The Via Project is a planned five-year dual-hemisphere spectroscopic survey targeting over 2 million stars with 100 m/s RV stability and transient spectroscopy to r~24 using instruments on MMT and Magellan/Clay telescopes starting in 2027.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
The paper advocates for a high-S/N UV spectroscopic survey of quasars to produce a legacy archive enabling detailed CGM, IGM, Milky Way, and AGN outflow studies.
citing papers explorer
-
The Via Project: Overview of the Science, Instrument, and Survey
The Via Project is a planned five-year dual-hemisphere spectroscopic survey targeting over 2 million stars with 100 m/s RV stability and transient spectroscopy to r~24 using instruments on MMT and Magellan/Clay telescopes starting in 2027.
-
High-S/N Quasar Observations with HST/COS: Deep Fields for Spectroscopy
The paper advocates for a high-S/N UV spectroscopic survey of quasars to produce a legacy archive enabling detailed CGM, IGM, Milky Way, and AGN outflow studies.