About: Rob Ivison

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

British astrophysicist

Attributes	Values
rdf:type	Item
description	United Kingdom karimba ŋun nyɛ doo (dag) astrophysicien britannique (fr) Brits onderzoeker (nl) British astrophysicist (en) astrofísico británico (es)
rdfs:label	Rob Ivison (ca) Rob Ivison (en) Rob Ivison (es) Rob Ivison (fr) Rob Ivison (nl) Rob Ivison (sl) Rob Ivison (ast)
skos:prefLabel	Rob Ivison (ca) Rob Ivison (en) Rob Ivison (es) Rob Ivison (fr) Rob Ivison (nl) Rob Ivison (sl) Rob Ivison (ast)
name	Rob Ivison (ca) Rob Ivison (en) Rob Ivison (es) Rob Ivison (fr) Rob Ivison (nl) Rob Ivison (sl) Rob Ivison (ast)
given name	wds:Q44376416-5489B389-3D71-489B-98BE-D170671939B5 wds:Q44376416-854ED7C1-3805-456F-A26E-8F48E328B217
given name	Rob Robert
image	wds:Q44376416-eae5a901-4713-f4c1-8958-6b8b553e1344
instance of	wds:Q44376416-1567FC58-303F-46BA-8F14-7B01A1AB6F9B
image
instance of	Homo sapiens
INSPIRE-HEP author ID	wds:Q44376416-0F4E9B0B-4490-4F5C-B7DC-432730DF425E
INSPIRE-HEP author ID	R.J.Ivison.1
skos:altLabel	R. J. Ivison (en) R.J. Ivison (en) Robert Ivison (en) Robert Ivison (es) Robert Ivison (fr) Robert Ivison (nl)
occupation	wds:Q44376416-447e5328-4820-7e6e-d5f2-60615326756d wds:Q44376416-667a56a9-45b1-ec72-e643-6bab39d31b3a
employer	wds:Q44376416-13779898-CD7B-429C-9C0C-1C1DB318C99C wds:Q44376416-155ECD68-87DD-44D8-8BF8-7DAD25535D43 wds:Q44376416-1e0db92a-40db-bcfd-2dea-657b3261deb3 wds:Q44376416-F6A7E40F-A6B8-47D0-BCAE-1DBA4BFB2B54
languages spoken, written or signed	wds:Q44376416-E7D12E74-311F-490F-83F6-87A28ABA48D6
sex or gender	wds:Q44376416-F14BE237-1744-450F-8FAD-70E2BD8F7D93
country of citizenship	wds:Q44376416-50F5F262-BCD8-46CF-98B7-BC45FA6369D4
Isidore scholar ID	wds:Q44376416-F58566DE-F1C2-4FF0-ACEB-F3527CF455DC
educated at	wds:Q44376416-C0EE8B61-A73E-4B4B-82FF-994A1EBFE0D3
family name	wds:Q44376416-7A1E1CDE-24FD-45B7-B5CC-A43760D90059
occupation	astrophysicist university teacher
employer	European Southern Observatory University of Edinburgh
languages spoken, written or signed	English
sex or gender	male
country of citizenship	United Kingdom
Isidore scholar ID	ivison_r_j
educated at	University of Central Lancashire
family name	Ivison
ORCID iD	wds:Q44376416-35877921-4ee3-88ed-964f-52328425d439
Dimensions author ID	wds:Q44376416-08A96607-12AA-4865-953E-AA5B89025AE2
ORCID iD	https://orcid.org/0000-0001-5118-1313
ORCID iD	0000-0001-5118-1313
Dimensions author ID	0605077727.45
is owl:sameAs of	Rob Ivison
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q44376416
is author of	Herschel imaging of 61 Vir: implications for the prevalence of debris in low-mass planetary systems Resolving debris discs in the far-infrared: Early highlights from the DEBRIS survey Detection of a noble gas molecular ion, 36ArH+, in the Crab Nebula TheHerschel-SPIRE instrument and its in-flight performance Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10¹¹ solar masses The nature of faint submillimetre-selected galaxies HerMES: deep galaxy number counts from a P(D) fluctuation analysis of SPIRE Science Demonstration Phase observations HerMES: COSMIC INFRARED BACKGROUND ANISOTROPIES AND THE CLUSTERING OF DUSTY STAR-FORMING GALAXIES HerMES: deep number counts at 250 μm, 350 μm and 500 μm in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background HerMES: current cosmic infrared background estimates can Be explained by known galaxies and their faint companions at z < 4 HerMES: SPIRE galaxy number counts at 250, 350, and 500 μm HerschelPACS and SPIRE imaging of CW Leonis SpitzerObservations of MAMBO Galaxies: Weeding Out Active Nuclei in Starbursting Protoellipticals Warm water vapour in the sooty outflow from a luminous carbon star Gone with the heat: a fundamental constraint on the imaging of dust and molecular gas in the early Universe The formation of cluster elliptical galaxies as revealed by extensive star formation. On the effect of the cosmic microwave background in high-redshift (sub-)millimeter observations Tracing the molecular gas in distant submillimetre galaxies via CO(1-0) imaging with the Expanded Very Large Array Submillimeter Galaxies atz∼ 2: Evidence for Major Mergers and Constraints on Lifetimes, IMF, and CO‐H2Conversion Factor A massive reservoir of low-excitation molecular gas at high redshift Rapid growth of black holes in massive star-forming galaxies A multiply imaged, submillimetre-selected ultraluminous infrared galaxy in a galaxy group atz∼ 2.5 SpitzerObservations of the SCUBA/VLA Sources in the Lockman Hole: Star Formation History of Infrared‐Luminous Galaxies Submillimetre observations of the Hubble Deep Field and Flanking Fields Herschel★-ATLAS/GAMA: dusty early-type galaxies and passive spirals The evolution of the dust temperatures of galaxies in the SFR–M∗ plane up to z ~ 2 The detection of dust in the central galaxies of distant cooling-flow clusters The Chandra deep protocluster survey: Ly{alpha} blobs are powered by heating, not cooling

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