Closed drphilmarshall closed 8 years ago
I didn't think we were going to use LensPop for the SW simulations. The sims I'm using are SimCT from Anu. I've setup Colin with LensPop though.
On 16 May 2016 at 11:40, Phil Marshall notifications@github.com wrote:
Assigned #11 https://github.com/DES-SL/BlueRings/issues/11 to @tcollett https://github.com/tcollett.
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OK, cool - the SimCT sims should have similar distributions. Do you have a catalog like the one I am talking about, with predicted colors as well as redshifts and masses? Anything would do to get started thinking about this and #6
On Mon, May 16, 2016 at 8:56 AM, Thomas Collett notifications@github.com wrote:
I didn't think we were going to use LensPop for the SW simulations. The sims I'm using are SimCT from Anu. I've setup Colin with LensPop though.
On 16 May 2016 at 11:40, Phil Marshall notifications@github.com wrote:
Assigned #11 https://github.com/DES-SL/BlueRings/issues/11 to @tcollett https://github.com/tcollett.
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Check out https://github.com/tcollett/LensPop/blob/master/lenses_DESa.txt
That's one example catalogue of discoverable lenses for DES coadds (full area at 5 year depth though). There's plenty of stochasticity in the catalogue though. I think Liz told me there's a bug in one of the columns (but I can't remember what it is - I think it's one of the discoverability flags; all of those lenses are discoverable)
Cheers, Tom
On 16 May 2016 at 11:59, Phil Marshall notifications@github.com wrote:
OK, cool - the SimCT sims should have similar distributions. Do you have a catalog like the one I am talking about, with predicted colors as well as redshifts and masses? Anything would do to get started thinking about this and #6
On Mon, May 16, 2016 at 8:56 AM, Thomas Collett notifications@github.com wrote:
I didn't think we were going to use LensPop for the SW simulations. The sims I'm using are SimCT from Anu. I've setup Colin with LensPop though.
On 16 May 2016 at 11:40, Phil Marshall notifications@github.com wrote:
Assigned #11 https://github.com/DES-SL/BlueRings/issues/11 to @tcollett https://github.com/tcollett.
— You are receiving this because you were mentioned. Reply to this email directly or view it on GitHub https://github.com/DES-SL/BlueRings/issues/11#event-661775813
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Great - that's almost exactly what we need. Do you have the z-band magnitudes to match? The SED modeling in #6 would need this, I think.
No I'm afraid not - I never simulated z band data. I could add it, but it would take a complete rerun sadly.
Why not clone the repo and try yourself sometime!
I'll see if I can find time - and also to think more about how to use this information. It'll be good to hear from James too, on what he can measure from the residuals. We can close this out, then - thanks Tom.
If you don't have the time I can do it (my comment about you doing it was tongue-in-cheek) - I don't think there's a rush.
On 16 May 2016 at 15:36, Phil Marshall notifications@github.com wrote:
Closed #11 https://github.com/DES-SL/BlueRings/issues/11.
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No, I agree - today I am mainly making sure everything is written down after last week! I think completing a SW PNG production pipeline is probably the first thing to get built: hopefully you, @bnord and James can do this assembly while we think about enhancements in parallel.
On Mon, May 16, 2016 at 12:43 PM, Thomas Collett notifications@github.com wrote:
If you don't have the time I can do it (my comment about you doing it was tongue-in-cheek) - I don't think there's a rush.
On 16 May 2016 at 15:36, Phil Marshall notifications@github.com wrote:
Closed #11 https://github.com/DES-SL/BlueRings/issues/11.
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Hey @tcollett - thinking about #6 but also more generally about interpreting BlueRings outputs, I think it would be helpful to provide access to the
LensPops
catalog from which the training set will be drawn, to drive algorithm development. This catalog can be reasonably assumed to be a fair sampling of the prior PDF for lens and source properties, which means we ought to be able to use it to help assess the plausibility of any Einstein radii we extract from the residual image analysis. I think we want the following columns, at least to start:What do you think? If the catalog you are using is small (<100k) you could check it in to a
data
folder in this repo. Otherwise, you could add a link to it from the README. Thanks!