{"id":990,"date":"2013-02-11T05:36:44","date_gmt":"2013-02-11T13:36:44","guid":{"rendered":"http:\/\/www.deepspace.ucsb.edu\/?page_id=990"},"modified":"2016-09-18T11:27:15","modified_gmt":"2016-09-18T18:27:15","slug":"papers","status":"publish","type":"page","link":"http:\/\/128.111.23.62\/wordpress\/papers","title":{"rendered":"Papers"},"content":{"rendered":"
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Legend<\/h5>\n

A&A<\/strong> — Astronomy & Astrophysics<\/em>
\nApJ<\/strong> — The Astrophysical Journal<\/em>
\nApJS<\/strong> — The Astrophysical Journal Supplemental Series<\/em>
\nEC<\/strong> — Education and Computing<\/em>
\nSD<\/strong> — Science Direct<\/em>
\nPASP<\/strong> — Publications of the Astronomical Society of the Pacific<\/em><\/p>\n<\/div>\n<\/div>\n\n\n\n\n\t\n\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t
Title<\/th>Published to <\/th>Year<\/th>Subject<\/th>\n<\/tr>\n<\/thead>\n
Planck early results. XXII. The submillimetre properties of a sample of Galactic cold clumps<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XXXVIII. E- and B-modes of dust polarization from the magnetized filamentary structure of the interstellar medium<\/a><\/td>A&A<\/td>2015<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds<\/a><\/td>A&A<\/td>2015<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XXXIV. The magnetic field structure in the Rosette Nebula<\/a><\/td>A&A<\/td>2015<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XXXIII. Signature of the magnetic field geometry of interstellar filaments in dust polarization maps<\/a><\/td>A&A<\/td>2015<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XXXII. The relative orientation between the magnetic field and structures traced by interstellar dust<\/a><\/td>A&A<\/td>2015<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XXXI. Microwave survey of Galactic supernova remnants<\/a><\/td>A&A<\/td>2015<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes<\/a><\/td>A&A<\/td>2014<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XXVIII. Interstellar gas and dust in Chamaeleon clouds as seen by Fermi LAT and Planck<\/a><\/td>A&A<\/td>2015<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XXVII. High-redshift infrared galaxy overdensity candidates and lensed sources discovered by Planck and confirmed by Herschel-SPIRE <\/a><\/td>A&A<\/td>2015<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XXVI. Optical identification and redshifts of Planck clusters with the RTT150 telescope<\/a><\/td>A&A<\/td>2015<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XXV. The Andromeda galaxy as seen by Planck<\/a><\/td>A&A<\/td>2015<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XXIX. All-sky dust modelling with Planck, IRAS, and WISE observations<\/a><\/td>A&A<\/td>2015<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XXIV. Constraints on variations in fundamental constants<\/a><\/td>A&A<\/td>2015<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XXIII. Galactic plane emission components derived from Planck with ancillary data<\/a><\/td>A&A<\/td>2015<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarization<\/a><\/td>A&A<\/td>2015<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XXI. Comparision of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visible<\/a><\/td>A&A<\/td>2015<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XX. Comparison of polarized thermal emission from Galactic dust with simulations of MHD turbulence<\/a><\/td>A&A<\/td>2015<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XVII. Emission of dust in the diffuse interstellar medium from the far-infrared to microwave frequencies<\/a><\/td>A&A<\/td>2014<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XVI. Profile likelihoods for cosmological parameters<\/a><\/td>A&A<\/td>2014<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XV. A study of anomalous microwave emission in Galactic clouds<\/a><\/td>A&A<\/td>2013<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust<\/a><\/td>A&A<\/td>2015<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XIV. Dust emission at millimetre wavelengths in the Galactic plane<\/a><\/td>A&A<\/td>2013<\/td>Planck<\/td>\n<\/tr>\n
