High-redshift galaxies and low-mass stars

Abstract

The sensitivity available to near-infrared surveys has recently allowed us to probe the galaxy population at z≈ 7 and beyond. The existingHubbleWide Field Camera 3 (WFC3) andVisible and Infrared Survey Telescope for Astronomy (VISTA) Infrared Camera (VIRCam) instruments allow deep surveys to be undertaken well beyond 1μm – a capability that will be further… (More)

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Cite this paper

@inproceedings{Wilkins2014HighredshiftGA, title={High-redshift galaxies and low-mass stars}, author={Stephen M. Wilkins and Elizabeth R. Stanway and Malcolm N. Bremer}, year={2014} }