Sarah Church
Professor of Physics
Administrative Appointments
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Senior Associate Vice Provost, Vice Provost for Teaching and Learning (2019 - Present)
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Senior Associate Vice Provost, Vice Provost Undergraduate Education (2016 - 2018)
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Director, Hanson Experimental Physics Laboratory (2013 - 2016)
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Professor, Stanford University (2012 - Present)
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Professor by Courtesy, SLAC PPA (2012 - Present)
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Chambers Fellow, Stanford University (2011 - 2011)
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Associate Professor by Courtesy, SLAC PPA (2007 - 2012)
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Associate Professor, Stanford University (2006 - 2012)
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Assistant Professor, Stanford University (1999 - 2005)
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Terman Fellowship, Stanford University (1999 - 1999)
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Senior Research Fellow, California Institute of Technology (1997 - 1998)
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Research Fellow, California Institute of Technology (1994 - 1997)
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Post-Graduate Research Physicist, University of California, Berkeley (1994 - 1994)
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Postdoctoral Research Assistant, Queen Mary Westfield College University of London (1989 - 1993)
Boards, Advisory Committees, Professional Organizations
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Selection Committee, DARE fellowships, Stanford University
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Collaborator, The Carbon Monoxide Mapping Array Pathfinder (COMAP) (2015 - Present)
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Member, Hansen Experimental Physics Laboratory, HEPL, Stanford University (2013)
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Chair, Committee on Undergraduate Standards and Policies, Stanford University (2013 - 2016)
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Director, Hansen Experimental Physics Laboratory, Stanford University (2013 - 2016)
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Visiting Committee, Dept. Physics, University of Miami (2013 - 2013)
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Chair, Graduate Advising, Stanford University (2012 - Present)
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Member, Convener Snowmass 2013 Cosmic Frontier, Particle Physics Astrophysics Community Planning Process (2012 - 2013)
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Member, University Course Evaluation Committee, Stanford University (2012 - 2013)
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Chair, Astronomy Astrophysics Advisory Committee, Astronomy Astrophysics (2011 - 2012)
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Member, JPL Astrophysics Advisory Committee, JPL Astrophysics (2010 - Present)
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Member, National Radio Astronomy Users Committee, National Radio Astronomy (2010 - Present)
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Principal Investigator, The Argus experiment (90 GHz spectrometer for GBT) (2009 - Present)
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Member, Astronomy Astrophysics Advisory Committee, Astronomy Astrophysics (2009 - 2012)
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Visiting Committee, Dept. Experimental Physics, U. Ireland, Maynooth (2009 - 2009)
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Member, SLAC PPA, Stanford University (2007)
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Deputy Director, Kavli Institute for Particle Astrophysics Cosmology, Stanford University (2007 - 2011)
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Member, NSF Office of Polar Programs Advisory Committee, National Science Foundation (2006 - 2008)
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Collaborator, QUIET CMB Polarization Experiment (2005 - 2012)
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Chair, Graduate Studies Committee, Stanford University (2005 - 2008)