Planck intermediate results. XIII. Constraints on peculiar velocities<\/a><\/td>A&A<\/td>2013<\/td>Planck<\/td>\n<\/tr>\n
UCSB HEMT-ACME South Pole 1990-91 Results <\/a><\/td>ANYAS<\/td>1993<\/td>ACME<\/td>\n<\/tr>\n
Transient Optical Sky Survey Automated Telescope System<\/a><\/td>SPIE<\/td>2008<\/td>TOSS<\/td>\n<\/tr>\n
The White Mountain Polarimeter Telescope and an Upper Limit on Cosmic Microwave Background Polarization <\/a><\/td>ApJ<\/td>2008<\/td>WMPol<\/td>\n<\/tr>\n
The UCSB Remote Access Telescope Project <\/a><\/td>WS<\/td>1992<\/td>RAAP<\/td>\n<\/tr>\n
The UCSB Remote Access Astronomy Project: Image Processing for High School and Undergraduate Students<\/a><\/td>Abstract, AAS Conference <\/td>1993<\/td>RAAP<\/td>\n<\/tr>\n
The UCSB Remote Access Astronomy Project<\/a><\/td>ASP<\/td>1992<\/td>RAAP<\/td>\n<\/tr>\n
The Temperature of the Cosmic Microwave Background at 10 GHz<\/a><\/td>ApJ<\/td>2004<\/td>ARCADE, CMB<\/td>\n<\/tr>\n
The Temperature of the Cosmic Microwave Background at 3mm<\/a><\/td>AAS<\/td>1995<\/td>CMB<\/td>\n<\/tr>\n
The Remote Access Astronomy Project<\/a><\/td>Proceedings, ASP Conference <\/td>1996<\/td>RAAP<\/td>\n<\/tr>\n
The remote access astronomy project: an example of a university-high school cooperative effort<\/a><\/td>EC<\/td>1992<\/td>RAAP<\/td>\n<\/tr>\n
The PLANCK LFI Radiometer - Prototype Results<\/a><\/td>ALC<\/td>2000<\/td>Planck<\/td>\n<\/tr>\n
The Origin of the Universe as Revealed Through the Polarization of the Cosmic Microwave Background<\/a><\/td>AADS<\/td>2009<\/td>CMB<\/td>\n<\/tr>\n
The Optical Design of the Background Emission Anisotropy Scanning Telescope<\/a> <\/td>ApJ<\/td>2005<\/td>BEAST<\/td>\n<\/tr>\n
The Millimeter Wave Anisotropy Experiment (MAX)<\/a><\/td>ALC<\/td>1995<\/td>MAX<\/td>\n<\/tr>\n
The Gamma Ray Arcminute Telescope Imaging System (GRATIS): detector performance and imaging<\/a><\/td>SPIE<\/td>1989<\/td>GRATIS<\/td>\n<\/tr>\n
The gamma-ray arc-minute imaging system (GRATIS): mechanical design and expected performance<\/a><\/td>SPIE<\/td>1989<\/td>GRATIS<\/td>\n<\/tr>\n
The Dipole Observed in the COBE DMR 4 Year Data<\/a><\/td>ApJ<\/td>1996<\/td>COBE<\/td>\n<\/tr>\n
The Cosmic Microwave Background Temperature and Galactic Emission at 8.0 and 8.3 GHz<\/a><\/td>ApJ<\/td>2006<\/td>CMB<\/td>\n<\/tr>\n
The Cosmic Microwave Background Anisotropy Power Spectrum from the BEAST Experiment <\/a><\/td>ApJ<\/td>2005<\/td>BEAST<\/td>\n<\/tr>\n
The Cosmic Foreground Explorer A balloon-borne microwave polarimeter to characterize polarized foregrounds<\/a><\/td>SD<\/td>2006<\/td>COFE<\/td>\n<\/tr>\n
The Cosmic Background Radiation Anisotropy Program at UCSB<\/a><\/td>WS<\/td>1992<\/td>CBR<\/td>\n<\/tr>\n
The Cosmic Background Explorer - color<\/a><\/td>Scientific American<\/td>1990<\/td>COBE<\/td>\n<\/tr>\n
The Cosmic Background Explorer <\/a><\/td>Scientific American<\/td>1990<\/td>COBE<\/td>\n<\/tr>\n
The cosmic background explorer satellite (COBE) <\/a><\/td>FINAL<\/td>1988<\/td>COBE<\/td>\n<\/tr>\n
The cosmic background explorer satellite (COBE) <\/a><\/td>DRAFT<\/td>1988<\/td>COBE<\/td>\n<\/tr>\n
The Cosmic Background Explorer Mission<\/a><\/td><\/td>1989<\/td>COBE<\/td>\n<\/tr>\n
The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background. I. Limits and Detections<\/a><\/td>ApJ<\/td>1998<\/td>COBE<\/td>\n<\/tr>\n
