Long-range dependency - Revision history

109.150.112.210: /* Further reading */ include Brockwell (2006)

2014-11-08T18:15:15Z

Further reading: include Brockwell (2006)

← Older revision		Revision as of 20:15, 8 November 2014
Line 1:		Line 1:
	~~{{other uses\|Clover (disambiguation)}}~~		If you ɑгe а bookie and oԝn an Apple iPad, yoս will be thrilled to know that there aгe any number of apps that сan help you take care of thе bookie աork ѡithout difficulty ԝhile on аppropriate. Wɦile you probaƅly don't want to rely on these apps to work full time over yoսr business, tҺey will save youг day іn case үou are away from theiг ѡork. Thеre aгe lots օf options for wherе to keep a bachelorette event and աhat tߋ dο. Really аre millions mаny other types of bonuses tҺɑt turn out to be a very gooԁ deal. Υоu can bet till Tuгn wіth yоur cards. Takе a lοok аt the 6 apps ʏoս can't do withoսt.<br><br>
	~~'''Clover''' would have been~~ an ~~experiment~~ to ~~measure the [[Polarization (waves)\|polarization]]~~ of ~~the [[Cosmic Microwave Background]]~~. ~~It was approved for funding in late 2004~~, ~~with the aim of having the full telescope operational by 2009~~. ~~The project was jointly run by [[Cardiff University]], [[Oxford University]], the [[Cavendish Astrophysics Group]]~~ and ~~the [[University~~ of ~~Manchester]]~~.~~<ref name="cardiff_webpage">{{cite web \| url=http://www~~.~~astro~~.~~cf.ac.uk/groups/instrumentation/projects/clover/ \| title=Clover Project page at Cardiff University \| accessdate=2007-07-31}}</ref>~~<~~ref name="oxford"~~>~~{{cite web \| url=http://www-astro.physics.ox.ac.uk/research/expcosmology/groupclover.html \| title = Clover Project page at Oxford \| accessdate=2007-07-31}}~~<~~/ref~~>

	~~The Clover Project was meant to consist of two independent telescopes~~, ~~one operating at 95~~ [~~[Hertz\|GHz~~]~~] with~~ the ~~other operating at both 150 and 225 [[Hertz\|GHz]]~~. ~~Both telescopes were~~ to ~~be sited near the [[Cosmic Background Imager\|CBI]] site~~ in ~~the [[Atacama\|Atacama Desert~~, ~~Chile]]. The two telescope [[Receiver (radio)\|receivers]] would have been large format [[focal plane array (astronomy)\|focal plane array]]s~~ of ~~either 100 or 200 [[bolometer\|bolometric detectors]]~~.<~~ref name="oxford" /~~>		While it holds true that үօu can read on and on aЬout ցreat moves and great winning strategies fօr thе different casino games, nothing beats experience еxactly ԝhat you learn from actual grinding. 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Јust find a site tɦat offers these free games ƴou cаn sit and play аll day if ƴou like. In fact, there's no download required and you don't eѵen end up Ьeing sign սp oг sign іn. Oг even betteг if you'гe preparing a escape tօ a casino ɑnd fix want to get in the groove. Вut since we're refering to free slots Cleopatra ɦere, we don't have to worry aЬоut Ьeing ripped ߋff because the ߋverall game is offered free аt ѕeveral sites cyberspace. Іt's а surperb ѡay to pass ѕome free time. Уоu'll fіnd that lots of the online casinos now havе access to a non-download version of vehicles аnd paid games.<br><br>25 for eаch bet within that gambling component. Sօ then start ԝith $50. 00 wɦich forms tҺе gambling component, thеn next stage is 5 percent of thіs, so now hɑving $0. 00, so now you enter а Casino game աith tеn percent of tҺis amߋunt, soon add up to $5.<br><br>Online casinos ԝill ǥenerally be lookіng to draw іn new players Ƅy providing attractive join bonuses. 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	~~The aim of the experiment was~~ to ~~measure the [[B~~-~~mode]] [[Polarization (waves)\|polarization]] of~~ the [~~[Cosmic Microwave Background~~]~~] between [[multipole]]s of 20 and 1000 down to a sensitivity limited by~~ the ~~foreground contamination due~~ to ~~[[gravitational lens\|lensing]]~~. ~~This would have allowed~~ the ~~detection~~ of ~~primordial [[gravitational waves]] in~~ the ~~universe so~~ long ~~as the ratio~~ of ~~scalar perturbations (caused by density fluctuations in the early universe)~~ to ~~the tensor perturbations caused~~ by ~~gravitational waves was greater than <math>r = 0~~.01<~~/math~~>.<~~ref name="oxford" /~~>

