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| [SSR2007] G1 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST00:14:38 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2007ApJ...654L..33S | 559 | X C | 14 | 7 | 82 | A very bright, highly magnified Lyman break galaxy at z = 3.07. | SMAIL I., SWINBANK A.M., RICHARD J., et al. | ||
| 2007MNRAS.379..308D | 779 | X C | 20 | 4 | 22 | Separation of the visible and dark matter in the Einstein ring LBG J213512.73-010143. | DYE S., SMAIL I., SWINBANK A.M., et al. | ||
| 2007ApJ...665..936C | 261 | X C | 6 | 11 | 81 | A detailed study of gas and star formation in a highly magnified Lyman Break Galaxy at z = 3.07. | COPPIN K.E.K., SWINBANK A.M., NERI R., et al. | ||
| 2008Natur.455..775S | 23 | 3 | 141 | The formation and assembly of a typical star-forming galaxy at redshift z ∼ 3. | STARK D.P., SWINBANK A.M., ELLIS R.E., et al. | ||||
| 2009ApJ...695.1537I | 353 | D | X C | 9 | 53 | 125 | Luminous infrared galaxies with the submillimeter array. II. Comparing the CO (3-2) sizes and luminosities of local and high-redshift luminous infrared galaxies. | IONO D., WILSON C.D., YUN M.S., et al. | |
| 2009ApJ...698.1273S | 81 | X | 2 | 7 | 88 | Detection of far-infrared and polycyclic aromatic hydrocarbon emission from the cosmic eye: probing the dust and star formation of Lyman break galaxies. | SIANA B., SMAIL I., SWINBANK A.M., et al. | ||
| 2010MNRAS.402.1467Q | 153 | X | 4 | 11 | 53 | A study of interstellar gas and stars in the gravitationally lensed galaxy `the cosmic eye' from rest-frame ultraviolet spectroscopy. | QUIDER A.M., SHAPLEY A.E., PETTINI M., et al. | ||
| 2010Natur.464..733S | 11 | 13 | 304 | Intense star formation within resolved compact regions in a galaxy at z = 2.3. | SWINBANK A.M., SMAIL I., LONGMORE S., et al. | ||||
| 2011Msngr.144...39R | 11 | 2 | Report on the workshop 'ALMA community days: Towards early science'. | RANDALL S. and TESTI L. |