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| XLS 17 , the SIMBAD biblio (4 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST16:37:06 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2014ApJ...788...74S | 16 | D | 1 | 44 | 121 | What is the physical origin of strong Lyα emission? II. Gas kinematics and distribution of Lyα emitters. | SHIBUYA T., OUCHI M., NAKAJIMA K., et al. | ||
|
2016ApJ...830...51S |
16 | D | 1 | 67525 | 168 | The FourStar galaxy evolution survey (ZFOURGE): ultraviolet to far-infrared catalogs, medium-bandwidth photometric redshifts with improved accuracy, stellar masses, and confirmation of quiescent galaxies to z ∼ 3.5. | STRAATMAN C.M.S., SPITLER L.R., QUADRI R.F., et al. | ||
| 2021MNRAS.505.1382M | 17 | D | 1 | 37 | 36 | The X-SHOOTER Lyman α survey at z = 2 (XLS-z2) I: what makes a galaxy a Lyman α emitter? | MATTHEE J., SOBRAL D., HAYES M., et al. | ||
| 2022MNRAS.510.4582N | 61 | D | X | 2 | 33 | 60 | The synchrony of production and escape: half the bright Lyα emitters at z ≃ 2 have Lyman continuum escape fractions ≃50. | NAIDU R.P., MATTHEE J., OESCH P.A., et al. |