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Member, NRC Committee to Review the Science Requirements for the ALMA Array, National Academies of Science (2005 - 2005)
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Member, Experimental Astrophysics Search Committees, Stanford University (2004 - 2006)
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Member, Cosmic Microwave Background Research, NSF/NASA/DOE Taskforce (2004 - 2005)
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Member, Kavli Institute of Particle Astrophysics Cosmology, KIPAC, Stanford University (2003)
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Member, NASA Structure Evolution of the Universe Road-Mapping Team (2001 - 2002)
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Principal Investigator, The QUaD (QUEST at DASI) CMB Polarization Experiment (2000 - 2010)
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Principal Investigator, The Sunyaev-Zel’dovich Infrared Experiment (SuZIE) (1999 - 2006)
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Member, NSF NASA Proposal Review Panels (1998)
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Collaborator, The Planck Satellite (1996 - 2012)
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Collaborator, ISO Long Wavelength Spectrometer Consortium Scientist (1994 - 1997)
Professional Education
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BA, Cambridge University, Natural Sciences (1986)
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PhD, Cambridge University (1991)
Current Research and Scholarly Interests
Experimental & Observational Astrophysics and Cosmology
2024-25 Courses
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Independent Studies (2)
- Research
PHYSICS 490 (Aut, Win, Spr) - Senior Thesis Research
PHYSICS 205 (Aut, Win, Spr)
- Research
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Prior Year Courses
2023-24 Courses
- Mechanics, Concepts, Calculations, and Context
PHYSICS 41E (Win) - Why College? Your Education and the Good Life
COLLEGE 101 (Aut)
2022-23 Courses
- Why College? Your Education and the Good Life
COLLEGE 101 (Aut)
- Mechanics, Concepts, Calculations, and Context
All Publications
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COMAP Early Science. VIII. A Joint Stacking Analysis with eBOSS Quasars
ASTROPHYSICAL JOURNAL
2024; 965 (1)
View details for DOI 10.3847/1538-4357/ad2dfc
View details for Web of Science ID 001194839300001
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GBT/Argus Observations of Molecular Gas in the Inner Regions of IC 342
ASTROPHYSICAL JOURNAL
2024; 963 (2)
View details for DOI 10.3847/1538-4357/ad2171
View details for Web of Science ID 001180043700001
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Dynamics in Star-forming Cores (DiSCo): project overview and the first look towards the B1 and NGC 1333 regions in Perseus
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2023; 527 (4): 10279-10293
View details for DOI 10.1093/mnras/stad3868
View details for Web of Science ID 001134499800006
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The Giant Low Surface Brightness Galaxy Malin 1: New Constraints for Its Molecular Gas Mass from GBT/ARGUS Observations
ASTROPHYSICAL JOURNAL LETTERS
2022; 940 (2)
View details for DOI 10.3847/2041-8213/aca146
View details for Web of Science ID 000892453700001
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COMAP Early Science. III. CO Data Processing
ASTROPHYSICAL JOURNAL
2022; 933 (2)
View details for DOI 10.3847/1538-4357/ac63ca
View details for Web of Science ID 000824060600001
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COMAP Early Science. II. Pathfinder Instrument
ASTROPHYSICAL JOURNAL
2022; 933 (2)
View details for DOI 10.3847/1538-4357/ac63c6
View details for Web of Science ID 000824067000001
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COMAP Early Science. VI. A First Look at the COMAP Galactic Plane Survey
ASTROPHYSICAL JOURNAL
2022; 933 (2)
View details for DOI 10.3847/1538-4357/ac63c8
View details for Web of Science ID 000824065300001
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COMAP Early Science. VII. Prospects for CO Intensity Mapping at Reionization
ASTROPHYSICAL JOURNAL
2022; 933 (2)
View details for DOI 10.3847/1538-4357/ac63c9
View details for Web of Science ID 000824065400001
