Repatch (from linux) of OSX IRAF

1 files changed, 179 insertions, 0 deletions

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+    addet - add the E-terms to a pre IAU 1976 mean place
+     afin - convert a sexagesimal character string to radians (s.p.)
+   airmas - compute the airmass at a given zenith distance 
+    altaz - compute altazimuth positions, velocities, accelerations
+      amp - convert a geocentric apparent to post IAU 1976 mean place
+    ampqk - convert a geocentric apparent to post IAU 1976 mean place 
+      aop - convert an apparent to observed place 
+    aoppa - pre-compute the set of apparent to observed place parameters 
+   aoppat - recompute the apparent to observed place sidereal time parameter 
+    aopqk - convert an apparent to observed place
+   atmdsp - apply atmospheric dispersion terms to refraction coefficients 
+     av2m - compute a rotation matrix from an axial vector (s.p.)
+     bear - compute the bearing of a point on a sphere w.r.t. another
+    caf2r - convert degrees, arcminutes, and arcseconds to radians
+    caldj - convert a Gregorian calendar date to a modified Julian date
+    calyd - convert a Gregorian calendar date to a Julian calendar year, day 
+     cc2s - convert Cartesian to spherical coordinates (s.p.)
+    cc62s - convert a 6-vector from Cartesian to spherical coordinates 
+    cd2tf - convert an interval in days to hours, minutes, and seconds 
+     cldj - convert a Gregorian calendar date to a modified Julian date
+     clyd - convert a Gregorian calendar date a Julian calendar year, day
+    cr2af - convert radians to degrees, arcminutes, and arcseconds
+    cr2tf - convert radians to hours, minutes, and seconds 
+     cs2c - convert spherical to Cartesian coordinates (s.p.)
+    cs2c6 - convert spherical position/velocity  to Cartesian coordinates
+    ctf2d - convert hours, minutes, and seconds to days 
+    ctf2r - convert hours, minutes, and seconds to radians 
+    daf2r - convert degrees, arcminutes, and arcseconds to radians (d.p) 
+    dafin - convert a sexagesimal character string to radians (d.p.)
+      dat - compute difference between TAI and UTC in seconds 
+    dav2m - compute a rotation matrix from an axial vector (d.p)
+    dbear - compute the bearing of a point on a sphere w.r.t. another (d.p.)
+    dbjin - convert a character string to a Besselian/Julian epoch 
+    dc62s - convert Cartesian position/velocity to spherical coordinates (d.p.)
+    dcc2s - convert Cartesian to spherical coordinates  (d.p)
+    dcmpf - convert linear fit coefficients to geometric parameters 
+    dcs2c - convert spherical to Cartesian coordinates (d.p)
+    dd2tf - convert interval in days to hours, minutes, and seconds (d.p.)
+     de2h - convert hour angle and declination to azimuth and elevation (d.p.)
+   deuler - convert Euler angles to a rotation matrix (d.p.)
+   dfltin - convert a character string to a floating point number (d.p.)
+     dh2e - convert azimuth and elevation to hour angle and declination (d.p.)
+    dimxv - apply a 3D reverse rotation to a 3-vector (d.p.)
+    djcal - convert an MJD to a Gregorian calendar date 
+     djcl - convert an MJD to a Gregorian year, month, and day 
+    dm2av - convert a rotation matrix to an axial vector (d.p)
+     dmat - solve a set of simultaneous equations (d.p.)
+    dmoon - compute approximate geocentric position/velocity of moon (d.p.)
+     dmxm - compute the product of two 3X3 matrices (d.p.)
+     dmxv - multiple a 3-vector by a rotation matrix (d.p.)
+     dpav - compute the bearing of a point on a sphere w.r.t. another (d.p.)
+    dr2af - convert radians to degrees, arcminutes, and arcseconds (d.p)
+    dr2tf - convert radians to hours, minutes, and seconds (d.p.)
+   drange - normalize an angle to the range -pi <= angle <= pi (d.p.)
+   dranrm - normalize an angle to the range 0 <= angle <= 2pi (d.p.)
+    ds2c6 - convert spherical position/velocity to Cartesian coordinates (d.p.)
