Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/835/172 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/ApJ/835/172 Kepler asteroseismic LEGACY sample. I. Oscillations (Lund+, 2017)
*================================================================================
*Standing on the shoulders of dwarfs: the Kepler asteroseismic LEGACY sample.
*I. Oscillation mode parameters.
* Lund M.N., Silva Aguirre V., Davies G.R., Chaplin W.J.,
* Christensen-Dalsgaard J., Houdek G., White T.R., Bedding T.R., Ball W.H.,
* Huber D., Antia H.M., Lebreton Y., Latham D.W., Handberg R., Verma K.,
* Basu S., Casagrande L., Justesen A.B., Kjeldsen H., Mosumgaard J.R.
* <Astrophys. J., 835, 172-172 (2017)>
* =2017ApJ...835..172L (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Parameters for the targets in the studied sample
integer*4 nr__
parameter (nr__=66) ! Number of records
character*139 ar__ ! Full-size record
character*8 KIC (nr__) ! KIC number
character*9 Name (nr__) ! Popular name
real*4 Kpmag (nr__) ! (mag) [5.8/11] Kepler magnitude
integer*4 numax (nr__) ! (uHz) [885/4197] Frequency of maximum amplitude
* ({nu}_max_) (1)
real*4 Dnu (nr__) ! (uHz) [48.4/173.5] Large frequency separation
* ({Delta}{nu}) (1)
integer*4 N (nr__) ! [22/59] Number of peak-bagged modes
character*6 Cat (nr__) ! Category according
* to Appourchaux+ (2012A&A...543A..54A);
* "F-like" or "Simple" (44 occurrences)
character*8 BkQ (nr__) ! Braketing quarters (2)
character*18 MgQ (nr__) ! Missing quarters (2)
integer*4 Teff (nr__) ! (K) [5180/6642] Effective temperature (3)
integer*4 e_Teff (nr__) ! (K) [50/180] Teff uncertainty (4)
integer*4 r_Teff (nr__) ! [1/6]? Reference for Teff (5)
real*4 v_Fe_H_ (nr__) ! ([-]) [-1/0.4] Metallicity (3)
real*4 e__Fe_H_ (nr__) ! ([-]) [0.02/0.2] [Fe/H] uncertainty (4)
integer*4 r__Fe_H_ (nr__) ! [1/6]? Reference for [Fe/H] (5)
real*4 logg (nr__) ! ([cm/s2]) [3.9/4.6] Log surface gravity from Paper II
* (Silva Aguirre+, 2017, J/ApJ/835/173)
real*4 e_logg (nr__) ! ([cm/s2]) [0.002/0.02] Negative uncertainty on logg
real*4 E_logg_1 (nr__) ! ([cm/s2]) [0.002/0.02] Positive uncertainty on logg
real*8 Vlos (nr__) ! (km/s) [-116/32]? Line-of-sight velocity (3)
real*4 e_Vlos (nr__) ! (km/s) [0.1]? Vlos uncertainty
real*4 vsini (nr__) ! (km/s) [0/24.1]? Rotational velocity (3)
real*4 e_vsini (nr__) ! (km/s) [0.5]? vsini uncertainty
*Note (1): For uncertainties in {nu}_max_ and {Delta}{nu} see Table 2.
*Note (2): First-last Kepler quarters during which the targets were observed in
* short-cadence (SC), and which quarters were missing in between.
*Note (3): Metallicities, temperatures, line of sight (LOS) velocities, and
* vsini values are adopted from the Stellar Parameters Classification
* tool (SPC; see Buchhave+ 2012, J/other/Nat/486.375) analysis of the
* targets unless otherwise indicated (see Note (5)).
*Note (4): Systematic uncertainties of +/-59K (Teff) and +/-0.062dex ([Fe/H])
* have been added in quadrature as suggested
* by Torres+ (2012, J/ApJ/757/161).
