[ARK2015] 4886 , the SIMBAD biblio

[ARK2015] 4886 , the SIMBAD biblio (67 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST12:57:18


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Title First 3 Authors
2014ApJ...795...93Z 118           X         3 33 52 Young galaxy candidates in the Hubble Frontier Fields. I. A2744. ZHENG W., SHU X., MOUSTAKAS J., et al.
2015ApJ...799...12I 16       D               2 128 172 Hubble frontier fields first complete cluster data: faint galaxies at z ∼ 5-10 for UV luminosity functions and cosmic reionization. ISHIGAKI M., KAWAMATA R., OUCHI M., et al.
2015ApJ...800...18A viz 17       D               1 64 149 New constraints on the faint end of the UV luminosity function at z ∼ 7-8 using the gravitational lensing of the Hubble frontier fields cluster A2744. ATEK H., RICHARD J., KNEIB J.-P., et al.
2015ApJ...800...84C 17       D               1 33 121 Frontier Fields: high-redshift predictions and early results. COE D., BRADLEY L. and ZITRIN A.
2015ApJ...804..103K 16       D               1 40 74 The sizes of z ∼ 6-8 lensed galaxies from the Hubble frontier fields Abell 2744 data. KAWAMATA R., ISHIGAKI M., SHIMASAKU K., et al.
2015MNRAS.450.3032M 20       D               1 15 149 New redshift z ≃ 9 galaxies in the Hubble Frontier Fields: implications for early evolution of the UV luminosity density. McLEOD D.J., McLURE R.J., DUNLOP J.S., et al.
2016ApJ...818...38S 16       D               1 87 48 The Grism Lens-Amplified Survey from Space (GLASS). III. A census of Lyα emission at z ≳ 7 from HST spectroscopy. SCHMIDT K.B., TREU T., BRADAC M., et al.
2016ApJ...819..114K viz 17       D               2 129 156 Precise strong lensing mass modeling of four Hubble frontier field clusters and a sample of magnified high-redshift galaxies. KAWAMATA R., OGURI M., ISHIGAKI M., et al.
2016ApJ...820...98L viz 16       D               1 142 43 Young galaxy candidates in the Hubble Frontier Fields. III. MACS J0717.5+3745. LAPORTE N., INFANTE L., TRONCOSO IRIBARREN P., et al.
2016ApJ...822....5I 241           X         6 14 10 A very compact dense galaxy overdensity with δ [?] 130 identified at z ∼ 8: implications for early protocluster and cluster core formation. ISHIGAKI M., OUCHI M. and HARIKANE Y.
2016A&A...590A..30M viz 16       D               1 14127 94 The ASTRODEEP Frontier Fields catalogues. I. Multiwavelength photometry of Abell-2744 and MACS-J0416. MERLIN E., AMORIN R., CASTELLANO M., et al.
2016A&A...590A..31C viz 16       D               1 14130 105 The ASTRODEEP Frontier Fields catalogues. II. Photometric redshifts and rest frame properties in Abell-2744 and MACS-J0416. CASTELLANO M., AMORIN R., MERLIN E., et al.
2016MNRAS.459.3812M 20       D               1 41 174 The z = 9-10 galaxy population in the Hubble Frontier Fields and CLASH surveys: the z = 9 luminosity function and further evidence for a smooth decline in ultraviolet luminosity density at z≥ 8. McLEOD D.J., McLURE R.J. and DUNLOP J.S.
2017ApJ...835..113L viz 17       D               1 166 327 Directly observing the galaxies likely responsible for reionization. LIVERMORE R.C., FINKELSTEIN S.L. and LOTZ J.M.
2017ApJ...837L..21L 959     A     X C       21 3 248 Dust in the reionization era: ALMA observations of a z = 8.38 gravitationally lensed galaxy. LAPORTE N., ELLIS R.S., BOONE F., et al.
2017ApJ...845..175J 51           X         1 2 20 Galaxy formation through filamentary accretion at z = 6.1. JONES G.C., WILLOTT C.J., CARILLI C.L., et al.
2018MNRAS.473.5363W 83               F     2 11 16 Dust-obscured star-forming galaxies in the early universe. WILKINS S.M., FENG Y., DI MATTEO T., et al.
2018ApJ...854...36I 99       D     X         3 21 12 A model connecting galaxy masses, star formation rates, and dust temperatures across cosmic time. IMARA N., LOEB A., JOHNSON B.D., et al.
2018ApJ...854...73I viz 16       D               2 443 240 Full-data results of Hubble Frontier Fields: UV luminosity functions at z ∼ 6-10 and a consistent picture of cosmic reionization. ISHIGAKI M., KAWAMATA R., OUCHI M., et al.
2018ApJ...855....4K viz 16       D               2 1029 127 Size-luminosity relations and UV luminosity functions at z = 6-9 simultaneously derived from the complete Hubble Frontier Fields data. KAWAMATA R., ISHIGAKI M., SHIMASAKU K., et al.
2018MNRAS.477..552B 713     A D     X C       17 7 92 Dusty galaxies in the Epoch of Reionization: simulations. BEHRENS C., PALLOTTINI A., FERRARA A., et al.
2018ApJ...862..156L viz 16       D               1 687 8 Magnification bias of distant galaxies in the Hubble Frontier Fields: testing wave versus particle dark matter predictions. LEUNG E., BROADHURST T., LIM J., et al.
2018ApJ...868...62G 58       D     X         2 31 7 Maximally dusty star-forming galaxies: supernova dust production and recycling in Local Group and high-redshift galaxies. GALL C. and HJORTH J.
2019MNRAS.484.4054K 46           X         1 4 16 Probing cosmic dawn: modelling the assembly history, SEDs, and dust content of selected z ∼ 9 galaxies. KATZ H., LAPORTE N., ELLIS R.S., et al.
2019ApJ...874...27T 263           X C       5 12 154 Detection of the far-infrared [O III] and dust emission in a galaxy at redshift 8.312: early metal enrichment in the heart of the reionization era. TAMURA Y., MAWATARI K., HASHIMOTO T., et al.
2019A&A...624L..13L 254           X         6 14 54 Dust production scenarios in galaxies at z ∼6-8.3. LESNIEWSKA A. and MICHALOWSKI M.J.
2019MNRAS.485.3947M 232       D     X         6 22 148 Inferences on the timeline of reionization at z ∼ 8 from the KMOS Lens-Amplified Spectroscopic Survey. MASON C.A., FONTANA A., TREU T., et al.
2019MNRAS.486.2197B 48           X         1 1 6 Ly α emission from galaxies in the Epoch of Reionization. BEHRENS C., PALLOTTINI A., FERRARA A., et al.
2019MNRAS.487L..81L 902     A D     X C F     20 2 49 The absence of [C II] 158 µm emission in spectroscopically confirmed galaxies at z > 8. LAPORTE N., KATZ H., ELLIS R.S., et al.
2019MNRAS.487.3007K 44           X         1 26 66 Kinematics of z >= 6 galaxies from [C II] line emission. KOHANDEL M., PALLOTTINI A., FERRARA A., et al.
2019MNRAS.490..540L 184       D     X C F     3 4 ~ Expected dust grain-size distributions in galaxies detected by ALMA at z > 7. LIU H.-M. and HIRASHITA H.
2019PASJ...71...71H 23       D               2 31 193 Big Three Dragons: A z = 7.15 Lyman-break galaxy detected in [O III] 88 μm, [C II] 158 μm, and dust continuum with ALMA. HASHIMOTO T., INOUE A.K., MAWATARI K., et al.
2019PASJ...71..109H 85             C       1 25 33 Detections of [O III] 88 μm in two quasars in the reionization epoch. HASHIMOTO T., INOUE A.K., TAMURA Y., et al.
2020MNRAS.493.4294B 219           X         5 14 97 ALMA uncovers the [C II] emission and warm dust continuum in a z = 8.31 Lyman break galaxy. BAKX T.J.L.C., TAMURA Y., HASHIMOTO T., et al.
