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  The Nature of the Host Galaxies of High- Redshift Damped Lyman-alpha Absorbers

Kanekar, N., Neeleman, M., Prochaska, J. X., & Rafelski, M. (2019). The Nature of the Host Galaxies of High- Redshift Damped Lyman-alpha Absorbers.

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Item Permalink: https://hdl.handle.net/21.11116/0000-0005-D0C0-6 Version Permalink: https://hdl.handle.net/21.11116/0000-0005-D0C1-5
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https://ui.adsabs.harvard.edu/abs/2019hst..prop15882K (Any fulltext)
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 Creators:
Kanekar, Nissim1, Author
Neeleman, Marcel1, Author
Prochaska, Jason X.1, Author
Rafelski, Marc1, Author
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1Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners, ou_2421692              

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 Abstract: Absorption-selected galaxies associated with damped Ly-alpha absorbers (DLAs) provide a unique opportunity to study the gas in 'typical' galaxies at high redshifts. We have recently used ALMA to detect [CII] 158 micron or CO emission from ten DLAs at z 2-4, and the VLA to detect CO(2-1) emission from one of the z 4 DLAs. We propose to continue this successful ALMA+VLA project, complementing the ALMA observations with (1) a VLA search for CO(1-0) or CO(2-1) emission from five DLA hosts at z 2-4 with ALMA detections of CO or [CII] 158 micron emission, and (2) an HST-WFC3 imaging of 4 of the 5 DLA host galaxies with ALMA+VLA observations, covering the restframe near-UV continuum. The VLA observations will yield molecular gas masses for all five galaxies, and

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 Dates: 2019
 Publication Status: Issued
 Pages: 15882
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Title: HST Proposal
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