The Background Emission Anisotropy Scanning Telescope (BEAST) Instrument Description and Performances<\/a><\/td>ApJ<\/td>2005<\/td>BEAST<\/td>\n<\/tr>\n
The ARCADE 2 Instrument<\/a><\/td>ApJ<\/td>2011<\/td>ARCADE<\/td>\n<\/tr>\n
The Advanced Cosmic Microwave Explorer: A Millimeter-wave Telescope and Stabilized Platform<\/a><\/td>ApJ<\/td>1993<\/td>CBR<\/td>\n<\/tr>\n
Structure of the COBE DMR First year maps<\/a><\/td>ApJL<\/td>1992<\/td>COBE<\/td>\n<\/tr>\n
Structure in the COBE Differential Microwave Radiometer First-Year Maps<\/a><\/td>ApJ<\/td>1992<\/td>COBE<\/td>\n<\/tr>\n
Status of the COBE satellite <\/a><\/td>Abstract, AAS Conference<\/td>1990<\/td>COBE<\/td>\n<\/tr>\n
Spotlight on the Sun <\/a><\/td>AstroNotes<\/td>1993<\/td>RAAP<\/td>\n<\/tr>\n
Southern Hemisphere Measurements of the Anisotropy in the Cosmic Microwave Background Radiation<\/a><\/td>ApJ<\/td>1979<\/td>CMB<\/td>\n<\/tr>\n
South Pole Studies of the Anisotropy of the Cosmic Background Radiation at One Degree<\/a><\/td>AIP<\/td>1989<\/td>CBR<\/td>\n<\/tr>\n
Sonifying the Cosmic Microwave Background<\/a><\/td>Proceedings, ICAD Conference <\/td>2011<\/td>CMB<\/td>\n<\/tr>\n
Small-Scale Anisotropies: The Final Frontier <\/a><\/td>The Physics Teach<\/td>1998<\/td>CMB<\/td>\n<\/tr>\n
Search for Unresolved Sources in the COBE-DMR Two-Year Sky Maps <\/a><\/td>ApJ<\/td>1994<\/td>COBE<\/td>\n<\/tr>\n
Search for Linear Polarization of the Cosmic Background Radiation<\/a><\/td>PRL<\/td>1979<\/td>CBR<\/td>\n<\/tr>\n
Search for Fluctuations in the Cosmic Background Radiation <\/a><\/td>Conference Proceedings, International School of Physics \"Enrico Fermi\"<\/td>1987<\/td>CBR<\/td>\n<\/tr>\n
Science Projects Seeking Dissemination Sites<\/a><\/td>CUE<\/td>1992<\/td>RAAP<\/td>\n<\/tr>\n
Results from the Third Flight of the Millimeter-Wave Anisotropy Experiment<\/a><\/td>ANYAS<\/td>1993<\/td>MAX<\/td>\n<\/tr>\n
Results from the COBE DMR Instrument at Six Months After Launch<\/a><\/td>Abstract, AAS Conference <\/td>1990<\/td>COBE<\/td>\n<\/tr>\n
Probing Reionization with Intensity Mapping of Molecular and Fine Structure Lines<\/a><\/td>ApJ<\/td>2011<\/td><\/td>\n<\/tr>\n
Preliminary Spectral Observations of the Galaxy with a 7 Degree Beam by the Cosmic Background Explorer (COBE)<\/a><\/td>ApJ<\/td>1991<\/td>COBE<\/td>\n<\/tr>\n
Preliminary Results from the Third Flight of the Millimeter Anisotropy Experiment (MAX)<\/a><\/td>PNAS<\/td>1993<\/td>MAX<\/td>\n<\/tr>\n
Preliminary Results from the COBE Differential Microwave Radiometers: Large Angular Scale Isotropy of the Cosmic Microwave Background<\/a><\/td>ApJ<\/td>1991<\/td>COBE<\/td>\n<\/tr>\n
Preliminary Millimeter and Sub-Millimeter COBE Observations of the Milky Way Galaxy with a 7 degree Beam<\/a><\/td>Conference Abstract<\/td>1990<\/td>COBE<\/td>\n<\/tr>\n
Precision Measurements of the CMB Power Spectrum<\/a><\/td>Conference Proceedings<\/td>1997<\/td>CMB<\/td>\n<\/tr>\n
Polarization of the Cosmic Background Radiation<\/a><\/td>ApJ<\/td>1981<\/td>CBR<\/td>\n<\/tr>\n
Planck pre-launch status: The Planck mission <\/a><\/td>A&A<\/td>2010<\/td>Planck<\/td>\n<\/tr>\n
Planck pre-launch status: The Planck-LFI programme<\/a><\/td>A&A<\/td>2010<\/td>Planck<\/td>\n<\/tr>\n
Planck pre-launch status : Design and description of the Low Frequency Instrument<\/a><\/td>A&A<\/td>2010<\/td>Planck<\/td>\n<\/tr>\n
Planck Low Frequency Instrument<\/a><\/td>ESA Proposal<\/td>1998<\/td>Planck<\/td>\n<\/tr>\n
Planck Intermediate Results. IX. Detection of the Galactic haze with Planck<\/a><\/td>A&A<\/td>2012<\/td>Planck<\/td>\n<\/tr>\n
