[AMH2017] ALMA-LAB5 , the SIMBAD biblio

[AMH2017] ALMA-LAB5 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST08:33:40


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Title First 3 Authors
2004AJ....128..569M 2 39 299 A SUBARU search for Lyα blobs in and around the protocluster region at redshift z = 3.1. MATSUDA Y., YAMADA T., HAYASHINO T., et al.
2005MNRAS.363.1398G 47 79 A submillimetre survey of Lyman α haloes in the SA22 protocluster at z= 3.1. GEACH J.E., MATSUDA Y., SMAIL I., et al.
2006ApJ...637L..89C 21 28 Ultraviolet-bright, high-redshift ultraluminous infrared galaxies. COLBERT J.W., TEPLITZ H., FRANCIS P., et al.
2009ApJ...692.1561W 240       D     X         7 50 27 Spitzer observations of extended Lyman-α clouds in the SSA22 field. WEBB T.M.A., YAMADA T., HUANG J.-S., et al.
2009ApJ...700....1G 278       D     X C F     6 38 106 The Chandra deep protocluster survey: Lyα blobs are powered by heating, not cooling. GEACH J.E., ALEXANDER D.M., LEHMER B.D., et al.
2011ApJ...728...59C 23 26 Polycyclic aromatic hydrocarbon emission within Lyα blobs. COLBERT J.W., SCARLATA C., TEPLITZ H., et al.
2011MNRAS.410L..13M 17       D               1 28 121 The Subaru Lyα blob survey: a sample of 100-kpc Lyα blobs at z= 3. MATSUDA Y., YAMADA T., HAYASHINO T., et al.
2012ApJ...750..116U 244       D     X C       6 39 24 Assembly of massive galaxies in a high-z protocluster. UCHIMOTO Y.K., YAMADA T., KAJISAWA M., et al.
2013MNRAS.430.2768T 15       D               1 44 15 Obscured star formation in Lyα blobs at z = 3.1. TAMURA Y., MATSUDA Y., IKARASHI S., et al.
2016ApJ...824...36C 17       D               1 37 84 The ubiquity of coeval starbursts in massive galaxy cluster progenitors. CASEY C.M.
2016MNRAS.460.4075H 16       D               2 38 9 The average submillimetre properties of Lyman α blobs at z = 3. HINE N.K., GEACH J.E., MATSUDA Y., et al.
2017ApJ...850..178A 16       D               3 45 7 Deep submillimeter and radio observations in the SSA22 field. I. Powering sources and the Lyα escape fraction of Lyα blobs. AO Y., MATSUDA Y., HENKEL C., et al.

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