+    ds2tp - project spherical coordinates onto the tangent plane (d.p)
+     dsep - compute the angle between two points on a sphere (d.p.)
+       dt - estimate the approximate difference between ET and UT in seconds
+    dtf2d - convert hours, minutes, and seconds to days (d.p)
+    dtf2r - convert hours, minutes, and seconds to radians (d.p.)
+    dtp2s - convert tangent plane to spherical coordinates (d.p.)
+    dtp2v - convert tangent plane coordinates to direction cosines (d.p.)
+   dtps2c - compute the spherical coordinates of the tangent point (d.p.)
+   dtpv2c - compute the direction cosines of the tangent point (d.p.)
+      dtt - compute the difference between TT and UTC in seconds
+    dv2tp - convert direction cosines to tangent plane coordinates (d.p)
+     dvdv - compute the scalar product of 2 3-vectors (d.p.)
+      dvn - normalize a 3-vector and compute the modulus (d.p.)
+     dvxv - compute the vector product of 2 3-vectors (d.p.)
+      e2h - convert hour angle and declination to azimuth and elevation (d.p.)
+    earth - compute approximate heliocentric position/velocity of earth 
+    ecleq - convert from ecliptic to equatorial FK5 coordinates 
+    ecmat - compute the equatorial FK5 to ecliptic coordinates rotation matrix
+     ecor - compute rv of earth and time correction to sun in given direction
+     eg50 - convert equatorial FK4 to IAU 1958 galactic coordinates 
+    el2ue - convert osculating orbital elements into universal form
+      epb - convert an MJD to a Besselian epoch
+    epb2d - convert a Besselian epoch to an MJD
+     epco - convert a Besselian/Julian epoch to match a given epoch
+      epj - convert an MJD to a Julian epoch 
+    epj2d - convert a Julian epoch to an MJD
+    eqecl - convert equatorial FK5 to ecliptic coordinates
+    eqeqx - compute the equation of the equinoxes
+    eqgal - convert equatorial FK5 to IAU 1958 galactic coordinates
+    etrms - compute the E-terms vector 
+    euler - convert Euler angles to a rotation matrix (s.p.)
+      evp - compute the barycentric/heliocentric velocity/position of earth
+    fitxy - fit a linear model to 2 sets of [x,y] coordinates
+    fk425 - convert equatorial FK4 to FK5 coordinates
+    fk45z - convert equatorial FK4 to FK5 coordinates excluding proper motion 
+    fk524 - convert equatorial FK5 to FK4 coordinates
+    fk54z - convert equatorial FK5 to FK4 coordinates excluding proper motion
+    fk52h - convert equatorial FK5 to ICRS coordinates
+    fk5hz - Convert equatorial FK5 to ICRS coordinates (0 ICRS proper motions)
+   flotin - convert a character string to a floating point number
+    galeq - convert IAU 1958 galactic to equatorial FK5 coordinates
+   galsup - convert IAU 1958 galactic to deVaucouleurs supergalactic coordinates
+     ge50 - convert IAU 1958 galactic to equatorial FK4 coordinates 
+     geoc - convert geodetic to geocentric position 
+     gmst - convert from UT1 to GMST 
+    gmsta - convert from UT1 to GMST while minimizing rounding errors
+      h2e - convert azimuth and elevation to hour angle and declination (s.p.)
+    h2fk5 - Convert equatorial ICRS to FK5 coordinates
+    hfk5z - Convert equatorial ICRS to FK5 coordinates (0 ICRS proper motions)
+     imxv - apply a 3D reverse rotation to a 3-vector (s.p.) 
+    intin - convert a character string into an integer
+     invf - invert the linear model computed from 2 sets of [x,y] coordinates 
+      kbj - select the epoch prefix B or J
+     m2av - convert a rotation matrix to an axial vector (s.p.) 
+      map - convert a post IAU 1976 mean to geocentric apparent place  
+    mappa - precompute the set of mean to geocentric apparent place parameters 
+    mapqk - convert a post IAU 1976 mean to geocentric apparent place
+   mapqkz - convert a post IAU 1976 mean to geocentric apparent place 
+     moon - compute approximate geocentric position/velocity of moon 
+      mxm - compute the product of two 3X3 matrices (s.p.) 
