Leiden University Scholarly Publications

Your Search

Enabled Filters

  • (-) = Boogaard, L.A.
  • (-) = Wisotzki, L.

Refine Results

Resource Type

Availability

Creation Date

Show more

Faculty

Collection

Author

Show more

Language

Search results

  • RSS Feed
(1 - 20 of 23)

Pages

Bipolar outflows out to 10 kpc for massive galaxies at redshift z ≈ 1
The MUSE eXtremely deep field: first panoramic view of an Mg II emitting intragroup medium
Deciphering stellar metallicities in the early Universe
Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at 1.5 < z < 6.4
The MUSE-Wide survey
The MUSE Extremely Deep Field
The ALMA spectroscopic survey in the Hubble Ultra Deep Field: constraining the molecular content at log(M*/M) 9.5 with CO stacking of MUSE-detected z >1.5 galaxies
The MUSE Hubble Ultra Deep Field Survey. XV. The mean rest-UV spectra of Ly emitters at z > 3
The nature of CR7 revealed with MUSE: a young starburst powering extended Ly emission at z = 6.6
Elevated ionizing photon production efficiency in faint high-equivalent-width Lyman-alpha emitters
The ALMA Spectroscopic Survey in the HUDF: Nature and Physical Properties of Gas-mass Selected Galaxies Using MUSE Spectroscopy
The ALMA Spectroscopic Survey in the HUDF: CO Luminosity Functions and the Molecular Gas Content of Galaxies through Cosmic History
The MUSE-Wide Survey: survey description and first data release
The MUSE-Wide Survey: A determination of the Lyman α emitter luminosity function at 3 < z < 6
Ionised gas structure of 100 kpc in an over-dense region of the galaxy group COSMOS-Gr30 at z 0.7
The MUSE Hubble Ultra Deep Field Survey. XI. Constraining the low-mass end of the stellar mass - star formation rate relation at z < 1
Properties and redshift evolution of star-forming galaxies with high [O III]/[O II] ratios with MUSE at 0.28 < z < 0.85
MUSE Spectroscopic Identifications of Ultra-faint Emission Line Galaxies with MUV~-15
The MUSE Hubble Ultra Deep Field Survey. II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies
The MUSE Hubble Ultra Deep Field Survey. IV. Global properties of C III] emitters

Pages