The level of flux model is not match with the data #928
Replies: 11 comments 11 replies
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You need to account for the passband luminosity and/or the distance. Please see the following tutorials and let us know if anything isn't clear: |
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Thank you for the clarification.
However, I got the another problem when I have tried to change the radius
of primary and secondary stars with the error likes this:
ValueError: Could not lookup ld_coeffs for ***@***.***
@***@***.***@dataset. Try changing ld_coeffs_source to a table that covers a
sufficient range of values or set ld_mode to 'manual' and manually provide
coefficients via ld_coeffs. Enable 'warning' logger to see out-of-bound
arrays.
How can we solve this problem?
Kittipong
…On Mon, Aug 26, 2024 at 7:09 PM Kyle Conroy ***@***.***> wrote:
You need to account for the passband luminosity and/or the distance.
Please see the following tutorials and let us know if anything isn't clear:
- passband luminosity
<https://phoebe-project.org/docs/latest/tutorials/pblum>
- distance <https://phoebe-project.org/docs/latest/tutorials/distance>
- third light <https://phoebe-project.org/docs/latest/tutorials/l3>
- Inverse problem example
<https://phoebe-project.org/docs/latest/examples/inverse_paper_examples>
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Kittipong Wangnok
+6684 828 6505
School of Physics
Institute of Science
Suranaree University of Technology
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I already input this parameter but still get the error with message:
ValueError: Could not lookup ld_coeffs for ***@***.***
@***@***.*** Try changing ld_coeffs_source_bol to a table that covers
a sufficient range of values or set ld_mode_bol to 'manual' and manually
provide coefficients via ld_coeffs_bol. Enable 'warning' logger to see
out-of-bound arrays.
How can I solve this problem
Kittipong
…On Mon, Aug 26, 2024 at 7:49 PM Kyle Conroy ***@***.***> wrote:
The error message is telling you what to do (effectively the same as your previous
question
<#924 (comment)>),
and there are also tutorials on these topics on the website that I linked
to in the response there. If you try that and are still running into
issues, please let us know!
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Kittipong Wangnok
+6684 828 6505
School of Physics
Institute of Science
Suranaree University of Technology
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Changing the radius of r1 and r2?
…On Tue, Aug 27, 2024 at 8:00 PM Kyle Conroy ***@***.***> wrote:
What have you tried that is still giving this message?
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Kittipong Wangnok
+6684 828 6505
School of Physics
Institute of Science
Suranaree University of Technology
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Since there is no reference of parameters for this system, I have tried to
change the parameters following the example that I have.
Moreover, How can I enable the warning logger?
Thanks
Kittipong
…On Tue, Aug 27, 2024 at 8:07 PM Kyle Conroy ***@***.***> wrote:
What are the masses/radii/temperatures? Can you enable the warning logger
and paste the output of the message that states the out-of-bounds values?
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Kittipong Wangnok
+6684 828 6505
School of Physics
Institute of Science
Suranaree University of Technology
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This is the set of parameters that I have:
b.set_value('incl@binary@component', 85)
b.set_value('q@binary@component', 0.5)
b.set_value('sma@binary@component', 7)
b.set_value('teff@primary@component', 4500)
b.set_value('teff@secondary@component', 6000)
b.set_value('requiv@primary@component', 35)
b.set_value('requiv@secondary@component', 10)
b.set_value('distance@system', 3.03)
b['ld_coeffs_source_bol@primary'] = 'phoenix' # Or 'ck2004' or 'auto'
b['ld_coeffs_source_bol@secondary'] = 'phoenix' # Or 'ck2004' or 'auto'
b.set_value('ld_mode', component='primary', dataset='lc01', value='manual')
b.set_value('ld_mode', component='secondary', dataset='lc01', value='manual')
b.set_value('ld_func', component='primary', dataset='lc01', value='logarithmic')
b.set_value('ld_func', component='secondary', dataset='lc01', value='logarithmic')
b.set_value_all('ld_mode_bol', value='manual')
b.set_value('atm@primary@phoebe01@phoebe@compute', value='blackbody')
b.set_value('atm@secondary@phoebe01@phoebe@compute', value='blackbody')
b.set_value('mass@primary@star@constraint', 3.00)
b.set_value('mass@secondary@star@constraint', 1.5)
When I tried to input:
b.set_value('period@binary@component', 310)
b.set_value('t0_supconj@binary@component', 58667.9)
I also get the error.
However, PHOEBE has the limitation of the binary period or not because my system is ~300 days.
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Ok
Kittipong Wangnok
+6684 828 6505
School of Physics
Institute of Science
Suranaree University of Technology
…On Tue, 27 Aug 2567 BE at 9:03 PM Kyle Conroy ***@***.***> wrote:
All of your messages sent through email are being censored by GitHub, can
you please go to the page and manually edit the messages so that they are
readable?
How can I enable the warning logger?
#924 (comment)
<#924 (comment)>
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I already update it
Thanks
Kittipong
…On Tue, Aug 27, 2024 at 9:03 PM Kyle Conroy ***@***.***> wrote:
All of your messages sent through email are being censored by GitHub, can
you please go to the page and manually edit the messages so that they are
readable?
How can I enable the warning logger?
#924 (comment)
<#924 (comment)>
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Kittipong Wangnok
+6684 828 6505
School of Physics
Institute of Science
Suranaree University of Technology
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I was just wondering, can phoebe model the system with a period more than
300+ days or not?
…On Wed, Aug 28, 2024 at 12:01 AM Kyle Conroy ***@***.***> wrote:
There are multiple ways to do that - have you tried anything that isn't
working?
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Kittipong Wangnok
+6684 828 6505
School of Physics
Institute of Science
Suranaree University of Technology
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After I input: I got this error: |
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I have tried to check from ck2004 to blackbody, but I still get the error.
However, I have used the initial input file from "Time" to "Phase", then I
can model and get the model with the good fit but the default period in the
model is 1 day (but actually the real period of the model we use to convert
from time to phase already).
Can I model this way, we can interpret the other parameters?
…On Sun, Sep 1, 2024 at 7:21 PM Andrej Prsa ***@***.***> wrote:
The exact same problem as before: you push your atmosphere parameters out
of bounds by changing the orbital period. You will need to adjust other
parameters accordingly so that Teff/logg/abun are within the supported
range, or switch to blackbody.
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Kittipong Wangnok
+6684 828 6505
School of Physics
Institute of Science
Suranaree University of Technology
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The shape of light curve look likes the data but the level is not the same, How can we solve this problem?
Thanks
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