|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| CANDELS EGS F160W J141910.9+524719.7 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST09:59:09 |
| 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 |
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 |
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. | ||
|
2024AJ....168..113C |
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. | ||
| 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...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...986..165T | 19 | D | 1 | 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. | ||
| 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. | |
| 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. |