Date: Thu, 28 Mar 2024 12:42:52 -0500 (CDT) Message-ID: <1738127769.168.1711647772699@os-confluence.ncsa.illinois.edu> Subject: Exported From Confluence MIME-Version: 1.0 Content-Type: multipart/related; boundary="----=_Part_167_1427553293.1711647772699" ------=_Part_167_1427553293.1711647772699 Content-Type: text/html; charset=UTF-8 Content-Transfer-Encoding: quoted-printable Content-Location: file:///C:/exported.html
Francisco Paz Chinch=C3=B3n
Run nightly calibrations over domeflats and bias. Beware the code automa= tically discards first exposure of each filetype of the night, for safety. = The nightly processing should run periodically, to make generation of super= cals smoother.
Note: Remember to delete precal runs after creating the Supercal, to= save disk space.
For a step-by-step, queries to select DB products, and discussion, refer= to the below repository. Remember visual inspection of each full-size= d CCD must be done, looking for structures.
Repository and documentation: https://github.com/paztronomer/skytemplates_build
For the step-by-step, codes, and discussion, refer to the below reposito= ry. This was done retrieving additional DECam data from NOAO.
Repository and documentation: https://github.com/paztronomer/uband_endeavor
The notebook and additional codes can be found in the repository below.<= /p>
Repository: https= ://github.com/paztronomer/skytemplates_wedge_mask
Use ~50 g-band exposures, following the step-by-step described in the fo= llowing repository. Remember to do a bit-by-bit comparison against past epo= chs, to check for some out of the normal variation.
Repository and documentation: https://github.com/paztronomer/bpm_calibrations
Repository: https://github.co= m/paztronomer/bpm_addmask
Repository and documentation: https://github.com/paztronomer/bpm_translation
Repository: https://github.com= /paztronomer/mask_check