About: Georgios Magdis

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Greek astrophysicist

Attributes	Values
rdf:type	Item
description	forskare (sv) 연구원 (ko) 研究者 (ja) изилдөөчү (ky) 研究者 (zh) ikertzaile greziarra (eu) onderzoeker uit Griekenland (nl) investigador grec (ca) investigador grego (gl) investigador grego (pt) investigador griegu (ast) ricercatore greco (it) Greek astrophysicist (en) astrofísico greco (es) astrophysicien grec (fr) réaltfhisiceoir Gréagach (ga) Έλληνας Αστροφυσικός (el)
rdfs:label	G Magdis (nl) Georgios Magdis (en) Georgios Magdis (es) Georgios Magdis (fr) Georgios Magdis (ga) Georgios Magdis (sq) Georgios Magdis (tr) Γεώργιος Μάγδης (el)
skos:prefLabel	G Magdis (nl) Georgios Magdis (en) Georgios Magdis (es) Georgios Magdis (fr) Georgios Magdis (ga) Georgios Magdis (sq) Georgios Magdis (tr) Γεώργιος Μάγδης (el)
name	G Magdis (nl) Georgios Magdis (en) Georgios Magdis (es) Georgios Magdis (fr) Georgios Magdis (ga) Georgios Magdis (sq) Georgios Magdis (tr) Γεώργιος Μάγδης (el)
Scopus author ID	wds:Q56421223-A36168E1-1890-4881-AE7A-BB02C1571A6E
Scopus author ID	14622946500
given name	wds:Q56421223-3C995842-5604-4515-94DF-F77071F652CF
given name	Georgios
instance of	wds:Q56421223-26EFFF71-EC0C-4837-8AF4-C73AD4D91AEE
instance of	Homo sapiens
AstroGen ID	wds:Q56421223-8A3EEE24-ABE1-47DA-A9F2-AB867D4E569F
AstroGen ID	46361
INSPIRE-HEP author ID	wds:Q56421223-5F3BEFA4-51EE-4B2D-8E41-3B508B7C73B5
INSPIRE-HEP author ID	G.Magdis.1
occupation	wds:Q56421223-00C6112C-CCC5-4392-B15D-9A95FA231484
employer	wds:Q56421223-23F2E4A3-D4D5-4F53-A5C5-C6B50F14CA32 wds:Q56421223-824E472E-A630-4433-B3E3-788045204BF8 wds:Q56421223-8925A7EA-0017-400D-B5E9-12204AC3C214 wds:Q56421223-94083583-4B69-4891-A13E-2222F940C803 wds:Q56421223-B94B046F-4174-4BEB-89B2-6C30BE607F1E wds:Q56421223-EF791C4C-D1CC-44F3-9A15-B150F5E73749
languages spoken, written or signed	wds:Q56421223-96449305-529D-4027-AD3F-73D96FD66343 wds:Q56421223-efac1049-494c-4a33-c0b3-e4db7e5bc601
place of birth	wds:Q56421223-70A83D4F-0B7E-423F-B51D-D17D94FEBD9A
sex or gender	wds:Q56421223-15B5452A-80CF-4CAF-A017-E00F1DEE3E40
country of citizenship	wds:Q56421223-83D0E4C1-FD33-4D2C-A1F0-021DC1E21C36
educated at	wds:Q56421223-2146C71B-FBCC-4372-B91C-C68A0E8896A2
official website	wds:Q56421223-7a92e699-40c4-2604-79fa-5b88263f6e50 wds:Q56421223-8DC87229-A7DB-4FF6-8F4C-23FD31F082A9
occupation	researcher
employer	University of Copenhagen University of Oxford University of Copenhagen Niels Bohr Institute Technical University of Denmark CEA Saclay
languages spoken, written or signed	Greek English
place of birth	Athens
sex or gender	male
country of citizenship	Groupement de recherche et d'études pour la civilisation européenne
educated at	University of Oxford
official website	http://www.georgiosmagdis.com/ https://curis.ku.dk/portal/en/persons/georgios-magdis(bb2c8ff6-621e-4570-ab1c-e007d2d15e40).html
ORCID iD	wds:Q56421223-D1C0EBD5-D05A-4397-99DD-0358D3D2021F
ORCID iD	https://orcid.org/0000-0002-4872-2294
ORCID iD	0000-0002-4872-2294
ResearcherID	wds:Q56421223-9EE00FF8-D8C3-4679-9981-CCAAED50BF76 wds:Q56421223-B0173CDC-F41D-4E2C-B537-20803D075B9D
ResearcherID	C-7295-2014 D-1276-2019
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q56421223
is author of	A mid-IR study of Hickson compact groups. II. Multiwavelength analysis of the complete GALEX-Spitzer sample The evolution of the dust and gas content in 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 Dissecting the cosmic infra-red background with Herschel/PEP The Herschel view of the dominant mode of galaxy growth from z = 4 to the present day The evolution of the dust temperatures of galaxies in the SFR–M∗ plane up to z ~ 2 GOODS-herschel: star formation, dust attenuation, and the FIR-radio correlation on the main sequence of star-forming galaxies up to z ~=4 The evolving interstellar medium of star-forming galaxies since z = 2 as probed by their infrared spectral energy distributions GOODS-herschel: gas-to-dust mass ratios and CO-to-H_2_ conversion factors in normal and starbursting galaxies at high-z Regularity underlying complexity: a redshift-independent description of the continuous variation of galaxy-scale molecular gas properties in the mass-star formation rate plane

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