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Spitzer acquired precision time series photometry in point-and-stare conditions for targeted science cases like transiting exoplanets or weather on brown dwarfs. Those data are housed as single per-c…
gully updated
4 years ago
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## Query
In the utility function, `photometry.utilities.mag2flux(mag, zp=20.60654144)`, what is the units of output flux? Is it in `e-/s` or in physical units `W/m^2`?
Also, what is the `zp` in…
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This notebook will form part of the series: Getting started with *Kepler* and *K2* data.
At Rebekah's request, I took Tutorial #4 and split it into two tutorials. Tutorial #4 is now "Understanding …
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To obtain the best solution as possible once we have the TLS results we need to fit the data properly. We choose
[Allesfitter](https://allesfitter.readthedocs.io/en/latest/index.html).
We will …
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This notebook will form part of the series: Getting started with _Kepler_ and _K2_ data products.
In this second notebook, we will focus on downloading and studying a target pixel file. This will i…
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This notebook will form part of the series: Getting started with _Kepler_ and _K2_ data products.
In this first notebook, we will focus on downloading and plotting a light curve for objects a user …
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I was trying to produce light curves from PRF photometry with TESS tpf. However, I encountered the error below saying the 'TessTargetPixelFile' object has no attribute 'prf_lightcurve'. It seems the T…
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Thanks for your help in the previous issue. I now encounter a different issue.
I am using the latest version of eleanor, astropy, astroquery, numpy.
I have flushed the content of the cache (`/home/m…
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The routine below needs to be adapted to process lightcurves for TESS objects in different sectors.
I have set cutout_size to 10, but the size of the resulting cutouts is only 4X4(see the output bel…
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Hi everyone, thank you for this great code!
I'm trying to create light curves for a few targets and I am running into an issue with collecting target data for three of these targets.
`ms = ele…