CASS - Recent changes [en]

calendar:News

2012-05-15T23:36:51Z

← Older revision		Revision as of 23:36, 15 May 2012
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	\|Image = Picture_1_2_t593.png		\|Image = Picture_1_2_t593.png
	\|Summary = NASA today launched a pair of small spacecraft that will give middle-school students an unprecedented opportunity to study the moon by way of cameras guided by undergraduates at UC San Diego. The university will use software to project the path that the GRAIL spacecraft will follow while orbiting the moon next year. Middle-school students can ask UCSD to use the spacecraft's MoonKam imaging systems to photograph specific spots on the surface. CASS Researcher Karen Flammer is involved in education and outreach for the GRAIL mission.}}		\|Summary = NASA today launched a pair of small spacecraft that will give middle-school students an unprecedented opportunity to study the moon by way of cameras guided by undergraduates at UC San Diego. The university will use software to project the path that the GRAIL spacecraft will follow while orbiting the moon next year. Middle-school students can ask UCSD to use the spacecraft's MoonKam imaging systems to photograph specific spots on the surface. CASS Researcher Karen Flammer is involved in education and outreach for the GRAIL mission.}}
		+
		+	{{FrontPageNews
		+	\|Date = 31 Aug 2011
		+	\|Title = Dr. Coil awarded the NSF CAREER Grant (2011)
		+	\|Link = http://www-physics.ucsd.edu/awards/awardstory.php?storyid=246
		+	\|Image = acoil.jpg
		+	\|Summary = Dr. Coil will carry out three complementary research projects to tackle several key outstanding questions in galaxy evolution. Her goal is to uncover the physical processes behind the dramatic evolution observed in galaxies and AGN in the latter half of cosmic history, focusing specifically on the build-up of stellar mass in galaxies, the role of environment on AGN accretion, and the prevalence and importance of outflowing galactic winds.}}

	{{FrontPageNews		{{FrontPageNews

calendar:Journal

2012-05-15T20:01:34Z

← Older revision		Revision as of 20:01, 15 May 2012
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-	== Journal Club ~~Meetings~~ ==	+	== Journal Club Seminars ==
	{{TOC right\|limit=3}}		{{TOC right\|limit=3}}
-	The ~~meetings~~ take place on Fridays from 12:00 - 1:00pm in 329 SERF. Pizza and ~~sodas~~ are served.	+	The seminars take place on Fridays from 12:00 - 1:00pm in 329 SERF. Pizza and soda are served.

-	~~Everybody~~ is welcome to attend and/or present. The ~~meetings~~ generally cover recent interesting journal articles or conference reports, and may introduce the topic of next week's seminar or a speaker's own results.	+	Everyone is welcome to attend and/or present. The seminars generally cover recent interesting journal articles or conference reports, and may introduce the topic of next week's seminar or a speaker's own results.

	Past journal club talks are archived [[calendar:journalarchive\|here]].		Past journal club talks are archived [[calendar:journalarchive\|here]].
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	\|Speaker2= Chang Feng		\|Speaker2= Chang Feng
	\|Institution = UCSD-CASS		\|Institution = UCSD-CASS
-	\|Title = <small>''Chang's title:''</small> "The interplay between primordial non-Gaussianity and gravitational lensing"	+	\|Title = <small>''Jon's title:''</small> "Searching for Primordial B-modes from the South Pole <br>with the Keck Telescope"
-	~~\|Title2=~~ }}	+	\|Title2 = <small>''Chang's title:''</small> "The interplay between primordial non-Gaussianity and <br>gravitational lensing"}}

	{{Seminars		{{Seminars
	\|Date = 05/25/2012		\|Date = 05/25/2012
-	\|Speaker = Scott Gustafson	+	\|Speaker = Zhibin Guo
-	\|Institution = UCSD-CASS	+	\|Speaker2 = Scott Gustafson
-	\|Title = ~~Title~~ TBA}}	+	\|Institution = Peking University & UCSD-CASS, respectively
		+	\|Title = <small>''Zhibin's title:''</small> "Turbulent magnetic reconnection"
		+	\|Title2 = <small>''Scott's title:''</small> TBA}}

	{{Seminars		{{Seminars
	\|Date = 06/01/2012		\|Date = 06/01/2012
-	\|Speaker =	+	\|Speaker = Lei Zhao
-	\|Title = }}	+	\|Speaker2 = Yusuke Kosuga
		+	\|Institution = UCSD-CASS
		+	\|Title = <small>''Lei's title:''</small> TBA
		+	\|Title2 = <small>''Yusuke's title:''</small> TBA}}