	~~It was hoped that the telescope would have spent around 2 years observing~~ a ~~total of around 1~~,~~000 [[degree~~ (~~angle~~)~~\|degree]]s~~ of ~~sky, made up of several patches~~ of ~~sky where polarized foregrounds ([[synchrotron]] and thermal dust emission) are at a minimum~~.<~~ref name="oxford" /~~>

	~~Clover was canceled in March 2009~~ as ~~[[Science and Technology Facilities Council\|STFC]] were unable to provide~~ the ~~requested additional funds~~ of 2.~~55 million pounds to finish~~ the ~~project~~.<~~ref name="IoP"~~>~~{{cite web \| url=http://physicsworld.com/cws/article/news/38547 \| title = It’s all over for Clover \| accessdate=2009-04-08}}~~<~~/ref~~>

	~~== Further reading ==~~
	~~=== Journal articles ===~~
	~~<!-- Ordered by year published -->~~
	* {{cite journal \| last=North \| first=C. ~~\| coauthors=et al~~. ~~\| url=http://www-astro~~.~~physics~~.ox.ac.~~uk/~cen/Papers/STT2007_Paper.pdf \| title=Clover - Measuring~~ the ~~CMB B~~-~~mode Polarisation \| journal=To appear in Proceedings~~ of ~~the 18th International Symposium on Space Terahertz Technology, Caltech, March 21–23, 2007 \| year=2007}}~~
	* {{cite journal \| last=Taylor \| first=A. \| coauthors=Clover collaboration \| title=CLOVER - A B-mode polarization instrument \| journal=New Astronomy Reviews \| volume=50 \| issue=11-12 \| year=2006 \| pages=993–998 \| doi=10.1016/j.newar.2006.09.026 \| arxiv=astro-ph/0610716 \|bibcode = 2006NewAR..50..~~993T }}~~
	* {{cite journal \| last=Audley \| first=M. ~~\| coauthors=et al~~. ~~\| title=TES imaging array technology for CLOVER \| journal=SPIE Orlando \| date=May 24–31~~, ~~2006 \| arxiv=astro-ph/0607067 \|bibcode = 2006SPIE~~.~~6275E~~..~~69A \|doi = 10~~.~~1117/12.670792 }}~~
	* {{cite journal \| last=Audley \| first=M. \| coauthors=et al. \| year=2006 \| pages=127 \| title=Prototype finline-coupled TES bolometers for ~~CLOVER \| journal=To appear in the Proceedings~~ of the ~~17th International Symposium on Space Terahertz Technology~~, ~~Paris~~, ~~May 10–12~~, ~~2006 \| bibcode=2006stt..conf..127A \| arxiv=astro-ph/0608285 }}~~
	* {{cite journal \| last=Taylor \| first=A. \| coauthors=et al. ~~\| title=CLOVER - A new instrument for measuring~~ the ~~B-mode polarization of the CMB \| journal=Proceedings of XXXIXth Rencontres de Moriond~~, ~~Editions Frontiers \| year=2004 \| arxiv=astro-ph/0407148 \|bibcode = 2004astro~~.ph..~~7148T }}~~

