CANDELS EGS F160W J141917.6+524949.0 , the SIMBAD biblio

CANDELS EGS F160W J141917.6+524949.0 , the SIMBAD biblio (29 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST03:02:39

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2014ApJS..214...24S viz 15       D               1 97940 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.
2015ApJ...803...34B viz 16       D               1 10313 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.
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.
2023ApJ...942L..17O 1833     A D     X C       42 4 20 A Candidate for the Least-massive Black Hole in the First 1.1 Billion Years of the Universe. ONOUE M., INAYOSHI K., DING X., et al.
2023ApJ...954L...4K 2916     A D S   X C       66 3 ~ Hidden Little Monsters: Spectroscopic Identification of Low-mass, Broad-line AGNs at z > 5 with CEERS. KOCEVSKI D.D., ONOUE M., INAYOSHI K., et al.
2023MNRAS.525.1353J 87           X         2 9 ~ EPOCHS VII: discovery of high-redshift (6.5 < z < 12) AGN candidates in JWST ERO and PEARLS data. JUODZBALIS I., CONSELICE C.J., SINGH M., et al.
2023ApJS..269...33N viz 17       D               1 187 ~ 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.
2023ApJ...959...39H 496       D     X C       11 14 ~ A JWST/NIRSpec First Census of Broad-line AGNs at z = 4-7: Detection of 10 Faint AGNs with MBH ∼ 106-108M⊙ and Their Host Galaxy Properties. HARIKANE Y., ZHANG Y., NAKAJIMA K., et al.
2023ApJ...959..100I 17       D               1 67 ~ JWST Identification of Extremely Low C/N Galaxies with [N/O] ≳ 0.5 at z ∼ 6-10 Evidencing the Early CNO-cycle Enrichment and a Connection with Globular Cluster Formation. ISOBE Y., OUCHI M., TOMINAGA N., et al.
2023MNRAS.526.3250S 87           X         2 5 ~ Are we surprised to find SMBHs with JWST at z ≥ 9? SCHNEIDER R., VALIANTE R., TRINCA A., et al.
2024ApJ...962..195B 18       D               1 158 ~ CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z > 2. BACKHAUS B.E., TRUMP J.R., PIRZKAL N., et al.
2024AJ....167..251L 108       D         F     9 20 ~ Radio Emission from High-redshift Active Galactic Nuclei in the JADES and CEERS Surveys. LATIF M.A., AFTAB A. and WHALEN D.J.
2024PASJ...76..219O viz 18       D               2 173 ~ Census for the rest-frame optical and UV morphologies of galaxies at z = 4-10: First phase of inside-out galaxy formation. ONO Y., HARIKANE Y., OUCHI M., et al.
2024MNRAS.531.4584S 18       D               1 22 ~ Diagnosing the massive-seed pathway to high-redshift black holes: statistics of the evolving black hole to host galaxy mass ratio. SCOGGINS M.T. and HAIMAN Z.
2024A&A...689A.128L 134           X C       2 5 ~ Size matters: are we witnessing super-Eddington accretion in high-redshift black holes from JWST? LUPI A., TRINCA A., VOLONTERI M., et al.
2024A&A...690A.182D 18       D               1 31 ~ Exploring a primordial solution for early black holes detected with JWST. DAYAL P.
2024ApJ...974L..26Y 18       D               3 17 ~ Stacking X-Ray Observations of “Little Red Dots”: Implications for Their Active Galactic Nucleus Properties. YUE M., EILERS A.-C., ANANNA T.T., et al.
2025ApJ...981...19L 19       D               1 23 ~ Tip of the Iceberg: Overmassive Black Holes at 4 < z < 7 Found by JWST Are Not Inconsistent with the Local ${{ \mathcal M }}_{\mathrm{BH}}-{{ \mathcal M }}_{\star }$ Relation. LI J., SILVERMAN J.D., SHEN Y., 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.
2025ApJ...983..165S 19       D               1 33 ~ Evolution of the M∗-MBH Relation from z ∼ 6 to the Present Epoch. SUN Y., RIEKE G.H., LYU J., et al.
2025ApJ...985...24C 19       D               1 22 ~ Unveiling the Cosmic Chemistry. II. “Direct” Te-based Metallicity of Galaxies at 3 < z < 10 with JWST/NIRSpec. CHAKRABORTY P., SARKAR A., SMITH R., et al.
2025ApJ...986..165T 578       D     X C       12 66 ~ Broad-line AGNs at 3.5 < z < 6: The Black Hole Mass Function and a Connection with Little Red Dots. TAYLOR A.J., FINKELSTEIN S.L., KOCEVSKI D.D., et al.
2025ApJ...986..177B 93             C       1 19 ~ Here There Be (Dusty) Monsters: High-redshift Active Galactic Nuclei Are Dustier than Their Hosts. BROOKS M., SIMONS R.C., TRUMP J.R., et al.
2025A&A...699A.336B 19       D               1 10 ~ CEERS: Possibly forging the first dust grains in the universe A population of galaxies with spectroscopically derived extremely low dust attenuation (GELDA) at 4.0 < z ≲ 11.4. BURGARELLA D., BUAT V., THEULE P., et al.
2025ApJ...991...74G 467           X C       9 5 ~ A Search for z = 5 Hα and Hβ + [O III] Dual-line Emitting Galaxies in the JWST CEERS Field: Implications for the Active Galactic Nucleus Abundance. GUO J., ONOUE M., INAYOSHI K., et al.
2025ApJ...991..217T 19       D               1 32 ~ JWST/NIRSpec Observations of High-ionization Emission Lines in Galaxies at High Redshift. TANG M., STARK D.P., PLAT A., et al.
2026Natur.649..574R 120       D         F     3 12 ~ Little red dots as young supermassive black holes in dense ionized cocoons. RUSAKOV V., WATSON D., NIKOPOULOS G.P., et al.
2026ApJ...999...70L 420       D     X C       8 20 ~ The Dichotomy in the Nuclear and Host-galaxy Properties of High-redshift Quasars. LI R., HO L.C. and CHEN C.-H.
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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