SP-2402: NB 300 series on variable stars #110
Conversation
|
Check out this pull request on See visual diffs & provide feedback on Jupyter Notebooks. Powered by ReviewNB |
| @@ -0,0 +1,800 @@ | |||
| { | |||
There was a problem hiding this comment.
(by using, e.g., [f]_psfFluxSigma, or some combination of the flux value percentiles from [f]_psfFluxPercentile05, 25, 50, 75, 95). We will also use r_psfFluxStetsonJ, which reports the Stetson J-index, an indicator of periodic variability.
Maybe move the first sentence to be outside of parenthesis, to be consistent with the Stetson J-index sentence.
Reply via ReviewNB
| @@ -0,0 +1,800 @@ | |||
| { | |||
There was a problem hiding this comment.
Maybe also add "applied in TAP query" to the line on r_scienceFluxMean, to be consistent with the point above it. Or remove both conditions from the list since they were already applied.
Reply via ReviewNB
| @@ -0,0 +1,800 @@ | |||
| { | |||
There was a problem hiding this comment.
Describe how we measure the period via Lomb-Scargle, and how the LC is phased.
Seems like this got left behind as a self-reminder
Reply via ReviewNB
| @@ -0,0 +1,800 @@ | |||
| { | |||
There was a problem hiding this comment.
The light curve that appears the least periodic, for diaObjectId 614435616184074318 seems to be classified as a quasar. I was hoping it would be obviously different within the 4 highlighted objects in the plots in section 2.3, but not sure how to exclude it yet.
Reply via ReviewNB
No description provided.