	~~== References ==~~
	~~{{Reflist\|1}}~~

	~~{{CMB experiments}}~~

	~~{{coord missing\|Chile}}~~

	~~[[Category:Cosmic microwave background experiments]]~~

en>Monkbot: Fix CS1 deprecated date parameter errors

2014-01-25T11:29:46Z

Fix CS1 deprecated date parameter errors

← Older revision		Revision as of 13:29, 25 January 2014
Line 1:		Line 1:
	~~Let me~~ ~~healthy food~~ [http://~~Www~~.~~Healthychefcreations~~.~~com~~/ ~~delivery~~] ~~first begin by introducing myself~~. My name ~~is Boyd Butts although it is not~~ the ~~name on my beginning certification~~. ~~One~~ of the ~~very best issues~~ in the ~~world for me is~~ to ~~do aerobics~~ and ~~now~~ [http://~~www.Nutrition411~~.com/~~patient-education-materials~~/~~grocery~~-~~shopping~~-~~and-food-preparation~~/~~item/889~~-~~diet~~-~~plans~~-~~with~~-~~meal-delivery/ I'm attempting] to healthy food delivery earn cash with it~~. ~~South Dakota is exactly where me and my husband live~~. ~~Hiring has been my [~~http://~~Www~~.~~Dailymail~~.Co.uk/~~femail~~/~~article-1305288~~/~~Diets~~-~~door~~-Do-~~latest~~-~~home~~-~~delivery~~-~~meal~~-~~packages~~-~~cut~~-~~mustard~~.~~html occupation]~~ for ~~some time but I've currently applied for another~~ 1~~.<br><br>my web page;~~ [~~http~~:~~//Mrk.im/fooddeliveryservices36486 http://Mrk.im/fooddeliveryservices36486~~]		{{other uses\|Clover (disambiguation)}}
			'''Clover''' would have been an experiment to measure the [[Polarization (waves)\|polarization]] of the [[Cosmic Microwave Background]]. It was approved for funding in late 2004, with the aim of having the full telescope operational by 2009. The project was jointly run by [[Cardiff University]], [[Oxford University]], the [[Cavendish Astrophysics Group]] and the [[University of Manchester]].<ref name="cardiff_webpage">{{cite web \| url=http://www.astro.cf.ac.uk/groups/instrumentation/projects/clover/ \| title=Clover Project page at Cardiff University \| accessdate=2007-07-31}}</ref><ref name="oxford">{{cite web \| url=http://www-astro.physics.ox.ac.uk/research/expcosmology/groupclover.html \| title = Clover Project page at Oxford \| accessdate=2007-07-31}}</ref>

			The Clover Project was meant to consist of two independent telescopes, one operating at 95 [[Hertz\|GHz]] with the other operating at both 150 and 225 [[Hertz\|GHz]]. Both telescopes were to be sited near the [[Cosmic Background Imager\|CBI]] site in the [[Atacama\|Atacama Desert, Chile]]. The two telescope [[Receiver (radio)\|receivers]] would have been large format [[focal plane array (astronomy)\|focal plane array]]s of either 100 or 200 [[bolometer\|bolometric detectors]].<ref name="oxford" />

			The aim of the experiment was to measure the [[B-mode]] [[Polarization (waves)\|polarization]] of the [[Cosmic Microwave Background]] between [[multipole]]s of 20 and 1000 down to a sensitivity limited by the foreground contamination due to [[gravitational lens\|lensing]]. This would have allowed the detection of primordial [[gravitational waves]] in the universe so long as the ratio of scalar perturbations (caused by density fluctuations in the early universe) to the tensor perturbations caused by gravitational waves was greater than <math>r = 0.01</math>.<ref name="oxford" />

			It was hoped that the telescope would have spent around 2 years observing a total of around 1,000 [[degree (angle)\|degree]]s of sky, made up of several patches of sky where polarized foregrounds ([[synchrotron]] and thermal dust emission) are at a minimum.<ref name="oxford" />

