The Ultimately Large Telescope: What Kind of Facility Do We Need to Detect Population III Stars?

• Published in: The Astrophysical journal Vol. 904; no. 2; pp. 145 - 150
• Main Authors: Schauer, Anna T. P., Drory, Niv, Bromm, Volker
• Format: Journal Article
• Language: English
• Published: Philadelphia The American Astronomical Society 01-12-2020; IOP Publishing
• Subjects: Astrophysics; Color; Early universe; Infrared telescopes; James Webb Space Telescope; Population III stars; Primary mirrors; Red shift; Space telescopes; Star & galaxy formation; Star formation
• ISSN: 0004-637X; 1538-4357
• DOI: 10.3847/1538-4357/abbc0b

The launch of the James Webb Space Telescope (JWST) will open up a new window for observations at the highest redshifts, reaching out to . However, even with this new facility, the first stars will remain out of reach, as they are born in small minihalos with luminosities too faint to be detected even by the longest exposure times. In this paper, we investigate the basic properties of the Ultimately Large Telescope, a facility that can detect Population III star formation regions at high redshift. Observations will take place in the near-infrared and therefore a Moon-based facility is proposed. An instrument needs to reach magnitudes as faint as 39 magAB, corresponding to a primary mirror size of about 100 m in diameter. Assuming JWST NIRCam filters, we estimate that Population III sources will have unique signatures in a color-color space and can be identified unambiguously.