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Wmap-Planck published presentations and documents on DocSlides.

Glenn Starkman
Glenn Starkman
by celsa-spraggs
Dept. of Physics/CERCA/ISO. Case Western Reserve ...
COBE and WMAP
COBE and WMAP
by kimberly
Zhuo ChengSupervisors Yi Mao and Jianfeng Zhou1Out...
What does the
What does the
by celsa-spraggs
Cosmic Microwave Background . tell us about our o...
Planck 2013 results, implications for cosmology
Planck 2013 results, implications for cosmology
by cheryl-pisano
Michele Liguori. Department of Physics and Astron...
Max Planck Institute
Max Planck Institute
by alexa-scheidler
for. Innovation . and. . Competition. | . Muni...
Glenn D. Starkman
Glenn D. Starkman
by jane-oiler
Craig . Copi. , . Dragan. . Huterer. & . Do...
An Uncooperative Universe:
An Uncooperative Universe:
by conchita-marotz
. . . large scale . a. nomalies. . in ....
I Neutrini in Cosmologia
I Neutrini in Cosmologia
by cheryl-pisano
Alessandro ...
Trispectrum
Trispectrum
by alexa-scheidler
Estimator of Primordial Perturbation in Equilate...
Kontakt: Max-Planck-Institut fü KohlenforschungSarah-Lena Gombert, Pr
Kontakt: Max-Planck-Institut fü KohlenforschungSarah-Lena Gombert, Pr
by wilson
LembkestraßeBismarkstraßeZeppelin-straßeDimbeck...
Cosmological constraints
Cosmological constraints
by reportcetic
f. rom . tSZ. -X cross-correlation. G.Hurier. Why....
Space environment and detection : lessons learned from
Space environment and detection : lessons learned from
by sandsomber
PLANCK/HFI. François PAJOT. . Institut d'Astrop...
Close Cycle Dilution for
Close Cycle Dilution for
by test
Space. Ph. Camus, . G. . Vermeulen, G. . Chaudhry...
Jan Hamann Rencontres de
Jan Hamann Rencontres de
by alida-meadow
Moriond. (Cosmology). 21. st. March 2016. Curre...
GEOGG141
GEOGG141
by calandra-battersby
Principles & Practice of Remote Sensing (PPRS...
Atomic Structure and Periodicity
Atomic Structure and Periodicity
by jane-oiler
Advanced Chemistry. Ms. . Grobsky. Food For Thoug...
Cosmic Microwave Background
Cosmic Microwave Background
by trish-goza
&. Primordial Gravitational Waves. Jun-Qing X...
Max-Planck-Institutf
Max-Planck-Institutf
by tatyana-admore
Max-Planck-Institutf
CMB large angular scale, full sky polarization anisotropy h
CMB large angular scale, full sky polarization anisotropy h
by luanne-stotts
The value of . reionization. fraction derived fr...
Neoclassical tests and large scale structure in quasi-linea
Neoclassical tests and large scale structure in quasi-linea
by debby-jeon
Uro. Å¡. . Seljak. UC Berkeley/LBNL. Dec 18. 2...
Theoretical
Theoretical
by cheryl-pisano
Challenges. . in the Post-Planck . Era. Scott Do...
Chapter 1 Thermal radiation and Planck’s postulate
Chapter 1 Thermal radiation and Planck’s postulate
by lois-ondreau
FUNDAMENTAL CONCEPTS OF QUANTUM PHYSICS. . Therm...
Planck Cosmology 2015
Planck Cosmology 2015
by tawny-fly
The nearly exact degeneracy -- i.e., nearly the s...
Understanding Leveraging
Understanding Leveraging
by sophie
Demand VariabilityRick BlairWho am IRick BlairVP I...
0 2 4 6 8 10 12 13.8
0 2 4 6 8 10 12 13.8
by tatiana-dople
billions of years after creation. CMB temperature...
NEUTRINO PHYSICS FROM
NEUTRINO PHYSICS FROM
by pamella-moone
COSMOLOGY. EVIDENCE FOR NEW PHYSICS?. STEEN . HA...
Removing foregrounds from CMB maps using non-
Removing foregrounds from CMB maps using non-
by cheryl-pisano
Gaussianity. measurement. Dr. . Rajib. . Saha. ...
Fifty Years of CMB Anisotropy Experiments (and Theory)
Fifty Years of CMB Anisotropy Experiments (and Theory)
by karlyn-bohler
….in 15 Minutes. Bruce Partridge. Haverford Col...
Anisotropies of Cosmic
Anisotropies of Cosmic
by tatiana-dople
Microwave . Background. and Its Polarization . A ...
Cosmology : Cosmic Microwave Background
Cosmology : Cosmic Microwave Background
by cheryl-pisano
& Large scale structure. Tarun So...
What is the solar system cosmically aligned
What is the solar system cosmically aligned
by liane-varnes
universe’s expansion WMAP 380,000 years after...
WMAP Ka-band (33 GHz)
WMAP Ka-band (33 GHz)
by pamella-moone
Synchrotron spectral indexWMAP Haze (courtesy Raji...
PIPER: Primordial Inflation Polarization Explorer
PIPER: Primordial Inflation Polarization Explorer
by lindy-dunigan
Jeffrey Hatef. Mentor: Dr. Alan . Kogut. Inflatio...
Primordial black hole formation
Primordial black hole formation
by trish-goza
in an . axion. -like . curvaton. model. 北嶋ç›...
TheVacuumWhatdowemeanbyVoid,Vacuum,Emptyness?Aconceptthatplaysacrucial
TheVacuumWhatdowemeanbyVoid,Vacuum,Emptyness?Aconceptthatplaysacrucial
by natalia-silvester
SolutionsofEinstein'sequationinvacuumcanhavedi ere...
Cosmology : Cosmic Microwave Background
Cosmology : Cosmic Microwave Background
by briana-ranney
& Large scale structure. Tarun So...
Max-Planck-Institut für extraterrestrische Physik and Halbleiterlabor, Germany
Max-Planck-Institut für extraterrestrische Physik and Halbleiterlabor, Germany
by jainy
Space Sciences Lab., UC Berkeley, USA. CNES. , Tou...
Perfecting Complex Assemblies of Covalent and Supramolecular Polymers via Biological Principles
Perfecting Complex Assemblies of Covalent and Supramolecular Polymers via Biological Principles
by eddey
DMR 2104554. 2021 Intellectual Merit. Virgil. . ...
Fermi/LAT observations of Dwarf Galaxies highly constrain a Dark Matter interpretation of Excess Po
Fermi/LAT observations of Dwarf Galaxies highly constrain a Dark Matter interpretation of Excess Po
by jocelyn
DPF 2015 – University of Michigan, Ann Arbor. . ...
[READ] - The Theory of Heat Radiation by Max Planck
[READ] - The Theory of Heat Radiation by Max Planck
by HoldenMclean
This is a reproduction of a book published before ...