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| [RSK2010] A 521 1 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST08:12:14 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2018MNRAS.477...18P | 17 | D | 1 | 17 | 33 | Kinematics, turbulence, and star formation of z ∼ 1 strongly lensed galaxies seen with MUSE. | PATRICIO V., RICHARD J., CARTON D., et al. | ||
| 2019MNRAS.489..224P | 41 | X | 1 | 13 | ~ | Resolved scaling relations and metallicity gradients on sub-kiloparsec scales at z ≃ 1. | PATRICIO V., RICHARD J., CARTON D., et al. | ||
| 2021ApJ...909...12G | 17 | D | 1 | 29 | 28 | Systematic difference between ionized and molecular gas velocity dispersions in z ∼ 1-2 disks and local analogs. | GIRARD M., FISHER D.B., BOLATTO A.D., et al. | ||
|
2022A&A...657A..25N |
4001 | A | D | S X C | 93 | 10 | 2 | Radial profiles of lensed z ∼ 1 galaxies on sub-kiloparsec scales. | NAGY D., DESSAUGES-ZAVADSKY M., RICHARD J., et al. |
| 2022MNRAS.516.2420M | 2624 | T K A | X C | 60 | 3 | 6 |
Multiply lensed star forming clumps in the A521-sys1 galaxy at redshift 1. |
MESSA M., DESSAUGES-ZAVADSKY M., RICHARD J., et al. | |
| 2023MNRAS.519.6222D | 3378 | K A | X C F | 76 | 5 | 2 | Molecular gas cloud properties at z ≃ 1 revealed by the superb angular resolution achieved with ALMA and gravitational lensing. | DESSAUGES-ZAVADSKY M., RICHARD J., COMBES F., et al. | |
| 2023MNRAS.520.2180C | 87 | C | 1 | 49 | 28 | Star formation at the smallest scales: a JWST study of the clump populations in SMACS0723. | CLAEYSSENS A., ADAMO A., RICHARD J., et al. | ||
| 2024MNRAS.529.2162M | 224 | X C F | 3 | 14 | ~ | Properties of the brightest young stellar clumps in extremely lensed galaxies at redshifts 4 to 5. | MESSA M., DESSAUGES-ZAVADSKY M., ADAMO A., et al. | ||
| 2025MNRAS.536.3090K | 187 | C F | 4 | 3 | ~ | Clumps as multiscale structures in cosmic noon galaxies. | KALITA B.S., SUZUKI T.L., KASHINO D., et al. |