53 Cuspis PPTs View free & download

CUSPIS CAM Storyboard: OPD case PowerPoint PPT Presentation

CUSPIS CAM Storyboard: OPD case - MID TERM REVIEW. EXIT. CUSPIS CAM Storyboard: OPD case. ABU. TCU. CAM: ... MID TERM REVIEW. EXIT. CAM Phase4.1: Trasportation conclusion and receipt generation ...

MID TERM REVIEW. EXIT. CUSPIS CAM Storyboard: OPD case. ABU. TCU. CAM: ... MID TERM REVIEW. EXIT. CAM Phase4.1: Trasportation conclusion and receipt generation ...

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CUSPIS HMI aspects: User interfaces, Context awareness and 3D fruition PowerPoint PPT Presentation

CUSPIS HMI aspects: User interfaces, Context awareness and 3D fruition - Example: 3D Model of Temple of Isis, Pompei archeological site - Italy ... a museum, a large building, an archeological site, etc.) and to easily identify ...

Example: 3D Model of Temple of Isis, Pompei archeological site - Italy ... a museum, a large building, an archeological site, etc.) and to easily identify ...

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Mid Term Review PowerPoint PPT Presentation

Mid Term Review - to describe the CUSPIS Cultural Asset Fruition (CAF) demonstrator that will ... Photo material: by qualified photographers, experienced on the cultural assets ...

to describe the CUSPIS Cultural Asset Fruition (CAF) demonstrator that will ... Photo material: by qualified photographers, experienced on the cultural assets ...

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SRDCE - SRDCE Ventriculus sinister M tvar ku ele. V horn ,roz en sti je vtokov ostium atrioventriculare sinistrum a v tokov ostium aortae.

SRDCE Ventriculus sinister M tvar ku ele. V horn ,roz en sti je vtokov ostium atrioventriculare sinistrum a v tokov ostium aortae.

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Diapositive 1 PowerPoint PPT Presentation

Diapositive 1 - Boris Kennes Market Development European GNSS Supervisory Authority

Boris Kennes Market Development European GNSS Supervisory Authority

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MTR - CA univocal identification is a necessary service requirement to realize other applications. The pre-requirement for the univocal identification is a CA catalogue: ...

CA univocal identification is a necessary service requirement to realize other applications. The pre-requirement for the univocal identification is a CA catalogue: ...

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Celine B - Title: Slide 1 Author: celine boehm Last modified by: celine boehm Created Date: 7/18/2005 8:02:37 AM Document presentation format: On-screen Show Company

Title: Slide 1 Author: celine boehm Last modified by: celine boehm Created Date: 7/18/2005 8:02:37 AM Document presentation format: On-screen Show Company

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Cosmology with the GMRT PowerPoint PPT Presentation

Cosmology with the GMRT - Title: PowerPoint Presentation Last modified by: ncra Created Date: 1/1/1601 12:00:00 AM Document presentation format: On-screen Show Other titles

Title: PowerPoint Presentation Last modified by: ncra Created Date: 1/1/1601 12:00:00 AM Document presentation format: On-screen Show Other titles

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Dan Hooper - Prospects depend on both the characteristics of the dark matter particle and its ... (Draco, Sagittarius, etc.) Little is known for certain about the halo ...

Prospects depend on both the characteristics of the dark matter particle and its ... (Draco, Sagittarius, etc.) Little is known for certain about the halo ...

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Diapositiva 1 PowerPoint PPT Presentation

Diapositiva 1 - A. Sesana1, F. Haardt1, P. Madau2 The Final Parsec: Orbital Decay of Massive Black Holes in Galactic Stellar Cusps 1 Universita` dell'Insubria, via Valleggio 11 ...

A. Sesana1, F. Haardt1, P. Madau2 The Final Parsec: Orbital Decay of Massive Black Holes in Galactic Stellar Cusps 1 Universita` dell'Insubria, via Valleggio 11 ...

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Dark Matter, Dark Energy: puzzles - Dark Matter, Dark Energy: puzzles

Dark Matter, Dark Energy: puzzles

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Galaxy%20formation PowerPoint PPT Presentation

Galaxy%20formation - Galaxy formation

Galaxy formation

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Gamma-ray bursts and hypernovae PowerPoint PPT Presentation

Gamma-ray bursts and hypernovae - GRB as superstrong cosmic explosions. Association with supernovae a critical view ... HETE2: GRB-X-ray rich-XRF (Lamb et al. 2003) Apparently continuous. transition ...