	{{Seminars		{{Seminars
	\|Date = 06/08/2012		\|Date = 06/08/2012
		+	\|Speaker = Pei-Chun Hsu
		+	\|Speaker2 = Wendell Misch
		+	\|Institution = UCSD-CASS
		+	\|Title = <small>''Pei-Chun's title:''</small> TBA
		+	\|Title2 = <small>''Wendell's title:''</small> TBA}}
		+
		+	{{Seminars
		+	\|Date = 06/15/2012
	\|Speaker = Darcy Barron		\|Speaker = Darcy Barron
-	\|~~Title~~ = Title TBA}}	+	\|Speaker2 = Christopher Lee
		+	\|Institution= UCSD-CASS
		+	\|Title = <small>''Darcy's title:''</small> TBA
		+	\|Title2 = <small>''Christopher's title:''</small> TBA}}

grads:Pchen

2012-05-11T20:43:39Z

Created page with "{{Profile | UserName = grads:pchen | Image = | FirstName = Pengfei | LastName = Chen | Email = pec008@ucsd.edu | Office = SERF 465 | Phone = }}"

New page

{{Profile
| UserName = grads:pchen
| Image =
| FirstName = Pengfei
| LastName = Chen
| Email = pec008@ucsd.edu
| Office = SERF 465
| Phone = }}

directory:Grad

2012-05-11T20:42:12Z

← Older revision		Revision as of 20:42, 11 May 2012
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	{{grads:dbardalezgagliuffi}}		{{grads:dbardalezgagliuffi}}
-	~~{{Grads:jjcherry}}~~
-	~~{{grads:acieplak}}~~
	{{grads:dbarron}}		{{grads:dbarron}}
		+	{{grads:pchen}}
		+	{{grads:jjcherry}}
		+	{{grads:acieplak}}
	{{grads:aday}}		{{grads:aday}}
	{{grads:gdobrowalski}}		{{grads:gdobrowalski}}

calendar:Journal

2012-05-11T17:48:36Z

← Older revision		Revision as of 17:48, 11 May 2012
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	\|Speaker2= Chang Feng		\|Speaker2= Chang Feng
	\|Institution = UCSD-CASS		\|Institution = UCSD-CASS
-	\|Title = ~~Titles TBA~~	+	\|Title = <small>''Chang's title:''</small> "The interplay between primordial non-Gaussianity and gravitational lensing"
	\|Title2= }}		\|Title2= }}

seminars:2011

2012-05-09T22:57:13Z

← Older revision		Revision as of 22:57, 9 May 2012
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	\|Position = Emeritus Professor of Physics		\|Position = Emeritus Professor of Physics
	\|Institution = UCSD (& Academia Sinica)		\|Institution = UCSD (& Academia Sinica)
-	\|Url =	+	\|Url = http://casswww.ucsd.edu/index.php/faculty:Fhshu
	\|Host = Pat Diamond		\|Host = Pat Diamond
	\|Title = "Climate Change and High-Throughput Biofuels"		\|Title = "Climate Change and High-Throughput Biofuels"
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	{{Seminars		{{Seminars
-	\|Date = 5/9/2012	+	\|Date = 5/8/2012
-	\|Speaker =	+	\|Note = (In lieu of regular Astrophysics Seminar on 5/9). Special Joint MAE/CER/CASS/Plasma Physics Seminar @ 4:00PM - EBU II, Room 479
-	\|Position =	+	\|Speaker = Frank H. Shu
-	\|Institution =	+	\|Position = Emeritus Professor of Physics
-	\|Url =	+	\|Institution = UCSD (& Academia Sinica)
-	\|Host =	+	\|Url = http://casswww.ucsd.edu/index.php/faculty:Fhshu
-	\|Title =	+	\|Host = George Tynan & Pat Diamond
-	\|Abstract =	+	\|Title = "Molten Salt Breeder Reactors"
		+	\|Abstract = We outline why Generation IV nuclear reactors, especially the Molten Salt Breeder Reactor (MSBR), represent more than a simple evolution of Generation III+ light water reactors (LWRs), but are a game changer in nuclear fission. In particular, we explain why the MSBR is safe with respect to possible accidents leading to the large-scale release of radioactivity, superior in terms of cost performance if used for process heat rather then turbine electricity generation, secure relative to nuclear proliferation, and sustainable with respect to nuclear waste disposal and the ability to provide the bulk of the clean energy needed for the millennium. Wediscuss the thermal, chemical, and mechanical challenges particular to developing this technology, and we explore a proposed approach using novel materials to build two-fluid MSBRs on a rapid enough schedule to make the world free of plutonium and net CO2 emission by roughly mid-century. We then summarize the laboratory experience of our group that suggests there are probably no technical showstoppers to the practical realization of such MSBRs. Finally, we project the feasibility of coupling the capacity of these facilities to the production of high-throughput biofuels that can rollback atmospheric greenhouse gases on a time scale of about two centuries to levels that would prevent the most catastrophic consequences of global warming.
	}}		}}

