MUSE-WIDE 721510776 , the SIMBAD biblio

MUSE-WIDE 721510776 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST21:44:00


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Title First 3 Authors
2006AJ....132..926C viz 15       D               2664 396 Galaxies in the Hubble Ultra Deep Field. I. Detection, multiband photometry, photometric redshifts, and morphology. COE D., BENITEZ N., SANCHEZ S.F., et al.
2006AJ....132.1729B viz 15       D               761 684 The Hubble Ultra Deep Field. BECKWITH S.V.W., STIAVELLI M., KOEKEMOER A.M., et al.
2015AJ....150...31R viz 16       D               1 9968 140 UVUDF: ultraviolet through near-infrared catalog and photometric redshifts of galaxies in the Hubble Ultra Deep Field. RAFELSKI M., TEPLITZ H.I., GARDNER J.P., et al.
2017A&A...608A...2I viz 16       D               1 1584 136 The MUSE Hubble Ultra Deep Field Survey. II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies. INAMI H., BACON R., BRINCHMANN J., et al.
2017A&A...608A...8L viz 16       D               1 186 164 The MUSE Hubble Ultra Deep Field Survey. VIII. Extended Lyman-α haloes around high-z star-forming galaxies. LECLERCQ F., BACON R., WISOTZKI L., et al.
2020ApJ...901...41S 305       D     X C       7 15 ~ Lyα radiative transfer: modeling spectrum and surface brightness profiles of Lyα-emitting galaxies at z = 3-6. SONG H., SEON K.-I. and HWANG H.S.
2021A&A...654A..80S viz 17       D               1 2058 14 Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at 1.5 < z < 6.4. SCHMIDT K.B., KERUTT J., WISOTZKI L., et al.
2022A&A...659A.183K viz 17       D               1 1923 13 Equivalent widths of Lyman α emitters in MUSE-Wide and MUSE-Deep. KERUTT J., WISOTZKI L., VERHAMME A., et al.
2022ApJS..259....3S 255           X C       5 13 ~ Lyα Radiative Transfer: A Stokes Vector Approach to Lyα Polarization. SEON K.-I., SONG H. and CHANG S.-J.
2025ApJ...988..103Y 112       D         F     3 9 ~ Lyα Radiative Transfer Modeling for 163 MUSE Lyα-emitting Galaxies at z = 3-6. YU S., SONG H. and SEON K.-I.

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