described in Section 2.2.
*Note (3): In Table 2, The Hoyer et al. (2013MNRAS.434...46H) BJD_TT_ times are
* equal to BJD_TDB_ for our purposes (Urban & Seidelmann 2012, Explanatory
* Supplement to the Astronomical Almanac (Mill Valley, CA: Univ. Science
* Books)). We omitted the timing measurements from Southworth et al. (2009,
* J/MNRAS/396/1023) because there were technical problems with the computer
* clock at the time of observation (Nikolov et al. 2012, J/A+A/539/A159). The
* two C. Baxter et al. (2019, in preparation) times were obtained from
* Spitzer/IRAC transit light curves in the 3.6 and 4.5 {mu}m channels.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6.dat' ! WASP-6b transit times, uncertainties,
and references
integer*4 nr__2
parameter (nr__2=18) ! Number of records
character*90 ar__2 ! Full-size record
real*8 Ttra_2 ! (d) Measured transit midtime (BJD_TDB_) (1)
real*8 e_Ttra_2 ! (d) [5e-05/0.00184] 1{sigma} uncertainty in Ttra (2)
integer*4 Epoch_2 ! [-4037/1925] Epoch
integer*4 H13_2 ! [0/1]? The midtime value was taken from
* Hoyer et al. (2013MNRAS.434...46H) (=1) or
* from Ref (=0) (only in Table 2)
character*25 Ref_2 ! Reference describing the original observations
* (3)
character*19 Bibcode_2 ! Bibcode of the reference
character*14 Com_2 ! Comment on Ref
*Note (1): In Table 5: all of the literature times except for the two
* Moyano et al. (2017MNRAS.471..650M) times are from the homogeneous
* Hoyer et al. (2012ApJ...748...22H) analysis.
* In Table 7: all of the literature times are from the homogeneous
* Wilkins et al. (2017ApJ...836L..24W) analysis.
* In Table 8: all of the literature times are from the homogeneous
* Petrucci et al. (2018MNRAS.473.5126P) analysis. Fourteen of the light curves
* were acquired by ETD observers (see Petrucci et al. 2018MNRAS.473.5126P).
*Note (2): {sigma}_Ttra_ was evaluated from the sampled posteriors by taking the
* maximum of the difference between the 84th percentile minus the median, and
* the median minus the 16th percentile. The resulting error variances then
* appeared to have been overestimated, so we lowered the uncertainties as
* described in Section 2.2.
*Note (3): In Table 2, The Hoyer et al. (2013MNRAS.434...46H) BJD_TT_ times are
* equal to BJD_TDB_ for our purposes (Urban & Seidelmann 2012, Explanatory
* Supplement to the Astronomical Almanac (Mill Valley, CA: Univ. Science
* Books)). We omitted the timing measurements from Southworth et al. (2009,
* J/MNRAS/396/1023) because there were technical problems with the computer
* clock at the time of observation (Nikolov et al. 2012, J/A+A/539/A159). The
* two C. Baxter et al. (2019, in preparation) times were obtained from
* Spitzer/IRAC transit light curves in the 3.6 and 4.5 {mu}m channels.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table7.dat' ! WASP-18b transit times, uncertainties,
and references
integer*4 nr__3
parameter (nr__3=58) ! Number of records
character*90 ar__3 ! Full-size record
real*8 Ttra_3 ! (d) Measured transit midtime (BJD_TDB_) (1)
real*8 e_Ttra_3 ! (d) [5e-05/0.00184] 1{sigma} uncertainty in Ttra (2)
integer*4 Epoch_3 ! [-4037/1925] Epoch
integer*4 H13_3 ! [0/1]? The midtime value was taken from
* Hoyer et al. (2013MNRAS.434...46H) (=1) or
* from Ref (=0) (only in Table 2)
character*25 Ref_3 ! Reference describing the original observations
* (3)
character*19 Bibcode_3 ! Bibcode of the reference
character*14 Com_3 ! Comment on Ref
*Note (1): In Table 5: all of the literature times except for the two
* Moyano et al. (2017MNRAS.471..650M) times are from the homogeneous
* Hoyer et al. (2012ApJ...748...22H) analysis.
* In Table 7: all of the literature times are from the homogeneous
* Wilkins et al. (2017ApJ...836L..24W) analysis.
* In Table 8: all of the literature times are from the homogeneous
* Petrucci et al. (2018MNRAS.473.5126P) analysis. Fourteen of the light curves
* were acquired by ETD observers (see Petrucci et al. 2018MNRAS.473.5126P).
*Note (2): {sigma}_Ttra_ was evaluated from the sampled posteriors by taking the
* maximum of the difference between the 84th percentile minus the median, and
* the median minus the 16th percentile. The resulting error variances then
* appeared to have been overestimated, so we lowered the uncertainties as
* described in Section 2.2.
*Note (3): In Table 2, The Hoyer et al. (2013MNRAS.434...46H) BJD_TT_ times are
* equal to BJD_TDB_ for our purposes (Urban & Seidelmann 2012, Explanatory
* Supplement to the Astronomical Almanac (Mill Valley, CA: Univ. Science
* Books)). We omitted the timing measurements from Southworth et al. (2009,
* J/MNRAS/396/1023) because there were technical problems with the computer
* clock at the time of observation (Nikolov et al. 2012, J/A+A/539/A159). The
* two C. Baxter et al. (2019, in preparation) times were obtained from
* Spitzer/IRAC transit light curves in the 3.6 and 4.5 {mu}m channels.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table8.dat' ! WASP-46b transit times, uncertainties,
and references
integer*4 nr__4
parameter (nr__4=62) ! Number of records
character*90 ar__4 ! Full-size record
real*8 Ttra_4 ! (d) Measured transit midtime (BJD_TDB_) (1)
real*8 e_Ttra_4 ! (d) [5e-05/0.00184] 1{sigma} uncertainty in Ttra (2)
integer*4 Epoch_4 ! [-4037/1925] Epoch
integer*4 H13_4 ! [0/1]? The midtime value was taken from
* Hoyer et al. (2013MNRAS.434...46H) (=1) or
* from Ref (=0) (only in Table 2)
character*25 Ref_4 ! Reference describing the original observations
* (3)
character*19 Bibcode_4 ! Bibcode of the reference
character*14 Com_4 ! Comment on Ref
*Note (1): In Table 5: all of the literature times except for the two
* Moyano et al. (2017MNRAS.471..650M) times are from the homogeneous
* Hoyer et al. (2012ApJ...748...22H) analysis.