GRB as superstrong cosmic explosions. Association with supernovae a critical view ... HETE2: GRB-X-ray rich-XRF (Lamb et al. 2003) Apparently continuous. transition ...

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Survival or disruption of CDM micro-haloes: implications for detection experiments PowerPoint PPT Presentation

Survival or disruption of CDM micro-haloes: implications for detection experiments - Survival or disruption of CDM micro-haloes: implications for detection ... after relaxation. Single encounter. c = 1.6. Varying impact parameter b. Arrow: rvir ...

Survival or disruption of CDM micro-haloes: implications for detection ... after relaxation. Single encounter. c = 1.6. Varying impact parameter b. Arrow: rvir ...

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Possible%20Dark%20Matter%20Signals%20from%20Antiprotons,%20Positrons,%20X-rays%20and%20%20Gamma-rays%20Ullrich%20Schwanke%20(Humboldt%20University,%20Berlin) - Right now, EGRET data (and more) can be described by scenarios with and without DM ... Explains EGRET data with a photon component from neutralino annihilation ...

Right now, EGRET data (and more) can be described by scenarios with and without DM ... Explains EGRET data with a photon component from neutralino annihilation ...

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Globular Cluters in Dwarf Galaxies PowerPoint PPT Presentation

Globular Cluters in Dwarf Galaxies - But, in fact, we do see both the clusters. and the field stars ... Clusters are not too interesting and are. observed only because they appear to ...

But, in fact, we do see both the clusters. and the field stars ... Clusters are not too interesting and are. observed only because they appear to ...

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Celine B - If DM is a fermion and coupled to heavy particles ... coupled to light particles (Z' ... Look like SUSY but relationship between the couplings and MF, ...

If DM is a fermion and coupled to heavy particles ... coupled to light particles (Z' ... Look like SUSY but relationship between the couplings and MF, ...

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Density Profile of Dark Matter Halos and Statistics of Strong Lensing - Statistics of strong gravitational lensing. Observational data. Conclusions. Future. Introduction ... In a concordant cosmology, how large is the core radius? ...

Statistics of strong gravitational lensing. Observational data. Conclusions. Future. Introduction ... In a concordant cosmology, how large is the core radius? ...

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Cosmology with the GMRT - Low and high resolution images of CH3CHO emission from SgrB2 made from a single ... Doppler shifts can be easily measured to high accuracy. ...

Low and high resolution images of CH3CHO emission from SgrB2 made from a single ... Doppler shifts can be easily measured to high accuracy. ...

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Search for Dark Matter The AMS-02 Experiment PowerPoint PPT Presentation

Search for Dark Matter The AMS-02 Experiment - ... magnet (BL2= 0.85 Tm2) Silicon Tracker (rigidity, charge) ... AMS on the International Space Station will provide enough statistics to perform a multi ...

... magnet (BL2= 0.85 Tm2) Silicon Tracker (rigidity, charge) ... AMS on the International Space Station will provide enough statistics to perform a multi ...

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Diapositiva 1 - MBHB M1 M2 on a Keplerian orbit with semimajor axis a and eccentricity e ... K is typically positive, but the eccentricity evoution of. the binary is modest ...

MBHB M1 M2 on a Keplerian orbit with semimajor axis a and eccentricity e ... K is typically positive, but the eccentricity evoution of. the binary is modest ...

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BoseEinstein Condensates as Galactic Dark Matter Halos Tonatiuh Matos, F' Siddhartha Guzman, Luis Ur PowerPoint PPT Presentation

BoseEinstein Condensates as Galactic Dark Matter Halos Tonatiuh Matos, F' Siddhartha Guzman, Luis Ur - Bose-Einstein Condensates as Galactic Dark Matter Halos ... Self-Annihilating DM. Repulsive DM. Fuzzy DM. Decaying DM. Scalar Field Dark Matter ...

Bose-Einstein Condensates as Galactic Dark Matter Halos ... Self-Annihilating DM. Repulsive DM. Fuzzy DM. Decaying DM. Scalar Field Dark Matter ...

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ASTR 540: Elliptical Galaxies PowerPoint PPT Presentation

ASTR 540: Elliptical Galaxies - `The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems' ... Lick Indices: Breaking Age/Metallicity Degeneracy. Age-s correlation? ...

