ZFOURGE CDFS 21442 , the SIMBAD biblio

ZFOURGE CDFS 21442 , the SIMBAD biblio (31 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST07:05:06


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Title First 3 Authors
2010A&A...512A..12B viz 15       D               1 4352 228 The Great Observatories Origins Deep Survey. VLT/VIMOS spectroscopy in the GOODS-South field: part II. BALESTRA I., MAINIERI V., POPESSO P., et al.
2011ApJ...729...48B 15       D               2 135 15 Differential morphology between rest-frame optical and ultraviolet emission from 1.5 < z < 3 star-forming galaxies. BOND N.A., GAWISER E. and KOEKEMOER A.M.
2011ApJ...743..146C viz 15       D               1 4132 61 Active and passive galaxies at z ∼ 2: rest-frame optical morphologies with WFC3. CAMERON E., CAROLLO C.M., OESCH P.A., 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.
2015A&A...576A.116V 882       S   X C       20 3 50 Peering through the holes: the far-UV color of star-forming galaxies at z ∼ 3-4 and the escaping fraction of ionizing radiation. VANZELLA E., DE BARROS S., CASTELLANO M., et al.
2016A&A...585A..51D 3156       S   X C       76 6 155 An extreme [OIII] emitter at z = 3.2: a low metallicity Lyman continuum source. DE BARROS S., VANZELLA E., AMORIN R., et al.
2016A&A...587A.133G 16       D               1 91 20 Limits on the LyC signal from z ∼ 3 sources with secure redshift and HST coverage in the E-CDFS field. GUAITA L., PENTERICCI L., GRAZIAN A., et al.
2016ApJ...825...41V 1042       S   X C       22 2 158 Hubble imaging of the ionizing radiation from a star-forming galaxy at z=3.2 with fesc>50%. VANZELLA E., DE BARROS S., VASEI K., et al.
2016ApJ...826L..24S 686       S   X         15 3 133 Q1549-C25: a clean source of Lyman-continuum emission at z = 3.15. SHAPLEY A.E., STEIDEL C.C., STROM A.L., et al.
2016ApJ...830...51S viz 16       D               1 67524 168 The FourStar galaxy evolution survey (ZFOURGE): ultraviolet to far-infrared catalogs, medium-bandwidth photometric redshifts with improved accuracy, stellar masses, and confirmation of quiescent galaxies to z ∼ 3.5. STRAATMAN C.M.S., SPITLER L.R., QUADRI R.F., et al.
2017ApJ...847...12N 773           X         19 11 20 The HDUV survey: six Lyman continuum emitter candidates at z ∼ 2 revealed by HST UV imaging. NAIDU R.P., OESCH P.A., REDDY N., et al.
2018ApJ...853..191S 48 12 Hubble Space Telescope Wide Field Camera 3 observations of escaping Lyman Continuum radiation from galaxies and weak AGN at redshifts z ∼ 2.3-4.1. SMITH B.M., WINDHORST R.A., JANSEN R.A., et al.
2018MNRAS.475.5133R viz 16       D               1 11242 2 Testing the hierarchical assembly of massive galaxies using accurate merger rates out to z ∼ 1.5. RODRIGUES M., PUECH M., FLORES H., et al.
2018MNRAS.476L..15V 253     A     X         5 2 129 Direct Lyman continuum and Ly α escape observed at redshift 4. VANZELLA E., NONINO M., CUPANI G., et al.
2018MNRAS.478.4851I 60           X         1 10 197 Low-redshift Lyman continuum leaking galaxies with high [O III]/[O II] ratios. IZOTOV Y.I., WORSECK G., SCHAERER D., et al.
2018ApJ...869..141C 165             C F     3 4 2 ZFOURGE: extreme 5007 Å emission may be a common early-lifetime phase for star-forming galaxies at z > 2.5. COHN J.H., LEJA J., TRAN K.-V.H., et al.
2019MNRAS.486.2215K 70           X         1 3 84 Understanding the escape of LyC and Lyα photons from turbulent clouds. KIMM T., BLAIZOT J., GAREL T., et al.
2020ApJ...888..109J 854           X         20 11 34 HST imaging of the ionizing radiation from a star-forming galaxy at z = 3.794. JI Z., GIAVALISCO M., VANZELLA E., et al.
2020MNRAS.491..468I 46           X         1 12 46 Diverse properties of Ly α emission in low-redshift compact star-forming galaxies with extremely high [O III]/[O II] ratios. IZOTOV Y.I., SCHAERER D., WORSECK G., et al.
2020MNRAS.491.1093V 1396     A     X C F     31 9 80 Ionizing the intergalactic medium by star clusters: the first empirical evidence. VANZELLA E., CAMINHA G.B., CALURA F., et al.
2020MNRAS.492.4858H 43           X         1 5 ~ Simulating star clusters across cosmic time - II. Escape fraction of ionizing photons from molecular clouds. HE C.-C., RICOTTI M. and GEEN S.
2020MNRAS.493L..65B 173           X C       3 7 24 Lyman continuum escape fraction in Ly α emitters at z ≃ 3.1. BIAN F. and FAN X.
2020ApJ...897...41S viz 17       D               1 122 ~ The Lyman continuum escape fraction of galaxies and AGN in the GOODS fields. SMITH B.M., WINDHORST R.A., COHEN S.H., et al.
2021MNRAS.508.3697G 90             C       2 7 27 Lyman-α transmission properties of the intergalactic medium in the CoDaII simulation. GRONKE M., OCVIRK P., MASON C., et al.
2021MNRAS.508.4443M 87           X         2 16 14 Upper limits on the escape fraction of ionizing radiation from galaxies at 2 <= z < 6. MESTRIC U., RYAN-WEBER E.V., COOKE J., et al.
2021ApJ...923L..28Y 44           X         1 7 ~ CDFS-6664: a candidate of Lyman-continuum emission at z ∼ 3.8 detected by the Hubble Deep UV Legacy Survey. YUAN F.-T., ZHENG Z.-Y., LIN R., et al.
2022MNRAS.510.4582N 270           X C       5 33 60 The synchrony of production and escape: half the bright Lyα emitters at z ≃ 2 have Lyman continuum escape fractions ≃50. NAIDU R.P., MATTHEE J., OESCH P.A., et al.
2022ApJ...933...50W 18       D               2 37 ~ The Physical Properties of Star-forming Galaxies with Strong [O III] Lines at z = 3.25. WEN R., AN F., ZHENG X.Z., et al.
2022MNRAS.517.1098S 48           X         1 5 15 Strong C IV emission from star-forming galaxies: a case for high Lyman continuum photon escape. SAXENA A., CRYER E., ELLIS R.S., et al.
2022MNRAS.517.2972M 91               F     1 9 10 An extreme blue nugget, UV-bright starburst at z = 3.613 with 90 per cent of Lyman continuum photon escape. MARQUES-CHAVES R., SCHAERER D., ALVAREZ-MARQUEZ J., et al.
2023MNRAS.520.4037M 19       D               1 33 2 Spectroscopy of CASSOWARY gravitationally lensed galaxies in SDSS: characterization of an extremely bright reionization-era analogue at z = 1.42. MAINALI R., STARK D.P., JONES T., et al.

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