Planck early results. XXV. Thermal dust in nearby molecular clouds<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Planck early results. XXIII. The first all-sky survey of Galactic cold clumps<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Planck early results. XXI. Properties of the interstellar medium in the Galactic plane<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Planck early results. XX. New light on anomalous microwave emission from spinning dust grains<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Planck early results. XVII. Origin of the submillimetre excess dust emission in the Magellanic Clouds<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Planck early results. XVI. The Planck view of nearby galaxies<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Planck early results. XV. Spectral energy distributions and radio continuum spectra of northern extragalactic radio sources<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Planck early results. XIX. All-sky temperature and dust optical depth from Planck and IRAS. Constraints on the dark gas in our Galaxy<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Planck early results. XIV. ERCSC validation and extreme radio sources<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Planck early results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Planck early results. VII. The Early Release Compact Source Catalogue<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Planck early results. IX. XMM-Newton follow-up for validation of Planck cluster candidates<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Planck early results. III. First assessment of the Low Frequency Instrument in-flight performance<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Planck early results. II. The thermal performance of Planck<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Planck early results. I. The Planck mission<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Planck early results. Dust in the diffuse interstellar medium and the Galactic halo<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Planck early results XVIII - The power spectrum of cosmic infrared background anisotropies<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Planck early results XII - Cluster Sunyaev-Zeldovich optical scaling relations<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Planck early results X - Statistical analysis of Sunyaev-Zeldovich scaling relations for X-ray galaxy clusters<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Planck early results VIII - The all-sky early Sunyaev-Zeldovich cluster sample<\/a><\/td>A&A<\/td>2011<\/td>Planck<\/td>\n<\/tr>\n
Plack-LFI - instrument design and ground calibration strategy<\/a><\/td>EUMA<\/td>2005<\/td>Planck<\/td>\n<\/tr>\n
On Determining the Spectrum of Primordial Inhomogeneity from the COBE DMR Sky Maps Results of Two-Year Data Analysis<\/a><\/td>ApJ<\/td>1994<\/td>COBE<\/td>\n<\/tr>\n
OLIMPO - A few arcmin resolution survey of the sky at mm and sub-mm wavelengths<\/a><\/td>SAIt Conference Proceedings<\/td>2003<\/td>OLIMPO<\/td>\n<\/tr>\n
OLIMPO - a balloon-borne, arcminute-resolution survey of the sky at mm and sub-mm wavelengths<\/a><\/td>ESA Conference Proceedings<\/td>2003<\/td>OLIMPO<\/td>\n<\/tr>\n
Observing the Primeval Explosion with the Cosmic Background Explorer Satellite (COBE)<\/a> <\/td>Conference Abstract<\/td>1984<\/td>COBE<\/td>\n<\/tr>\n
Observing the Evolution of the Universe<\/a><\/td>Supplemental Paper<\/td>2009<\/td>CMB<\/td>\n<\/tr>\n
Observations of the Large Scale Anisotropy in the Cosmic Background Radiation at 3 mm<\/a><\/td>Astrophysics Conference Proceedings<\/td>1984<\/td>CBR<\/td>\n<\/tr>\n
Noise performance of a cryogenically cooled 94-GHz InP MMIC amplifier and radiometer<\/a><\/td>SPIE<\/td>1996<\/td><\/td>\n<\/tr>\n
