Science scope:
broad spectrum of ground-breaking stellar astrophysics,
telling us how stars work, live and die...
With Gaia & TESS there are transformational space missions
that focus on imaging/photometry/astrometry (some spectra) of bright stars.
The proposed program is tailored towards a spectroscopic survey that
in many ways ideally complements this:
-- it is all sky
-- it is matched in apparent magnitude
-- it is time-domain
-- it is dust-penetrating (disk/young stars)
Natural operational meshing of stellar astrophysics & DISCO
It is focussed on
-- age-chemo-orbital mapping of the entire galaxy
-- binary stars across the HR (as calibrators, stellar evolution, SF,SN)
-- astroseimsology to understand stellar evolution (need spectra)
-- planet hosts
It is a full sky program, with APOGEE and BOSS (1 each) in both hemispheres,
2/3 is multi-epoch observations; 2/3 APOGEE; 1/3 BOSS; still based on a 10min minimal cadence.
"Surprise" element:
Instead of a ROBOT, a 4-5 fold-set of 300 APOGEE fibers, feeding 4-5 gang connectors,
still using plug plates would enable:
-- simultaneous use of 300 APOGEE and 500 BOSS fibers
--> better use of instrument/detectors
-- more flexibility in fiber placement
This would mean:
-- minimal new hardware development
(RV improvement; fiber cart upgrade with BOSS and more APOGEE fibers)
-- move 1 BOSS spectrograph to LCO
-- plug plate costs in two hemisphere continues
-- could start 2019
All science can be done in minimally 3 years; comfortably 4 years;
minimum 25 Million x 10min x spectrum
few million fiberx10min open (for BOSS)
Much of the same science would work within fiber-robot framework,
too, in comparable survey duration.
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