CANDELS EGS F160W J141955.9+525721.7 , the SIMBAD biblio

CANDELS EGS F160W J141955.9+525721.7 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST02:56:44


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Title First 3 Authors
2017ApJS..229...32S viz 16       D               1 37883 113 CANDELS multi-wavelength catalogs: source identification and photometry in the CANDELS Extended Groth Strip. STEFANON M., YAN H., MOBASHER B., et al.
2022ApJ...939L..31H 45           X         1 8 22 Has JWST Already Falsified Dark-matter-driven Galaxy Formation? HASLBAUER M., KROUPA P., ZONOOZI A.H., et al.
2023Natur.616..266L 24       D               1 18 142 A population of red candidate massive galaxies ∼600 Myr after the Big Bang. LABBE I., VAN DOKKUM P., NELSON E., et al.
2023ApJ...955L..12B 104       D     X         3 13 ~ Sizes and Mass Profiles of Candidate Massive Galaxies Discovered by JWST at 7 < z < 9: Evidence for Very Early Formation of the Central ∼100 pc of Present-day Ellipticals. BAGGEN J.F.W., VAN DOKKUM P., LABBE I., et al.
2024MNRAS.528.7052C 18       D               1 96 ~ JWST spectroscopy of z ∼ 5-8 UV-selected galaxies: new constraints on the evolution of the Ly α escape fraction in the reionization era. CHEN Z., STARK D.P., MASON C., et al.
2024MNRAS.530.2935D 18       D               1 36 ~ ΛCDM not dead yet: massive high-z Balmer break galaxies are less common than previously reported. DESPREZ G., MARTIS N.S., ASADA Y., et al.
2024ApJ...969L..13W 824       D     X C       18 7 ~ RUBIES: Evolved Stellar Populations with Extended Formation Histories at z ∼ 7-8 in Candidate Massive Galaxies Identified with JWST/NIRSpec. WANG B., LEJA J., DE GRAAFF A., et al.
2024ApJ...970...63L 18       D               3 13 ~ Age of Massive Galaxies at Redshift 8. LOPEZ-CORREDOIRA M., MELIA F., WEI J.-J., et al.
2024AJ....168..113C viz 18       D               1 123 ~ Evidence for a Shallow Evolution in the Volume Densities of Massive Galaxies at z = 4-8 from CEERS. CHWOROWSKY K., FINKELSTEIN S.L., BOYLAN-KOLCHIN M., et al.
2024ApJ...977L..13B 376       D     X         9 4 ~ The Small Sizes and High Implied Densities of “Little Red Dots” with Balmer Breaks Could Explain Their Broad Emission Lines without an Active Galactic Nucleus. BAGGEN J.F.W., VAN DOKKUM P., BRAMMER G., et al.
2025ApJ...978...89H 187           X C       3 18 ~ EPOCHS. IV. SED Modeling Assumptions and Their Impact on the Stellar Mass Function at 6.5 ≤ z ≤ 13.5 Using PEARLS and Public JWST Observations. HARVEY T., CONSELICE C.J., ADAMS N.J., et al.
2025ApJ...980L..27I 47           X         1 7 ~ Extremely Dense Gas around Little Red Dots and High-redshift Active Galactic Nuclei: A Nonstellar Origin of the Balmer Break and Absorption Features. INAYOSHI K. and MAIOLINO R.
2025ApJ...980...36L 47           X         1 10 ~ Little Red Dots: Rapidly Growing Black Holes Reddened by Extended Dusty Flows. LI Z., INAYOSHI K., CHEN K., et al.
2025ApJ...982...23J 47           X         1 14 ~ On the Significance of Rare Objects at High Redshift: The Impact of Cosmic Variance. JESPERSEN C.K., STEINHARDT C.L., SOMERVILLE R.S., et al.
2025ApJ...983L..26T 19       D               1 25 ~ Lack of Rest-frame Ultraviolet Variability in Little Red Dots Based on HST and JWST Observations. TEE W.L., FAN X., WANG F., et al.
2025MNRAS.538.3210B 187             C F     2 8 ~ Accelerated by dark matter: a high-redshift pathway to efficient galaxy-scale star formation. BOYLAN-KOLCHIN M.
2025ApJ...986..126K 19       D               1 32 ~ The Rise of Faint, Red Active Galactic Nuclei at z > 4: A Sample of Little Red Dots in the JWST Extragalactic Legacy Fields. KOCEVSKI D.D., FINKELSTEIN S.L., BARRO G., et al.
2025ApJ...991..217T 3937       D S   X C       83 32 ~ JWST/NIRSpec Observations of High-ionization Emission Lines in Galaxies at High Redshift. TANG M., STARK D.P., PLAT A., et al.
2026ApJ...999...30C 50           X         1 8 ~ A z ≃ 0.4 Galaxy Reflecting the High-redshift Little Red Dots: An Extended Starburst with an Overmassive Black Hole. CHEN X., ICHIKAWA K., AKIYAMA M., et al.
2026A&A...707A..75T 100             C       1 9 ~ The warm outer layer of a little red dot as the source of [Fe II] and collisional Balmer lines with scattering wings. TORRALBA A., MATTHEE J., PEZZULLI G., et al.

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