https://pfspipe.ipmu.jp/jira This file is an XML representation of an issue en-us 8.3.4 803005 13-09-2019 https://pfspipe.ipmu.jp/jira/browse/PIPE2D-367 DRP 2-D Pipeline <p>Fit available model templates with HSC photometry and PSF spectroscopy to derive the probability P(Teff, log g, Z), given the input stellar parameters.</p> <p>There are multiple techniques for performing this work, and these will be the subject of individual tickets. The results of those tickets should be compared in order to determine the best approach.</p> PIPE2D-367

Derive P(Teff, log g, Z) from model templates

Task Normal Open Unresolved Masayuki Tanaka hassan flux-calibration model-spectra-fitting Tue, 19 Feb 2019 17:53:11 +0000 Fri, 14 Jul 2023 06:26:04 +0000 0 2 <p>We are currently using P(Teff,logg,Z,alpha) from the broad-band photometry and that from the spectral ftting. The broad-band fitting is done, but we are still working on (or improving) the spectral fitting part.</p> Blocks PIPE2D-374 PIPE2D-836 PIPE2D-369 PIPE2D-368 Duplicate PIPE2D-305 PIPE2D-306 Development Rank 0|02qpti:f