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| AzTEC J095953.83+021847.9 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST22:47:57 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
2011MNRAS.415.3831A 
|
15 | D | 1 | 196 | 119 | AzTEC millimetre survey of the COSMOS field – III. Source catalogue over 0.72 deg2 and plausible boosting by large-scale structure. | ARETXAGA I., WILSON G.W., AGUILAR E., et al. | ||
| 2013MNRAS.431..662J | 15 | D | 1 | 53 | 17 | X-ray detections of submillimetre galaxies: active galactic nuclei versus starburst contribution. | JOHNSON S.P., WILSON G.W., WANG Q.D., et al. | ||
|
2013MNRAS.436.1919C
|
15 | D | 3 | 161 | 145 | Characterization of Scuba-2 450µm and 850µm selected galaxies in the COSMOS field. | CASEY C.M., CHEN C.-C., COWIE L.L., et al. | ||
|
2017A&A...608A..15B
|
95 | D | C | 1 | 148 | 62 | An ALMA survey of submillimeter galaxies in the COSMOS field: Multiwavelength counterparts and redshift distribution. | BRISBIN D., MIETTINEN O., ARAVENA M., et al. | |
|
2018ApJ...864...56J
|
87 | C | 1 | 14 | 98 | "Super-deblended" dust emission in galaxies. II. Far-IR to (Sub)millimeter photometry and high-redshift galaxy candidates in the full COSMOS field. | JIN S., DADDI E., LIU D., et al. | ||
| 2021A&A...646A.174A | 17 | D | 1 | 35 | ~ | Environments of a sample of AzTEC submillimetre galaxies in the COSMOS field. | ALVAREZ CRESPO N., SMOLIC V., FINOGUENOV A., et al. | ||
| 2023ApJ...956...72M | 4031 | A | X C | 92 | 7 | ~ | A Near-infrared-faint, Far-infrared-luminous Dusty Galaxy at z ∼ 5 in COSMOS-Web. | McKINNEY J., MANNING S.M., COOPER O.R., et al. | |
| 2025ApJ...979..229M | 93 | X | 2 | 11 | ~ | SCUBADive. I. JWST+ALMA Analysis of 289 Submillimeter Galaxies in COSMOS-web. | McKINNEY J., CASEY C.M., LONG A.S., et al. | ||
| 2025MNRAS.539.2409D | 93 | X | 2 | 3 | ~ | No evidence (yet) for increased star-formation efficiency at early times. | DONNAN C.T., DUNLOP J.S., McLURE R.J., et al. |
