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/SCIDB-65 Science Database <p>Run survey simulations (cosmology, galaxy evolution, and maybe galactic archaeology as well) based on the HSC PDR1 data and generate psfObject files.</p> SCIDB-65

prototype v2: run survey simulation

Story Normal Done Done Kiyoto Yabe Masayuki Tanaka Wed, 14 Nov 2018 04:48:54 +0000 Tue, 19 Mar 2019 08:19:19 +0000 Tue, 19 Mar 2019 08:19:19 +0000 0 1 <p>For the purpose of v2, we do not need to fully simulate the survey.  We (randomly) chose the GAMA15H field for the cosmology survey and applied the magntiude and color cuts in [the latest cosmology document|<a href="https://sumire.pbworks.com/w/file/128479866/ssp_cosmology_princeton2018.pdf" class="external-link" rel="nofollow">https://sumire.pbworks.com/w/file/128479866/ssp_cosmology_princeton2018.pdf</a>.]  We got 1.2xe5 objects over ~10sqdeg.</p> <p> </p> <p>Yabe-kun ran the simulation.  GE survey is only in UD-COSMOS and followed the selection criteria in the document from the Princeton meeting in September.  We did not include the Ly alpha emitters.  The redshifts of the target galaxies are the many-band photo-z's and we assumed two SED shapes, quiescent and star forming, based on the NUVr selection.  GA in the GAMA15H field and we again followed the latest selection criteria, but we simulate only the MW-disk/stream targets, not dwarf spheroidals.</p> Development Epic Link SCIDB-64 Rank 0|s001pc: