NAME Himiko , the SIMBAD biblio

NAME Himiko , the SIMBAD biblio (101 results) C.D.S. - SIMBAD4 rel 1.8 - 2023.09.26CEST13:28:38

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Title First 3 Authors
2009ApJ...696.1164O 800       D     X C F     19 3 137 Discovery of a giant Lyα emitter near the reionization epoch. OUCHI M., ONO Y., EGAMI E., et al.
2010ApJ...723..869O 30       D               1 18 563 Statistics of 207 Lyα emitters at a redshift near 7: constraints on reionization and galaxy formation models. OUCHI M., SHIMASAKU K., FURUSAWA H., et al.
2010ApJ...724.1524O 97           X         2 4 163 Stellar populations of Lyα emitters at z ∼ 6-7: constraints on the escape fraction of ionizing photons from galaxy building blocks. ONO Y., MASAMI O., SHIMASAKU K., et al.
2012ApJ...751L..24W 882     A S   X C       21 5 13 A deep search for CO J = 2-1 emission from a Lyα blob at z ∼ 6.595. WAGG J. and KANEKAR N.
2012ApJ...752...93W 1093     A D     X C       28 11 43 Evidence for low extinction in actively star-forming galaxies at z > 6.5. WALTER F., DECARLI R., CARILLI C., et al.
2012A&A...547A..51G 16       D               1 115 62 The size-luminosity relation at z=7 in CANDELS and its implication on reionization. GRAZIAN A., CASTELLANO M., FONTANA A., et al.
2013MNRAS.432L...6B 237           X   F     5 2 6 Identifying Lyman α emitters powered by AGNs. BAEK S. and FERRARA A.
2013ApJS..206...10G viz 16       D               1 34915 252 CANDELS multiwavelength catalogs: source identification and photometry in the CANDELS UKIDSS ultra-deep survey field. GALAMETZ A., GRAZIAN A., FONTANA A., et al.
2013MNRAS.432.2696M viz 16       D               1 209 345 A new multifield determination of the galaxy luminosity function at z = 7-9 incorporating the 2012 Hubble ultra-deep field imaging. McLURE R.J., DUNLOP J.S., BOWLER R.A.A., et al.
2013MNRAS.433.1567V 310     A     X         8 2 44 Far-infrared line emission from high-redshift galaxies. VALLINI L., GALLERANI S., FERRARA A., et al.
2013ApJ...772...99J 16       D               1 68 51 Physical properties of spectroscopically confirmed galaxies at z ≥ 6. I. Basic characteristics of the rest-frame UV continuum and Lyα emission. JIANG L., EGAMI E., MECHTLEY M., et al.
2013ApJ...773..153J 79               F     1 46 42 Physical properties of spectroscopically confirmed galaxies at z ≥ 6. II. Morphology of the rest-frame UV continuum and Lyα emission. JIANG L., EGAMI E., FAN X., et al.
2013ApJ...778..102O 4041     A S   X C       101 16 177 An intensely star-forming galaxy at z ∼ 7 with low dust and metal content revealed by deep ALMA and HST observations. OUCHI M., ELLIS R., ONO Y., et al.
2014ApJ...782L..23H 41           X         1 4 15 Shaping the dust mass-star-formation rate relation. HJORTH J., GALL C. and MICHALOWSKI M.J.
2014MNRAS.438.2483M 254       D     X         7 13 14 Extreme galaxies during reionization: testing ISM and disc models. MUNOZ J.A. and FURLANETTO S.R.
2014ApJ...784...99G 477       S   X C       10 24 31 Search for [C II] emission in z = 6.5-11 star-forming galaxies. GONZALEZ-LOPEZ J., RIECHERS D.A., DECARLI R., et al.
2014ApJ...785...64S 42           X         1 5 26 What is the physical origin of strong Lyα emission? I. Demographics of Lyα emitter structures. SHIBUYA T., OUCHI M., NAKAJIMA K., et al.
2014ApJ...787....9W 120           X         3 4 15 Constraining the Lyα escape fraction with far-infrared observations of Lyα emitters. WARDLOW J.L., MALHOTRA S., ZHENG Z., et al.
2014MNRAS.440.2375M 40           X         1 22 32 A 10 deg2 Lyman α survey at z=8.8 with spectroscopic follow-up: strong constraints on the luminosity function and implications for other surveys. MATTHEE J.J.A., SOBRAL D., SWINBANK A.M., et al.
2014MNRAS.440.2810B viz 772       D     X C       19 40 174 The bright end of the galaxy luminosity function at z ≃ 7: before the onset of mass quenching ? BOWLER R.A.A., DUNLOP J.S., McLURE R.J., et al.
2014ApJ...788L..30D 42           X         1 4 23 Dust formation, evolution, and obscuration effects in the very high-redshift universe. DWEK E., STAGUHN J., ARENDT R.G., et al.
2014ApJ...792...34O 2463           X C       61 34 104 ALMA observation of 158 µm [C II] line and dust continuum of a z = 7 normally star-forming galaxy in the epoch of reionization. OTA K., WALTER F., OHTA K., et al.
2014A&A...568A..62D 95       D       C       2 467 300 The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types. DE LOOZE I., CORMIER D., LEBOUTEILLER V., et al.
2014AJ....148...73M 119           X         3 10 11 Close companions to two high-redshift quasars. McGREER I.D., FAN X., STRAUSS M.A., et al.
2014A&A...569A..98T 280           X C       6 17 75 Dust and gas in luminous proto-cluster galaxies at z = 4.05: the case for different cosmic dust evolution in normal and starburst galaxies. TAN Q., DADDI E., MAGDIS G., et al.
2014ApJ...795....5O 334       D     X C       8 36 59 Faint submillimeter galaxies revealed by multifield deep ALMA observations: number counts, spatial clustering, and a dark submillimeter line emitter. ONO Y., OUCHI M., KURONO Y., et al.
2014MNRAS.443.1704H 1455     A     X C F     35 7 17 Constraining dust formation in high-redshift young galaxies. HIRASHITA H., FERRARA A., DAYAL P., et al.
2014MNRAS.443.3795R 79           X         2 18 12 Spectroscopy of 7 radio-loud QSOs at 2 < z < 6: giant Lyman α emission nebulae accreting on to host galaxies. ROCHE N., HUMPHREY A. and BINETTE L.
2014ApJ...796...96B 238           X C       5 31 13 ALMA observations of the host galaxy of GRB 090423 at z = 8.23: deep limits on obscured star formation 630 million years after the Big Bang. BERGER E., ZAUDERER B.A., CHARY R.-R., et al.
2015ApJ...799..166B 41           X         1 7 11 Cosmic evolution of dust in galaxies: methods and preliminary results. BEKKI K.
2015A&A...574A..14C 70           X         1 6 183 Very extended cold gas, star formation and outflows in the halo of a bright quasar at z >6. CICONE C., MAIOLINO R., GALLERANI S., et al.
2015A&A...574A..19S 1368     A D     X C       34 23 69 New constraints on dust emission and UV attenuation of z = 6.5-7.5 galaxies from millimeter observations. SCHAERER D., BOONE F., ZAMOJSKI M., et al.
2015ApJ...800L..29K 60           X         1 1 20 First infrared-based implications for the dust attenuation and star formation of typical Lyα emitters. KUSAKABE H., SHIMASAKU K., NAKAJIMA K., et al.
2015ApJ...801..122S 100       D       C       2 33 146 High-precision photometric redshifts from Spitzer/Irac: extreme [3.6] - [4.5] colors identify galaxies in the redshift range z ∼ 6.6 - 6.9. SMIT R., BOUWENS R.J., FRANX M., et al.
2015ApJ...803L...8R 40           X         1 8 3 Supernova remnant mass accumulated during the star formation history of the z = 3.8 radio galaxies 4C41.17 and TN J2007-1316. ROCCA-VOLMERANGE B., DROUART G. and DE BREUCK C.
2015ApJ...803...34B viz 136       D     X         4 10321 1045 UV luminosity functions at redshifts z ∼ 4 to z ∼ 10: 10,000 galaxies from HST legacy fields. BOUWENS R.J., ILLINGWORTH G.D., OESCH P.A., et al.
2015Natur.519..327W 31 9 282 A dusty, normal galaxy in the epoch of reionization. WATSON D., CHRISTENSEN L., KNUDSEN K.K., et al.
2015A&A...577A..80M 224       D   O X         6 13 97 Dust production 680-850 million years after the Big Bang. MICHALOWSKI M.J.
2015ApJ...806..108B 16       D               1 14 4 LBT/LUCI spectroscopic observations of zÅ=7 galaxies. BIAN F., STARK D.P., FAN X., et al.
2015ApJ...807..180W 133           X         3 11 148 Star formation and the interstellar medium in z > 6 UV-luminous Lyman-break galaxies. WILLOTT C.J., CARILLI C.L., WAGG J., et al.
2015ApJ...808..139S 874       D S   X C       19 5 275 Evidence for PopIII-like stellar populations in the most luminous lyman-α emitters at the epoch of reionization: spectroscopic confirmation. SOBRAL D., MATTHEE J., DARVISH B., et al.
2015MNRAS.451L..70M 67       D     X         2 11 123 The dust mass in z > 6 normal star-forming galaxies. MANCINI M., SCHNEIDER R., GRAZIANI L., et al.
2015MNRAS.451..400M 426           X         10 6 153 Identification of the brightest Lyα emitters at z = 6.6: implications for the evolution of the luminosity function in the reionization era. MATTHEE J., SOBRAL D., SANTOS S., et al.
2015MNRAS.451.2050Z 2169 T K A D     X C F     52 9 20 Deep rest-frame far-UV spectroscopy of the giant Lyman α emitter `
2015ApJ...813...36V 90             C       2 14 144 On the [CII]-SFR relation in high redshift galaxies. VALLINI L., GALLERANI S., FERRARA A., et al.
2015ApJ...814...76O 48           X         1 3 25 Simulator of galaxy Millimeter/Submillimeter emission (SiGAME): the [C ii]-SFR relationship of massive z = 2 main sequence galaxies. OLSEN K.P., GREVE T.R., NARAYANAN D., et al.
2015MNRAS.453L..88Z 40           X         1 11 7 Early science with the Large Millimeter Telescope: dust constraints in a z ∼ 9.6 galaxy. ZAVALA J.A., MICHALOWSKI M.J., ARETXAGA I., et al.
2015MNRAS.453.2465P 58           X         1 4 73 The brightest Lyα emitter: Pop III or black hole? PALLOTTINI A., FERRARA A., PACUCCI F., et al.
2016ApJ...816...16J 16       D               3 44 23 Physical properties of spectroscopically confirmed galaxies at z ≥ 6. III. Stellar populations from SED modeling with secure Lyα emission and redshifts. JIANG L., FINLATOR K., COHEN S.H., et al.
2015MNRAS.452.1817B 172           X         4 14 161 The galaxy luminosity function at z~= 6 and evidence for rapid evolution in the bright end from z~=7 to 5. BOWLER R.A.A., DUNLOP J.S., McLURE R.J., et al.
2016ApJS..222....1F viz 43           X         1 40 108 ALMA census of faint 1.2 mm sources down to ∼ 0.02 mJy: extragalactic background light and dust-poor, high-z galaxies. FUJIMOTO S., OUCHI M., ONO Y., et al.
2016MNRAS.462.2184H 92           X         2 4 46 Exploring the nature of the Lyman-α emitter CR7. HARTWIG T., LATIF M.A., MAGG M., et al.
2017ApJ...836L...2B 47           X         1 7 44 ALMA C II 158 µm detection of a redshift 7 lensed galaxy behind RX J1347.1-1145. BRADAC M., GARCIA-APPADOO D., HUANG K.-H., et al.
2016MNRAS.462L...6K 49           X         1 12 97 [C II] emission in z ∼ 6 strongly lensed, star-forming galaxies. KNUDSEN K.K., RICHARD J., KNEIB J.-P., et al.
2017MNRAS.465.2540P 66           X         1 4 100 Zooming on the internal structure of z ~= 6 galaxies. PALLOTTINI A., FERRARA A., GALLERANI S., et al.
2017MNRAS.465.3475W 42           X         1 4 6 Dust evolution processes in normal galaxies at z > 6 detected by ALMA. WANG W.-C., HIRASHITA H. and HOU K.-C.
2017MNRAS.466.3612B 1198     A D     X C       29 31 129 Unveiling the nature of bright z ~= 7 galaxies with the Hubble Space Telescope. BOWLER R.A.A., DUNLOP J.S., McLURE R.J., et al.
2017MNRAS.467..768R 123           X         3 7 4 A multiply imaged z ∼ 6.3 Lyman α emitter candidate behind Abell 2261. RYDBERG C.-E., ZITRIN A., ZACKRISSON E., et al.
2017MNRAS.468.1505M 79           X         1 3 114 Simulating the dust content of galaxies: successes and failures. McKINNON R., TORREY P., VOGELSBERGER M., et al.
2017MNRAS.469..448B 99           X         2 3 51 No evidence for Population III stars or a direct collapse black hole in the z = 6.6 Lyman α emitter 'CR7'. BOWLER R.A.A., McLURE R.J., DUNLOP J.S., et al.
2017ApJ...846..105O viz 18       D               2 36 76 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...846..134J 99       D     X         3 40 8 A Magellan M2FS spectroscopic survey of galaxies at 5.5 < z < 6.8: program overview and a sample of the brightest Lyα emitters. JIANG L., SHEN Y., BIAN F., et al.
2017ApJ...851..145M 388           X         9 5 91 ALMA reveals metals yet no dust within multiple components in CR7. MATTHEE J., SOBRAL D., BOONE F., et al.
2017MNRAS.471.4128P 103             C       1 4 85 The impact of chemistry on the structure of high-z galaxies. PALLOTTINI A., FERRARA A., BOVINO S., et al.
2017MNRAS.472.4587H 2678     A D S   X C F     63 2 6 Dust masses of z > 5 galaxies from SED fitting and ALMA upper limits. HIRASHITA H., BURGARELLA D. and BOUWENS R.J.
2018ApJ...853...81C 42           X         1 3 ~ Observing galaxy mergers at the epoch of reionization. CHAIKIN E.A., TYULNEVA N.V. and KAUROV A.A.
2018MNRAS.473.5363W 252           X   F     5 11 16 Dust-obscured star-forming galaxies in the early universe. WILKINS S.M., FENG Y., DI MATTEO T., et al.
2017MNRAS.472..772M viz 511       D     X C       12 48 66 Spectroscopic properties of luminous Ly α emitters at z ~= 6-7 and comparison to the Lyman-break population. MATTHEE J., SOBRAL D., DARVISH B., et al.
2018ApJ...854L...7C 1038 T   A     X C       23 6 60 ALMA detection of extended [C II] emission in
Himiko at z = 6.6.
2018ApJ...856..109O 86           X         2 9 22 Large-scale environment of a z = 6.61 luminous quasar probed by Lyα emitters and Lyman break galaxies. OTA K., VENEMANS B.P., TANIGUCHI Y., et al.
2018ApJ...859...84H 143       D     X         4 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.
2018MNRAS.477.2817S viz 43           X         1 42 71 The nature of luminous Ly α emitters at z ∼ 2-3: maximal dust-poor starbursts and highly ionizing AGN. SOBRAL D., MATTHEE J., DARVISH B., et al.
2018MNRAS.478.1170C 437       D     X         11 38 108 Kiloparsec-scale gaseous clumps and star formation at z = 5-7. CARNIANI S., MAIOLINO R., AMORIN R., et al.
2018A&A...619A.136M viz 134           X C       2 7 63 Confirmation of double peaked Lyα emission at z=6.593. Witnessing a galaxy directly contributing to the reionisation of the Universe. MATTHEE J., SOBRAL D., GRONKE M., et al.
2019ApJ...871..109P 145       D     X         4 28 1 Multiband optical and near-infrared properties of faint submillimeter galaxies with serendipitous ALMA detections. PATIL P., NYLAND K., LACY M., et al.
2018PASJ...70S..15S 18       D               1 104 117 SILVERRUSH. III. Deep optical and near-infrared spectroscopy for Lyα and UV-nebular lines of bright Lyα emitters at z = 6-7. SHIBUYA T., OUCHI M., HARIKANE Y., et al.
2019A&A...623A.157S 2 27 57 Predicting Lyα escape fractions with a simple observable. Lyα in emission as an empirically calibrated star formation rate indicator. SOBRAL D. and MATTHEE J.
2019A&A...624L..13L 344           X         8 14 54 Dust production scenarios in galaxies at z ∼6-8.3. LESNIEWSKA A. and MICHALOWSKI M.J.
2019ApJ...879...28H 44           X         1 46 57 SILVERRUSH. VII. Subaru/HSC identifications of protocluster candidates at z ∼ 6-7: implications for cosmic reionization. HIGUCHI R., OUCHI M., ONO Y., et al.
2019MNRAS.487.3007K 19       D               2 26 66 Kinematics of z >= 6 galaxies from [C II] line emission. KOHANDEL M., PALLOTTINI A., FERRARA A., et al.
2019ApJ...881..124M 147       D     X         4 34 73 Resolved UV and [C II] structures of luminous galaxies within the epoch of reionization. MATTHEE J., SOBRAL D., BOOGAARD L.A., et al.
2019ApJ...883..142H 17       D               1 89 67 SILVERRUSH. VIII. Spectroscopic identifications of early large-scale structures with protoclusters over 200 Mpc at z ∼ 6-7: strong associations of dusty star-forming galaxies. HARIKANE Y., OUCHI M., ONO Y., et al.
2019ApJ...887..107F 47           X         1 20 93 First identification of 10 kpc [C II] 158 µm halos around star-forming galaxies at z = 5-7. FUJIMOTO S., OUCHI M., FERRARA A., et al.
2020MNRAS.492.1778M 44           X         1 3 ~ Resolved Lyman-α properties of a luminous Lyman-break galaxy in a large ionized bubble at z = 6.53. MATTHEE J., SOBRAL D., GRONKE M., et al.
2019PASJ...71...71H 406       D     X C       9 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.
2020ApJ...891..177Z 888       D     X C       20 8 ~ CHORUS. III. Photometric and spectroscopic properties of Lyα blobs at z = 4.9-7.0. ZHANG H., OUCHI M., ITOH R., et al.
2020MNRAS.494.1071G 105       D         F     2 54 62 The assembly of dusty galaxies at z >= 4: statistical properties. GRAZIANI L., SCHNEIDER R., GINOLFI M., et al.
2020MNRAS.494.3453T 218           X         5 6 ~ Modelling a bright z = 6 galaxy at the faint end of the AGN luminosity function. TREBITSCH M., VOLONTERI M. and DUBOIS Y.
2020MNRAS.495.1577I 90           X         2 8 27 Radiative equilibrium estimates of dust temperature and mass in high-redshift galaxies. INOUE A.K., HASHIMOTO T., CHIHARA H., et al.
2020ApJ...896...93H 19       D               1 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.498.3043M 132           X         3 12 12 The nature of CR7 revealed with MUSE: a young starburst powering extended Ly α emission at z = 6.6. MATTHEE J., PEZZULLI G., MACKENZIE R., et al.
2020A&A...641A..32H 44           X         1 19 ~ A Lyα nebula at z ∼ 3.3. HIBON P., TANG F. and THOMAS R.
2020MNRAS.499.5136C 48           X         1 14 65 Missing [C II] emission from early galaxies. CARNIANI S., FERRARA A., MAIOLINO R., et al.
2021MNRAS.500.3083C 360           X C       7 5 10 Constraints on the [C II] luminosity of a proto-globular cluster at z ∼ 6 obtained with ALMA. CALURA F., VANZELLA E., CARNIANI S., et al.
2021MNRAS.502.3210L 18       D               1 23 16 The IRX-β relation of high-redshift galaxies. LIANG L., FELDMANN R., HAYWARD C.C., et al.
2021ApJ...908L..30P 90           X         2 7 ~ RELICS-DP7: spectroscopic confirmation of a dichromatic Primeval Galaxy at z ∼ 7. PELLICCIA D., STRAIT V., LEMAUX B.C., et al.
2021ApJ...911...78O viz 108       D     X         3 181 17 SILVERRUSH X: machine learning-aided selection of 9318 LAEs at z = 2.2, 3.3, 4.9, 5.7, 6.6, and 7.0 from the HSC SSP and CHORUS survey data. ONO Y., ITOH R., SHIBUYA T., et al.
2022ApJ...926..230N 159       D     X         4 42 8 The Magellan M2FS Spectroscopic Survey of High-z Galaxies: Lyα Emitters at z ≃ 6.6 and the Evolution of Lyα Luminosity Function over z ≃ 5.7-6.6. NING Y., JIANG L., ZHENG Z.-Y., et al.
2022A&A...660A.137G viz 47           X         1 21 3 Tomography of the environment of the COSMOS/AzTEC-3 submillimeter galaxy at z ∼ 5.3 revealed by Lyα and MUSE observations. GUAITA L., ARAVENA M., GURUNG-LOPEZ S., et al.
2022A&A...663A.172M 112       D       C       5 20 1 The interstellar medium of high-redshift galaxies: Gathering clues from C III] and [C II] lines. MARKOV V., CARNIANI S., VALLINI L., et al.
2022MNRAS.517.5642E 19       D               1 31 29 The REBELS ALMA Survey: efficient Ly α transmission of UV-bright z ≃ 7 galaxies from large velocity offsets and broad line widths. ENDSLEY R., STARK D.P., BOUWENS R.J., et al.

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