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COMAP Early Science. V. Constraints and Forecasts at z similar to 3
ASTROPHYSICAL JOURNAL
2022; 933 (2)
View details for DOI 10.3847/1538-4357/ac63c7
View details for Web of Science ID 000824062700001
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COMAP Early Science. I. Overview
ASTROPHYSICAL JOURNAL
2022; 933 (2)
View details for DOI 10.3847/1538-4357/ac63cc
View details for Web of Science ID 000824063200001
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COMAP Early Science. IV. Power Spectrum Methodology and Results
ASTROPHYSICAL JOURNAL
2022; 933 (2)
View details for DOI 10.3847/1538-4357/ac63c5
View details for Web of Science ID 000824063600001
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Neutral versus Ion Line Widths in Barnard 5: Evidence for Penetration by Magnetohydrodynamic Waves
ASTROPHYSICAL JOURNAL
2021; 912 (1)
View details for DOI 10.3847/1538-4357/abebdd
View details for Web of Science ID 000646371800001
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Forecasting [C ii] Line-intensity Mapping Measurements between the End of Reionization and the Epoch of Galaxy Assembly
ASTROPHYSICAL JOURNAL
2020; 892 (1)
View details for DOI 10.3847/1538-4357/ab798f
View details for Web of Science ID 000522409100001
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Investigating the complex velocity structures within dense molecular cloud cores with GBT-Argus
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2019; 490 (1): 527–39
View details for DOI 10.1093/mnras/stz2633
View details for Web of Science ID 000496922300040
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Cross-correlating Carbon Monoxide Line-intensity Maps with Spectroscopic and Photometric Galaxy Surveys
ASTROPHYSICAL JOURNAL
2019; 872 (2)
View details for DOI 10.3847/1538-4357/ab0027
View details for Web of Science ID 000460814000009
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An Ammonia Spectral Map of the L1495-B218 Filaments in the Taurus Molecular Cloud. II. CCS and HC7N Chemistry and Three Modes of Star Formation in the Filaments
ASTROPHYSICAL JOURNAL
2019; 871 (2)
View details for DOI 10.3847/1538-4357/aaf887
View details for Web of Science ID 000457048700002
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On Estimation of Contamination from Hydrogen Cyanide in Carbon Monoxide Line-intensity Mapping
ASTROPHYSICAL JOURNAL
2017; 846 (1)
View details for DOI 10.3847/1538-4357/aa8624
View details for Web of Science ID 000409527500010
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CONNECTING CO INTENSITY MAPPING TO MOLECULAR GAS AND STAR FORMATION IN THE EPOCH OF GALAXY ASSEMBLY
ASTROPHYSICAL JOURNAL
2016; 817 (2)
View details for DOI 10.3847/0004-637X/817/2/169
View details for Web of Science ID 000369437900086
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Argus: A 16-pixel Millimeter-Wave Spectrometer for the Green Bank Telescope
SPIE-INT SOC OPTICAL ENGINEERING. 2014
View details for DOI 10.1117/12.2055655
View details for Web of Science ID 000354387400018
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NOVEL COMPACT WAVEGUIDE DUAL CIRCULAR POLARIZER
PROGRESS IN ELECTROMAGNETICS RESEARCH-PIER
2013; 136: 1-16
View details for Web of Science ID 000314747900001
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Low Noise Amplifiers for 140 GHz Wide-Band Cryogenic Receivers
IEEE. 2013
View details for Web of Science ID 000369754300344
- The QUIET Instrument ApJ 2013; 768: 9
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Note: Cryogenic microstripline-on-Kapton microwave interconnects
REVIEW OF SCIENTIFIC INSTRUMENTS
2012; 83 (8)
Abstract
Simple broadband microwave interconnects are needed for increasing the size of focal plane heterodyne radiometer arrays. We have measured loss and crosstalk for arrays of microstrip transmission lines in flex circuit technology at 297 and 77 K, finding good performance to at least 20 GHz. The dielectric constant of Kapton substrates changes very little from 297 to 77 K, and the electrical loss drops. The small cross-sectional area of metal in a printed circuit structure yields overall thermal conductivities similar to stainless steel coaxial cable. Operationally, the main performance tradeoffs are between crosstalk and thermal conductivity. We tested a patterned ground plane to reduce heat flux.
