|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| CANDELS UDS F160W J021658.60-051444.9 , the SIMBAD biblio (26 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST04:54:55 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2013ApJS..206...10G |
15 | D | 1 | 34915 | 252 | CANDELS multiwavelength catalogs: source identification and photometry in the CANDELS UKIDSS ultra-deep survey field. | GALAMETZ A., GRAZIAN A., FONTANA A., et al. | ||
|
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. | ||
|
2016ApJ...830...51S |
16 | D | 1 | 67525 | 168 | The FourStar galaxy evolution survey (ZFOURGE): ultraviolet to far-infrared catalogs, medium-bandwidth photometric redshifts with improved accuracy, stellar masses, and confirmation of quiescent galaxies to z ∼ 3.5. | STRAATMAN C.M.S., SPITLER L.R., QUADRI R.F., et al. | ||
|
2020ApJ...897...44S |
16 | D | 1 | 123 | ~ | Selection of massive evolved galaxies at 3 <= z <= 4.5 in the CANDELS fields. | SHAHIDI A., MOBASHER B., NAYYERI H., et al. | ||
| 2024MNRAS.531.3187M | 242 | D | X F | 5 | 30 | ~ | The origin of large emission line widths in massive galaxies at redshifts z ∼ 3-4. | MARTINEZ-MARIN M., GLAZEBROOK K., NANAYAKKARA T., et al. | |
| 2025ApJ...980L..27I | 140 | X C | 2 | 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...984..121W | 2827 | A | X C | 60 | 4 | ~ | RUBIES: JWST/NIRSpec Confirmation of an Infrared-luminous, Broad-line Little Red Dot with an Ionized Outflow. | WANG B., DE GRAAFF A., DAVIES R.L., et al. | |
| 2025A&A...697A.189D | 47 | X | 1 | 3 | ~ | RUBIES: A complete census of the bright and red distant Universe with JWST/NIRSpec. | DE GRAAFF A., BRAMMER G., WEIBEL A., et al. | ||
| 2025ApJ...986..126K | 252 | D | X C | 5 | 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...989L...7T | 47 | X | 1 | 6 | ~ | CAPERS-LRD-z9: A Gas-enshrouded Little Red Dot Hosting a Broad-line Active Galactic Nucleus at z = 9.288. | TAYLOR A.J., KOKOREV V., KOCEVSKI D.D., et al. | ||
| 2025ApJ...990L..61C | 93 | C | 1 | 2 | ~ | An Upper Limit of 106M⊙ in Dust from ALMA Observations in 60 Little Red Dots. | CASEY C.M., AKINS H.B., FINKELSTEIN S.L., et al. | ||
| 2025A&A...701A.168D | 47 | X | 1 | 7 | ~ | A remarkable ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a little red dot at z = 3.5. | DE GRAAFF A., RIX H.-W., NAIDU R.P., et al. | ||
| 2025ApJ...991L..10S | 1372 | D | X C | 29 | 3 | ~ | A Confirmed Deficit of Hot and Cold Dust Emission in the Most Luminous Little Red Dots. | SETTON D.J., GREENE J.E., SPILKER J.S., et al. | |
| 2025ApJ...991...37A | 187 | X C | 3 | 8 | ~ | COSMOS-Web: The Overabundance and Physical Nature of “Little Red Dots”-Implications for Early Galaxy and SMBH Assembly. | AKINS H.B., CASEY C.M., LAMBRIDES E., et al. | ||
| 2025ApJ...994...86R | 233 | X C | 4 | 22 | ~ | Deciphering the Nature of Virgil: An Obscured Active Galactic Nucleus Lurking within an Apparently Normal Lyα Emitter during Cosmic Reionization. | RINALDI P., PEREZ-GONZALEZ P.G., RIEKE G.H., et al. | ||
| 2025ApJ...994..113L | 93 | X | 2 | 6 | ~ | The Balmer Break and Optical Continuum of Little Red Dots from Super-Eddington Accretion. | LIU H., JIANG Y.-F., QUATAERT E., et al. | ||
| 2025A&A...703A..36L | 1148 | A | X C | 24 | 11 | ~ | A big red dot at cosmic noon. | LOIACONO F., GILLI R., MIGNOLI M., et al. | |
| 2025ApJ...994L..42C | 588 | A | X C | 12 | 2 | ~ | Dust Budget Crisis in Little Red Dots. | CHEN K., LI Z., INAYOSHI K., et al. | |
| 2025ApJ...995..118S | 233 | X C | 4 | 3 | ~ | Little Red Dots at an Inflection Point: Ubiquitous V-shaped Turnover Consistently Occurs at the Balmer Limit. | SETTON D.J., GREENE J.E., DE GRAAFF A., et al. | ||
| 2025A&A...704A.313D | 187 | X C | 3 | 9 | ~ | Active galactic nuclei-heated dust revealed in “little red dots”. | DELVECCHIO I., DADDI E., MAGNELLI B., et al. | ||
| 2026ApJ...996..129G | 1020 | D | S X C | 19 | 3 | ~ | What You See Is What You Get: Empirically Measured Bolometric Luminosities of Little Red Dots. | GREENE J.E., SETTON D.J., FURTAK L.J., et al. | |
| 2026ApJ...997...48B | 600 | X C | 11 | 7 | ~ | A Comprehensive Photometric Selection of “Little Red Dots” in MIRI Fields: An Infrared-Bright Little Red Dot at z = 3.1386 with Warm Dust Emission. | BARRO G., PEREZ-GONZALEZ P.G., KOCEVSKI D.D., et al. | ||
| 2026ApJ...997..218A | 520 | D | X | 11 | 4 | ~ | Tentative Detection of Neutral Gas in a Little Red Dot at z = 4.46. | AKINS H.B., CASEY C.M., CHISHOLM J., et al. | |
| 2026ApJ..1000L..18H | 100 | C | 1 | 6 | ~ | The X-Ray Dot: Exotic Dust or a Late-stage Little Red Dot? | HVIDING R.E., DE GRAAFF A., LIU H., et al. | ||
| 2026ApJ..1000...59M | 150 | X C | 2 | 10 | ~ | Counting Little Red Dots at z < 4 with Ground-based Surveys and Spectroscopic Follow-up. | MA Y., GREENE J.E., SETTON D.J., et al. |