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Manuel Aravena

Identifiers

  • name variant Manuel Aravena 0.60 · backfill

Papers (25)

  1. A Deep Study of the Spiral Galaxy W2246f astro-ph.GA · 2026 · author #5
  2. The ALPINE-CRISTAL-JWST Survey: Gas-phase abundance gradients of main sequence star-forming galaxies and their kinematics at $4 < z < 6$ astro-ph.GA · 2026 · author #22
  3. The ALPINE-CRISTAL-JWST Survey: The Fast Metal Enrichment of Massive Galaxies at z~5 astro-ph.GA · 2025 · author #13
  4. Source structure and molecular gas properties from high-resolution CO imaging of SPT-selected dusty star-forming galaxies astro-ph.GA · 2019 · author #5
  5. The CO Luminosity Density at High-z (COLDz) Survey: A Sensitive, Large Area Blind Search for Low-J CO Emission from Cold Gas in the Early Universe with the Karl G. Jansky Very Large Array astro-ph.GA · 2018 · author #14
  6. ALMA resolves the molecular gas in a young low-metallicity starburst galaxy at z=1.7 astro-ph.GA · 2017 · author #7
  7. An ALMA survey of submillimeter galaxies in the COSMOS field: Multiwavelength counterparts and redshift distribution astro-ph.GA · 2017 · author #3
  8. JVLA 1.5GHz continuum observation of CLASH clusters I: radio properties of the BCGs astro-ph.GA · 2017 · author #9
  9. An ALMA survey of submillimetre galaxies in the COSMOS field: Physical properties derived from energy balance spectral energy distribution modelling astro-ph.GA · 2017 · author #4
  10. On the Kennicutt-Schmidt scaling law of submillimetre galaxies astro-ph.GA · 2017 · author #4
  11. An ALMA survey of submillimetre galaxies in the COSMOS field: The extent of the radio-emitting region revealed by 3 GHz imaging with the Very Large Array astro-ph.GA · 2017 · author #5
  12. (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies IV. Physical properties derived from spectral energy distributions astro-ph.GA · 2016 · author #5
  13. ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Molecular gas reservoirs in high-redshift galaxies astro-ph.GA · 2016 · author #3
  14. ALMA spectroscopic survey in the Hubble Ultra Deep Field: CO luminosity functions and the evolution of the cosmic density of molecular gas astro-ph.GA · 2016 · author #3
  15. ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Survey Description astro-ph.GA · 2016 · author #3
  16. ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-selected z=2-10 galaxies as a function of UV-continuum Slope and Stellar Mass astro-ph.GA · 2016 · author #2
  17. ALMA Imaging and Gravitational Lens Models of South Pole Telescope-Selected Dusty, Star-Forming Galaxies at High Redshifts astro-ph.GA · 2016 · author #3
  18. Globular Cluster Populations: Results Including S$^4$G Late-Type Galaxies astro-ph.GA · 2015 · author #3
  19. (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies - II. The spatial extent of the radio-emitting regions astro-ph.GA · 2015 · author #7
  20. (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies - I. Multiwavelength identifications and redshift distribution astro-ph.GA · 2015 · author #4
  21. Globular Cluster Populations: First Results from S$^4$G Early-Type Galaxies astro-ph.GA · 2014 · author #2
  22. The Spitzer Survey of Stellar Structure in Galaxies (S^4G) astro-ph.CO · 2010 · author #38
  23. Cold molecular gas in massive disk galaxies at z=1.5 astro-ph.CO · 2010 · author #1
  24. Environment of MAMBO galaxies in the COSMOS field astro-ph.CO · 2009 · author #1
  25. Properties of the molecular gas in a starbursting QSO at z=1.83 in the COSMOS field astro-ph · 2008 · author #1

Mentions

  • 1411.4615 #2 · backfill · confidence 0.70 Manuel Aravena
  • 2605.29014 #5 · arxiv_oai · confidence 0.70 Manuel Aravena
  • 2510.16106 #13 · arxiv_oai · confidence 0.70 Manuel Aravena
  • 1010.1592 #38 · backfill · confidence 0.70 Manuel Aravena
  • 1005.4965 #1 · backfill · confidence 0.70 Manuel Aravena
  • 0911.4297 #1 · backfill · confidence 0.70 Manuel Aravena
  • 0809.2337 #1 · backfill · confidence 0.70 Manuel Aravena

Frequent Coauthors