What CORA needs the SST team to confirm. This model is reverse-engineered from public open source (the NSLS2/sst-*-profile-collection endstation repos and the shared NSLS-II-SST/sst-base package): the EPICS PVs are read from the TOML device manifests and the sst-base device classes, but vendor identities, physical positions, and the per-endstation configuration are not. Each row is a fact the beamline team owns. It is a delete-on-answer queue.
The two undulator periods and gap / phase ranges (soft EPU60, tender U42). The devices (SR:C07-ID:G1A{SST1:1}, {SST2:1}) are confirmed from the sst-base energy classes; soft range about 71-2250 eV.
Two insertion devices, identity-only.
The InsertionDevice settings.
PSS-1
Blocks-go-live
The PSS search-and-secure permit-leaf PVs. Only the shutters (XF:07ID-PPS{Sh:FE}, XF:07IDA-PPS{PSh:n}) are in source.
The permit signal is a confirm note, not a guessed PV.
The Enclosure permit signals.
ENC-1
Nice-to-have
The branch-to-hutch mapping and the physical hutch names / numbering (not in source): which endstations (RSoXS, NEXAFS on the soft SST-1 branch; HAXPES on the tender SST-2 branch; plus UCAL, VPPEM) sit in which enclosures? The PV zone numbers (07ID1 / 07ID2 / 07ID6) do not map one-to-one to a branch.
An optics hutch plus a soft (SST-1) and a tender (SST-2) experiment enclosure.
The soft PGM grating set and the tender DCM crystal cut and ranges. Both monochromators (Mono:PGM1, Mono:DCM1) are in source.
One GratingMonochromator and one Monochromator Asset, settings blank.
The Monochromator settings.
ENERGY-1
Nice-to-have
Is energy scanned as the measurement (NEXAFS absorption sweeps the soft PGM across an edge), warranting the energy-scan Capability the catalog anticipates?
NEXAFS mapped to deferred Capabilities; energy-scan deferred (the BMM question).
The HAXPES Scienta SES hemispherical analyzer model, lens modes, and pass-energy / kinetic-energy controls.
An ElectronAnalyzer Asset (catalog Family, graduated at this 2nd sighting after ESM) presenting the Detector Role.
The analyzer model.
DET-1
Blocks-go-live
Which detectors are live per endstation: the RSoXS Greateyes WAXS CCD (a second SAXS-arm CCD is commented out), the HAXPES analyzer, the NEXAFS microcalorimeter and drain-current / partial-electron-yield channels.
The WAXS CCD, the analyzer, and the microcalorimeter modelled; the SAXS arm excluded.
The detector roster per endstation.
TEMP-1
Nice-to-have
Which sample-environment thermal units are live per endstation (the Lakeshore controllers).
One TemperatureController Asset; the others noted.
The sample-environment Assets.
DIAG-1
Nice-to-have
The flux-channel map (the I0 mesh / diode, the drain-current and ion-chamber SR570 channels) and the BeamPositionMonitor sensor fold-vs-promote hold.
The endstations and in-situ accessories deferred at this design phase: the NEXAFS endstation detail (drain-current / partial-electron-yield channels), the UCAL microcalorimeter ADR cryostat, the VPPEM microscope, the HAXPES flood gun and source-measure unit, and the RSoXS syringe pump. None fits an existing family cleanly. How does CORA model these?
Deferred; the main RSoXS / HAXPES / NEXAFS-TES legs are modelled; the rest are named here.
Do the soft-scattering (RSoXS), absorption (NEXAFS), and photoemission (HAXPES) Capabilities enter CORA's catalog, or stay deferred? This is the same owner-scope decision the other scattering / spectroscopy / photoemission beamlines opened.
Capabilities deferred (rendered unlinked), no Practice recorded.