What CORA needs the MOGNO team to confirm before the model can be trusted.
MOGNO was reverse-engineered from two published papers (Campoi et al. 2025, the software architecture; Archilha et al. 2022, the beamline) and the public Sirius MOGNO facility page. Unlike the NSLS-II and Diamond scaffolds, there is no public controls configuration to read, so MOGNO carries no real control handles at all: the device families are inferred from the papers, and every handle, model, and PV namespace is an open question. This is CORA's first Sirius Site and first South American facility. Each row below is a fact the beamline team owns, not a CORA modelling choice (those are on Model). It is a delete-on-answer queue. Priorities are Blocks-build, Blocks-go-live, and Nice-to-have.
The detector roster and per-station pairing: which of Pimega (Si photon-counting), the sCMOS indirect chain, and the CdTe Medipix/Mobipix are installed and active at each station.
One detector position bound to Camera until staff confirm; the FXI multi-camera precedent.
The detector Assets.
CAM-2
Nice-to-have
The scintillator material and thickness and the Optique Peter microscope objective set for the indirect chain.
A Scintillator (e.g. LuAG:Ce) coupled via a microscope.
The indirect-chain detail.
MAG-1
Nice-to-have
The cone-beam magnification rule (how sample-along-cone position maps to magnification).
A PseudoAxis over the sample and detector distances; rule deferred. The FXI Magnification precedent.
The magnification Asset.
DATA-1
Blocks-go-live
The acquisition file format and layout: HDF5 / NeXus / DXchange exchange/data + flat + dark, and the metadata schema injected into the file.
A single main data file carrying projections, flat, dark, and metadata; format pending.