Conversion of standardized ReadMe file for
file /./ftp/cats/J/MNRAS/448/1044 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-Mar-28 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/MNRAS/448/1044 Simulation data for 50 planetary model systems (Hansen+, 2015) *================================================================================ *Secular effects of tidal damping in compact planetary systems. * Hansen B.M.S., Murray N. * <Mon. Not. R. Astron. Soc., 448, 1044-1059 (2015)> * =2015MNRAS.448.1044H (SIMBAD/NED BibCode) C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'tablea1.dat' ! Initial Conditions for each of the 50 model systems integer*4 nr__ parameter (nr__=294) ! Number of records character*60 ar__ ! Full-size record integer*4 Model (nr__) ! [1/50] Model system number integer*4 Num (nr__) ! [1/10] Condition number real*4 a (nr__) ! (AU) Semi-major axis, in AU real*4 M (nr__) ! (Mgeo) Planet mass, in earth mass real*4 v_e_ (nr__) ! Eccentricity <e^2^>^1/2^ (1) real*4 omega (nr__) ! (deg) Longitude of periastron {omega} real*4 v_i_ (nr__) ! (deg) Inclination <i^2^>^1/2^ (1) real*4 Omega_1 (nr__) ! (deg) Longitude of ascending node {Omega} character*14 emode (nr__) ! Indicates to which eccentricity oscillation * mode(s) each planet is strongly coupled (2) *Note (1): The eccentricities and inclinations are shown as the average of each * planet over the secular oscillations given the initial configuration. *Note (2): Modes are numbered by frequency, with one being the highest frequency * mode. In most cases, this is the frequency of the mode dominated by * the innermost planet, although this is sometimes superseded if there * is a near-commensurability in the system. * The numerical labels indicate which planets (counting from inside out) * are strongly coupled in the sense defined in Section 2.1. c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'tablea2.dat' ! Final conditions of model systems shown in Table A1, after 10^10^ yr of evolution with Q'_p_=10 integer*4 nr__1 parameter (nr__1=245) ! Number of records character*60 ar__1 ! Full-size record integer*4 Model_1 (nr__1) ! [1/50] Model system number integer*4 Num_1 (nr__1) ! [1/10] Condition number real*4 a_1 (nr__1) ! (AU) Semi-major axis, in AU real*4 M_1 (nr__1) ! (Mgeo) Planet mass, in earth mass real*4 v_e__1 (nr__1) ! Eccentricity <e^2^>^1/2^ (1) real*4 omega_2 (nr__1) ! (deg) Longitude of periastron {omega} real*4 v_i__1 (nr__1) ! (deg) Inclination <i^2^>^1/2^ (1) real*4 Omega_3 (nr__1) ! (deg) Longitude of ascending node {Omega} character*14 emode_1 (nr__1) ! Indicates to which eccentricity oscillation * mode(s) each planet is strongly coupled (2) *Note (1): The eccentricities and inclinations are shown as the average of each * planet over the secular oscillations given the initial configuration. *Note (2): Modes are numbered by frequency, with one being the highest frequency * mode. In most cases, this is the frequency of the mode dominated by * the innermost planet, although this is sometimes superseded if there * is a near-commensurability in the system. * The numerical labels indicate which planets (counting from inside out) * are strongly coupled in the sense defined in Section 2.1. C============================================================================= C Loading file 'tablea1.dat' ! Initial Conditions for each of the 50 model * systems C Format for file interpretation 1 format( + I2,1X,I2,1X,F5.3,1X,F6.3,1X,F5.3,1X,F6.2,1X,F6.3,1X,F6.2,1X, + A14) C Effective file loading open(unit=1,status='old',file= +'tablea1.dat') write(6,*) '....Loading file: tablea1.dat' do i__=1,294 read(1,'(A60)')ar__ read(ar__,1) + Model(i__),Num(i__),a(i__),M(i__),v_e_(i__),omega(i__), + v_i_(i__),Omega_1(i__),emode(i__) c ..............Just test output........... write(6,1) + Model(i__),Num(i__),a(i__),M(i__),v_e_(i__),omega(i__), + v_i_(i__),Omega_1(i__),emode(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'tablea2.dat' ! Final conditions of model systems shown in * Table A1, after 10^10^ yr of evolution with * Q'_p_=10 C Format for file interpretation 2 format( + I2,1X,I2,1X,F5.3,1X,F6.3,1X,F5.3,1X,F6.2,1X,F6.3,1X,F6.2,1X, + A14) C Effective file loading open(unit=1,status='old',file= +'tablea2.dat') write(6,*) '....Loading file: tablea2.dat' do i__=1,245 read(1,'(A60)')ar__1 read(ar__1,2) + Model_1(i__),Num_1(i__),a_1(i__),M_1(i__),v_e__1(i__), + omega_2(i__),v_i__1(i__),Omega_3(i__),emode_1(i__) c ..............Just test output........... write(6,2) + Model_1(i__),Num_1(i__),a_1(i__),M_1(i__),v_e__1(i__), + omega_2(i__),v_i__1(i__),Omega_3(i__),emode_1(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= stop end