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

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

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 ev...

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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
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Abstract 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.
AbstractList 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 mag AB , 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.
The launch of the James Webb Space Telescope (JWST) will open up a new window for observations at the highest redshifts, reaching out to \(z\approx 15\). 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.
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.
Author Bromm, Volker
Drory, Niv
Schauer, Anna T. P.
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  surname: Bromm
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Snippet 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...
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...
The launch of the James Webb Space Telescope (JWST) will open up a new window for observations at the highest redshifts, reaching out to \(z\approx 15\)....
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SubjectTerms Astrophysics
Color
Early universe
Infrared telescopes
James Webb Space Telescope
Population III stars
Primary mirrors
Red shift
Space telescopes
Star & galaxy formation
Star formation
Title The Ultimately Large Telescope: What Kind of Facility Do We Need to Detect Population III Stars?
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