-
The METS ingest service returns different values depending on the version:
2.5 - returns experiment ID
3.0 - returns absolute file path for placement of files on the target system
Perhaps the synchr…
-
The METS ingest service returns different values depending on the version:
2.5 - returns experiment ID
3.0 - returns absolute file path for placement of files on the target system
Perhaps the synchr…
-
The METS ingest service returns different values depending on the version:
2.5 - returns experiment ID
3.0 - returns absolute file path for placement of files on the target system
Perhaps the synchr…
-
The METS ingest service returns different values depending on the version:
2.5 - returns experiment ID
3.0 - returns absolute file path for placement of files on the target system
Perhaps the synchr…
-
The dREL in ``cif_core.dic`` calculates the complex structure factor based on the structural model. To do this, it must handle dispersion. Dispersion becomes more significant the more accurate the exp…
-
Hi,
I was seeing whether I could use the Lnu_fun in your code to compute the emission in sources unrelated to shocks. Checking the code, it seems to me that Lnu_fun takes as arguments mu and mu_e,…
-
In GitLab by Weijun Zhou on 06 Nov 2018, 03:15 UTC (GitLab issue GL#1852)
Dear all,
I'm working on the synchrotron radiation generation by the electrons in the WFLA. Therefore, the trajectory of th…
-
Pointed out by @dagewa the other day, in `FormatCBFFullPilatus.py` we explicitly override the beam polarisation to synchotron values:
https://github.com/cctbx/cctbx_project/blob/c8767224cd85600d3cc6c…
-
First effort to define radiation devices:
> "Radiation source": http://purl.obolibrary.org/obo/NCIT_C138129
A device designed to emit radiation, either for external use or implantable. …
-
I'm trying to use your code to simulate galactic foreground around 1.4 GHz, and I find that most your model components are high frequency, except the 408 MHz all sky survey. So is it OK to use your co…