+      mxv - multiply a 3-vector by a rotation matrix (s.p.) 
+      nut - compute the nutation matrix for a given date
+     nutc - compute the nutation components for a given date 
+      oap - convert from observed to apparent place 
+    oapqk - convert from observed to apparent place
+      obs - look up an entry in a list of groundbased observing stations 
+       pa - compute the parallactic angle from the hour angle and declination
+      pav - compute the bearing of a point on a sphere w.r.t. another
+      pcd - apply pincushion/barrel distortion to tangent plane coordinates 
+    pda2h - compute the hour angle corresponding to a given azimuth 
+    pdq2h - compute the hour angle corresponding to a given parallactic angle 
+   pertel - update osculating orbital elements by applying perturbations
+   pertue - update universal elements by applying perturbations
+   planel - compute the approximate heliocentric position/velocity of a planet 
+   planet - compute the approximate heliocentric position/velocity of a planet 
+   plante - compute approximate topocentric apparent position of a planet 
+       pm - apply the correction for proper motion to a star 
+    polmo - correct site longitude and latitude for polar motion
+    prebn - compute the FK4 matrix of precession between two epochs
+     prec - compute the FK5 matrix of precession between two epochs 
+   preces - precess coordinates in either the FK4 or FK5 systems 
+    precl - compute the longterm matrix of precession between two epochs 
+   precss - precess coordinates in either the FK4 or FK5 systems
+   prenut - compute the FK5 matrix of precession and nutation 
+    pv2el - convert J2000 position and velocity to osculating elements
+    pv2ue - convert instantaneous position and velocity to universal element set
+    pvobs - compute the geocentric position / velocity of an observing station 
+      pxy - apply a linear model to a set of expected and measured [x,y] 
+    range - normalize an angle to the range -pi <= angle <= pi (s.p.) 
+   ranorm - normalize an angle to the range 0 <= angle <= 2pi (s.p.) 
+      rcc - compute the difference between TDB and TT in seconds 
+   rdplan - compute approximate topocentric apparent position of a planet 
+    refco - compute the refraction coefficients 
+   refcoq - compute the refraction coefficients (fast version)
+    refro - compute the atmospheric refraction for optical and radio wavelengths
+     refv - apply the refraction correction to a Cartesian 3-vector 
+     refz - apply the refraction correction to a zenith distance 
+   rverot - compute the earth rotation velocity component in a given direction 
+   rvgalc - compute the dynamical LSR velocity component in a given direction 
+     rvlg - compute the solar velocity component in a given direction
+   rvlsrd - compute the peculiar solar velocity component in a given direction
+   rvlsrk - compute the standard solar velocity component in a given direction 
+     s2tp - project spherical coordinates onto the tangent plane (s.p.) 
+      sep - compute the angle between two points on a sphere (s.p.) 
+     smat - solve a set of simultaneous equations (s.p.) 
+    subet - remove the E-terms from a pre IAU 1976 catalog position
+   supgal - convert deVaucouleurs supergalactic to IAU 1958 galactic coordinates
+      svd - compute the SVD factorization of a matrix 
+   svdcov - compute the covariance matrix from the SVD factorization 
+   svdsol - solve a set of simultaneous equations using SVD factorization 
+     tp2s - convert tangent plane to spherical coordinates (s.p.) 
+     tp2v - convert tangent plane coordinates to direction cosines (s.p.) 
+    tps2c - compute the spherical coordinates of the tangent point (s.p.)
+    tpv2c - compute the direction cosines of the tangent point (s.p.) 
+    ue2el - convert universal elements into heliocentric osculating elements
+    ue2pv - compute heliocentric position and velocity from universal form
+    unpcd - remove pincushion/barrel distortion from distorted coordinates 
+     v2tp - convert direction cosines to tangent plane coordinates (s.p.) 
+      vdv - convert the scale production of two 3-vectors (s.p.)
+       vn - normalize a 3-vector and compute the modulus (s.p.) 
+      vxv - compute the vector product of two 3-vectors (s.p.) 
+    xy2xy - apply a computed linear model to a set of [x,y] 
+       zd -  convert hour angle and declination to zenith distance