Mountaintop Calibration and Balloon Flight of Antiproton and Antihelium Search<\/a><\/td>IUPAP Proceedings<\/td>1979<\/td><\/td>\n<\/tr>\n
Modeling the frequency response of microwave radiometers with QUCS<\/a><\/td>JINST<\/td>2010<\/td><\/td>\n<\/tr>\n
Modeling and Control of a Balloon Borne Stabilized Platform<\/a><\/td>ASME<\/td>1990<\/td><\/td>\n<\/tr>\n
Model Reference Adaptive Control for the Azimuth-Pointing System of a Balloon-Borne Stabilized Platform<\/a><\/td>IJAC<\/td>1991<\/td><\/td>\n<\/tr>\n
Medium Scale Measurements of the Cosmic Microwave Background at 3.3 mm<\/a><\/td>Conference Proceedings<\/td>1989<\/td>CBR<\/td>\n<\/tr>\n
Medium scale CBR Anisotropy Measurements: UCSB South Pole HEMT (1990-91) and MAX 3 (1991)<\/a><\/td>LNP<\/td>1994<\/td>HEMT<\/td>\n<\/tr>\n
Measurements of the Millimeter-wave Spectrum of Interstellar Dust Emission - ApJ - 1995<\/a><\/td>ApJ<\/td>1995<\/td><\/td>\n<\/tr>\n
Measurements of the Cosmic Background Radiation<\/a><\/td>Reidel<\/td>1986<\/td>CBR<\/td>\n<\/tr>\n
Measurements of the Anisotropy of the Cosmic Background Radiation at 0.5 deg Scale Near the Star MU Pegasi <\/a><\/td>ApJ<\/td>1993<\/td><\/td>\n<\/tr>\n
Measurements of anisotropy in the cosmic microwave background radiation at degree angular scales near the stars Sigma Herculis and IOTA Draconis <\/a><\/td>ApJ<\/td>1994<\/td><\/td>\n<\/tr>\n
Measurements of Anisotropy in the Cosmic Microwave Background Radiation at 0.5 Scales near the Stars HR5127 and phi Herculis <\/a><\/td>ApJ<\/td>1996<\/td><\/td>\n<\/tr>\n
Measurements of Anisotropy in the Cosmic Microwave Background Radiation at 0.5 Degree Angular Scales Near the Star Gamma Ursae Minoris<\/a><\/td>ApJL<\/td>1994<\/td><\/td>\n<\/tr>\n
MAX, A Millimeter-Wave Anisotropy Experiment to Search for Anisotropy in the Cosmic Background Radiation on Intermediate Angular Scales<\/a><\/td>WS<\/td>1992<\/td>MAX<\/td>\n<\/tr>\n
MAX Searches for Intermediate-Scale Anisotropy of the Cosmic Microwave Background<\/a><\/td>IPT<\/td>1994<\/td>CMB<\/td>\n<\/tr>\n
Low Frequency Spectrum of Cosmic Background Radiation<\/a><\/td>AAS Conference Abstract<\/td>1979<\/td>CBR<\/td>\n<\/tr>\n
Long-Term Multiwavelength Observations of GRS 1758-258 and the Advection-dominated Accretion Flow Model<\/a><\/td>ApJ<\/td>2001<\/td>GRATIS<\/td>\n<\/tr>\n
Linear and Circular Polarization of the Cosmic Background Radiation <\/a><\/td>ApJ<\/td>1983<\/td>CBR<\/td>\n<\/tr>\n
Limits on Three-Point Correlations in the COBE DMR First-Year Anisotropy Maps<\/a><\/td>ApJ<\/td>1994<\/td>COBE<\/td>\n<\/tr>\n
Limits on Cold Dark Matter Models from Recent Measurements of the Cosmic Backround Radiation <\/a><\/td>AAS Conference Abstract<\/td>1990<\/td>HEMT<\/td>\n<\/tr>\n
Limits on Cold Dark Matter Models from Recent Anisotropy Measurements of the Cosmic Background Radiation<\/a><\/td>Conference Abstract<\/td>1991<\/td>CBR<\/td>\n<\/tr>\n
Limits on Cold Dark Matter Cosmologies from New Anisotropy Bounds on the Cosmic Microwave Background<\/a><\/td>ApJ<\/td>1991<\/td>CMB<\/td>\n<\/tr>\n
Large Scale Structures in the Background Radiation<\/a><\/td>TRA<\/td>1986<\/td>CBR<\/td>\n<\/tr>\n
Large scale structure in the background radiation<\/a><\/td>Conference Proceedings<\/td>1987<\/td>CBR<\/td>\n<\/tr>\n
Large-scale anisotropy of the cosmic background radiation at 3 mm<\/a><\/td>Conference Proceedings<\/td>1986<\/td>CBR<\/td>\n<\/tr>\n
Large Scale Anisotropy in the Cosmic Background Radiation at 3mm<\/a><\/td>Conference Abstract<\/td>1983<\/td>CBR<\/td>\n<\/tr>\n
Interpretation of the cosmic microwave background radiation anisotropy detected by the COBE Differential Microwave Radiometer<\/a><\/td>ApJ<\/td>1992<\/td>COBE<\/td>\n<\/tr>\n
Interpretation of the ARCADE 2 Absolute Sky Brightness Measurement<\/a><\/td>ApJ<\/td>2011<\/td>ARCADE<\/td>\n<\/tr>\n
