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Lens position matching via some suitable LRG catalog #22
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In the future, we might also consider drawing from PS1 itself, or other surveys. See #2 |
…rightest galaxies in each redshift range. #22
…es first before positioning? #22
OK, I made an initial foray, trying to select sensible galaxies from CFHTLS (basically the brightest galaxies in each of 6 broadish redshift bins - I checked that we cannot query by color directly). Here's my notebook, in a CFHTLS branch (that I pulled your notes into as well, Mike). From this I think I conclude that its best to first paint the OM10 lenses with reasonable colors, extrapolating from SDSS (like we do with the quasars), and then go looking for a suitably faint and correctly colored object to position the system. I worry that we won't have enough red objects unless we go looking for them specifically - I might need to download a lot of CFHTLS galaxies at some point soon. |
Hey Phil, |
Sweet! I'll give it a try :-) On Mon, Jul 20, 2015 at 12:02 PM, Mike Baumer notifications@github.com
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Downloading CFHTLS galaxies is getting painful. Let's switch to using SDSS LRGs for the sky positioning - and start using the painted-on lens colors to find a good LRG to use when simulating images. |
Try matching on one color; check that others are sensible? |
…e colors - and maybe a better algorithm? #22
Hmm. I downloaded the SDSS LRGs and checked them in. They're very bright! Mostly brighter than i=19 or so. This is too bright for PS1QLS. So, back to CFHTLS. I think the next thing to do is to use the SDSS-painted OM10 lens colors to define the CFHTLS wget statement, in a |
That’s unfortunate, but I can work on the matching algorithm in parallel while you sort out the CFHTLS selection. Thanks for doing all that wget legwork!
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OK, I upgraded the download script and it is running. Can you try it out as well, @mbaumer, and see whether the new |
BTW You'll see from the issue22 notebook that download errors are common - it still might be worth looking for a better way to get all the CFHTLS galaxies we need... |
We use CFHTLS red galaxies to decide where to plop down our simulated lenses on sky, by matching nearest neighbors (in redshift and velocity dispersion--although the latter is not for long) between catalogs.
Apparent cuts on the CFHTLS LRG magnitudes in our current reference catalog ($OM10_DIR/data/CFHTLS_LRGs.txt) limit our matching ability on an OM10-PS1 sample to 73%
@drphilmarshall , can you investigate loosening these cuts to expand our CFHTLS reference catalog? You can use the following plot as a guide:
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