180 citations · 3.8k across the 123 of their papers we have counts for
11 papers · 1 filter
Stellar populations and physical properties of starbursts in the Antennae galaxy from self-consistent modelling of MUSE spectra
M. L. P. Gunawardhana, J. Brinchmann, P. M. Weilbacher +6
We have modelled the stellar and nebular continua and emission-line intensity ratios of massive stellar populations in the Antennae galaxy using high resolution and self-consistent…
Nature and physical properties of ALMA selected galaxies using MUSE spectroscopy
Leindert A. Boogaard
Mapping the molecular gas content of the universe is key to our understanding of the build-up of galaxies over cosmic time. Spectral line scans in deep fields, such as the Hubble U…
The ALMA Spectroscopic Survey in the HUDF: Nature and physical properties of gas-mass selected galaxies using MUSE spectroscopy
Leindert A. Boogaard, Roberto Decarli, Jorge González-López +31
We discuss the nature and physical properties of gas-mass selected galaxies in the ALMA spectroscopic survey (ASPECS) of the Hubble Ultra Deep Field (HUDF). We capitalize on the de…
The ALMA Spectroscopic Survey in the HUDF: CO luminosity functions and the molecular gas content of galaxies through cosmic history
Roberto Decarli, Fabian Walter, Jorge Gónzalez-López +34
We use the results from the ALMA large program ASPECS, the spectroscopic survey in the Hubble Ultra Deep Field (HUDF), to constrain CO luminosity functions of galaxies and the resu…
The ALMA Spectroscopic Survey in the HUDF: CO emission lines and 3 mm continuum sources
Jorge González-López, Roberto Decarli, Ricardo Pavesi +29
The ALMA SPECtroscopic Survey in the {\it Hubble} Ultra Deep Field is an ALMA large program that obtained a frequency scan in the 3\,mm band to detect emission lines from the molec…
The ALMA Spectroscopic Survey in the HUDF: the molecular gas content of galaxies and tensions with IllustrisTNG and the Santa Cruz SAM
Gergö Popping, Annalisa Pillepich, Rachel S. Somerville +27
The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS) provides new constraints for galaxy formation models on the molecular gas properties of galaxies. We compare r…
The evolution of the cosmic molecular gas density
Fabian Walter, Chris Carilli, Roberto Decarli +38
One of the last missing pieces in the puzzle of galaxy formation and evolution through cosmic history is a detailed picture of the role of the cold gas supply in the star-formation…
The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Evolution of the molecular gas in CO-selected galaxies
Manuel Aravena, Roberto Decarli, Jorge Gónzalez-López +31
We analyze the interstellar medium properties of a sample of sixteen bright CO line emitting galaxies identified in the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (AS…
Resolved UV and [CII] structures of luminous galaxies within the epoch of reionisation
J. Matthee, D. Sobral, L. A. Boogaard +7
We present new deep ALMA and HST/WFC3 observations of MASOSA and VR7, two luminous Ly emitters (LAEs) at , for which the UV continuum level differ by a factor four. No IR…
Exploring HeII1640 emission line properties at
Themiya Nanayakkara, Jarle Brinchmann, Leindert Boogaard +10
Deep optical spectroscopic surveys of galaxies provide us a unique opportunity to investigate rest-frame ultra-violet (UV) emission line properties of galaxies at .…
The mean H EW and Lyman-continuum photon production efficiency for faint galaxies
Daniel Lam, Rychard J. Bouwens, Ivo Labbe +9
We present the first measurements of the Lyman-continuum photon production efficiency at -5 for galaxies fainter than 0.2 (19 mag). $ξ_{\textr…