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	\|Speaker = Joel Ullom		\|Speaker = Joel Ullom
	\|Position =		\|Position =
-	\|Institution = NIST	+	\|Institution = National Institute of Standards and Technology (NIST), Boulder, CO
	\|Url = http://www.nist.gov/cgi-bin/wwwph/cso.nist.gov?Query=joel+ullom&submit=Enter		\|Url = http://www.nist.gov/cgi-bin/wwwph/cso.nist.gov?Query=joel+ullom&submit=Enter
	\|Host = Brian Keating		\|Host = Brian Keating
-	\|Title = ~~Title TBA~~	+	\|Title = "Cryogenic Sensors for Astrophysics and Terrestrial Materials Analysis"
-	\|Abstract = ~~Abstract TBA~~	+	\|Abstract = Sensors operating at temperatures near 100 mK bring exquisite sensitivity to a startlingly broad range of applications. These sensors often consist of thin superconducting films that are electrically biased in the superconducting-to-normal transition where their resistance is a strong function of temperature and hence deposited energy or power. Devices designed for gamma-ray and alpha-particle spectroscopy are able to measure the energy of single 5 MeV events with resolving powers greater than 5,000, perhaps the highest resolving power ever achieved in an energy-dispersive measurement. These devices provide new capabilities in the arena of nuclear forensics, treaty verification, and nuclear materials accounting. Kilopixel arrays of transition-edge sensors are also being used in contemporary probes of the cosmic microwave background such as ACTPol and SPTPol. Despite significant differences between these applications, the sensing elements are remarkably similar. I will review transition-edge sensor development at NIST and discuss a range of applications including submillimeter and millimeter-wave astronomy, as well as emerging applications that include nuclear materials analysis, time-resolved X-ray spectroscopy, and synchrotron science.
	}}		}}

directory:Grad

2012-05-09T20:53:48Z

← Older revision		Revision as of 20:53, 9 May 2012
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	{{grads:clee}}		{{grads:clee}}
	{{grads:wlee}}		{{grads:wlee}}
-	~~{{grads:slin}}~~
	{{grads:fmatuda}}		{{grads:fmatuda}}
	{{grads:ajmendez}}		{{grads:ajmendez}}
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	<!-- {{grads:rwagner}} Not a student any more -->		<!-- {{grads:rwagner}} Not a student any more -->
	{{grads:hxu}}		{{grads:hxu}}
		+	{{grads:slin}}
	{{grads:lzhao}}		{{grads:lzhao}}

faculty:Krumpe

2012-05-09T19:44:10Z

← Older revision		Revision as of 19:44, 9 May 2012
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	{{Profile		{{Profile
	\| UserName = faculty:krumpe		\| UserName = faculty:krumpe
-	\| Image =	+	\| Image = krumpe.jpg
	\| FirstName = Mirko		\| FirstName = Mirko
	\| LastName = Krumpe		\| LastName = Krumpe