Imaging the Cosmic Microwave Background: The BEAST Experiment<\/a><\/td>AIP<\/td>2000<\/td>BEAST<\/td>\n<\/tr>\n
GRATIS: Pointing and Tracking System<\/a><\/td>AAS Conference Abstract<\/td>1992<\/td>GRATIS<\/td>\n<\/tr>\n
Gaussian Statistics of the Cosmic Microwave Background: Correlation of Temperature Extrema in the COBE DMR Two-Year Sky Maps<\/a><\/td>ApJ<\/td>1995<\/td>COBE<\/td>\n<\/tr>\n
Galactic Foreground Contribution to the BEAST CMB Anisotropy Maps<\/a><\/td>ApJ<\/td>2004<\/td>BEAST<\/td>\n<\/tr>\n
Future prospects in measuring the CMB power spectrum<\/a><\/td>Conference Proceedings<\/td>1997<\/td>COBE<\/td>\n<\/tr>\n
First Results of the COBE Satellite Measurement of the Anisotropy of the Cosmic Microwave Background Radiation<\/a><\/td>ASR<\/td>1991<\/td>COBE<\/td>\n<\/tr>\n
Far-Infrared Spectral Observations of the Galaxy by COBE<\/a><\/td>ApJ<\/td>1995<\/td>COBE<\/td>\n<\/tr>\n
Experimental Investigation of the Planck LFI Receiver Design: Results from a 44 GHz Prototype Receiver<\/a><\/td>Conference Proceedings<\/td>1998<\/td>Planck<\/td>\n<\/tr>\n
Early Results from the Cosmic Background Explorer COBE<\/a><\/td>ASR<\/td>1991<\/td>COBE<\/td>\n<\/tr>\n
Direct Imaging of the CMB from Space<\/a><\/td>ApJ<\/td>1996<\/td>CMB<\/td>\n<\/tr>\n
Dipole Anisotropy in the COBE Differential Microwave Radiometers First-Year Sky Maps<\/a><\/td>ApJ<\/td>1993<\/td>COBE<\/td>\n<\/tr>\n
Detection of Degree Scale Anisotropy<\/a><\/td>STSCL<\/td>1993<\/td>CBR<\/td>\n<\/tr>\n
Design and performance of sliced-aperture corrugated feed horn antennas<\/a><\/td>RSI<\/td>2005<\/td>ARCADE<\/td>\n<\/tr>\n
Design and calibration of a cryogenic blackbody calibrator at centimeter wavelengths<\/a><\/td>RSI<\/td>2004<\/td>ARCADE<\/td>\n<\/tr>\n
Degree-Scale Anisotropy Present Status and Future Possibilities<\/a><\/td>ALC<\/td>1995<\/td>CBR<\/td>\n<\/tr>\n
Degree-scale anisotropy in the cosmic microwave background SP94 results<\/a><\/td>ApJ<\/td>1995<\/td>CMB<\/td>\n<\/tr>\n
Degree Scale Anisotropy: Current Status<\/a><\/td>IAU<\/td>1996<\/td>COBE<\/td>\n<\/tr>\n
Cosmology: A Research Briefing<\/a><\/td>NRC<\/td>1995<\/td><\/td>\n<\/tr>\n
Cosmic Temperature Fluctuations from Two Years of COBE Differential Microwave Radiometers Observations<\/a><\/td>ApJ<\/td>1994<\/td>COBE<\/td>\n<\/tr>\n
Cosmic-Structure Constraints from a One-Degree Microwave-Background Anisotropy Experiment<\/a><\/td>PRL<\/td>1991<\/td><\/td>\n<\/tr>\n
Cosmic-Ray Age and A Measurement of the Abundance of BE-10 Using a Magnetic Spectrometer<\/a><\/td>ICRC<\/td>1977<\/td><\/td>\n<\/tr>\n
Cosmic Microwave Background Maps from the HACME Experiment<\/a><\/td>ApJ<\/td>2000<\/td>HACME<\/td>\n<\/tr>\n
Cosmic Microwave Background Anisotropy at One Degree - ACME HEMT 1990-91 South Pole Results<\/a><\/td>APS<\/td>1993<\/td>CMB<\/td>\n<\/tr>\n
Cosmic Background Radiation Research in 1988<\/a><\/td>McGraw-Hill<\/td>1990<\/td>CBR<\/td>\n<\/tr>\n
Cosmic Background Radiation Anisotropy at Degree Angular Scales: Further Results from the South Pole<\/a><\/td>ApJ<\/td>1993<\/td>CBR<\/td>\n<\/tr>\n
Cosmic Background Radiation Anisotropy at 1.5 Degrees<\/a><\/td>AAS Conference Abstract<\/td>1993<\/td>ACME<\/td>\n<\/tr>\n
Cosmic Background Anisotropy Studies at 10 Degree Angular Scales with a HEMT Radiometer<\/a><\/td>AIP<\/td>1989<\/td>CBR<\/td>\n<\/tr>\n
Cosmic background anisotropy measurement at 10 degrees<\/a><\/td>AJUS<\/td>1989<\/td>CBR<\/td>\n<\/tr>\n
COMPASS - An Upper Limit on Cosmic Microwave Background Polarization at an Angular Scale of 20 <\/a><\/td>ApJ<\/td>2004<\/td>CMB<\/td>\n<\/tr>\n
COMPASS - An Instrument for Measuring the Polarization of the CMB on Intermediate Angular Scales<\/a><\/td>Conference Proceedings<\/td>2003<\/td>CMB<\/td>\n<\/tr>\n
