-
_From @demitri on August 26, 2014 23:23_
### Trillian Data Needs
This document will describe the data needs in detail for the [Trillian project](http://trillianverse.com). Trillian is an attempt to a…
-
### Project URL
https://pypi.org/project/nmma
### Does this project already exist?
- [X] Yes
### New Limit
300
### Update issue title
- [X] I have updated the title.
### Which indexes
PyPI, T…
-
_Issue [JP-1655](https://jira.stsci.edu/browse/JP-1655) was created on JIRA by [Nestor Espinoza](https://jira.stsci.edu/secure/ViewProfile.jspa?name=nespinoza):_
Currently, the outlier_detection st…
-
### Description
I am using a python module for gravitational wave computations called gwfast (https://github.com/CosmoStatGW/gwfast) which requires astropy=5.2.1 and for which I need to compute ti…
-
Leave below as comments your memos that grapple with the topic of the existential threat of nuclear war and nuclear holocaust, inspired by the readings ([2021 Doomsday Clock Statement](https://thebull…
-
**Submitting author:** @athob (Adrien C. R. Thob)
**Repository:** https://github.com/athob/py-ananke
**Branch with paper.md** (empty if default branch):
**Version:** v1.0.0
**Editor:** @warrickball
*…
-
Gummi posed a good question in the final draft re-read: what about the possibility that the TESS out-of-transit modulations are just instrumental artifacts-- momentum dumps and background, etc. We ha…
-
Transition dynamics in the $Λ_{s}$CDM model: Implications for bound cosmic structures
**Authors**: Evangelos A. Paraskevas, Arman Cam, Leandros Perivolaropoulos, Ozgur Akarsu
**TL;DR**: The paper i…
-
Because our validation set contains a large amount of low SNR signals that are "hopeless", random guessing actually performs better, since for theses signals below the noise floor, our trained model w…
-
Hi,
I was wondering about what would be the appropriate value to be reported as SNR for a given planet after the fit is done with the next steps:
1 Initial out of transit estimation of noise
2 Fina…