View details for DOI 10.1063/1.4737185
View details for Web of Science ID 000308406500081
View details for PubMedID 22938347
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A G-band cryogenic MMIC heterodyne receiver module for astronomical applications
INTERNATIONAL JOURNAL OF MICROWAVE AND WIRELESS TECHNOLOGIES
2012; 4 (3): 283-289
View details for DOI 10.1017/S1759078712000189
View details for Web of Science ID 000313630900005
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Technology developments for a large-format heterodyne MMIC array at W-band
INTERNATIONAL JOURNAL OF MICROWAVE AND WIRELESS TECHNOLOGIES
2012; 4 (3): 299-307
View details for DOI 10.1017/S1759078712000293
View details for Web of Science ID 000313630900007
- Second Season QUIET Observations: Measurements of the CMB Polarization Power Spectrum at 95 GHz Astrophysics Journal 2012; 760: 145
- W-band heterodyne receiver module with 27 K noise temperature 2012 IEEE MTT-S International Microwave Symposium Digest (MTT). IEEE, Piscataway, NJ 2012: 1-3
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Planck early results. VI. The High Frequency Instrument data processing
ASTRONOMY & ASTROPHYSICS
2011; 536
View details for DOI 10.1051/0004-6361/201116462
View details for Web of Science ID 000298485100007
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Planck early results. IV. First assessment of the High Frequency Instrument in-flight performance
ASTRONOMY & ASTROPHYSICS
2011; 536
View details for DOI 10.1051/0004-6361/201116487
View details for Web of Science ID 000298485100005
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MEASURING THE GALAXY CLUSTER BULK FLOW FROM WMAP DATA
ASTROPHYSICAL JOURNAL
2011; 737 (2)
View details for DOI 10.1088/0004-637X/737/2/98
View details for Web of Science ID 000294013600052
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THE QUaD GALACTIC PLANE SURVEY. II. A COMPACT SOURCE CATALOG
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
2011; 195 (1)
View details for DOI 10.1088/0067-0049/195/1/8
View details for Web of Science ID 000292590200008
- First Season QUIET Observations: Measurements of Cosmic Microwave Background Polarization Power Spectra at 43 GHz in the Multipole Range 25 <= \ell <= 475 Astrophysical Journal 2011; 741: 111
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A G-Band Cryogenic MMIC Heterodyne Receiver Module for Astronomical Applications
IEEE. 2011: 523–26
View details for Web of Science ID 000411595800133
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Technology developments for a scalable heterodyne MMIC array at W-band
IEEE. 2011: 527–30
View details for Web of Science ID 000411595800134
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THE QUaD GALACTIC PLANE SURVEY. I. MAPS AND ANALYSIS OF DIFFUSE EMISSION
ASTROPHYSICAL JOURNAL
2010; 722 (2): 1057-1077
View details for DOI 10.1088/0004-637X/722/2/1057
View details for Web of Science ID 000284075400008
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Planck pre-launch status: The Planck mission
ASTRONOMY & ASTROPHYSICS
2010; 520
View details for DOI 10.1051/0004-6361/200912983
View details for Web of Science ID 000283064200002
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Planck pre-launch status: The HFI instrument, from specification to actual performance
ASTRONOMY & ASTROPHYSICS
2010; 520
View details for DOI 10.1051/0004-6361/200912975
View details for Web of Science ID 000283064200010
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Planck pre-launch status: The optical architecture of the HFI
ASTRONOMY & ASTROPHYSICS
2010; 520
View details for DOI 10.1051/0004-6361/200913039
View details for Web of Science ID 000283064200012
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PARAMETER ESTIMATION FROM IMPROVED MEASUREMENTS OF THE COSMIC MICROWAVE BACKGROUND FROM QUaD
ASTROPHYSICAL JOURNAL
2010; 716 (2): 1040-1046
View details for DOI 10.1088/0004-637X/716/2/1040
View details for Web of Science ID 000278459000011
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CHARACTERIZATION OF THE MILLIMETER-WAVE POLARIZATION OF CENTAURUS A WITH QUaD
ASTROPHYSICAL JOURNAL
2010; 710 (2): 1541-1550