*Note (5): Reference as follows:
* 1 = Pinsonneault et al. (2012, J/ApJS/199/30)
* 2 = Pinsonneault et al. (2014, J/ApJS/215/19)
* 3 = the SAGA project (Casagrande+ 2014, J/ApJ/787/110;
* see http://www.mso.anu.edu.au/saga/saga_home.html)
* 4 = Ramirez et al. (2009, J/A+A/508/L17)
* 5 = Chaplin et al. (2014, J/ApJS/210/1)
* 6 = Huber et al. (2013, J/ApJ/767/127)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6.dat' ! *Extracted mode parameters and quality control
(Equations in section 3.2.3) for all sources
including the Sun
integer*4 nr__1
parameter (nr__1=2927) ! Number of records
character*96 ar__1 ! Full-size record
character*8 KIC_1 (nr__1) ! Kepler Input Catalog Identifier or "Sun"
integer*4 n_1 (nr__1) ! [8/31] Radial order
integer*4 l (nr__1) ! [0/3] Angular degree
real*8 Freq (nr__1) ! (uHz) [527.6/5729.7] Frequency
real*8 e_Freq (nr__1) ! (uHz) [0.03/6] Lower error on Freq
real*8 E_Freq_1 (nr__1) ! (uHz) [0.03/6] Upper error on Freq
real*8 Amp (nr__1) ! (ppm) [0.05/6.5]? Amplitude
real*8 e_Amp (nr__1) ! (ppm) [0.02/0.8]? Lower error on Amp
real*8 E_Amp_1 (nr__1) ! (ppm) [0.03/0.7]? Upper error on Amp
real*8 Width (nr__1) ! (uHz) [0.2/14.9]? Line width
real*8 e_Width (nr__1) ! (uHz) [0.04/4.3]? Lower error on Width
real*8 E_Width_1 (nr__1) ! (uHz) [0.04/7.5]? Upper error on Width
character*1 l_lnK (nr__1) ! Limit flag on lnK
real*4 lnK (nr__1) ! ([-]) [-1.4/6] Natural log of Bayes factor
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table7.dat' ! *The calculated mode frequency difference ratios
r_01,10,02(n)_ (Equation 16) for all sources
including the Sun
integer*4 nr__2
parameter (nr__2=2541) ! Number of records
character*42 ar__2 ! Full-size record
character*8 KIC_2 (nr__2) ! Kepler Input Catalog Identifier or "Sun"
character*5 Type (nr__2) ! Ratio type (r_01_, r_02_ or r_10_) (1)
integer*4 n_2 (nr__2) ! [10/30] Radial order
real*8 Ratio (nr__2) ! [-0.02/0.15] Mode frequency difference ratio
real*8 e_Ratio (nr__2) ! [0.0003/0.07] Lower error on Ratio
real*8 E_Ratio_1 (nr__2) ! [0.0003/0.06] Upper error on Ratio
*Note (1): Corresponding to the frequency ratios defined as
* (Roxburgh & Vorontsov 2003A&A...411..215R):
* r_01_(n)=d_01_(n)/{Delta}{nu}_1_(n),
* r_10_(n)=d_10_(n)/{Delta}{nu}_0_(n+1),
* r_02_(n)=({nu}_n,0_-{nu}_n-1,2_)/{Delta}{nu}_1_(n)
* See Equation 16 in section 3.3.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table8.dat' ! *Calculated second differences {Delta}_2_{nu}(n,l)
(Equation 20) for all sources and the Sun
integer*4 nr__3
parameter (nr__3=2489) ! Number of records
character*41 ar__3 ! Full-size record
character*8 KIC_3 (nr__3) ! Kepler Input Catalog Identifier or "Sun"
integer*4 n_3 (nr__3) ! [9/30] Radial order
integer*4 l_1 (nr__3) ! [0/3] Angular degree
real*8 Del2nu (nr__3) ! (uHz) [-11.4/12.1] Calculated 2nd difference
* {Delta}_2_{nu} (1)
real*8 e_Del2nu (nr__3) ! (uHz) [0.05/15.5] Lower error in Del2nu
real*8 E_Del2nu_1 (nr__3) ! (uHz) [0.06/12.1] Upper error in Del2nu
*Note (1): The second differences - Equation (20):
* {Delta}_2_{nu}(n,l)={nu}_n-1,l_-2{nu}_n,l_+{nu}_n+1,l_
C=============================================================================
C Loading file 'table1.dat' ! Parameters for the targets in the studied sample
C Format for file interpretation
1 format(
+ A8,1X,A9,1X,F5.2,1X,I4,1X,F5.1,1X,I2,1X,A6,1X,A8,1X,A18,1X,I4,
+ 1X,I3,1X,I1,1X,F5.2,1X,F4.2,1X,I1,1X,F5.3,1X,F5.3,1X,F5.3,1X,
+ F7.2,1X,F4.2,1X,F5.2,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,66
read(1,'(A139)')ar__
read(ar__,1)
+ KIC(i__),Name(i__),Kpmag(i__),numax(i__),Dnu(i__),N(i__),
+ Cat(i__),BkQ(i__),MgQ(i__),Teff(i__),e_Teff(i__),r_Teff(i__),
+ v_Fe_H_(i__),e__Fe_H_(i__),r__Fe_H_(i__),logg(i__),
+ e_logg(i__),E_logg_1(i__),Vlos(i__),e_Vlos(i__),vsini(i__),
+ e_vsini(i__)
if(ar__(84:84) .EQ. '') r_Teff(i__) = iNULL__
if(ar__(97:97) .EQ. '') r__Fe_H_(i__) = iNULL__
if(ar__(117:123) .EQ. '') Vlos(i__) = rNULL__
if(ar__(125:128) .EQ. '') e_Vlos(i__) = rNULL__
if(ar__(130:134) .EQ. '') vsini(i__) = rNULL__
if(ar__(136:139) .EQ. '') e_vsini(i__) = rNULL__
c ..............Just test output...........