File:Krumpe.jpg

2012-05-09T19:44:03Z

uploaded "[[File:Krumpe.jpg]]"

faculty:Krumpe

2012-05-09T19:11:09Z

← Older revision		Revision as of 19:11, 9 May 2012
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	{{Profile		{{Profile
-	\| UserName = faculty:~~Mkrumpe~~	+	\| UserName = faculty:krumpe
	\| Image =		\| Image =
	\| FirstName = Mirko		\| FirstName = Mirko

faculty:Miyaji

2012-05-09T19:10:40Z

← Older revision		Revision as of 19:10, 9 May 2012
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	{{Profile		{{Profile
-	\| UserName = faculty:~~tmiyaji~~	+	\| UserName = faculty:miyaji
	\| Image =		\| Image =
	\| FirstName = Takamitsu		\| FirstName = Takamitsu

directory:Faculty

2012-05-09T19:10:17Z

← Older revision	Revision as of 19:10, 9 May 2012
(One intermediate revision not shown)

faculty:Miyaji

2012-05-09T19:09:18Z

← Older revision		Revision as of 19:09, 9 May 2012
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	{{Profile		{{Profile
-	\| UserName = faculty:~~miyaji~~	+	\| UserName = faculty:tmiyaji
	\| Image =		\| Image =
	\| FirstName = Takamitsu		\| FirstName = Takamitsu

directory:Faculty

2012-05-09T19:08:37Z

← Older revision	Revision as of 19:08, 9 May 2012
(2 intermediate revisions not shown)

faculty:Krumpe

2012-05-09T19:05:25Z

← Older revision		Revision as of 19:05, 9 May 2012
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	{{Profile		{{Profile
-	\| UserName = faculty:~~krumpe~~	+	\| UserName = faculty:Mkrumpe
	\| Image =		\| Image =
	\| FirstName = Mirko		\| FirstName = Mirko

faculty:Eburbidge

2012-05-09T19:04:33Z

← Older revision		Revision as of 19:04, 9 May 2012
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	\|Position = Professor Emeritus		\|Position = Professor Emeritus
	\|Email = eburbidge@ucsd.edu		\|Email = eburbidge@ucsd.edu
-	\|Office = SERF ~~327~~	+	\|Office = SERF 330
	\|Image = eburbidge.jpg		\|Image = eburbidge.jpg
	\|BiblioPDF = eburbidge.pdf		\|BiblioPDF = eburbidge.pdf
-	\|Phone = ~~<!--~~(858) 534-~~6626 Needs to be corrected.-->~~	+	\|Phone = (858) 534-4477
	\|adslink = http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?author=Burbidge,+Margaret&version=1		\|adslink = http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?author=Burbidge,+Margaret&version=1
	\|spireslink = http://www.slac.stanford.edu/spires/find/hep/www?rawcmd=FIND+A+Burbidge,+Margaret&FORMAT=www&SEQUENCE=ds(d)		\|spireslink = http://www.slac.stanford.edu/spires/find/hep/www?rawcmd=FIND+A+Burbidge,+Margaret&FORMAT=www&SEQUENCE=ds(d)
	\|Research = Theoretical astrophysics: Physics of active galaxies & quasi-stellar objects, nonthermal radiation processes, cosmology		\|Research = Theoretical astrophysics: Physics of active galaxies & quasi-stellar objects, nonthermal radiation processes, cosmology
	}}		}}

faculty:Fhshu

2012-05-09T19:01:41Z

← Older revision		Revision as of 19:01, 9 May 2012
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	\|Position = Distinguished Professor Emeritus, University Professor Emeritus		\|Position = Distinguished Professor Emeritus, University Professor Emeritus
	\|Email = fhshu@ucsd.edu		\|Email = fhshu@ucsd.edu
-	\|Office = SERF ~~427~~	+	\|Office = SERF 330
-	\|Phone = (858) ~~822~~-~~1214~~	+	\|Phone = (858) 534-4477
	\|adslink = http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?author=Shu,+Frank&version=1		\|adslink = http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?author=Shu,+Frank&version=1
	}}		}}

faculty:Gburbidge

2012-05-09T18:58:34Z

← Older revision		Revision as of 18:58, 9 May 2012
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	\| FirstName = Geoffrey		\| FirstName = Geoffrey
	\| LastName = Burbidge		\| LastName = Burbidge
-	\| Position = Professor Burbidge passed ~~<br/>~~ away on Jan. 26,2010	+	\| Position = Professor Burbidge passed away on Jan. 26, 2010
	\| Email =		\| Email =
	\| Office =		\| Office =

faculty:Miyaji

2012-05-09T18:55:53Z

Created page with "{{Profile | UserName = faculty:miyaji | Image = | FirstName = Takamitsu | LastName = Miyaji | Position = Visiting Associate Research Scientist | Email = miyaji@astrosen.unam.mx ..."

