LSSTprep | Richards group LSST prep work
kandi X-RAY | LSSTprep Summary
kandi X-RAY | LSSTprep Summary
LSSTprep is a Jupyter Notebook library. LSSTprep has no bugs, it has no vulnerabilities, it has a Permissive License and it has low support. You can download it from GitHub.
Repository for Richards group LSST prep work, specifically related to the AGN SC. Maintained by gtr@physics.drexel.edu. Training set -- Notebooks related to the AGN classification training set that we are building for LSST. We are currently focusing on the SDSS Stripe 82 region, collected optical photometry and light curves from SDSS, Mid-infrared photometry from Spitzer, proper motion and parallax measurements from GAIA. We are still adding more data. opSim -- Tutorial notebook to help people get started analyzing the cadence opSim. Adapted by Weixiang and Gordon from notebooks referenced therein. Cadence -- Notebooks related to exploring the effect of different cadences (particular, so-called "rolling" cadences) on the identification of AGNs in LSST via variability. Led by Weixiang Yu. We will be simulating WFD and DDF light curves of theoretical AGNs (both damped random walks and damped harmonic oscillators--with a range of parameters) and seeing how changing the observing cadences affects our ability both to identify the objects as variable AGN and, furthermore, to accurately recover their model parameters. LCmerge -- Notebooks related to trying to understand how we can best merge light curves from multiple bands to produce a single light curve, both for the purpose of deciding whether an object is variable or not and for determining the properties of the variability. Started by Drexel undergrad Jared Haughton (Drexel 2018), currently maintained by Drexel undergrad co-op student Rachel Buttry (Drexel 2019). GAIA -- Notebooks related to determining under what conditions GAIA can be used to improve quasar selection in LSST. The bottom line is roughly that all quasars brighter than $i=20$ will be detected by GAIA, but essentially no quasars fainter than $i=22$ will be. Currently maintained by Drexel undergrad co-op student Bee Martin (Drexel 2020). Photoz -- Notebooks exploring different aspect of photo-z's for AGNs in LSST. Currently maintained by Drexel undergrad co-op student Bee Martin (Drexel 2020). The point is to demonstrate that photo-z in the LSST era will need to consider AGNs with significant contributions from their host galaxy where photo-z algorithms for quasars are more prone to fail (due to host contamination) and where photo-z algorithms for galaxies are also more prone to fail (due to central engine contamination). We compare the effectiveness of 4 galaxy photo-z algorithms used by DES with our own Nadaraya-Watson based quasar photo-z algorithm.
Repository for Richards group LSST prep work, specifically related to the AGN SC. Maintained by gtr@physics.drexel.edu. Training set -- Notebooks related to the AGN classification training set that we are building for LSST. We are currently focusing on the SDSS Stripe 82 region, collected optical photometry and light curves from SDSS, Mid-infrared photometry from Spitzer, proper motion and parallax measurements from GAIA. We are still adding more data. opSim -- Tutorial notebook to help people get started analyzing the cadence opSim. Adapted by Weixiang and Gordon from notebooks referenced therein. Cadence -- Notebooks related to exploring the effect of different cadences (particular, so-called "rolling" cadences) on the identification of AGNs in LSST via variability. Led by Weixiang Yu. We will be simulating WFD and DDF light curves of theoretical AGNs (both damped random walks and damped harmonic oscillators--with a range of parameters) and seeing how changing the observing cadences affects our ability both to identify the objects as variable AGN and, furthermore, to accurately recover their model parameters. LCmerge -- Notebooks related to trying to understand how we can best merge light curves from multiple bands to produce a single light curve, both for the purpose of deciding whether an object is variable or not and for determining the properties of the variability. Started by Drexel undergrad Jared Haughton (Drexel 2018), currently maintained by Drexel undergrad co-op student Rachel Buttry (Drexel 2019). GAIA -- Notebooks related to determining under what conditions GAIA can be used to improve quasar selection in LSST. The bottom line is roughly that all quasars brighter than $i=20$ will be detected by GAIA, but essentially no quasars fainter than $i=22$ will be. Currently maintained by Drexel undergrad co-op student Bee Martin (Drexel 2020). Photoz -- Notebooks exploring different aspect of photo-z's for AGNs in LSST. Currently maintained by Drexel undergrad co-op student Bee Martin (Drexel 2020). The point is to demonstrate that photo-z in the LSST era will need to consider AGNs with significant contributions from their host galaxy where photo-z algorithms for quasars are more prone to fail (due to host contamination) and where photo-z algorithms for galaxies are also more prone to fail (due to central engine contamination). We compare the effectiveness of 4 galaxy photo-z algorithms used by DES with our own Nadaraya-Watson based quasar photo-z algorithm.
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LSSTprep has a low active ecosystem.
It has 3 star(s) with 2 fork(s). There are 9 watchers for this library.
It had no major release in the last 12 months.
LSSTprep has no issues reported. There are no pull requests.
It has a neutral sentiment in the developer community.
The latest version of LSSTprep is v0
Quality
LSSTprep has no bugs reported.
Security
LSSTprep has no vulnerabilities reported, and its dependent libraries have no vulnerabilities reported.
License
LSSTprep is licensed under the MIT License. This license is Permissive.
Permissive licenses have the least restrictions, and you can use them in most projects.
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LSSTprep releases are available to install and integrate.
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