write(6,1)
+ KIC(i__),Name(i__),Kpmag(i__),numax(i__),Dnu(i__),N(i__),
+ Cat(i__),BkQ(i__),MgQ(i__),Teff(i__),e_Teff(i__),r_Teff(i__),
+ v_Fe_H_(i__),e__Fe_H_(i__),r__Fe_H_(i__),logg(i__),
+ e_logg(i__),E_logg_1(i__),Vlos(i__),e_Vlos(i__),vsini(i__),
+ e_vsini(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table6.dat' ! *Extracted mode parameters and quality control
* (Equations in section 3.2.3) for all sources
* including the Sun
C Format for file interpretation
2 format(
+ A8,1X,I2,1X,I1,1X,F10.5,1X,F7.5,1X,F7.5,1X,F7.5,1X,F7.5,1X,
+ F7.5,1X,F8.5,1X,F7.5,1X,F7.5,1X,A1,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table6.dat')
write(6,*) '....Loading file: table6.dat'
do i__=1,2927
read(1,'(A96)')ar__1
read(ar__1,2)
+ KIC_1(i__),n_1(i__),l(i__),Freq(i__),e_Freq(i__),
+ E_Freq_1(i__),Amp(i__),e_Amp(i__),E_Amp_1(i__),Width(i__),
+ e_Width(i__),E_Width_1(i__),l_lnK(i__),lnK(i__)
if(ar__1(42:48) .EQ. '') Amp(i__) = rNULL__
if(ar__1(50:56) .EQ. '') e_Amp(i__) = rNULL__
if(ar__1(58:64) .EQ. '') E_Amp_1(i__) = rNULL__
if(ar__1(66:73) .EQ. '') Width(i__) = rNULL__
if(ar__1(75:81) .EQ. '') e_Width(i__) = rNULL__
if(ar__1(83:89) .EQ. '') E_Width_1(i__) = rNULL__
c ..............Just test output...........
write(6,2)
+ KIC_1(i__),n_1(i__),l(i__),Freq(i__),e_Freq(i__),
+ E_Freq_1(i__),Amp(i__),e_Amp(i__),E_Amp_1(i__),Width(i__),
+ e_Width(i__),E_Width_1(i__),l_lnK(i__),lnK(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table7.dat' ! *The calculated mode frequency difference ratios
* r_01,10,02(n)_ (Equation 16) for all sources
* including the Sun
C Format for file interpretation
3 format(A8,1X,A5,1X,I2,1X,F8.5,1X,F7.5,1X,F7.5)
C Effective file loading
open(unit=1,status='old',file=
+'table7.dat')
write(6,*) '....Loading file: table7.dat'
do i__=1,2541
read(1,'(A42)')ar__2
read(ar__2,3)
+ KIC_2(i__),Type(i__),n_2(i__),Ratio(i__),e_Ratio(i__),
+ E_Ratio_1(i__)
c ..............Just test output...........
write(6,3)
+ KIC_2(i__),Type(i__),n_2(i__),Ratio(i__),e_Ratio(i__),
+ E_Ratio_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table8.dat' ! *Calculated second differences {Delta}_2_{nu}(n,l)
* (Equation 20) for all sources and the Sun
C Format for file interpretation
4 format(A8,1X,I2,1X,I1,1X,F9.5,1X,F8.5,1X,F8.5)
C Effective file loading
open(unit=1,status='old',file=
+'table8.dat')
write(6,*) '....Loading file: table8.dat'
do i__=1,2489
read(1,'(A41)')ar__3
read(ar__3,4)
+ KIC_3(i__),n_3(i__),l_1(i__),Del2nu(i__),e_Del2nu(i__),
+ E_Del2nu_1(i__)
c ..............Just test output...........
write(6,4)
+ KIC_3(i__),n_3(i__),l_1(i__),Del2nu(i__),e_Del2nu(i__),
+ E_Del2nu_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end