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| [BBC2005] 31.1 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST03:22:39 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2012MNRAS.427.1953C | 512 | D | S X C F | 11 | 32 | 71 | The low-mass end of the fundamental relation for gravitationally lensed star-forming galaxies at 1 < z < 6. | CHRISTENSEN L., RICHARD J., HJORTH J., et al. | |
| 2012MNRAS.427.1973C | 934 | D | S X C | 23 | 10 | 68 | Gravitationally lensed galaxies at 2 < z < 3.5: direct abundance measurements of Ly α emitters. | CHRISTENSEN L., LAURSEN P., RICHARD J., et al. | |
| 2014MNRAS.445.3200S | 483 | D | X C | 12 | 22 | 175 | Ultraviolet emission lines in young low-mass galaxies at z ≃ 2: physical properties and implications for studies at z > 7. | STARK D.P., RICHARD J., SIANA B., et al. | |
| 2018MNRAS.481.3520P | 297 | D | X F | 7 | 13 | 7 | Testing strong line metallicity diagnostics at z ∼ 2. | PATRICIO V., CHRISTENSEN L., RHODIN H., et al. | |
| 2020MNRAS.491.1427S | 392 | D | X | 10 | 21 | 117 | The MOSDEF survey: direct-method metallicities and ISM conditions at z 1.5-3.5. | SANDERS R.L., SHAPLEY A.E., REDDY N.A., et al. | |
| 2020ApJ...893....1B | 16 | D | 2 | 42 | 17 | A comparison of UV and optical metallicities in star-forming galaxies. | BYLER N., KEWLEY L.J., RIGBY J.R., et al. | ||
| 2020PASP..132c3001N | 181 | D | X | 5 | 11 | ~ | Estimating electron temperatures in ionized nebulae: the Direct Method and its limitations. | NICHOLLS D.C., KEWLEY L.J. and SUTHERLAND R.S. | |
| 2020ApJ...903..150J | 17 | D | 1 | 32 | 41 | The mass-metallicity relation at z ≃ 8: direct-method metallicity constraints and near-future prospects. | JONES T., SANDERS R., ROBERTS-BORSANI G., et al. | ||
| 2023MNRAS.520.4037M | 17 | D | 1 | 33 | 2 | Spectroscopy of CASSOWARY gravitationally lensed galaxies in SDSS: characterization of an extremely bright reionization-era analogue at z = 1.42. | MAINALI R., STARK D.P., JONES T., et al. |