* In Table 7: all of the literature times are from the homogeneous
* Wilkins et al. (2017ApJ...836L..24W) analysis.
* In Table 8: all of the literature times are from the homogeneous
* Petrucci et al. (2018MNRAS.473.5126P) analysis. Fourteen of the light curves
* were acquired by ETD observers (see Petrucci et al. 2018MNRAS.473.5126P).
*Note (2): {sigma}_Ttra_ was evaluated from the sampled posteriors by taking the
* maximum of the difference between the 84th percentile minus the median, and
* the median minus the 16th percentile. The resulting error variances then
* appeared to have been overestimated, so we lowered the uncertainties as
* described in Section 2.2.
*Note (3): In Table 2, The Hoyer et al. (2013MNRAS.434...46H) BJD_TT_ times are
* equal to BJD_TDB_ for our purposes (Urban & Seidelmann 2012, Explanatory
* Supplement to the Astronomical Almanac (Mill Valley, CA: Univ. Science
* Books)). We omitted the timing measurements from Southworth et al. (2009,
* J/MNRAS/396/1023) because there were technical problems with the computer
* clock at the time of observation (Nikolov et al. 2012, J/A+A/539/A159). The
* two C. Baxter et al. (2019, in preparation) times were obtained from
* Spitzer/IRAC transit light curves in the 3.6 and 4.5 {mu}m channels.
C=============================================================================
C Loading file 'table2.dat' ! WASP-4b transit times, uncertainties,
* and references
C Format for file interpretation
1 format(F13.5,1X,F7.5,1X,I5,1X,I1,1X,A25,1X,A19,1X,A14)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,59
read(1,'(A90)')ar__
read(ar__,1)Ttra,e_Ttra,Epoch,H13,Ref,Bibcode,Com
if(ar__(29:29) .EQ. '') H13 = iNULL__
c ..............Just test output...........
write(6,1)Ttra,e_Ttra,Epoch,H13,Ref,Bibcode,Com
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table5.dat' ! WASP-5b transit times, uncertainties,
* and references
C Format for file interpretation
2 format(F13.5,1X,F7.5,1X,I5,1X,I1,1X,A25,1X,A19,1X,A14)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,39
read(1,'(A90)')ar__1
read(ar__1,2)
+ Ttra_1,e_Ttra_1,Epoch_1,H13_1,Ref_1,Bibcode_1,Com_1
if(ar__1(29:29) .EQ. '') H13_1 = iNULL__
c ..............Just test output...........
write(6,2)
+ Ttra_1,e_Ttra_1,Epoch_1,H13_1,Ref_1,Bibcode_1,Com_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table6.dat' ! WASP-6b transit times, uncertainties,
* and references
C Format for file interpretation
3 format(F13.5,1X,F7.5,1X,I5,1X,I1,1X,A25,1X,A19,1X,A14)
C Effective file loading
open(unit=1,status='old',file=
+'table6.dat')
write(6,*) '....Loading file: table6.dat'
do i__=1,18
read(1,'(A90)')ar__2
read(ar__2,3)
+ Ttra_2,e_Ttra_2,Epoch_2,H13_2,Ref_2,Bibcode_2,Com_2
if(ar__2(29:29) .EQ. '') H13_2 = iNULL__
c ..............Just test output...........
write(6,3)
+ Ttra_2,e_Ttra_2,Epoch_2,H13_2,Ref_2,Bibcode_2,Com_2
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table7.dat' ! WASP-18b transit times, uncertainties,
* and references
C Format for file interpretation
4 format(F13.5,1X,F7.5,1X,I5,1X,I1,1X,A25,1X,A19,1X,A14)
C Effective file loading
open(unit=1,status='old',file=
+'table7.dat')
write(6,*) '....Loading file: table7.dat'
do i__=1,58
read(1,'(A90)')ar__3
read(ar__3,4)
+ Ttra_3,e_Ttra_3,Epoch_3,H13_3,Ref_3,Bibcode_3,Com_3
if(ar__3(29:29) .EQ. '') H13_3 = iNULL__
c ..............Just test output...........
write(6,4)
+ Ttra_3,e_Ttra_3,Epoch_3,H13_3,Ref_3,Bibcode_3,Com_3
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table8.dat' ! WASP-46b transit times, uncertainties,
* and references
C Format for file interpretation
5 format(F13.5,1X,F7.5,1X,I5,1X,I1,1X,A25,1X,A19,1X,A14)
C Effective file loading
open(unit=1,status='old',file=
+'table8.dat')
write(6,*) '....Loading file: table8.dat'
do i__=1,62
read(1,'(A90)')ar__4
read(ar__4,5)
+ Ttra_4,e_Ttra_4,Epoch_4,H13_4,Ref_4,Bibcode_4,Com_4
if(ar__4(29:29) .EQ. '') H13_4 = iNULL__
c ..............Just test output...........
write(6,5)
+ Ttra_4,e_Ttra_4,Epoch_4,H13_4,Ref_4,Bibcode_4,Com_4
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end