PLENS
PLENS is
Keith Horne 's fortran code to fit
lightcurves of microlensing events.
2008 Nov LCOGT microlens workshop :
horne_plens.pdf .
horne_bayes.pdf .
all talks .
ftp_ogle to ftp OGLE data.
rsync_year to rsync all lightcurves of given year
rsync_event to rsync all lightcurves of given event
PLENS uses PGPLOT for graphics.
The code is continually under development.
plens.tar.gz
, tarball with all files listed below.
plens.exe
, executable image.
plens.com
, script to compile plens.
plens_a.com
, script to create archive of plens subroutines.
plens.inc
, include file with common blocks for global variables.
plens.for
, plens main programme.
plens.a
archive with plens subroutines.
lens1.for
, single lens subroutines.
lens2.for
, binary lens subroutines.
asp.for
, multiple lens subroutines.
dzw.for
, detection zone area subroutines.
misc.for
, miscillaneous subroutines.
test390.dat
, lightcurve data file for testing.
plens.fit
runs plens.exe to fit and make standard plots.
plens.fitb for blend grid.
plens.fitc for Chi^2 map.
plens.fitp for P(det|a).
plens.test
runs plens.fit* on test390.dat.
pspl fit: test390_4_(
a,
b,
m,
n,
r,
g,
y,
z,
mr,
mn,
mb).ps
+blending: test390_5_(
a,
b,
m,
n,
r,
g,
y,
z,
mr,
mn,
mb.
bb).ps
+sigmag0: test390_6_(
a,
b,
m,
n,
r,
g,
y,
z,
mr,
mn,
mb.
bb).ps
+erbscl: test390_7_(
a,
b,
m,
n,
r,
g,
y,
z,
mr,
mn,
mb.
bb).ps
Chi^2(x,y): test390_5_(
c,
mc,
mrc,
mnc).ps
Chi^2(lnu,az): test390_5_(
l,
ml,
mrl,
mnl).ps
Chi^2(t,f): test390_5_(
v,
mv,
mrv,
mnv).ps
P(det|a): test390_5_(
p,
pc,
mpc.
pl,
mpl.
pv,
mpv).ps
Keith Horne (kdh1 at st-andrews.ac.uk)