[MYH2004] LAB 18 , the SIMBAD biblio

[MYH2004] LAB 18 , the SIMBAD biblio (16 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:01:42

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		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 127       D     X         4 50 27 Spitzer observations of extended Lyman-α clouds in the SSA22 field. WEBB T.M.A., YAMADA T., HUANG J.-S., et al.
2009NewAR..53...54Y 37           X         1 5 2 Lymanalpha Blobs: Discussions in Heidelberg. YAMADA T.
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.
2011MNRAS.410L..13M 55       D     X         2 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.
2013MNRAS.430.2768T 707       D     X C       18 44 15 Obscured star formation in Lyα blobs at z = 3.1. TAMURA Y., MATSUDA Y., IKARASHI S., et al.
2014ApJ...784..171Y 712       D     X C       18 14 12 Pinpointing the molecular gas within an Lyα blob at z ∼ 2.7. YANG Y., WALTER F., DECARLI R., 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 448       D     X C       11 38 9 The average submillimetre properties of Lyman α blobs at z = 3. HINE N.K., GEACH J.E., MATSUDA Y., et al.
2016MNRAS.461.2944A 173       D     X C F     3 14 12 ALMA observations of a z [?] 3.1 protocluster: star formation from active galactic nuclei and Lyman-alpha blobs in an overdense environment. ALEXANDER D.M., SIMPSON J.M., HARRISON C.M., et al.
2017ApJ...850..178A 16       D               1 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.
2017MNRAS.471.1280T 18       D               1 13 73 The KMOS Deep Survey (KDS) - I. Dynamical measurements of typical star-forming galaxies at z ~= 3.5. TURNER O.J., CIRASUOLO M., HARRISON C.M., et al.
2018PASJ...70L...6K 1581       D     X C       39 6 2 A high dust emissivity index β for a CO-faint galaxy in a filamentary Lyα nebula at z = 3.1 . KATO Y., MATSUDA Y., IONO D., et al.
2026ApJ...998..345M 50           X         1 4 ~ ODIN: A New Lyα Blob Selection Method, Sample, and Statistical Analysis at z ∼ 3.1. MOON B., YANG Y., LEE K.-S., et al.

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