			Clover was canceled in March 2009 as [[Science and Technology Facilities Council\|STFC]] were unable to provide the requested additional funds of 2.55 million pounds to finish the project.<ref name="IoP">{{cite web \| url=http://physicsworld.com/cws/article/news/38547 \| title = It’s all over for Clover \| accessdate=2009-04-08}}</ref>

			== Further reading ==
			=== Journal articles ===
			<!-- Ordered by year published -->
			* {{cite journal \| last=North \| first=C. \| coauthors=et al. \| url=http://www-astro.physics.ox.ac.uk/~cen/Papers/STT2007_Paper.pdf \| title=Clover - Measuring the CMB B-mode Polarisation \| journal=To appear in Proceedings of the 18th International Symposium on Space Terahertz Technology, Caltech, March 21–23, 2007 \| year=2007}}
			* {{cite journal \| last=Taylor \| first=A. \| coauthors=Clover collaboration \| title=CLOVER - A B-mode polarization instrument \| journal=New Astronomy Reviews \| volume=50 \| issue=11-12 \| year=2006 \| pages=993–998 \| doi=10.1016/j.newar.2006.09.026 \| arxiv=astro-ph/0610716 \|bibcode = 2006NewAR..50..993T }}
			* {{cite journal \| last=Audley \| first=M. \| coauthors=et al. \| title=TES imaging array technology for CLOVER \| journal=SPIE Orlando \| date=May 24–31, 2006 \| arxiv=astro-ph/0607067 \|bibcode = 2006SPIE.6275E..69A \|doi = 10.1117/12.670792 }}
			* {{cite journal \| last=Audley \| first=M. \| coauthors=et al. \| year=2006 \| pages=127 \| title=Prototype finline-coupled TES bolometers for CLOVER \| journal=To appear in the Proceedings of the 17th International Symposium on Space Terahertz Technology, Paris, May 10–12, 2006 \| bibcode=2006stt..conf..127A \| arxiv=astro-ph/0608285 }}
			* {{cite journal \| last=Taylor \| first=A. \| coauthors=et al. \| title=CLOVER - A new instrument for measuring the B-mode polarization of the CMB \| journal=Proceedings of XXXIXth Rencontres de Moriond, Editions Frontiers \| year=2004 \| arxiv=astro-ph/0407148 \|bibcode = 2004astro.ph..7148T }}

			== References ==
			{{Reflist\|1}}

			{{CMB experiments}}

			{{coord missing\|Chile}}

			[[Category:Cosmic microwave background experiments]]

84.212.99.233: /* Short-range dependence vs. long-range dependence */

2012-01-14T17:19:51Z

Short-range dependence vs. long-range dependence

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← Older revision		Revision as of 20:15, 8 November 2014
Line 1:		Line 1:
	~~{{other uses\|Clover (disambiguation)}}~~		If you ɑгe а bookie and oԝn an Apple iPad, yoս will be thrilled to know that there aгe any number of apps that сan help you take care of thе bookie աork ѡithout difficulty ԝhile on аppropriate. Wɦile you probaƅly don't want to rely on these apps to work full time over yoսr business, tҺey will save youг day іn case үou are away from theiг ѡork. Thеre aгe lots օf options for wherе to keep a bachelorette event and աhat tߋ dο. Really аre millions mаny other types of bonuses tҺɑt turn out to be a very gooԁ deal. Υоu can bet till Tuгn wіth yоur cards. Takе a lοok аt the 6 apps ʏoս can't do withoսt.<br><br>
	~~'''Clover''' would have been~~ an ~~experiment~~ to ~~measure the [[Polarization (waves)\|polarization]]~~ of ~~the [[Cosmic Microwave Background]]~~. ~~It was approved for funding in late 2004~~, ~~with the aim of having the full telescope operational by 2009~~. ~~The project was jointly run by [[Cardiff University]], [[Oxford University]], the [[Cavendish Astrophysics Group]]~~ and ~~the [[University~~ of ~~Manchester]]~~.~~<ref name="cardiff_webpage">{{cite web \| url=http://www~~.~~astro~~.~~cf.ac.uk/groups/instrumentation/projects/clover/ \| title=Clover Project page at Cardiff University \| accessdate=2007-07-31}}</ref>~~<~~ref name="oxford"~~>~~{{cite web \| url=http://www-astro.physics.ox.ac.uk/research/expcosmology/groupclover.html \| title = Clover Project page at Oxford \| accessdate=2007-07-31}}~~<~~/ref~~>

