SAS-LBG SSA22a-M28 , the SIMBAD biblio

SAS-LBG SSA22a-M28 , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.7 - 2021.06.18CEST21:06:56


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Title First 3 Authors
2018PASJ...70...65U 44           X         1 66 ~ ALMA deep field in SSA22: Survey design and source catalog of a 20 arcmin2 survey at 1.1 mm. UMEHATA H., HATSUKADE B., SMAIL I., et al.
2017ApJ...835...98U 17       D               1 52 17 ALMA deep field in SSA22: source catalog and number counts. UMEHATA H., TAMURA Y., KOHNO K., et al.
2017ApJ...850..178A 17       D               3 45 4 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.
2016MNRAS.455.3333K 1020       D S   X C F     22 25 15 An extremely dense group of massive galaxies at the centre of the protocluster at z = 3.09 in the SSA22 field. KUBO M., YAMADA T., ICHIKAWA T., et al.
2016MNRAS.460.4075H 17       D               4 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 518       D     X C F     11 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.
2015ApJ...799...38K 16       D               1 45 22 NIR spectroscopic observation of massive galaxies in the protocluster at z = 3.09. KUBO M., YAMADA T., ICHIKAWA T., et al.
2015ApJ...804...26A 99       D       C       3 26 ~ A deep narrowband imaging search for C IV and He II emission from Lyα blobs. ARRIGONI BATTAIA F., YANG Y., HENNAWI J.F., et al.
2015ApJ...815L...8U 43           X         1 18 36 ALMA deep field in SSA22: a concentration of dusty starbursts in a z = 3.09 protocluster core. UMEHATA H., TAMURA Y., KOHNO K., et al.
2014ApJ...795...33E 18       D               1 37 79 The Lyα properties of faint galaxies at z ∼ 2-3 with systemic redshifts and velocity dispersions from Keck-MOSFIRE. ERB D.K., STEIDEL C.C., TRAINOR R.F., et al.
2013ApJ...765...47N viz 177       D     X C       4 178 111 A refined estimate of the ionizing emissivity from galaxies at z ≃ 3: spectroscopic follow-up in the SSA22a field. NESTOR D.B., SHAPLEY A.E., KORNEI K.A., et al.
2013MNRAS.430.2768T 16       D               1 44 15 Obscured star formation in Lyα blobs at z = 3.1. TAMURA Y., MATSUDA Y., IKARASHI S., et al.
2012ApJ...750..116U 334       D     X C       8 39 24 Assembly of massive galaxies in a high-z protocluster. UCHIMOTO Y.K., YAMADA T., KAJISAWA M., et al.
2011ApJ...728...59C 16       D               1 23 26 Polycyclic aromatic hydrocarbon emission within Lyα blobs. COLBERT J.W., SCARLATA C., TEPLITZ H., et al.
2011ApJ...736...18N viz 94       D       C       4 154 99 Narrowband imaging of escaping lyman-continuum emission in the SSA22 field. NESTOR D.B., SHAPLEY A.E., STEIDEL C.C., et al.
2010MNRAS.401.1521M viz 16       D               1 245 93 On the stellar masses of IRAC detected Lyman break galaxies at z ∼ 3. MAGDIS G.E., RIGOPOULOU D., HUANG J.-S., et al.
2009ApJ...692.1561W 15       D               1 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 325       D     X C F     7 38 56 The Chandra deep protocluster survey: Lyα blobs are powered by heating, not cooling. GEACH J.E., ALEXANDER D.M., LEHMER B.D., et al.
2005MNRAS.363.1398G 47 56 A submillimetre survey of Lyman α haloes in the SA22 protocluster at z= 3.1. GEACH J.E., MATSUDA Y., SMAIL I., et al.
2004AJ....128..569M 2 39 177 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.
2003ApJ...592..728S viz 2596 511 Lyman break galaxies at redshift z ∼ 3: survey description and full data set. STEIDEL C.C., ADELBERGER K.L., SHAPLEY A.E., et al.
1998ApJ...492..428S 7 20 455 A large structure of galaxies at redshift z ∼ 3 and its cosmological implications. STEIDEL C.C., ADELBERGER K.L., DICKINSON M., et al.

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2021.06.18-21:06:56

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