Filter your results
- 2
- 1
- 3
- 2
- 1
- 1
- 2
- 3
- 3
- 2
- 2
- 2
- 2
- 2
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 3
- 3
- 2
- 2
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
|
|
sorted by
|
|
Larger sizes of massive quiescent early-type galaxies in clusters than in the field at 0.8 < z < 1.5Monthly Notices of the Royal Astronomical Society, 2014, 441 (1), pp.203-223. ⟨10.1093/mnras/stu496⟩
Journal articles
hal-02366114v1
|
||
|
THE NEXT GENERATION VIRGO CLUSTER SURVEY. XV. THE PHOTOMETRIC REDSHIFT ESTIMATION FOR BACKGROUND SOURCESThe Astrophysical Journal, 2014, 797 (2), ⟨10.1088/0004-637X/797/2/102⟩
Journal articles
hal-01441980v1
|
||
|
Euclid preparation. III. Galaxy cluster detection in the wide photometric survey, performance and algorithm selectionAstronomy and Astrophysics - A&A, 2019, 627, pp.A23. ⟨10.1051/0004-6361/201935088⟩
Journal articles
cea-02166503v1
|