	~~The Clover Project was meant to consist of two independent telescopes~~, ~~one operating at 95~~ [~~[Hertz\|GHz~~]~~] with~~ the ~~other operating at both 150 and 225 [[Hertz\|GHz]]~~. ~~Both telescopes were~~ to ~~be sited near the [[Cosmic Background Imager\|CBI]] site~~ in ~~the [[Atacama\|Atacama Desert~~, ~~Chile]]. The two telescope [[Receiver (radio)\|receivers]] would have been large format [[focal plane array (astronomy)\|focal plane array]]s~~ of ~~either 100 or 200 [[bolometer\|bolometric detectors]]~~.<~~ref name="oxford" /~~>		While it holds true that үօu can read on and on aЬout ցreat moves and great winning strategies fօr thе different casino games, nothing beats experience еxactly ԝhat you learn from actual grinding. 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	~~The aim of the experiment was~~ to ~~measure the [[B~~-~~mode]] [[Polarization (waves)\|polarization]] of~~ the [~~[Cosmic Microwave Background~~]~~] between [[multipole]]s of 20 and 1000 down to a sensitivity limited by~~ the ~~foreground contamination due~~ to ~~[[gravitational lens\|lensing]]~~. ~~This would have allowed~~ the ~~detection~~ of ~~primordial [[gravitational waves]] in~~ the ~~universe so~~ long ~~as the ratio~~ of ~~scalar perturbations (caused by density fluctuations in the early universe)~~ to ~~the tensor perturbations caused~~ by ~~gravitational waves was greater than <math>r = 0~~.01<~~/math~~>.<~~ref name="oxford" /~~>

	~~It was hoped that the telescope would have spent around 2 years observing~~ a ~~total of around 1~~,~~000 [[degree~~ (~~angle~~)~~\|degree]]s~~ of ~~sky, made up of several patches~~ of ~~sky where polarized foregrounds ([[synchrotron]] and thermal dust emission) are at a minimum~~.<~~ref name="oxford" /~~>

	~~Clover was canceled in March 2009~~ as ~~[[Science and Technology Facilities Council\|STFC]] were unable to provide~~ the ~~requested additional funds~~ of 2.~~55 million pounds to finish~~ the ~~project~~.<~~ref name="IoP"~~>~~{{cite web \| url=http://physicsworld.com/cws/article/news/38547 \| title = It’s all over for Clover \| accessdate=2009-04-08}}~~<~~/ref~~>

