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Real Light Curves. The light curves published on web pages are usually very carefully selected because they look impressive. In reality, not all light curves look so good. Here are some of mine. TW Dra has a range of over 2 mags … but in 2009, I never managed to catch it in eclipse. - PowerPoint PPT Presentation
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Real Light Curves
The light curves published on web pages are usually very carefully selected
because they look impressive.
In reality, not all light curves look so good. Here are some of mine ...
TW Dra has a
range of over 2 mags
… but in 2009, I never
managed to catch it in eclipse
TW Dra in 2009
6.7
7
7.3
7.6
7.9
8.2
8.5
8.8
9.1
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1
Phase
Mag
nit
ud
e
Sometimes you miss seeing the primary eclipse,
… but do catch the secondary
eclipse
Here,, the maximum near phase 0.1 and the
eclipses near phases 0.35 & 0.8
can be seen,
but the maximum near phase
0.6 was almost
missed !
W UMa in 2009
7.9
8
8.1
8.2
8.3
8.4
8.5
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1
Phase
Ma
gn
itu
de
Sometimes you can’t see mid eclipse
because the EB
becomes too faint for you to see.
At mid eclipse,
RW Tau is around mag
11.0
The start of this eclipse of TV Cas (7.3-8.1) started in daylight.
Cloud then intervened before the
eclipse was over
TV Cas : 2010 Feb 5
7.7
7.75
7.8
7.85
7.9
7.95
8
8.05
8.1
18:00 19:12 20:24 21:36
Mag
nit
ud
e
If you observe low amplitude
EBs, scatter will be a problem.
However, the general pattern of
variation can still be seen
GK Cep in 2009
7.10
7.15
7.20
7.25
7.30
7.35
7.40
7.45
7.50
7.55
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1
Phase
Ma
gn
itu
de
When you first start
observing, you expect
that eclipses will be
symmetrical.
Not all are, as is shown by this RZ Cas light
curve
Whenever possible, its best to observe
the whole eclipse in one night.
Otherwise different
sky conditions or changes in the light
curve shape will
lead to scatter
Beta Lyrae, however,
has eclipses that last
more than a day
… so you have to
observe on many
different nights
LY Aur has a period very close to 4
days.
This means that you keep catching it at
the same phases for
months on end.
In 2009, this wasn’t too bad
because eclipses were occurring at
night.
LY Aur in 2009
6.9
7
7.1
7.2
7.3
7.4
7.5
7.6
7.7
7.8
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1
Phase
Mag
nit
ud
e
In 2007, however, eclipses
were occurring
during daylight.
Hence the light curve
was less impressive
LY Aur in 2007
6.8
6.9
7
7.1
7.2
7.3
7.4
7.5
7.6
7.7
7.8
0.0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1.0
Phase
Mag
nit
ud
e
The lesson is to not be put off if your some of your light curves are
disappointing
It happens to everyone – but every so often, you will have more luck
The secondary eclipse of RZ Cas is
usually said to be too
small to be seen
visually.
But it does show up
near phase 0.5 in this light curve from 2009
RZ Cas in 2009 (SAC elements)
6.0
6.2
6.4
6.6
6.8
7.0
7.2
7.4
7.6
7.8
8.0
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1
Phase
Mag
nit
ud
e