Microlensing light curves — live


Most recently received data from OGLE, MOA, MiNDSTEp, PLANET/RoboNet, MONET and MicroFUN, along with model light curve from SIGNALMEN



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Please select site(s) or group(s) to be monitored for new data
  Surveys

    O OGLE
    K MOA

  MiNDSTEp, PLANET/RoboNet, MONET

    Z Danish 1.54m
    U UTas 1.0m
    W Perth 0.6m
    F Boyden 1.5m
    A SAAO 1.0m
    R LNA/OPD 0.6m
    H Faulkes North 2.0m
    I Faulkes South 2.0m
    J Liverpool 2.0m
    P MONET North 1.2m
    Q MONET South 1.2m

  MicroFUN

    c CTIO 1.3m
    y CTIO 1.0m
    z Hereford Arizona 0.35m
    l Mt Lemmon 1.0m
    m MDM 2.4m
    o Palomar 60''
    r Regent Lane
    d Possum 11''
    a Auckland 0.4m
    h Hunters Hill 0.35m
    t Southern Stars 11''
    f Farm Cove 0.35m
    k Kumeu Obs 0.35m
    v Vintage Lane 0.4m
    p CBA Perth 0.25m
    w Wise 1.0m E2V
    i Wise 1.0m SITe
    b Bronberg 0.35m
    x Campo Catino 0.5m


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all this season
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The observed flux at time t reads F(t) = FS A(t) + FB, where the source flux FS and the background flux FB are specific to each observing site and filter, while A(t) denotes the theoretical magnification. In order to put different data sets (ti, Fi, σFi) on the same plot, we show the theoretical magnitude shift Δm = 2.5 lg A(t) along with mi = 2.5 lg Ai and the error bar σmi = [2.5/ln(10)] [σFi/|FS Ai|]. Epochs for which Ai ≤ 0 are marked by small stars below the abscissa.
PLEASE NOTE THE FOLLOWING:
SIGNALMEN modelling ©2006–2008 Martin Dominik & Nicholas Rattenbury
SM plotting package ©1987–1999 Robert Lupton & Patricia Monger
SM macros ©1999–2008 Martin Dominik
Data processing ©2007–2008 Martin Dominik
Top-level interface ©2007–2008 Martin Dominik

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