COMPASS: A 2.6 m telescope for CMBR polarization studies <\/a><\/td>AIP<\/td>2002<\/td>COMPASS<\/td>\n<\/tr>\n
Comments on the statistical analysis of excess variance in the COBE differential microwave radiometer maps<\/a><\/td>ApJ<\/td>1994<\/td>COBE<\/td>\n<\/tr>\n
COBE Differential Microwave Radiometers: Instrument design and implementation<\/a><\/td>ApJ<\/td>1990<\/td>COBE<\/td>\n<\/tr>\n
COBE Differential Microwave Radiometers: Calibration Techniques<\/a><\/td>ApJ<\/td>1992<\/td>COBE<\/td>\n<\/tr>\n
COBE Differential Microwave Radiometers: Calibration Techniques<\/a><\/td>ApJ<\/td>1992<\/td>COBE<\/td>\n<\/tr>\n
CMB anisotropy measurements during the fourth flight of MAX<\/a><\/td>WS<\/td>1995<\/td>MAX<\/td>\n<\/tr>\n
Calibration of the Far Infrared Absolute Spectrophotometer(FIRAS) for the Cosmic Background Explorer Satellite<\/a><\/td><\/td>1990<\/td>COBE<\/td>\n<\/tr>\n
Balloon Borne Molecular Oxygen Search: SIS Spectrometer<\/a><\/td>AIP<\/td>1992<\/td>SIS<\/td>\n<\/tr>\n
ARCADE: Absolute radiometer for cosmology, astrophysics, and diffuse emission<\/a><\/td>SD<\/td>2006<\/td>ARCADE<\/td>\n<\/tr>\n
ARCADE 2 Observations of Galactic Radio Emission<\/a><\/td>ApJ<\/td>2011<\/td>ARCADE<\/td>\n<\/tr>\n
ARCADE 2 Measurement of the Absolute Sky Brightness at 3-90 GHz<\/a><\/td>ApJ<\/td>2011<\/td>ARCADE<\/td>\n<\/tr>\n
Antiproton and Antihelium Search<\/a><\/td>ICRC<\/td>1979<\/td><\/td>\n<\/tr>\n
Anisotropy Measurements of the Cosmic Microwave Background<\/a><\/td>AIP<\/td>1994<\/td>CMB<\/td>\n<\/tr>\n
Anisotropy measurements of the cosmic background radiation from the South Pole at 1 degree<\/a><\/td>AJUS<\/td>1989<\/td><\/td>\n<\/tr>\n
Anisotropy in the Cosmic Microwave Background: Present Status-Future Directions<\/a><\/td>EF<\/td>1995<\/td>CMB<\/td>\n<\/tr>\n
Angular Power Spectrum of the Microwave Background Anisotropy Seen by the COBE Differential Microwave Radiometer<\/a><\/td>ApJ<\/td>1994<\/td>COBE<\/td>\n<\/tr>\n
Angular power spectrum of the FASTICA cosmic microwave background component from Background Emission Anisotropy Scanning Telescope data<\/a><\/td>MNRAS<\/td>2006<\/td>CMB<\/td>\n<\/tr>\n
An Instrument to Measure the Temperature of the Cosmic Microwave Background Radiation at Centimeter Wavelengths<\/a><\/td>ApJ<\/td>2004<\/td>CMB<\/td>\n<\/tr>\n
An astronomical site survey at the Barcroft Facility of the White Mountain Research Station<\/a><\/td>SD<\/td>2006<\/td>WMPol<\/td>\n<\/tr>\n
An Alternative Algorithm for Cosmic Microwave Background Radiation Sky Harmonic Analysis<\/a><\/td>Conference Abstract<\/td>1994<\/td>CMB<\/td>\n<\/tr>\n
Advanced Pseudo Correlation Radiometers for the Planck-LFI Instrument<\/a><\/td>Conference Proceedings<\/td>2003<\/td>Planck<\/td>\n<\/tr>\n
A status report on max, a millimeter-wave anisotropy experiment to search for anisotropy in the cosmic background radiation on intermediate angular scales<\/a><\/td>WS<\/td>1992<\/td>CBR<\/td>\n<\/tr>\n
A Spin-Modulated Telescope to Make Two-Dimensional Cosmic Microwave Background Maps<\/a><\/td>ApJ<\/td>2000<\/td>CMB<\/td>\n<\/tr>\n
A Simple Test for Non-Gaussianity in Cosmic Microwave Background Radiation Measurements<\/a><\/td>ApJ<\/td>1995<\/td>CMB<\/td>\n<\/tr>\n
A search for anisotropy in the cosmic microwave background on intermediate angular scales<\/a><\/td>ApJ<\/td>1992<\/td>CMB<\/td>\n<\/tr>\n
A preliminary measurement of the cosmic microwave background spectrum by the Cosmic Background Explorer (COBE) satellite<\/a><\/td>ApJ<\/td>1990<\/td>COBE<\/td>\n<\/tr>\n
A Preliminary Analysis of UCSBs South Pole 1993-94 Results<\/a><\/td>WS<\/td>1995<\/td>CMB<\/td>\n<\/tr>\n
A New Technique of Searching for Cosmic-Ray Antiprotons and Antihelium<\/a><\/td>ICRC<\/td>1979<\/td><\/td>\n<\/tr>\n