View details for DOI 10.1088/0004-637X/710/2/1541
View details for Web of Science ID 000274233300048
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Development of a 150 GHz MMIC module prototype for large-scale CMB radiation experiments
Conference on Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V
SPIE-INT SOC OPTICAL ENGINEERING. 2010
View details for DOI 10.1117/12.857872
View details for Web of Science ID 000285838800072
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Development of MMIC receivers for cosmic microwave background interferometry
Conference on Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V
SPIE-INT SOC OPTICAL ENGINEERING. 2010
View details for DOI 10.1117/12.857830
View details for Web of Science ID 000285838800071
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COSMOLOGICAL PARAMETERS FROM THE QUAD CMB POLARIZATION EXPERIMENT
ASTROPHYSICAL JOURNAL
2009; 701 (2): 857-864
View details for DOI 10.1088/0004-637X/701/2/857
View details for Web of Science ID 000268761500001
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SMALL ANGULAR SCALE MEASUREMENTS OF THE COSMIC MICROWAVE BACKGROUND TEMPERATURE POWER SPECTRUM FROM QUaD
ASTROPHYSICAL JOURNAL LETTERS
2009; 700 (2): L187-L191
View details for DOI 10.1088/0004-637X/700/2/L187
View details for Web of Science ID 000268157500030
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QUaD: A HIGH-RESOLUTION COSMIC MICROWAVE BACKGROUND POLARIMETER
ASTROPHYSICAL JOURNAL
2009; 692 (2): 1221-1246
View details for DOI 10.1088/0004-637X/692/2/1221
View details for Web of Science ID 000263674700019
- Coherent detectors Journal of Physics: Conference Series 2009: 012002
- Second third season QUaD CMB temperature polarization power spectra The Astrophysical Journal 2009; 692 (2): 1247-1270
- Parity Violation Constraints Using Cosmic Microwave Background Polarization Spectra from 2006 2007 Observations by the QUaD Polarimeter Physical Review Letters 2009; 102 (16): 161302
- Improved Measurements of the Temperature Polarization of the Cosmic Microwave Background from QUaD The Astrophysical Journal 2009; 705: 978-999
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The quasi-optical design of the QUaD telescope
INFRARED PHYSICS & TECHNOLOGY
2008; 51 (4): 277-286
View details for DOI 10.1016/j.infrared.2007.10.001
View details for Web of Science ID 000254984100001
- First Season QUaD CMB Temperature Polarization Power Spectra ApJ 2008; 674: 22–28
- Modelling of the optical performance of millimeter-wave instruments in MODAL SPIE edited by Linden, K. J., Sadwick, L. P. 2007: 64720D
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Corrugated waveguide band edge filters for CMB experiments in the far infrared
INFRARED PHYSICS & TECHNOLOGY
2005; 46 (6): 493-505
View details for DOI 10.1016/j.infrared.2004.10.001
View details for Web of Science ID 000230224800006
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Millimeter-wave profiled corrugated horns for the QUaD cosmic background polarization experiment
INTERNATIONAL JOURNAL OF INFRARED AND MILLIMETER WAVES
2005; 26 (4): 505-523
View details for DOI 10.1007/s10762-005-4069-7
View details for Web of Science ID 000228194400002
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Recent results from the SuZIE experiment: An investigation of SZ scaling relationships
Meeting on Observing Dark Energy
ASTRONOMICAL SOC PACIFIC. 2005: 157–166
View details for Web of Science ID 000233599200017
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Measurements of Sunyaev-Zel'dovich effect scaling relations for clusters of galaxies
ASTROPHYSICAL JOURNAL
2004; 617 (2): 829-846
View details for Web of Science ID 000225968200009
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Effects of submillimeter and radio point sources on the recovery of Sunyaev-Zel'dovich galaxy cluster parameters
ASTROPHYSICAL JOURNAL
2004; 612 (1): 96-107
View details for Web of Science ID 000223634400009
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Scientific optimization of a ground-based CMB polarization experiment
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2004; 349 (1): 321-335
View details for DOI 10.1111/j.1365-2966.2004.07506.x