`The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems' ... Lick Indices: Breaking Age/Metallicity Degeneracy. Age-s correlation? ...

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Observational Evidence for Extra Dimensions from Dark Matter PowerPoint PPT Presentation

Observational Evidence for Extra Dimensions from Dark Matter - mx 8 10-(25-22) cm2/GeV (Spergel & Steinhardt 2000, PRL) Nature of this self-interaction is unknown: Introduce a new interaction beyond the Standard Model? ...

mx 8 10-(25-22) cm2/GeV (Spergel & Steinhardt 2000, PRL) Nature of this self-interaction is unknown: Introduce a new interaction beyond the Standard Model? ...

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Dan Hooper - Excluded by EGRET. Excluded by HESS. GLAST Reach. GLAST Reach (neglecting BG) ... EGRET's galactic gamma ray spectrum. EGRET's extragalactic gamma ray spectrum ...

Excluded by EGRET. Excluded by HESS. GLAST Reach. GLAST Reach (neglecting BG) ... EGRET's galactic gamma ray spectrum. EGRET's extragalactic gamma ray spectrum ...

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Astrophysics and Cosmology with TeV gamma-rays - Astrophysics and Cosmology with TeV gammarays

Astrophysics and Cosmology with TeV gammarays

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Dwarf Dark Matter Halos in CDM cosmology : small scales, big problems PowerPoint PPT Presentation

Dwarf Dark Matter Halos in CDM cosmology : small scales, big problems - Open Questions in Dwarf Galaxy Formation. Is the 'missing satellites problem' still a problem? (can we reproduce dwarf galaxy numbers and spatial distribution? ...

Open Questions in Dwarf Galaxy Formation. Is the 'missing satellites problem' still a problem? (can we reproduce dwarf galaxy numbers and spatial distribution? ...

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Halos in a warm dark matter cosmology Astrophysical Probes of the Nature of Dark Matter, Irvine, Mar PowerPoint PPT Presentation

Halos in a warm dark matter cosmology Astrophysical Probes of the Nature of Dark Matter, Irvine, Mar - Q = ?/ v2 3/2 for collisionless particles Q can not increase. ... 3 halos. X same halo. Density profiles with vth (Avila-Reese et al. 2001) ...

Q = ?/ v2 3/2 for collisionless particles Q can not increase. ... 3 halos. X same halo. Density profiles with vth (Avila-Reese et al. 2001) ...

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Does dark matter really exist PowerPoint PPT Presentation

Does dark matter really exist - MOND in the MW. Tully-Fisher relation. HSB & LSB galaxies. Giant elliptical galaxies ... to DM, non-circular motions in (l,v) vanish (even shallow halo smoothes bumps) ...

MOND in the MW. Tully-Fisher relation. HSB & LSB galaxies. Giant elliptical galaxies ... to DM, non-circular motions in (l,v) vanish (even shallow halo smoothes bumps) ...

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AMS : A COSMIC RAY OBSERVATORY ON THE INTERNATIONAL SPACE STATION Carlo Bosio INFN Roma La Sapienza PowerPoint PPT Presentation

AMS : A COSMIC RAY OBSERVATORY ON THE INTERNATIONAL SPACE STATION Carlo Bosio INFN Roma La Sapienza - AMS : A COSMIC RAY OBSERVATORY. ON THE INTERNATIONAL SPACE ... Astrophysics/Cosmology dependence: 9/14/09. Carlo Bosio SUSY 04. 15. DM searches with positrons ...

AMS : A COSMIC RAY OBSERVATORY. ON THE INTERNATIONAL SPACE ... Astrophysics/Cosmology dependence: 9/14/09. Carlo Bosio SUSY 04. 15. DM searches with positrons ...

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Looking for signals from dark matter annihilation PowerPoint PPT Presentation

Looking for signals from dark matter annihilation - COS-B and EGRET (20keV~30GeV) observed diffuse gamma rays, measured its spectra. ... EGRET data requires the neutralino mass be in the range 40~50 GeV and DM ...

COS-B and EGRET (20keV~30GeV) observed diffuse gamma rays, measured its spectra. ... EGRET data requires the neutralino mass be in the range 40~50 GeV and DM ...