New page

{{Profile
| UserName = faculty:miyaji
| Image =
| FirstName = Takamitsu
| LastName = Miyaji
| Position = Visiting Associate Research Scientist
| Email = miyaji@astrosen.unam.mx
| Office =
| Lab =
| Phone =
| Fax = (858) 534-0177
| adslink = http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?author=Miyaji,+Takamitsu&version=1
| spireslink = http://www.slac.stanford.edu/spires/find/hep/www?rawcmd=FIND+A+Miyaji,+Takamitsu&FORMAT=www&SEQUENCE=ds(d)
| Web0 =
| Web0Title =
| Web1 =
| Web1Title =
| Web2 =
| Web2Title =
| ResearchShort = Conducts collaborative research in CASS with Associate Professor of Physics Alison Coil and Visiting Assistant Project Scientist Mirko Krumpe on clustering of galaxies and their evolution.
| Research = Dr. Miyaji conducts collaborative research in CASS with Associate Professor of Physics Alison Coil and Visiting Assistant Project Scientist Mirko Krumpe on clustering of galaxies and their evolution. Their work on the cross correlation between X-ray emitting galaxies in the Rosat All-Sky Survey and the red galaxies of the Sloan Digital Sky Survey allowed for the first-time determination of the full distribution of AGN dark matter haloes.
| Biography = PhD 1994, University of Maryland. Dr. Takamitsu Miyaji holds a Visiting Associate Research Scientist appointment in CASS. His home institution is the Universidad Nacional Autonoma de Mexico (UNAM), Ensenada, BC, Mexico, where he is currently an Investigador Tutular B (Associate Professor Level).
| Projects = He is presently working with the Japanese AKARI team to correlate X-ray galaxies as detected by the Chandra X-ray Observatory with specifically selected AKARI sources to identify those AGN in the AKARI North Ecliptic Pole survey that have Compton-thick accretion. This is directly related to galaxy evolution and structure.
| Publications =
| Description =
| Accomplishments =
| Expertise =
}}

faculty:Krumpe

2012-05-09T18:43:22Z

New page

{{Profile
| UserName = faculty:krumpe
| Image =
| FirstName = Mirko
| LastName = Krumpe
| Position = Visiting Assistant Project Scientist
| Email = mkrumpe@ucsd.edu
| Office =
| Lab =
| Phone =
| Fax = (858) 534-0177
| adslink = http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?author=Krumpe,+Mirko&version=1
| spireslink = http://www.slac.stanford.edu/spires/find/hep/www?rawcmd=FIND+A+Krumpe,+Mirko&FORMAT=www&SEQUENCE=ds(d)
| Web0 =
| Web0Title =
| Web1 =
| Web1Title =
| Web2 =
| Web2Title =
| ResearchShort = Conducts collaborative research in CASS with Associate Professor of Physics Alison Coil and Visiting Associate Research Scientist Takamitsu Miyaji on clustering of galaxies and their evolution.
| Research = Dr. Krumpe conducts collaborative research in CASS with Associate Professor of Physics Alison Coil and Visiting Associate Research Scientist Takamitsu Miyaji on clustering of galaxies and their evolution. Their work on the cross correlation between X-ray emitting galaxies in the Rosat All-Sky Survey and the red galaxies of the Sloan Digital Sky Survey allowed for the first-time determination of the full distribution of AGN dark matter haloes.
| Biography = PhD 2008, magna cum laude, AIP, Potsdam, Germany. Dr. Mirko Krumpe holds a Visiting Assistant Project Scientist appointment in CASS. His home institution is the European Organisation for Astronomical Research in the Southern Hemisphere (ESO), Garching, Germany, where he is currently a Postdoctoral Fellow. Previously, he served as a Postdoctoral Scholar in CASS.
| Projects = He is presently working with the Japanese AKARI team to correlate X-ray galaxies as detected by the Chandra X-ray Observatory with specifically selected AKARI sources to identify those AGN in the AKARI North Ecliptic Pole survey that have Compton-thick accretion. This is directly related to galaxy evolution and structure.
| Publications =
| Description =
| Accomplishments =
| Expertise =
}}

directory:Faculty

2012-05-09T18:15:07Z

← Older revision		Revision as of 18:15, 9 May 2012
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	----		----
	=== Visiting Researchers ===		=== Visiting Researchers ===
		+	{{faculty:krumpe}}
		+	{{faculty:miyaji}}

