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| AzTEC J100025.56+021530.1 , the SIMBAD biblio (20 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST13:19:32 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2007ApJS..172..132B | 58 | 144 | COSBO: the MAMBO 1.2 millimeter imaging survey of the COSMOS field. | BERTOLDI F., CARILLI C., ARAVENA M., et al. | |||||
| 2010ApJ...708L..36A | 75 | F | 1 | 30 | 24 | Environment of MAMBO galaxies in the COSMOS field. | ARAVENA M., BERTOLDI F., CARILLI C., et al. | ||
|
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. | ||
| 2019ApJ...887...55C | 3766 | A | S X C | 91 | 8 | 47 | Physical characterization of an unlensed, dusty star-forming galaxy at z = 5.85. | CASEY C.M., ZAVALA J.A., ARAVENA M., et al. | |
| 2020ApJ...900...68C | 123 | X C | 2 | 12 | ~ | Far-infrared photometric redshifts: a new approach to a highly uncertain enterprise. | CASEY C.M. | ||
|
2020A&A...644A.144D |
85 | C | 1 | 9 | 28 | In pursuit of giants. I. The evolution of the dust-to-stellar mass ratio in distant dusty galaxies. | DONEVSKI D., LAPI A., MALEK K., et al. | ||
| 2021MNRAS.505.4838L | 170 | X C | 3 | 4 | 15 | ALMA Lensing Cluster Survey: a strongly lensed multiply imaged dusty system at z >= 6. | LAPORTE N., ZITRIN A., ELLIS R.S., et al. | ||
|
2021ApJ...923..215C |
980 | D | S X C | 22 | 13 | 33 | Mapping Obscuration to Reionization with ALMA (MORA): 2 mm efficiently selects the highest-redshift obscured galaxies. | CASEY C.M., ZAVALA J.A., MANNING S.M., et al. | |
| 2022ApJ...925...23M | 347 | X C | 7 | 4 | 26 | Characterization of Two 2 mm detected Optically Obscured Dusty Star-forming Galaxies. | MANNING S.M., CASEY C.M., ZAVALA J.A., et al. | ||
| 2022A&A...659A.154I | 383 | X C | 8 | 13 | 3 | NOEMA confirmation of an optically dark ALMA-AzTEC submillimetre galaxy at z = 5.24. A late-stage starburst prior to quenching. | IKARASHI S., IVISON R.J., COWLEY W.I., et al. | ||
|
2022A&A...667A...9P |
85 | X | 2 | 21 | 6 | Unveiling the warm and dense ISM in z > 6 quasar host galaxies via water vapor emission. | PENSABENE A., VAN DER WERF P., DECARLI R., et al. | ||
| 2023MNRAS.523.3119W | 148 | D | X | 4 | 27 | 1 | An empirical study of dust properties at the earliest epochs. | WITSTOK J., JONES G.C., MAIOLINO R., et al. | |
| 2021RNAAS...5...15Z | 84 | C | 1 | 3 | ~ | A Tentative Emission Line at z = 5.8 from a 3 mm Selected Galaxy. | ZAVALA J.A. | ||
| 2023ApJ...956...72M | 44 | X | 1 | 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. | ||
| 2024A&A...684A..56K | 45 | X | 1 | 18 | ~ | Probing the interstellar medium of the quasar BRI 0952-0115 An analysis of [C II], [C II], CO, OH, and H2O. | KADE K., KNUDSEN K.K., BEWKETU BELETE A., et al. | ||
| 2025ApJ...979..229M | 187 | X | 4 | 11 | ~ | SCUBADive. I. JWST+ALMA Analysis of 289 Submillimeter Galaxies in COSMOS-web. | McKINNEY J., CASEY C.M., LONG A.S., et al. | ||
| 2025ApJ...980...12S | 47 | X | 1 | 12 | ~ | A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at z = 4-6. | SUN F., WANG F., YANG J., et al. | ||
| 2025MNRAS.539.2409D | 47 | X | 1 | 3 | ~ | No evidence (yet) for increased star-formation efficiency at early times. | DONNAN C.T., DUNLOP J.S., McLURE R.J., et al. | ||
| 2025ApJ...991...37A | 93 | C | 1 | 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. | ||
| 2026ApJ...998L..36Z | 100 | C | 1 | 2 | ~ | ALMA and JWST Identification of Faint Dusty Star-forming Galaxies up to z ∼ 8 and Their Connection with Other Galaxy Populations. | ZAVALA J.A., FAISST A.L., ARAVENA M., et al. |