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EGRETs Excess of Diffuse Gamma Rays as Dark Matter Tracer PowerPoint PPT Presentation

EGRETs Excess of Diffuse Gamma Rays as Dark Matter Tracer - EGRET's Excess of Diffuse Gamma Rays. as Dark Matter Tracer. Pearl Sandick ... Whole halo contributes to diffuse ? ray intensity, but only diffusion region (R ...

EGRET's Excess of Diffuse Gamma Rays. as Dark Matter Tracer. Pearl Sandick ... Whole halo contributes to diffuse ? ray intensity, but only diffusion region (R ...

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Dan Hooper - Less dependent on understanding of halo profile, diffusion parameters ... (Draco, Sagittarius, etc.) Little is known for certain about the halo profiles of such ...

Less dependent on understanding of halo profile, diffusion parameters ... (Draco, Sagittarius, etc.) Little is known for certain about the halo profiles of such ...

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O ensino da - ... informando as compet ncias e habilidades esperadas dos alunos. Matriz de refer ncia de L ngua Portuguesa COMPREENDE o conjunto de habilidades previstas como ...

... informando as compet ncias e habilidades esperadas dos alunos. Matriz de refer ncia de L ngua Portuguesa COMPREENDE o conjunto de habilidades previstas como ...

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EGRETs Excess of Diffuse Gamma Rays as Dark Matter Tracer - Spectra 'optimized' to explain EGRET GeV excess without DM (does not work well ... scenarios that were compatible with both the BESS and EGRET measurements! ...

Spectra 'optimized' to explain EGRET GeV excess without DM (does not work well ... scenarios that were compatible with both the BESS and EGRET measurements! ...

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The Milky Way Galaxy PowerPoint PPT Presentation

The Milky Way Galaxy - Bulges and disks. We live at edge of disk. Disadvantage: structure obscured by 'dust' ... Radial migration leads to big spread in [Fe/H] at given age. Velocity ...

Bulges and disks. We live at edge of disk. Disadvantage: structure obscured by 'dust' ... Radial migration leads to big spread in [Fe/H] at given age. Velocity ...

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Dark Matter halos at galaxy scale PowerPoint PPT Presentation

Dark Matter halos at galaxy scale - DISK KINEMATICS. Sufue & Rubin 2001. DISK KINEMATICS. Decomposing luminosity. distribution of Andromeda Galaxy (Tenjes et al. 1994) ...

DISK KINEMATICS. Sufue & Rubin 2001. DISK KINEMATICS. Decomposing luminosity. distribution of Andromeda Galaxy (Tenjes et al. 1994) ...

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Astrophysical Constraints on Dark Matter Candidate PowerPoint PPT Presentation

Astrophysical Constraints on Dark Matter Candidate - Self gravitating system of collisionless particles with ... 2: substructure abundance. Moore et al. 1999, ApJ, 524, L19. Self-Interacting Dark Matter (SIDM) ...

Self gravitating system of collisionless particles with ... 2: substructure abundance. Moore et al. 1999, ApJ, 524, L19. Self-Interacting Dark Matter (SIDM) ...

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Indirect - ... y:z:{:|:}:~:: : : : : : : : : : : : : : : : : : : : : : : : : : : : : : :P : : : ... aSZ$J ) Rsv _u*H 3 c d_ aP~ 4g bk ] E gy zG ]~ Op ...

... y:z:{:|:}:~:: : : : : : : : : : : : : : : : : : : : : : : : : : : : : : :P : : : ... aSZ$J ) Rsv _u*H 3 c d_ aP~ 4g bk ] E gy zG ]~ Op ...

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CDM cusps in LSB galaxies by means of stellar kinematics PowerPoint PPT Presentation

CDM cusps in LSB galaxies by means of stellar kinematics - Long-slit spectroscopy (VLT/FORS2) VLT/IFU-VIMOS. Dynamical modeling ... Fit parameter using Metropolis algorithm. NOTE: no use of gas kinematics. minor axis ...

Long-slit spectroscopy (VLT/FORS2) VLT/IFU-VIMOS. Dynamical modeling ... Fit parameter using Metropolis algorithm. NOTE: no use of gas kinematics. minor axis ...

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The influence of baryons on the matter distribution and shape of dark matter halos PowerPoint PPT Presentation

The influence of baryons on the matter distribution and shape of dark matter halos - Dynamic Friction by sinking galaxies (El-Zant et al. ... Stellar mass dominate center part of clusters and groups of galaxies. ...

