[HOS2013] COSMOS-30679 , the SIMBAD biblio

[HOS2013] COSMOS-30679 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST11:00:02


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Title First 3 Authors
2013ApJ...765...70H 1308       D     X C       33 9 107 Gas motion study of Lyα emitters at z ∼ 2 using FUV and optical spectral lines. HASHIMOTO T., OUCHI M., SHIMASAKU K., et al.
2013ApJ...769....3N 1407     A D     X C       36 15 110 First spectroscopic evidence for high ionization state and low oxygen abundance in Lyα emitters. NAKAJIMA K., OUCHI M., SHIMASAKU K., et al.
2014ApJ...780...20R 212       D     X         6 12 15 The dynamical masses, densities, and star formation scaling relations of Lyα galaxies. RHOADS J.E., MALHOTRA S., RICHARDSON M.L.A., et al.
2014ApJ...788...74S 17       D               1 44 121 What is the physical origin of strong Lyα emission? II. Gas kinematics and distribution of Lyα emitters. SHIBUYA T., OUCHI M., NAKAJIMA K., et al.
2014ApJS..214...24S viz 16       D               1 66903 733 3D-HST WFC3-selected photometric catalogs in the five CANDELS/3D-HST fields: photometry, photometric redshifts, and stellar masses. SKELTON R.E., WHITAKER K.E., MOMCHEVA I.G., et al.
2014MNRAS.442..900N 51           X         1 11 272 Ionization state of inter-stellar medium in galaxies: evolution, SFR-M*-Z dependence, and ionizing photon escape. NAKAJIMA K. and OUCHI M.
2014ApJ...796...64C viz 16       D               1 91 20 Hubble Space Telescope emission line galaxies at z ∼ 2: the Lyα escape fraction. CIARDULLO R., ZEIMANN G.R., GRONWALL C., et al.
2015ApJ...812..157H 454       D     X C       11 16 56 A close comparison between observed and modeled Lyα lines for z ∼ 2.2 Lyα emitters. HASHIMOTO T., VERHAMME A., OUCHI M., et al.
2016ApJS..225...27M viz 16       D               1 19341 548 The 3D-HST survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for ∼ 100,000 galaxies. MOMCHEVA I.G., BRAMMER G.B., VAN DOKKUM P.G., et al.
2017MNRAS.465.1543H 41           X         1 18 16 Lyα emitters with very large Lyα equivalent widths, EW0(Lyα) ~= 200-400 Å, at z ∼ 2. HASHIMOTO T., OUCHI M., SHIMASAKU K., et al.
2018ApJ...859...84H 83           X         2 87 105 SILVERRUSH. V. Census of Lyα, [O III] λ5007, Hα, and [C II] 158 µm line emission with ∼1000 LAEs at z = 4.9-7.0 revealed with Subaru/HSC. HARIKANE Y., OUCHI M., SHIBUYA T., et al.

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