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Results: 1-11 |
Results: 11

Authors: Plovnick, RH Richards, EA
Citation: Rh. Plovnick et Ea. Richards, New combustion synthesis route to TiB2-Al2O3, MATER RES B, 36(7-8), 2001, pp. 1487-1493

Authors: Richards, EA
Citation: Ea. Richards, Galaxy evolution in the reddest possible filter, ASTRO SP SC, 276(2-4), 2001, pp. 1169-1178

Authors: Chapman, SC Richards, EA Lewis, GF Wilson, G Barger, AJ
Citation: Sc. Chapman et al., The nature of the bright submillimeter galaxy population: A radio-preselected sample with I >similar to 25, ASTROPHYS J, 548(2), 2001, pp. L147-L151

Authors: Barger, AJ Cowie, LL Mushotzky, RF Richards, EA
Citation: Aj. Barger et al., The nature of the hard X-ray background sources: Optical, near-infrared, submillimeter, and radio properties, ASTRONOM J, 121(2), 2001, pp. 662-682

Authors: Haarsma, DB Partridge, RB Windhorst, RA Richards, EA
Citation: Db. Haarsma et al., Faint radio sources and star formation history, ASTROPHYS J, 544(2), 2000, pp. 641-658

Authors: Richards, EA
Citation: Ea. Richards, The nature of radio emission from distant galaxies: The 1.4 GHz observations, ASTROPHYS J, 533(2), 2000, pp. 611-630

Authors: Richards, EA
Citation: Ea. Richards, The nature of radio emission from distant galaxies, PUB AST S P, 112(773), 2000, pp. 1001-1002

Authors: Barger, AJ Cowie, LL Richards, EA
Citation: Aj. Barger et al., Mapping the evolution of high-redshift dusty galaxies with submillimeter observations of a radio-selected sample, ASTRONOM J, 119(5), 2000, pp. 2092-2109

Authors: Richards, EA Fomalont, EB Kellermann, KI Windhorst, RA Partridge, RB Cowie, LL Barger, AJ
Citation: Ea. Richards et al., Optically faint microjansky radio sources, ASTROPHYS J, 526(2), 1999, pp. L73-L76

Authors: Richards, EA
Citation: Ea. Richards, Radio identification of submillimeter sources in the Hubble Deep Field, ASTROPHYS J, 513(1), 1999, pp. L9-L12

Authors: Campos, A Yahil, A Windhorst, RA Richards, EA Pascarelle, S Impey, C Petry, C
Citation: A. Campos et al., A cluster or filament of galaxies at redshift z=2.5?, ASTROPHYS J, 511(1), 1999, pp. L1-L4
Risultati: 1-11 |