Dynamic Friction by sinking galaxies (El-Zant et al. ... Stellar mass dominate center part of clusters and groups of galaxies. ...

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Lars Bergstrm PowerPoint PPT Presentation

Lars Bergstrm - Enhanced flux possible thanks to halo density profile and substructure (as predicted by CDM) ... profile needed for DM substructure; some fine-tuning to get ...

Enhanced flux possible thanks to halo density profile and substructure (as predicted by CDM) ... profile needed for DM substructure; some fine-tuning to get ...

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GLAST Development Status, Science Opportunities - GLAST Development Status, Science Opportunities

GLAST Development Status, Science Opportunities

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Nessun titolo diapositiva PowerPoint PPT Presentation

Nessun titolo diapositiva - 2- too many satellites, 3- dwarf galaxies less clustered than bright ones ... (SDSS data); 3- galaxies along filaments in warm dark matter sims is probably ...

2- too many satellites, 3- dwarf galaxies less clustered than bright ones ... (SDSS data); 3- galaxies along filaments in warm dark matter sims is probably ...

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Observations of HIPASS radio galaxies with 6dF PowerPoint PPT Presentation

Observations of HIPASS radio galaxies with 6dF - HI mass function optical luminosity function. most baryonic mass in low surface ... HIPASS (HI) remaining fuel star formation future. failed star formation ...

HI mass function optical luminosity function. most baryonic mass in low surface ... HIPASS (HI) remaining fuel star formation future. failed star formation ...

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Will GLAST Identify Dark Matter PowerPoint PPT Presentation

Will GLAST Identify Dark Matter - ... Dark Matter ... variability tests would help identify local dark matter annihilation sources ... 4 - Sanchez-Conde, Miguel; Angel Dark matter in draco: new ...

... Dark Matter ... variability tests would help identify local dark matter annihilation sources ... 4 - Sanchez-Conde, Miguel; Angel Dark matter in draco: new ...

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Making Galaxies Red and Dead Without Feedback PowerPoint PPT Presentation

Making Galaxies Red and Dead Without Feedback - High mass and spatial resolution is a necessary condition in order to obtain ... High resolution SPH simulations without feedback produce normal, massive but ...

High mass and spatial resolution is a necessary condition in order to obtain ... High resolution SPH simulations without feedback produce normal, massive but ...

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Dynamics of substructures: On survivors and debris PowerPoint PPT Presentation

Dynamics of substructures: On survivors and debris - If radial and constant anisotropy: too fastly rising dispersion near the centre, ... the anisotropy has to be tangential. This is why NFW profiles require 0 ...

If radial and constant anisotropy: too fastly rising dispersion near the centre, ... the anisotropy has to be tangential. This is why NFW profiles require 0 ...

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The Physics of AMS02 PowerPoint PPT Presentation

The Physics of AMS02 - The Physics of AMS-02. Francesca Spada INFN Rome. on behalf of the ... P.Maestro, PhD thesis, 2003. Francesca Spada / INFN Rome The Physics of AMS-02. 15 ...

The Physics of AMS-02. Francesca Spada INFN Rome. on behalf of the ... P.Maestro, PhD thesis, 2003. Francesca Spada / INFN Rome The Physics of AMS-02. 15 ...

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Search for Dark Matter The AMS02 Experiment - For these and other benchmark scenarios, boost factors needed to fit HEAT data ... Center) visible signal in cuspy profile scenarios or other boost factors. ...

For these and other benchmark scenarios, boost factors needed to fit HEAT data ... Center) visible signal in cuspy profile scenarios or other boost factors. ...

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Folie 1 - ... with data from Integral, Egret, WMAP, Haslam, secondary CR production ... EGRET data set upper limit of few % on DMA contribution to synchrotron spectra, ...

... with data from Integral, Egret, WMAP, Haslam, secondary CR production ... EGRET data set upper limit of few % on DMA contribution to synchrotron spectra, ...

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physcol - physcol

physcol

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CHAPTERS 5 - Usually end in ase. Amylase = enzyme that catalyzes the. chemical digestion ... Icter (G) = an oriole. Jaune (F) = yellow. TERMS (Volvulus, Intussusception) ...

Usually end in ase. Amylase = enzyme that catalyzes the. chemical digestion ... Icter (G) = an oriole. Jaune (F) = yellow. TERMS (Volvulus, Intussusception) ...

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