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{{Short description|English-American physicist}}
{{Orphan|date=August 2017}}
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'''Clement Laurence Pryke''' (born 1968 in [[Wallasey]], [[Cheshire]], UK) is an English-American physicist, focusing in astrophysics and cosmology, particularly on the cosmic microwave background.<ref>{{cite arXiv|author=Pryke, C.|year=2012|title=The Quest for Gravity Wave B-modes|class=astro-ph.IM |eprint=1209.2768}}</ref><ref>{{cite web|url=https://cesta.umn.edu/team/clem-pryke|title=Clem Pryke &#124; Center for Excellence in Sensing Technologies & Analytics }}</ref>

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'''Clement Laurence Pryke''' (born 1968 in [[Wallasey]], [[Cheshire]], UK) is an English-American physicist, focusing in astrophysics and cosmology, particularly on the cosmic microwave background.<ref>{{cite web|url=https://cesta.umn.edu/team/clem-pryke|title=Clem Pryke &#124; Center for Excellence in Sensing Technologies & Analytics }}</ref>


==Education and career==
==Education and career==
Pryke worked from 1988 to 1989 as a research assistant at Thorn EMI Central Research Labs in the UK. He graduated in physics from the [[University of Leeds]] in 1992 with a B.Sc. and in 1996 with a Ph.D. His Ph.D. thesis ''Instrumentation development and experimental design for a next generation detector of the highest energy cosmic rays'' was supervised by [[Alan Andrew Watson]]. At the [[Enrico Fermi Institute]] of the University of Chicago, Pryke was from 1996 to 1999 a McCormick Fellow, from 1999 to 2000 a research scientist, and from 2001 to 2002 a senior research associate.<ref name=CV>{{cite web|title=Curriculum Vita and Publication List for Clement Pryke|website=University of Minnesota|url=http://spud.spa.umn.edu/~pryke/cv.pdf}}</ref> From 2002 to 2010 he was an assistant professor in the department of astronomy and astrophysics of the University of Chicago.<ref name=CV/><ref>{{cite web|url=https://lambda.gsfc.nasa.gov/product/suborbit/PYTHON/astro.uchicago.edu/people/clement-pryke.shtml.html|title=The Department of Astronomy & Astrophysics - Profile: Clement Pryke | website=astro.uchicago.edu}}</ref> In the department of physics and astronomy of the [[University of Minnesota]], he was from 2010 to 2018 an associate professor and is since 2018 a full professor.<ref name=UMinnesota>{{cite web|url=https://cse.umn.edu/physics/clement-pryke|title=Clement Pryke|website=School of Physics and Astronomy, University of Minnesota }}</ref><ref>{{cite web|url=https://cse.umn.edu/physics/news/pryke-leads-research-effort-improves-constraints-physics-big-bang|title=Pryke leads research effort that improves constraints on Physics of Big Bang |website=School of Physics and Astronomy, University of Minnesota}}</ref>
Pryke worked from 1988 to 1989 as a research assistant at Thorn EMI Central Research Labs in the UK.<ref name=CV/> He graduated in physics from the [[University of Leeds]] in 1992 with a B.Sc. and in 1996 with a Ph.D.<ref name=UMinnesota/> His Ph.D. thesis ''Instrumentation development and experimental design for a next generation detector of the highest energy cosmic rays''<ref>{{cite web|title=''Instrumentation development and experimental design for a next generation detector of the highest energy cosmic rays'' by Clement Pryke|website=University of Leeds|url=https://leeds.primo.exlibrisgroup.com/discovery/fulldisplay?docid=alma991017175999705181&context=L&vid=44LEE_INST:VU1&lang=en&search_scope=My_Inst_CI_not_ebsco&adaptor=Local%20Search%20Engine&tab=AlmostEverything&query=any,contains,Pryke,AND&query=any,contains,clement,AND&mode=advanced&offset=0}}</ref> was supervised by [[Alan Andrew Watson]]. At the [[Enrico Fermi Institute]] of the University of Chicago, Pryke was from 1996 to 1999 a McCormick Fellow, from 1999 to 2000 a research scientist, and from 2001 to 2002 a senior research associate.<ref name=CV>{{cite web|title=Curriculum Vita and Publication List for Clement Pryke|website=University of Minnesota|url=http://spud.spa.umn.edu/~pryke/cv.pdf}}</ref> From 2002 to 2010 he was an assistant professor in the department of astronomy and astrophysics of the University of Chicago.<ref name=CV/><ref>{{cite web|url=https://lambda.gsfc.nasa.gov/product/suborbit/PYTHON/astro.uchicago.edu/people/clement-pryke.shtml.html|title=The Department of Astronomy & Astrophysics - Profile: Clement Pryke | website=astro.uchicago.edu}}</ref> In the department of physics and astronomy of the [[University of Minnesota]], he was from 2010 to 2018 an associate professor and is since 2018 a full professor.<ref name=UMinnesota>{{cite web|url=https://cse.umn.edu/physics/clement-pryke|title=Clement Pryke|website=School of Physics and Astronomy, University of Minnesota }}</ref><ref>{{cite web|url=https://cse.umn.edu/physics/news/pryke-leads-research-effort-improves-constraints-physics-big-bang|title=Pryke leads research effort that improves constraints on Physics of Big Bang |website=School of Physics and Astronomy, University of Minnesota}}</ref>


