DLA abundances in the CUBES’s spectral window

Molaro, P.

doi:10.1007/s10509-014-2017-5

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2020

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“…It might be possible to detect uncontaminated metal lines (of, e.g., D, O I, N I, S II) in the spectra of these objects. Considering that damped Lyman-α systems are likely galaxies at an early stage of their evolution, studies of these objects can contribute to the understanding of the early chemical enrichment of the Universe (Molaro, 2014).…”

Section: Extragalactic Sciencementioning

confidence: 99%

Near-UV Spectroscopy with the VLT

Smiljanic

2020

Preprint

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The 39-meter European Extremely Large Telescope (E-ELT) is expected to have very low throughput in the blue part of the visible spectrum. Because of that, a blue-optimised spectrograph at the 8-meter Very Large Telescope could potentially be competitive against the E-ELT at wavelengths shorter than 400 nm. A concept study for such an instrument was concluded in 2012. This would be a high-throughput, medium resolution (R ∼ 20 000) spectrograph, operating between 300 and 400 nm. It is currently expected that construction of this instrument will start in the next few years. In this contribution, I present a summary of the instrument concept and of some of the possible Galactic and extragalactic science cases that motivate such a spectrograph.

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Section: Extragalactic Sciencementioning

confidence: 99%

Near-UV Spectroscopy with the VLT

Smiljanic

2020

Preprint

View full text Add to dashboard Cite

show abstract

DLA abundances in the CUBES’s spectral window

Cited by 1 publication

References 35 publications

Near-UV Spectroscopy with the VLT

Near-UV Spectroscopy with the VLT

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