View details for Web of Science ID 000220152700034
- Bandwidth characteristics of corrugated waveguidehorn feeds for CMB experiments SPIE 2004: 713
- Measuring the cosmic microwave background polarization with the QUaD experiment SPIE 2004: 84
- The quasi-optical design of the QUaD Telescope SPIE 2004: 396
- Recent Results from the SuZIE Experiment: An Investigation of SZ Scaling Relationships Observing Dark Energy 2004: 157
- Effects of sub-mm radio point sources on the recovery of Sunyaev-Zeldovich galaxy cluster parameters Astrophysical Journal 2004; 612: 96
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QUEST on DASI: a South Pole CMB polarization experiment
Workshop on the Cosmic Microwave Background Radiation and its Polarization
ELSEVIER SCI LTD. 2003: 1083–89
View details for DOI 10.1016/j.newar.2003.09.033
View details for Web of Science ID 000187665800026
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Peculiar velocity limits from measurements of the spectrum of the Sunyaev-Zeldovich effect in six clusters of galaxies
ASTROPHYSICAL JOURNAL
2003; 592 (2): 674-691
View details for Web of Science ID 000184408100003
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The effect of bandpass uncertainties on component separation
ASTROPHYSICAL JOURNAL
2003; 582 (2): L63-L66
View details for Web of Science ID 000180282800001
- BOOMERANG: A Balloon-borne Millimeter Wave Telescope Total Power Receiver for Mapping Anisotropy in the Cosmic Microwave Background Astrophysical Journal 2003; 148: 527
- Electromagnetic modelling of few-moded Winston cones in the far-infrared Ed. Marco De Petri Massimo Gervasi, AIP Conf. Proc. 2002: 295
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QUEST - A 2.6-m mm-wave telescope for CMB polarization studies
Workshop on Astrophysical Polarized Backgrounds
AMER INST PHYSICS. 2002: 159–163
View details for Web of Science ID 000175483200026
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A determination of the Hubble constant using measurements of X-ray emission and the Sunyaev-Zeldovich effect at millimeter wavelengths in the cluster Abell 1835
ASTROPHYSICAL JOURNAL
2000; 538 (2): 505-516
View details for Web of Science ID 000088824800005
- A determination of the Hubble constant using measurements of X-ray emission the SZ effect at mm wavelengths in the cluster A1835 APJ 2000; 538: 505
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The high frequency instrument of Planck: Design and performances
Workshop on Cosmic Microwave Background and the Planck Mission
GORDON BREACH PUBLISHING, TAYLOR & FRANCIS GROUP. 2000: 161-?
View details for Web of Science ID 000088375200004
- The Abell 2163 Spectrum from Infrared to Millimetre Wavelengths edited by Laureijs, R. J., Leech, K. 1999: 171
- Cosmic Microwave Background Experiments, 1999 Microwave Foregrounds edited by Oliveira-Costa, A. d., Tegmark, M. 1999
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A 96-GHz ortho-mode transducer for the Polatron
IEEE MICROWAVE AND GUIDED WAVE LETTERS
1998; 8 (12): 421-423
View details for Web of Science ID 000078591300003
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First measurement of the submillimeter Sunyaev-Zeldovich effect
ASTROPHYSICAL JOURNAL
1998; 507 (1): L5-L8
View details for Web of Science ID 000077779500002
- Measuring the cosmic microwave background anisotropy power spectrum using Boomerang Topological Defects in Cosmology World Scientific Publishers. 1998: 135
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An upper limit to arcminute-scale anisotropy in the cosmic microwave background radiation at 142 GHz
ASTROPHYSICAL JOURNAL
1997; 484 (2): 523-537
View details for Web of Science ID A1997XP94100002
- Limits on the Peculiar Velocities of Two Distant Clusters Using the Kinematic Sunyaev-Zel'dovich Effect Astrophysical Journal, Astrophysical Journal 1997; 481: 35
- A Compact High-Efficiency Feed Structure for Cosmic Microwave Background Astronomy at Millimeter Wavelengths Submillimetre Far-Infrared Space Instrumentation 1997: 77
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Observations of the Sunyaev-Zel'dovich effect at millimeter wavelengths from the Caltech submillimeter observatory