postdocs:Aleks

2012-05-09T18:14:22Z

← Older revision		Revision as of 18:14, 9 May 2012
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	\|Image = aleks.jpg		\|Image = aleks.jpg
	\|Phone = (858) 822-4463		\|Phone = (858) 822-4463
-	\|Web0 = [http://www.cge.uci.edu/fellows.html ~~http://www.cge.uci.edu/fellows.html]~~	+	\|Web0 = http://www.cge.uci.edu/fellows.html
	\|adslink = http://goo.gl/bElhq		\|adslink = http://goo.gl/bElhq
	\|spireslink = http://www.slac.stanford.edu/spires/find/hep/www?rawcmd=FIND+A+Diamond-Stanic,+Aleks&FORMAT=www&SEQUENCE=ds(d)		\|spireslink = http://www.slac.stanford.edu/spires/find/hep/www?rawcmd=FIND+A+Diamond-Stanic,+Aleks&FORMAT=www&SEQUENCE=ds(d)
	\|Research = Co-evolution of galaxies and their supermassive black holes. Galaxy outflows and their role in regulating star formation.		\|Research = Co-evolution of galaxies and their supermassive black holes. Galaxy outflows and their role in regulating star formation.
	}}		}}

directory:Faculty

2012-05-09T18:00:15Z

← Older revision		Revision as of 18:00, 9 May 2012
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	=== Academic Coordinator / Outreach ===		=== Academic Coordinator / Outreach ===
	{{faculty:flammer}}		{{faculty:flammer}}
		+
		+
		+	----
		+	=== Visiting Researchers ===

postdocs:Aleks

2012-05-09T17:57:29Z

← Older revision		Revision as of 17:57, 9 May 2012
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	\|adslink = http://goo.gl/bElhq		\|adslink = http://goo.gl/bElhq
	\|spireslink = http://www.slac.stanford.edu/spires/find/hep/www?rawcmd=FIND+A+Diamond-Stanic,+Aleks&FORMAT=www&SEQUENCE=ds(d)		\|spireslink = http://www.slac.stanford.edu/spires/find/hep/www?rawcmd=FIND+A+Diamond-Stanic,+Aleks&FORMAT=www&SEQUENCE=ds(d)
-	\|Research = ~~Black hole growth, galaxy~~ evolution.	+	\|Research = Co-evolution of galaxies and their supermassive black holes. Galaxy outflows and their role in regulating star formation.
	}}		}}

directory:Main

2012-05-09T17:53:15Z

← Older revision		Revision as of 17:53, 9 May 2012
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	<!-- Removed and replaced with just the		<!-- Removed and replaced with just the
	== Directory ==		== Directory ==
-	The Center for Astrophysics and Space Sciences(CASS) is located in ~~the top two floors of~~ the Science and Engineering Research Facility(SERF). CASS currently consists of [[directory:Faculty\|faculty]], [[directory:postdoc\|postdoctoral scholars]], [[directory:Grad\|graduate students]], [[directory:staff\|technical staff]], and [[directory:admin\|administrative staff]].	+	The Center for Astrophysics and Space Sciences (CASS) is located in the Science and Engineering Research Facility (SERF). CASS currently consists of [[directory:Faculty\|faculty]], [[directory:postdoc\|postdoctoral scholars]], [[directory:Grad\|graduate students]], [[directory:staff\|technical staff]], and [[directory:admin\|administrative staff]].

	-->		-->

faculty:Aorlando

2012-05-09T17:42:22Z

← Older revision		Revision as of 17:42, 9 May 2012
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	\|Office = SERF 330A		\|Office = SERF 330A
	\|Image =		\|Image =
-	\|Phone =	+	\|Phone = (858) 534-8609
	\|adslink = http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?author=Orlando,+Angiola&version=1		\|adslink = http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?author=Orlando,+Angiola&version=1
	\|Research = Experimental and observational cosmology. Observations of cosmic microwave background temperature and polarization anisotropies, and their use to search for evidence of Inflation, constrain cosmological parameters and study the evolution of structure. Development of cryogenic detectors for astrophysics and cosmology. Experimental techniques for measurement from mm to infrared wavelengths.		\|Research = Experimental and observational cosmology. Observations of cosmic microwave background temperature and polarization anisotropies, and their use to search for evidence of Inflation, constrain cosmological parameters and study the evolution of structure. Development of cryogenic detectors for astrophysics and cosmology. Experimental techniques for measurement from mm to infrared wavelengths.
	}}		}}