1997/02/06 by D. J. Thompson, D. Thompson, Thompson, D.
Physics and Astronomy · #Astrobiology #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Astrophysics (astro-ph) #FOS: Physical sciences #Infrared #Physics #Scientific Research and Discoveries #Star (game theory) #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9702062
3 pages, LaTeX, no figures, uses World Scientific Press style file. To appear in the proceedings from the 18th Texas Symposium (1996)
arxiv created 1997/02/06 · openalex publication_date 1997/02/06 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The success of the Hubble Deep Field (HDF) data in identifying galaxies at redshifts up to ~3 has been quite spectacular. It is possible to extend this to even higher redshifts using infrared techniques, several of which are briefly described in this paper.