CANDELS EGS F160W J142019.5+525819.9 , the SIMBAD biblio

CANDELS EGS F160W J142019.5+525819.9 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST05:16:49

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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
2012A&A...547A..51G 15       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.
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.
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.
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.
2023A&A...679A..12M 17       D               1 7 ~ Dust attenuation law in JWST galaxies at z ∼ 7-8. MARKOV V., GALLERANI S., PALLOTTINI A., et al.
2023ApJ...959...39H 104       D       C       4 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.526.1657T 104       D         F     5 25 ~ JWST/NIRSpec spectroscopy of z = 7-9 star-forming galaxies with CEERS: new insight into bright Lyα emitters in ionized bubbles. TANG M., STARK D.P., CHEN Z., 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.531.4974Z 403           X C F     7 6 ~ TRINITY IV: predictions for supermassive black holes at z ≳ 6. ZHANG H., BEHROOZI P., VOLONTERI M., et al.
2024ApJ...971...21H 18       D               1 64 ~ Characterizing the Average Interstellar Medium Conditions of Galaxies at z ∼ 5.6-9 with Ultraviolet and Optical Nebular Lines. HU W., PAPOVICH C., DICKINSON 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...980..138H 19       D               1 68 ~ JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z ∼ 7-14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe. HARIKANE Y., INOUE A.K., ELLIS R.S., 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...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...986..165T 140           X         3 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.
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...995...24K 93             C       1 18 ~ Challenging the Active Galactic Nucleus Scenario for JWST/NIRSpec Little Red Dot and Non-Little Red Dot Broad Hα Emitters in Light of Nondetection of NIRCam Photometric Variability and X-Ray. KOKUBO M. and HARIKANE Y.

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