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We propose "quickbrick" similar to what the Lyman-alpha forest group did for QSOs at the Argonne 2015 workshop: go directly from templates to brick files, skipping over the intermediate steps. This i…
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I'll need the following for each candidate. Some of these are in the Paper 1 table, but others aren't. @dfm, ideally the photometry would be able to be machine-grabable (via either ketu or kplr?) so …
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When trying to verify my recent installation of Lemon it will go nearly to the end but then it fails with a mismatch on the flux value. The output looks like this:
```
test_get_coords_file (test_qph…
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I think the following is all we need:
- [x] **Tim**: finish stellar properties where they are currently broken
- [ ] **Dan**: Table and subsection on planet properties
- [x] **Tim**: False positive pr…
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Python 2.7, astropy 1.0.1
Hi,
I am starting to work with images that have SIP distoorions in their WCS. My example image is from Spitzer and does contain the SIP keywords. When creating the WCS obj…
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The Getting Started section of the astropy docs should have an analysis thread that highlights the integrated functionality of Astropy. Some example that hits a bunch of the major subpackages and pre…
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WFC3 data, like ACS data, also requires/can take advantage of CTE correction. We may want to add it to our pipeline. Some information on it is here:
- http://www.stsci.edu/hst/wfc3/ins_performance/CTE…
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User's experience is that suddenly photometry can't be measured in the middle of an accept. This was the second time I had this bug, after processing reals in a validate instance for about half an hou…
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Nothing prevents the XML file produced by _offsets.py_ from containing information for duplicate images -- that is, images whose observation date is exactly the same. This causes the next module of th…
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David, Can you find the fundamental references for SDSS (York et al), SDSS-II (don't know), SDSS-III (maybe Ahn et al??), and put them into method.tex where I have left placeholders? Follow the conv…