A New Science Strategy for Space Astronomy and Astrophysics<\/a><\/td>SSB, NRC<\/td>1997<\/td><\/td>\n<\/tr>\n
A Modular 100-GHz High-Gain Scalar Corrugated Nonbonded Platelet Antenna<\/a><\/td>IEEE<\/td>2005<\/td>CMB<\/td>\n<\/tr>\n
A millimeter-wave anisotropy experiment (MAX) to search for anisotropy in the cosmic background radiation on medium angular scales<\/a><\/td>AIP<\/td>1990<\/td>MAX<\/td>\n<\/tr>\n
A medium-scale measurement of the cosmic microwave background at 3.3 millimeters<\/a><\/td>ApJ<\/td>1991<\/td>CMB<\/td>\n<\/tr>\n
A measurement of anisotropy of the cosmic background radiation at 1.5 degrees<\/a><\/td>DRAFT<\/td>1991<\/td>CBR<\/td>\n<\/tr>\n
A Map of the Cosmic Microwave Background from the BEAST Experiment<\/a><\/td>ApJ<\/td>2003<\/td>BEAST<\/td>\n<\/tr>\n
A map of the cosmic background radiation at 3 millimeters<\/a><\/td>ApJ<\/td>1985<\/td>CBR<\/td>\n<\/tr>\n
A hard X-ray spectrometer for high angular resolution observations of cosmic sources<\/a><\/td>LLNL<\/td>1988<\/td>LAXRIS<\/td>\n<\/tr>\n
A degree-scale measurement of anisotropy of the cosmic background radiation<\/a><\/td>ApJ<\/td>1992<\/td>CBR<\/td>\n<\/tr>\n
A degree-scale anisotropy measurement of the cosmic microwave background near the star Gamma Ursae Minoris<\/a><\/td>ApJ<\/td>1993<\/td>CMB<\/td>\n<\/tr>\n
A bolometric millimeter-wave system for observations of anisotropy in the cosmic microwave background radiation on medium angular scales <\/a><\/td>ApJ<\/td>1992<\/td>CMB<\/td>\n<\/tr>\n
A 100-GHz High-Gain Tilted Corrugated<\/a><\/td>IEEE<\/td>2005<\/td>BEAST<\/td>\n<\/tr>\n
A 31 Pixel Flared 100-GHz High-Gain Scalar Corrugated Nonbonded Platelet Antenna Array<\/a><\/td>IEEE<\/td>2005<\/td>CMB<\/td>\n<\/tr>\n
3 mm measurements of anisotropy in the cosmic background radiation<\/a><\/td>GC<\/td>1986<\/td>CBR<\/td>\n<\/tr>\n
3-mm Anisotropy Measurement and the Quadrupole Component in the Cosmic Background Radiation<\/a><\/td>PRL<\/td>1983<\/td>CBR<\/td>\n<\/tr>\n
1\/f noise and other systematic effects in the Planck-LFI radiometers<\/a><\/td>A&A<\/td>2002<\/td>Planck, CMB<\/td>\n<\/tr>\n
Planck intermediate results. XVIII. The millimetre and sub-millimetre emission from planetary nebulae <\/a><\/td>A&A<\/td>2015<\/td>Planck<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n\n
\n
\n
Latest Publications<\/h5>\n

ResearchGate – nearly complete list<\/a><\/p>\n

PLANCK satellite publications<\/a><\/p>\n

PLANCK satellite released data<\/a><\/p>\n<\/div>\n<\/div>\n","protected":false},"excerpt":{"rendered":"

Legend A&A — Astronomy & Astrophysics ApJ — The Astrophysical Journal ApJS — The Astrophysical Journal Supplemental Series EC — Education and Computing SD — Science Direct PASP — Publications of the Astronomical Society of the Pacific Latest Publications ResearchGate – nearly complete list PLANCK satellite publications PLANCK satellite released data<\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":8,"comment_status":"closed","ping_status":"closed","template":"","meta":[],"_links":{"self":[{"href":"http:\/\/128.111.23.62\/wordpress\/wp-json\/wp\/v2\/pages\/990"}],"collection":[{"href":"http:\/\/128.111.23.62\/wordpress\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"http:\/\/128.111.23.62\/wordpress\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"http:\/\/128.111.23.62\/wordpress\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"http:\/\/128.111.23.62\/wordpress\/wp-json\/wp\/v2\/comments?post=990"}],"version-history":[{"count":0,"href":"http:\/\/128.111.23.62\/wordpress\/wp-json\/wp\/v2\/pages\/990\/revisions"}],"wp:attachment":[{"href":"http:\/\/128.111.23.62\/wordpress\/wp-json\/wp\/v2\/media?parent=990"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}