ESA Symposium on the Far InfraRed and Submillimetre Universe
EUROPEAN SPACE AGENCY. 1997: 169–174
View details for Web of Science ID A1997BJ82Z00024
- A Determination of the Hubble Constant from X-ray Observations Measurements of the Sunyaev Zel'dovich Effect in A2163 Astrophysical Journal 1997; 480: 449
- Using SuZIE Arcminute-Scale CMB Anisotropy Data to Probe Open Flat-Λ CDM Cosmogenies Astrophysical Journal 1997; 479: 17
- Bolometric Detector Systems for IR Mm-wave Space Astronomy Submillimetre Far-Infrared Space Instrumentation 1997: 105
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The ISO long-wavelength spectrometer
ASTRONOMY & ASTROPHYSICS
1996; 315 (2): L38-L42
View details for Web of Science ID A1996VU26600003
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LWS observations of the colliding galaxies NGC 4038/39
ASTRONOMY & ASTROPHYSICS
1996; 315 (2): L97-L100
View details for Web of Science ID A1996VU26600016
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Molecular line CO (2->1) observations of ultraluminous IRAS galaxies
ASTRONOMY & ASTROPHYSICS
1996; 305 (3): 747-755
View details for Web of Science ID A1996TR76900016
- Calibration Performance of the ISO Long Wavelength Spectrometer ISO Consortium Paper 1996: L43
- Non-Linear Effects in Doped-Ge Photoconductors Appl. Opt. 1996; 35: 1597
- LWS-spectroscopy of Herbig-Haro Objects Molecular Outflows in the Cha II Dark Cloud ISO Consortium Paper 1996: L321
- Photo-dissociation the CN:HCN ratio: observations of a third Bar in OMC1 Mon. Not. R. astr. Soc. 1996; 283: 1179
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PREDICTING RESIDUAL LEVELS OF ATMOSPHERIC SKY NOISE IN GROUND-BASED OBSERVATIONS OF THE COSMIC BACKGROUND-RADIATION
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
1995; 272 (3): 551-569
View details for Web of Science ID A1995QF01500011
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Measurements of submillimetre emission noise from Mauna Kea
Multi-Feed Systems for Radio Telescopes Workshop
ASTRONOMICAL SOC PACIFIC. 1995: 295–308
View details for Web of Science ID A1995BD96S00034
- An Arcminute Resolution Search at 4.7 cm-1 for Point Sources Confusion to Measurements of CMB Anisotropy Astrophysical Journal 1995; 440: L33
- The Detector Signal Processing Chain Of The ISO Long Wavelength Spectrometer Experimental Astronomy 1994; 4: 213
- Measuring the performance of the ISO LWS Infrared Spaceborne Remote Sensing 1994
- An Upper Limit on the Fine Scale Anisotropy of the Background Radiation at 800um Mon. Not. R. astr. Soc. 1993; 261: 705
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PERFORMANCE-CHARACTERISTICS OF DOPED-GE PHOTOCONDUCTORS FOR THE INFRARED SPACE-OBSERVATORY LONG-WAVELENGTH SPECTROMETER
Conference on Infrared Detector and Instrumentation
SPIE - INT SOC OPTICAL ENGINEERING. 1993: 116–125
View details for Web of Science ID A1993BZ73X00015
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TESTING THE LONG-WAVELENGTH SPECTROMETER FOR ISO
Conference on Infrared Detector and Instrumentation
SPIE - INT SOC OPTICAL ENGINEERING. 1993: 272–280
View details for Web of Science ID A1993BZ73X00029
- Ionising Radiation- Induced Effects in Doped-Germanium FIR Photoconductors Photon Detectors for Space Instrumentation 1992: 309
- Extrinsic Photoconductor Detectors for the Wavelength Range 2 to 240um Photon Detectors for Space Instrumentation 1992: 289
- Non- Linear effects in Doped-Germanium Photoconductors for the ISO Long Wavelength Spectrometer Photon Detectors for Space Instrumentation 1992: 261
- Performance Testing of Doped-Germanium Photoconductors for the ISO Long Wavelength Spectrometer Photon Detectors for Space Instrumentation 1992: 255
- Short-baseline Interferometry Atmospheric Effects Radio Astronomical Seeing edited by Baldwin, J. B., Wang, S. 1990: 48
- Performance Testing on Ge:Ga Ge:Be detectors for the ISO Long Wavelength Spectrometer From Ground-Based to Space-Borne Sub-mm Astronomy 1990: 359
- Measurements of Day-time Astronomical “Seeing” on Mauna Kea made with the James Clerk Maxwell Telescope Radio Astronomical Seeing edited by Baldwin, J. B., Wang, S. 1990: 75