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| [ESS2003] Q2346-BX405 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST19:24:02 |
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| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2006ApJ...645.1062F | 8 | 16 | 427 | SINFONI integral field spectroscopy of z ∼ 2 UV-selected galaxies: rotation curves and dynamical evolution. | FORSTER SCHREIBER N.M., GENZEL R., LEHNERT M.D., et al. | ||||
| 2006ApJ...646..107E | 1 | 116 | 456 | The stellar, gas, and dynamical masses of star-forming galaxies at z ∼ 2. | ERB D.K., STEIDEL C.C., SHAPLEY A.E., et al. | ||||
2006ApJ...647..128E 
|
16 | D | 115 | 362 | Hα observations of a large sample of galaxies at z ∼ 2: implications for star formation in high-redshift galaxies. | ERB D.K., STEIDEL C.C., SHAPLEY A.E., et al. | |||
| 2009ApJ...697.2057L | 19 | D | 1 | 43 | 347 | The kiloparsec-scale kinematics of high-redshift star-forming galaxies. | LAW D.R., STEIDEL C.C., ERB D.K., et al. | ||
|
2009ApJ...706.1364F
|
96 | D | F | 8 | 72 | 945 | The SINS survey: SINFONI integral field spectroscopy of z ∼ 2 star-forming galaxies. | FORSTER SCHREIBER N.M., GENZEL R., BOUCHE N., et al. | |
| 2010ApJ...722.1895E | 113 | X | 3 | 23 | 23 | Tadpole galaxies in the Hubble Ultra Deep Field. | ELMEGREEN B.G. and ELMEGREEN D.M. | ||
| 2011ARA&A..49..525S | 153 | C F | 2 | 42 | 129 | Physical properties of galaxies from z = 2-4. | SHAPLEY A.E. | ||
| 2015MNRAS.451.3001T | 16 | D | 1 | 37 | 17 | On the road to precision cosmology with high-redshift HII galaxies. | TERLEVICH R., TERLEVICH E., MELNICK J., et al. | ||
| 2016MNRAS.463.1144W | 16 | D | 1 | 131 | 10 | The H II galaxy Hubble diagram strongly favours Rh = ct over ΛCDM. | WEI J.-J., WU X.-F. and MELIA F. | ||
|
2021MNRAS.505.1441G
|
17 | D | 1 | 246 | 34 | Independent cosmological constraints from high-z H II galaxies: new results from VLT-KMOS data. | GONZALEZ-MORAN A.L., CHAVEZ R., TERLEVICH E., et al. |
