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Hi Tim,
Over the past few days I've been wondering how hard could it be to tune `VESPA` so that one can readily apply it to TESS photometry.
A few things came up:
— A magnitude for the band in …
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### Version
1
### DataCap Applicant
jevticgallonsd1466
### Project ID
x
### Data Owner Name
Space Telescope Science Institute.
### Data Owner Country/Region
United States
### Data Owner Indu…
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Hello,
What parameters/settings are needed to fit sigle lined binaries within allesfitter?
Unfortunately, I could only find samples for double lines EBs and exoplanets.
Thanks
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# Add Time Domain Data to AstroPile
Add time domain photometric data (e.g. PLAsTiCC/Young Supernova Experiment) and spectroscopic data (e.g. Kaepora) to AstroPile.
Contacts:
Participants: Ben B…
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I'm leading an AAVSO workshop that will introduce amateur astronomers to analyzing TESS data using lightkurve. The initial goal will be to use TESS photometry to refine the classifications and periods…
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This issue is a final wrap up of the Kepler-Focus Lightkurve Tutorial project, which created 21 new Lightkurve tutorials. The tutorials were merged to the [STScI notebook repository](https://github.co…
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Can we have an option to return the HDU list in case the user wants to add keywords to the headers?
Currently, I need to save moving TPFs with extra information about the asteroid in the header, e.g.…
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Asteroseismology can unlock stellar properties such as mass and radius independently from other methods. Until recently, asteroseismic analyses were only carried out in the frequency domain, by using …
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##### Description
The Kepler Point Spread Function (PSF), like any real-world optical instrument, depends on its location in the focal plane, both *x, y*, and radial distance *z*. The conspicuous …
gully updated
6 years ago
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While generating the LC of a source in a moderately crowded field, I found that the circles representing the Gaia sources are slightly off compared to the TESS sources in plot_gaia_overlay. The shift…