Planck Collaboration
Planck observations of M33
... GHz. Planck has extracted the CMB over the whole sky using four different methods: SMICA, a non- parametric method that computes the CMB map by linearly combining all of the Planck maps with weights that ...
14
Planck 2015 results VI LFI mapmaking
... The Planck Collaboration acknowledges the support of: ESA; CNES, and CNRS / INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MINECO, ...the Planck ...
23
Planck 2015 results XXVIII The Planck catalogue of galactic cold clumps
... in Planck Collaboration XXIII ...the Planck sur- vey (353−857 GHz, 850−350μm) with the far-infrared IRAS (Neugebauer et ...Furthermore, Planck has provided the first uniform submillimetre ...
28
Planck 2015 results XX Constraints on inflation
... The Planck Collaboration acknowledges the support of: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); ...
65
Planck intermediate results XLIX Parity violation constraints from polarization data
... The Planck Collaboration acknowledges the support of: ESA; CNES, and CNRS / INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); ...
13
Planck 2015 results IV Low Frequency Instrument beams and window functions
... Max Planck Institute for Astrophysics Planck Analysis Centre (MPAC), funded by the Space Agency of the German Aerospace Center (DLR) under grant 50OP0901 with resources of the German Federal Ministry of ...
22
Planck intermediate results XXV. The Andromeda galaxy as seen by Planck
... (see Planck Collaboration Int. XV 2014; additionally Planck Collaboration XVII 2011 found a ratio of approximately 1:2000 for the Small Magellanic Cloud) and it is sensitive to dust ...
23
Planck 2015 results XV Gravitational lensing
... The Planck Collaboration acknowledges the support of: ESA; CNES and CNRS / INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); ...
28
Planck 2015 results XXVII The second Planck catalogue of Sunyaev Zeldovich sources
... (Planck Collaboration XII ...the Planck sky model (Planck Collaboration XII ...(Planck Collaboration XXVI 2016), and harmoni- cally infilled using the same process as for ...
38
Candidate high z proto clusters among the Planck compact sources, as revealed by Herschel SPIRE
... In our catalogue, for sources not assigned a counter- part, the median detection level in the PCCS and PCCS2 is 5.4 ± 0.5σ , near the detection threshold of 5σ (for our proto-clusters, this is similar at 5.4 ± 0.3σ ...
28
Planck 2015 results XIII Cosmological parameters
... (Planck Collaboration XXIV ...in Planck Collaboration XX (2014) we quantified with a “hydro- static bias” parameter, (1 − b), with a fiducial value of ...the Planck cluster ...entire ...
63
Planck intermediate results XLVII Planck constraints on reionization history
... The Thomson scattering of CMB photons o ff ionized elec- trons induces secondary anisotropies at di ff erent stages of the reionization process. In particular, we are interested here in the e ff ect of photons scattering ...
19
Planck 2015 results XVIII Background geometry and topology of the Universe
... 2006c; Bridges et al. 2007). Recall that the Bianchi densi- ties ( Ω B m and Ω B Λ ) are decoupled from the standard cosmol- ogy in the flat-decoupled-Bianchi model considered here and, as found previously, are ...
21
Planck 2015 results XXIV Cosmology from Sunyaev Zeldovich cluster counts
... in Planck Collaboration XX ...the Planck cat- alogue construction agree with each other and can be reasonably modelled by a simple analytical expression derived by assum- ing noise is the dominant ...
19
Planck 2015 results V LFI calibration
... nine Planck frequency channels is essential in component separation, where we disentangle the CMB from the vari- ous Galactic and extragalactic foreground emission processes (Planck Collaboration IX ...
24
Planck 2015 results XVI Isotropy and statistics of the CMB
... 2013 Planck data (Planck Collaboration XXVII ...the Planck full mission data set, though based only on the full ve- locity estimator (β), which is the sum of the modulation and the aberration ...
62
Planck intermediate results XLVI Reduction of large scale systematic effects in HFI polarization maps and estimation of the reionization optical depth
... (Planck Collaboration VIII 2016), but it solves simultaneously for absolute calibration, leakage of temperature into polarization, and various other sources of systematic er- ...final Planck data ...
52
Inertial effects in suspension dynamics
... With the inclusion of hydrodynamic interactions, the force field and diffusivity in the Fokker-Planck equation become complex functions of the particle configuration, making it extremely difficult to obtain an ...
294
Symmetry Analysis of the Fokker Planck Equation
... The Fokker-Planck equation (FPE, for short) is a linear PDE that describes the transition probability density of a Markov process. It is also known as the Kolmogorov diffusion equation and is used to model many ...
10
Planck Scale Gravity Test at PETRA
... A simple theoretical framework is established allowing to access extremely small distances in laboratory, pro- vided a vacuum refraction index growing with photon energy. Such vacuum is suggested by wide range of grav- ...
18