CANDELS EGS F160W J142034.9+525802.2 , the SIMBAD biblio

CANDELS EGS F160W J142034.9+525802.2 , the SIMBAD biblio (15 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST10:12:06


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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.
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 322       D     X C       7 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.
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.
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 93             C       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.
2025ApJ...986..177B 19       D               3 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.

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