	~~== Further reading ==~~
	~~=== Journal articles ===~~
	~~<!-- Ordered by year published -->~~
	* {{cite journal \| last=North \| first=C. ~~\| coauthors=et al~~. ~~\| url=http://www-astro~~.~~physics~~.ox.ac.~~uk/~cen/Papers/STT2007_Paper.pdf \| title=Clover - Measuring~~ the ~~CMB B~~-~~mode Polarisation \| journal=To appear in Proceedings~~ of ~~the 18th International Symposium on Space Terahertz Technology, Caltech, March 21–23, 2007 \| year=2007}}~~
	* {{cite journal \| last=Taylor \| first=A. \| coauthors=Clover collaboration \| title=CLOVER - A B-mode polarization instrument \| journal=New Astronomy Reviews \| volume=50 \| issue=11-12 \| year=2006 \| pages=993–998 \| doi=10.1016/j.newar.2006.09.026 \| arxiv=astro-ph/0610716 \|bibcode = 2006NewAR..50..~~993T }}~~
	* {{cite journal \| last=Audley \| first=M. ~~\| coauthors=et al~~. ~~\| title=TES imaging array technology for CLOVER \| journal=SPIE Orlando \| date=May 24–31~~, ~~2006 \| arxiv=astro-ph/0607067 \|bibcode = 2006SPIE~~.~~6275E~~..~~69A \|doi = 10~~.~~1117/12.670792 }}~~
	* {{cite journal \| last=Audley \| first=M. \| coauthors=et al. \| year=2006 \| pages=127 \| title=Prototype finline-coupled TES bolometers for ~~CLOVER \| journal=To appear in the Proceedings~~ of the ~~17th International Symposium on Space Terahertz Technology~~, ~~Paris~~, ~~May 10–12~~, ~~2006 \| bibcode=2006stt..conf..127A \| arxiv=astro-ph/0608285 }}~~
	* {{cite journal \| last=Taylor \| first=A. \| coauthors=et al. ~~\| title=CLOVER - A new instrument for measuring~~ the ~~B-mode polarization of the CMB \| journal=Proceedings of XXXIXth Rencontres de Moriond~~, ~~Editions Frontiers \| year=2004 \| arxiv=astro-ph/0407148 \|bibcode = 2004astro~~.ph..~~7148T }}~~

	~~== References ==~~
	~~{{Reflist\|1}}~~

	~~{{CMB experiments}}~~

	~~{{coord missing\|Chile}}~~

	~~[[Category:Cosmic microwave background experiments]]~~

← Older revision		Revision as of 13:29, 25 January 2014
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	~~Let me~~ ~~healthy food~~ [http://~~Www~~.~~Healthychefcreations~~.~~com~~/ ~~delivery~~] ~~first begin by introducing myself~~. My name ~~is Boyd Butts although it is not~~ the ~~name on my beginning certification~~. ~~One~~ of the ~~very best issues~~ in the ~~world for me is~~ to ~~do aerobics~~ and ~~now~~ [http://~~www.Nutrition411~~.com/~~patient-education-materials~~/~~grocery~~-~~shopping~~-~~and-food-preparation~~/~~item/889~~-~~diet~~-~~plans~~-~~with~~-~~meal-delivery/ I'm attempting] to healthy food delivery earn cash with it~~. ~~South Dakota is exactly where me and my husband live~~. ~~Hiring has been my [~~http://~~Www~~.~~Dailymail~~.Co.uk/~~femail~~/~~article-1305288~~/~~Diets~~-~~door~~-Do-~~latest~~-~~home~~-~~delivery~~-~~meal~~-~~packages~~-~~cut~~-~~mustard~~.~~html occupation]~~ for ~~some time but I've currently applied for another~~ 1~~.<br><br>my web page;~~ [~~http~~:~~//Mrk.im/fooddeliveryservices36486 http://Mrk.im/fooddeliveryservices36486~~]		{{other uses\|Clover (disambiguation)}}
			'''Clover''' would have been an experiment to measure the [[Polarization (waves)\|polarization]] of the [[Cosmic Microwave Background]]. It was approved for funding in late 2004, with the aim of having the full telescope operational by 2009. The project was jointly run by [[Cardiff University]], [[Oxford University]], the [[Cavendish Astrophysics Group]] and the [[University of Manchester]].<ref name="cardiff_webpage">{{cite web \| url=http://www.astro.cf.ac.uk/groups/instrumentation/projects/clover/ \| title=Clover Project page at Cardiff University \| accessdate=2007-07-31}}</ref><ref name="oxford">{{cite web \| url=http://www-astro.physics.ox.ac.uk/research/expcosmology/groupclover.html \| title = Clover Project page at Oxford \| accessdate=2007-07-31}}</ref>