Pryke was elected in 2016 a Fellow of the [[American Physical Society]].<ref>{{cite web|title=APS Fellow Archive|website=American Physical Society|url=https://www.aps.org/programs/honors/fellowships/archive-all.cfm?initial=&year=2016&unit_id=&institution=University+of+Minnesota}} (search on year=2016 and institution=University of Minnesota)</ref> He was involved with the [[Degree Angular Scale Interferometer]] (DASI), and [[QUaD]] microwave background polarization experiments, and is currently co-PI of the [[BICEP and Keck Array]] collaboration.<ref name=UMinnesota/>
Pryke was elected in 2016 a [[Fellow of the American Physical Society]], "for groundbreaking measurement and data analyses of the polarization of cosmic microwave background radiation, and for using the data to provide strong constraints on the composition and initial conditions of the early universe".<ref>{{cite web|title=APS Fellow Archive|website=American Physical Society|url=https://www.aps.org/programs/honors/fellowships/archive-all.cfm?initial=&year=2016&unit_id=&institution=University+of+Minnesota}} (search on year=2016 and institution=University of Minnesota)</ref> He was involved with the [[Degree Angular Scale Interferometer]] (DASI),<ref>{{cite journal|author=Kovac, J. M.|author2=Leitch, E. M.|author3=Pryke, C.|author4=Carlstrom, J. E.|author5=Halverson, N. W.|author6=Holzapfel, W. L.|year=2002|title=Detection of polarization in the cosmic microwave background using DASI|journal=Nature|volume=420|issue=6917|pages=772–787|doi=10.1038/nature01269|pmid=12490941 |arxiv=astro-ph/0209478 |bibcode=2002Natur.420..772K |s2cid=4359884 }}</ref> and [[QUaD]] microwave background polarization experiments, and is currently co-PI of the [[BICEP and Keck Array]] collaboration.<ref name=UMinnesota/><ref>{{cite journal|author=Pryke, C.|title=Searching for the imprint of cosmic inflation|journal=Nature Astronomy|volume=4|page=1204|year=2020|issue=12 |doi=10.1038/s41550-020-01260-5|bibcode=2020NatAs...4.1204P |s2cid=230587954 }}</ref>


==References==
==References==

Latest revision as of 07:45, 28 August 2022

Clement Laurence Pryke (born 1968 in Wallasey, Cheshire, UK) is an English-American physicist, focusing in astrophysics and cosmology, particularly on the cosmic microwave background.[1][2]

Education and career

[edit]

Pryke worked from 1988 to 1989 as a research assistant at Thorn EMI Central Research Labs in the UK.[3] He graduated in physics from the University of Leeds in 1992 with a B.Sc. and in 1996 with a Ph.D.[4] His Ph.D. thesis Instrumentation development and experimental design for a next generation detector of the highest energy cosmic rays[5] was supervised by Alan Andrew Watson. At the Enrico Fermi Institute of the University of Chicago, Pryke was from 1996 to 1999 a McCormick Fellow, from 1999 to 2000 a research scientist, and from 2001 to 2002 a senior research associate.[3] From 2002 to 2010 he was an assistant professor in the department of astronomy and astrophysics of the University of Chicago.[3][6] In the department of physics and astronomy of the University of Minnesota, he was from 2010 to 2018 an associate professor and is since 2018 a full professor.[4][7]

Pryke was elected in 2016 a Fellow of the American Physical Society, "for groundbreaking measurement and data analyses of the polarization of cosmic microwave background radiation, and for using the data to provide strong constraints on the composition and initial conditions of the early universe".[8] He was involved with the Degree Angular Scale Interferometer (DASI),[9] and QUaD microwave background polarization experiments, and is currently co-PI of the BICEP and Keck Array collaboration.[4][10]

References

[edit]
  1. ^ Pryke, C. (2012). "The Quest for Gravity Wave B-modes". arXiv:1209.2768 [astro-ph.IM].
  2. ^ "Clem Pryke | Center for Excellence in Sensing Technologies & Analytics".
  3. ^ a b c "Curriculum Vita and Publication List for Clement Pryke" (PDF). University of Minnesota.
  4. ^ a b c "Clement Pryke". School of Physics and Astronomy, University of Minnesota.
  5. ^ "Instrumentation development and experimental design for a next generation detector of the highest energy cosmic rays by Clement Pryke". University of Leeds.
  6. ^ "The Department of Astronomy & Astrophysics - Profile: Clement Pryke". astro.uchicago.edu.
  7. ^ "Pryke leads research effort that improves constraints on Physics of Big Bang". School of Physics and Astronomy, University of Minnesota.
  8. ^ "APS Fellow Archive". American Physical Society. (search on year=2016 and institution=University of Minnesota)
  9. ^ Kovac, J. M.; Leitch, E. M.; Pryke, C.; Carlstrom, J. E.; Halverson, N. W.; Holzapfel, W. L. (2002). "Detection of polarization in the cosmic microwave background using DASI". Nature. 420 (6917): 772–787. arXiv:astro-ph/0209478. Bibcode:2002Natur.420..772K. doi:10.1038/nature01269. PMID 12490941. S2CID 4359884.
  10. ^ Pryke, C. (2020). "Searching for the imprint of cosmic inflation". Nature Astronomy. 4 (12): 1204. Bibcode:2020NatAs...4.1204P. doi:10.1038/s41550-020-01260-5. S2CID 230587954.


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