2020MNRAS.494.1071G 146       D     X   F     3 54 62 The assembly of dusty galaxies at z >= 4: statistical properties. GRAZIANI L., SCHNEIDER R., GINOLFI M., et al.
2020ApJ...896...93H 104       D     X         3 50 106 Large population of ALMA galaxies at z > 6 with very high [O III] 88 µm to [C II] 158 µm flux ratios: evidence of extremely high ionization parameter or PDR deficit? HARIKANE Y., OUCHI M., INOUE A.K., et al.
2020MNRAS.497.3440R 745       D     X C F     16 12 54 Interpreting the Spitzer/IRAC colours of 7 <= z <= 9 galaxies: distinguishing between line emission and starlight using ALMA. ROBERTS-BORSANI G.W., ELLIS R.S. and LAPORTE N.
2020MNRAS.498..164K 128           X         3 39 32 New methods for identifying Lyman continuum leakers and reionization-epoch analogues. KATZ H., DUROVCIKOVA D., KIMM T., et al.
2020ApJ...903..150J 18       D               2 32 41 The mass-metallicity relation at z ≃ 8: direct-method metallicity constraints and near-future prospects. JONES T., SANDERS R., ROBERTS-BORSANI G., et al.
2020MNRAS.499.1701B 553           X C F     11 5 ~ Theoretical clues about dust accumulation and galaxy obscuration at high and low redshift. BARBOSA-SANTOS J.H., LIMA NETO G.B. and FRIACA A.C.S.
2020MNRAS.499.3417Y 272       D     X   F     6 9 ~ An analytic model for [O III] fine structure emission from high redshift galaxies. YANG S. and LIDZ A.
2020MNRAS.499.5136C 660       D S   X C F     13 14 65 Missing [C II] emission from early galaxies. CARNIANI S., FERRARA A., MAIOLINO R., et al.
2020A&A...643A...3S 51           X         1 10 89 The ALPINE-ALMA [C II] survey. Little to no evolution in the [C II]-SFR relation over the last 13 Gyr. SCHAERER D., GINOLFI M., BETHERMIN M., et al.
2021A&A...646A..26B 218           X   F     4 16 ~ A puzzling non-detection of [O III] and [C II] from a z ≃ 7.7 galaxy observed with ALMA. BINGGELI C., INOUE A.K., HASHIMOTO T., et al.
2021MNRAS.504..723Y 192       D     X C       4 10 ~ The prospects for observing [O III] 52 micron emission from galaxies during the Epoch of Reionization. YANG S., LIDZ A. and POPPING G.
2021MNRAS.505.5543V 454       D     X   F     10 15 29 High [O III]/[C II] surface brightness ratios trace early starburst galaxies. VALLINI L., FERRARA A., PALLOTTINI A., et al.
2021MNRAS.507.1175M 44           X         1 2 ~ Dust grain growth at high redshift: starburst-driven CMB-dark supershells. MARTINEZ-GONZALEZ S., SILICH S. and TENORIO-TAGLE G.
2021MNRAS.508L..58B 94               F     2 6 42 Accurate dust temperature determination in a z = 7.13 galaxy. BAKX T.J.L.C., SOMMOVIGO L., CARNIANI S., et al.
2022MNRAS.510.5603K 111       D         F     2 9 29 The nature of high [O III]_88 µ m_/[C II]_158 µm_ galaxies in the epoch of reionization: Low carbon abundance and a top-heavy IMF? KATZ H., ROSDAHL J., KIMM T., et al.
2022MNRAS.513.3122S 359     A D     X C       8 30 49 The ALMA REBELS Survey: cosmic dust temperature evolution out to z ∼ 7. SOMMOVIGO L., FERRARA A., PALLOTTINI A., et al.
2022ApJ...931..160B 46           X         1 50 96 Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z > 6.5 Universe. BOUWENS R.J., SMIT R., SCHOUWS S., et al.
