Survey Specifications

• Survey of all known Class 0 and Class I protostars in the Perseus Molecular Cloud
• ~600 hours of Submillimeter Array Observations
• Subcompact and Extended configuration
• 230 GHz (1.3 mm) and 345 GHz (870 μm, Subcompact only)
• Dust continuum + spectral lines
• 1.3 mm lines: CO(2-1), C¹⁸O(2-1), ¹³CO(2-1), N₂D⁺(3-2)
• 870 μm lines: CO(3-2), HCO⁺(4-3), H¹³CO⁺(4-3)
• Some additional lines for some tracks that used the SWARM correlator