About: Manuel Aravena

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An Entity of Type : wikibase:Item, within Data Space : wikidata.demo.openlinksw.com associated with source document(s)

researcher

Attributes	Values
rdf:type	Item
description	forskare (sv) researcher (en) 연구원 (ko) 研究者 (ja) araştırmacı (tr) wetenschapper (nl) дослідник (uk) वैज्ञानिक (hi) изилдөөчү (ky) 研究者 (zh) հետազոտող (hy)
rdfs:label	Manuel Aravena (en) Manuel Aravena (es) Manuel Aravena (fr) Manuel Aravena (nl) Manuel Aravena (ast)
skos:prefLabel	Manuel Aravena (en) Manuel Aravena (es) Manuel Aravena (fr) Manuel Aravena (nl) Manuel Aravena (ast)
name	Manuel Aravena (en) Manuel Aravena (es) Manuel Aravena (fr) Manuel Aravena (nl) Manuel Aravena (ast)
given name	wds:Q56900372-AA4AAE6D-0C42-4E10-AF67-EB0BE9551D6E
given name	Manuel
instance of	wds:Q56900372-5909A156-F97C-477A-B909-F9B14BFB4A8C
instance of	Homo sapiens
skos:altLabel	M. Aravena (en)
occupation	wds:Q56900372-0736F42E-AEFF-4130-9308-7C88FD5A5244
employer	wds:Q56900372-481ED7B1-6F27-4BB2-8351-01A4C51C1C33 wds:Q56900372-B6B408CD-5DB6-4C41-92F9-04E5B3750042 wds:Q56900372-EEAA6FE7-5050-43C6-8E08-C11F8F247F41
languages spoken, written or signed	wds:Q56900372-42aac848-4802-bc4c-8277-37e6e4ca78e7 wds:Q56900372-D798F7B7-704F-409E-8053-902AC16B958B
sex or gender	wds:Q56900372-6784BA85-F08D-4547-A6A1-B322A72499CD
VIAF ID	wds:Q56900372-2015e645-235e-471a-9a42-49e6bef9d38b
GND ID	wds:Q56900372-f66f7619-cd7c-4048-bace-a83ca618675b
educated at	wds:Q56900372-7BFFA2DE-B2AD-45DF-B803-68762FF469B9
family name	wds:Q56900372-C1284E5D-7ECB-43C1-999F-E36214267F52
official website	wds:Q56900372-3C152845-DEFB-4B57-A464-709B5C0AB076
VIAF ID	http://viaf.org/viaf/86009595
GND ID	https://d-nb.info/gnd/137832648
occupation	researcher
employer	European Southern Observatory National Radio Astronomy Observatory Diego Portales University
languages spoken, written or signed	Spanish English
sex or gender	male
VIAF ID	86009595
GND ID	137832648
educated at	University of Bonn
family name	Aravena
official website	http://www.astro.udp.cl/~maravena/
ORCID iD	wds:Q56900372-25681B7D-DDD8-4DE0-B1F4-D2A68F657275
Dimensions author ID	wds:Q56900372-8747FC31-FEC9-4CC6-BCA5-786BA5B6FEF9
ORCID iD	https://orcid.org/0000-0002-6290-3198
ORCID iD	0000-0002-6290-3198
Dimensions author ID	011041333453.58
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q56900372
is author of	The multiple merger assembly of a hyperluminous obscured quasar at redshift 4.6 Cold molecular gas in massive, star-forming disk galaxies at z = 1.5 Imaging the molecular gas in a submillimeter galaxy at z = 4.05: cold mode accretion or a Major merger? Deep observations of CO line emission from star-forming galaxies in a cluster candidate atz=1.5 ALLSMOG: an APEX Low-redshift Legacy Survey for MOlecular Gas – I. Molecular gas scaling relations, and the effect of the CO/H2 conversion factor Spatially Resolved [C ii] Emission in SPT0346-52: A Hyper-starburst Galaxy Merger at z ∼ 5.7 COSBO: The MAMBO 1.2 Millimeter Imaging Survey of the COSMOS Field CO excitation of normal star-forming galaxies out to z = 1.5 as regulated by the properties of their interstellar medium CO(1–0) line imaging of massive star-forming disc galaxies at z=1.5–2.2 The redshift distribution of dusty star-forming galaxies from the SPT survey Stellar masses and star formation rates of lensed, dusty, star-forming galaxies from the SPT survey Extragalactic millimeter-wave point-source catalog, number counts and statistics from 771 deg^2^ of the SPT-SZ survey Imaging atomic and highly excited molecular gas in a z = 6.42 quasar host galaxy: copious fuel for an eddington-limited starburst at the end of cosmic reionization TheSpitzerSurvey of Stellar Structure in Galaxies Quest for COSMOS submillimeter galaxy counterparts using CARMA and VLA: identifying three high-redshift starburst galaxies (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies The ALMA spectroscopic survey in the Hubble Ultra Deep Field: molecular gas reservoirs in high-redshift galaxies ALMA redshifts of millimeter-selected galaxies from the SPT survey: the redshift distribution of dusty star-forming galaxies The redshift and nature of AzTEC/COSMOS 1: a starburst galaxy at z = 4.6 Physical properties ofz> 4 submillimeter galaxies in the COSMOS field Environment of MAMBO galaxies in the COSMOS field A molecular line scan in the Hubble Deep Field North Millimeter imaging of submillimeter galaxies in the COSMOS field: redshift distribution Grand design and flocculent spirals in the Spitzer survey of stellar structure in galaxies (S^4^G) [C II] line emission in massive star-forming galaxies at z = 4.7 The strikingly uniform, highly turbulent interstellar medium of the most luminous galaxy in the universe VALES. II. The physical conditions of interstellar gas in normal star-forming galaxies up to z = 0.2 revealed by ALMA ALMA imaging and gravitational lens models of South Pole telescope - Selected dusty, star-forming galaxies at high redshifts An ALMA survey of submillimeter galaxies in the COSMOS field: Multiwavelength counterparts and redshift distribution The ALMA spectroscopic survey in the Hubble Ultra Deep Field: search for [CII] line and dust emission in 6 < z < 8 galaxies A molecular line scan in the Hubble Deep Field North: constraints on the CO luminosity function and the cosmic H_2_Density The ALMA Frontier Fields Survey. I. 1.1 mm continuum detections in Abell 2744, MACS J0416.1-2403 and MACS J1149.5+2223 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 The ALMA spectroscopic survey in the Hubble Ultra Deep Field: continuum number counts, resolved 1.2 mm extragalactic background, and properties of the faintest dusty star-forming galaxies 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 (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies. II. The spatial extent of the radio-emitting regions

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