			The Clover Project was meant to consist of two independent telescopes, one operating at 95 [[Hertz\|GHz]] with the other operating at both 150 and 225 [[Hertz\|GHz]]. Both telescopes were to be sited near the [[Cosmic Background Imager\|CBI]] site in the [[Atacama\|Atacama Desert, Chile]]. The two telescope [[Receiver (radio)\|receivers]] would have been large format [[focal plane array (astronomy)\|focal plane array]]s of either 100 or 200 [[bolometer\|bolometric detectors]].<ref name="oxford" />

			The aim of the experiment was to measure the [[B-mode]] [[Polarization (waves)\|polarization]] of the [[Cosmic Microwave Background]] between [[multipole]]s of 20 and 1000 down to a sensitivity limited by the foreground contamination due to [[gravitational lens\|lensing]]. This would have allowed the detection of primordial [[gravitational waves]] in the universe so long as the ratio of scalar perturbations (caused by density fluctuations in the early universe) to the tensor perturbations caused by gravitational waves was greater than <math>r = 0.01</math>.<ref name="oxford" />

			It was hoped that the telescope would have spent around 2 years observing a total of around 1,000 [[degree (angle)\|degree]]s of sky, made up of several patches of sky where polarized foregrounds ([[synchrotron]] and thermal dust emission) are at a minimum.<ref name="oxford" />

			Clover was canceled in March 2009 as [[Science and Technology Facilities Council\|STFC]] were unable to provide the requested additional funds of 2.55 million pounds to finish the project.<ref name="IoP">{{cite web \| url=http://physicsworld.com/cws/article/news/38547 \| title = It’s all over for Clover \| accessdate=2009-04-08}}</ref>

			== Further reading ==
			=== Journal articles ===
			<!-- Ordered by year published -->
			* {{cite journal \| last=North \| first=C. \| coauthors=et al. \| url=http://www-astro.physics.ox.ac.uk/~cen/Papers/STT2007_Paper.pdf \| title=Clover - Measuring the CMB B-mode Polarisation \| journal=To appear in Proceedings of the 18th International Symposium on Space Terahertz Technology, Caltech, March 21–23, 2007 \| year=2007}}
			* {{cite journal \| last=Taylor \| first=A. \| coauthors=Clover collaboration \| title=CLOVER - A B-mode polarization instrument \| journal=New Astronomy Reviews \| volume=50 \| issue=11-12 \| year=2006 \| pages=993–998 \| doi=10.1016/j.newar.2006.09.026 \| arxiv=astro-ph/0610716 \|bibcode = 2006NewAR..50..993T }}
			* {{cite journal \| last=Audley \| first=M. \| coauthors=et al. \| title=TES imaging array technology for CLOVER \| journal=SPIE Orlando \| date=May 24–31, 2006 \| arxiv=astro-ph/0607067 \|bibcode = 2006SPIE.6275E..69A \|doi = 10.1117/12.670792 }}
			* {{cite journal \| last=Audley \| first=M. \| coauthors=et al. \| year=2006 \| pages=127 \| title=Prototype finline-coupled TES bolometers for CLOVER \| journal=To appear in the Proceedings of the 17th International Symposium on Space Terahertz Technology, Paris, May 10–12, 2006 \| bibcode=2006stt..conf..127A \| arxiv=astro-ph/0608285 }}
			* {{cite journal \| last=Taylor \| first=A. \| coauthors=et al. \| title=CLOVER - A new instrument for measuring the B-mode polarization of the CMB \| journal=Proceedings of XXXIXth Rencontres de Moriond, Editions Frontiers \| year=2004 \| arxiv=astro-ph/0407148 \|bibcode = 2004astro.ph..7148T }}

			== References ==
			{{Reflist\|1}}

			{{CMB experiments}}

			{{coord missing\|Chile}}

			[[Category:Cosmic microwave background experiments]]