[MTS2007] 66 , the SIMBAD biblio

[MTS2007] 66 , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.7 - 2020.01.25CET15:22:14


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Title First 3 Authors
2019ApJ...872..117G 47           X         1 55 ~ Confirming Herschel candidate protoclusters from ALMA/VLA CO observations. GOMEZ-GUIJARRO C., RIECHERS D.A., PAVESI R., et al.
2019ApJ...882..168P 4824       D     X C       103 20 ~ Low star formation efficiency in typical galaxies at z = 5-6. PAVESI R., RIECHERS D.A., FAISST A.L., et al.
2019ApJ...886...29S 205       D     X         5 10 ~ Fast outflows identified in early star-forming galaxies at z = 5-6. SUGAHARA Y., OUCHI M., HARIKANE Y., et al.
2019MNRAS.487.1689P 93               F     1 15 ~ Deep into the structure of the first galaxies: SERRA views. PALLOTTINI A., FERRARA A., DECATALDO D., et al.
2018A&A...609A.130L viz 49 13 The [CII] 158 µm line emission in high-redshift galaxies. LAGACHE G., COUSIN M. and CHATZIKOS M.
2018A&A...617A.131S 672           X         15 16 ~ "Zombie" or active? An alternative explanation to the properties of star-forming galaxies at high redshift. SATURNI F.G., MANCINI M., PEZZULLI E., et al.
2018ApJ...859...84H 18       D               1 39 13 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.
2018ApJ...861...43P 1550     A     X C       34 13 4 Hidden in plain sight: a massive, dusty starburst in a galaxy protocluster at z = 5.7 in the COSMOS field. PAVESI R., RIECHERS D.A., SHARON C.E., et al.
2018ApJ...861...95H 45           X         1 31 5 SHINING, a survey of far-infrared lines in nearby galaxies. II. Line-deficit models, AGN impact, [C II]-SFR scaling relations, and mass-metallicity relation in (U)LIRGs. HERRERA-CAMUS R., STURM E., GRACIA-CARPIO J., et al.
2018MNRAS.473.1909G 45           X         1 17 10 Alma suggests outflows in z∼ 5.5 galaxies. GALLERANI S., PALLOTTINI A., FERUGLIO C., et al.
2018MNRAS.477..552B 180           X C       3 7 7 Dusty galaxies in the Epoch of Reionization: simulations. BEHRENS C., PALLOTTINI A., FERRARA A., et al.
2018MNRAS.478.1170C 376       D     X         9 38 6 Kiloparsec-scale gaseous clumps and star formation at z = 5-7. CARNIANI S., MAIOLINO R., AMORIN R., et al.
2017ApJ...834....5S 88             C       1 19 28 The spatially resolved [CII] cooling line deficit in galaxies. SMITH J.D.T., CROXALL K., DRAINE B., et al.
2017ApJ...845...41B 192       D     X C       4 13 12 Dust properties of C II detected z ∼ 5.5 galaxies: new HST/WFC3 near-IR observations. BARISIC I., FAISST A.L., CAPAK P.L., et al.
2017ApJ...846..105O viz 17       D               2 35 14 SIGAME simulations of the [C II], [O I] and [O III] line emission from star-forming galaxies at z ~= 6. OLSEN K., GREVE T.R., NARAYANAN D., et al.
2017ApJ...847...21F 975       D     X C       22 47 17 Are high-redshift galaxies hot? Temperature of z > 5 galaxies and implications for their dust properties. FAISST A.L., CAPAK P.L., YAN L., et al.
2017ApJ...850..180J 696     A D S   X         16 19 8 Dynamical characterization of galaxies at z ∼ 4-6 via tilted ring fitting to ALMA [C II] observations. JONES G.C., CARILLI C.L., SHAO Y., et al.
2016ApJ...832..151P 1976       D S   X C       45 12 16 ALMA reveals weak [N II] emission in "typical" galaxies and intense starbursts at z = 5-6. PAVESI R., RIECHERS D.A., CAPAK P.L., et al.
2015Natur.522..455C 10 15 153 Galaxies at redshifts 5 to 6 with systematically low dust content and high [C II] emission. CAPAK P.L., CARILLI C., JONES G., et al.
2012ApJ...760..128M viz 16       D               1 237 41 Lyα emission from high-redshift sources in COSMOS. MALLERY R.P., MOBASHER B., CAPAK P., et al.
2009ApJ...701..915T 16       D               1 127 18 Hubble space Telescope/Advanced camera for surveys morphology of Lyα emitters at redshift 5.7 in the COSMOS field. TANIGUCHI Y., MURAYAMA T., SCOVILLE N.Z., et al.
2007ApJS..172..523M viz 15       D               121 73 Lyα emitters at redshift 5.7 in the COSMOS field. MURAYAMA T., TANIGUCHI Y., SCOVILLE N.Z., et al.

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2020.01.25-15:22:14

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