2022MNRAS.514.1148Y 18       D               1 90 19 The size-luminosity relation of lensed galaxies at z ∼ 6-9 in the Hubble Frontier Fields. YANG L., LEETHOCHAWALIT N., TREU T., et al.
2022MNRAS.515.3126I viz 18       D               1 46 45 The ALMA REBELS Survey: dust continuum detections at z > 6.5. INAMI H., ALGERA H.S.B., SCHOUWS S., et al.
2022MNRAS.515.5813P 45           X         1 7 ~ Intensity mapping from the sky: synergizing the joint potential of [O III] and [C II] surveys at reionization. PADMANABHAN H., BREYSSE P., LIDZ A., et al.
2022A&A...664L...5B 45           X         1 4 ~ A tentative ∼1000 km s–1 offset between the [CII] 158 µm and Lyα line emission in a star-forming galaxy at z = 7.2. BAIER-SOTO R., HERRERA-CAMUS R., FORSTER SCHREIBER N.M., et al.
2022MNRAS.516.1612H 108       D       C       2 10 6 Analytic models of dust temperature in high-redshift galaxies. HIRASHITA H. and CHIANG I.-D.
2022ApJ...938L..13R 93               F     1 11 33 Early Results from GLASS-JWST. I: Confirmation of Lensed z ≥ 7 Lyman-break Galaxies behind the Abell 2744 Cluster with NIRISS. ROBERTS-BORSANI G., MORISHITA T., TREU T., et al.
2022MNRAS.517.5930S 90               F     1 27 10 A new look at the infrared properties of z ∼ 5 galaxies. SOMMOVIGO L., FERRARA A., CARNIANI S., et al.
2023ApJ...947L..24M 719       D     X C       15 18 31 Early Results from GLASS-JWST. XIV. A Spectroscopically Confirmed Protocluster 650 Million Years after the Big Bang. MORISHITA T., ROBERTS-BORSANI G., TREU T., et al.
2023ApJ...948....3U 93             C       1 9 ~ Detections of [C II] 158 μm and [O III] 88 μm in a Local Lyman Continuum Emitter, Mrk 54, and Its Implications to High-redshift ALMA Studies. URA R., HASHIMOTO T., INOUE A.K., et al.
2023ApJ...950...94L 140           X C       2 6 5 Cosmic Sands: The Origin of Dusty, Star-forming Galaxies in the Epoch of Reionization. LOWER S., NARAYANAN D., LI Q., et al.
2023ApJ...953..140N 47           X         1 7 ~ Simulations of High-redshift [O III] Emitters: Chemical Evolution and Multiline Diagnostics. NAKAZATO Y., YOSHIDA N. and CEVERINO D.
2023ApJ...955L...2H 1232       D     X C       26 6 ~ Reionization and the ISM/Stellar Origins with JWST and ALMA (RIOJA): The Core of the Highest-redshift Galaxy Overdensity at z = 7.88 Confirmed by NIRSpec/JWST. HASHIMOTO T., ALVAREZ-MARQUEZ J., FUDAMOTO Y., et al.
2023ApJ...956...61A 93             C       1 3 ~ Two Massive, Compact, and Dust-obscured Candidate z ≃ 8 Galaxies Discovered by JWST. AKINS H.B., CASEY C.M., ALLEN N., et al.
2023ApJ...956..139I 19       D               1 13 ~ Redshift Evolution of Electron Density in the Interstellar Medium at z ∼ 0-9 Uncovered with JWST/NIRSpec Spectra and Line-spread Function Determinations. ISOBE Y., OUCHI M., NAKAJIMA K., et al.
2023ApJ...957...39L 159       D     X C       3 11 ~ Evolution of the Mass-Metallicity Relation from Redshift z ≈ 8 to the Local Universe. LANGEROODI D., HJORTH J., CHEN W., et al.
2023ApJS..269...33N 19       D               1 19 ~ JWST Census for the Mass-Metallicity Star Formation Relations at z = 4-10 with Self-consistent Flux Calibration and Proper Metallicity Calibrators. NAKAJIMA K., OUCHI M., ISOBE Y., et al.

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