436 Rosat PPTs View free & download

Autor: Rosate Descarga ofrecida por: www.prevention-world.com PowerPoint PPT Presentation

Autor: Rosate Descarga ofrecida por: www.prevention-world.com - Title: Presentaci n General Author: RICARDO ZAMBRANO Last modified by: Enrique Ruiz Atilano Created Date: 7/2/1998 11:10:18 PM Document presentation format

Title: Presentaci n General Author: RICARDO ZAMBRANO Last modified by: Enrique Ruiz Atilano Created Date: 7/2/1998 11:10:18 PM Document presentation format

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Instrument: ROSAT PSPC - Instrument: ROSAT PSPC

Instrument: ROSAT PSPC

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Autor: Rosate Descarga ofrecida por: www'preventionworld'com - Rojo cero: No es combustible. Amarillo cero: No es reactivo. Blanco OXY: Es ... debe estar l mpio de materiales combustibles o que representen peligro de fuego ...

Rojo cero: No es combustible. Amarillo cero: No es reactivo. Blanco OXY: Es ... debe estar l mpio de materiales combustibles o que representen peligro de fuego ...

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Solar wind charge exchange and the ROSAT skymaps PowerPoint PPT Presentation

Solar wind charge exchange and the ROSAT skymaps - New sky-map. Background subtracted. 3/4 keV band ... Movie. Final ... be improved by observations from the Moon or other place outside the bow shock. ...

New sky-map. Background subtracted. 3/4 keV band ... Movie. Final ... be improved by observations from the Moon or other place outside the bow shock. ...

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Discrepancy between average WMAP observed and ROSAT predicted SunyaevZel'dovich Effect profiles of 3 PowerPoint PPT Presentation

Discrepancy between average WMAP observed and ROSAT predicted SunyaevZel'dovich Effect profiles of 3 - Discrepancy between average WMAP observed and ROSAT predicted Sunyaev-Zel'dovich ... The S-Z effect may be probe of cluster non-thermal processes, not cosmology. ...

Discrepancy between average WMAP observed and ROSAT predicted Sunyaev-Zel'dovich ... The S-Z effect may be probe of cluster non-thermal processes, not cosmology. ...

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Constraints%20on%20Neutron%20Star%20Cooling%20using%20Chandra%20Observations%20of%20PSR%20B1509-58,%20PSR%20B1951 32,%20and%20RX%20J0007.0 7303 - London, 27 Apr 2006. 1. Constraints on Neutron Star Cooling using Chandra ... EGRET. Pulsations observed with ROSAT and EGRET with periods matching the radio solution ...

London, 27 Apr 2006. 1. Constraints on Neutron Star Cooling using Chandra ... EGRET. Pulsations observed with ROSAT and EGRET with periods matching the radio solution ...

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EXIST Concept for BHFP: Hard X-ray Black Hole Surveys in Space and Time PowerPoint PPT Presentation

EXIST Concept for BHFP: Hard X-ray Black Hole Surveys in Space and Time - Hard X-ray (10-600 keV) sky not yet surveyed to ROSAT sensitivity. ... Zenith pointer - scanning & nodding for full-sky coverage each orbit (95min) ...

Hard X-ray (10-600 keV) sky not yet surveyed to ROSAT sensitivity. ... Zenith pointer - scanning & nodding for full-sky coverage each orbit (95min) ...

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Degeneracy - White dwarf in X-ray from ROSAT The gas (mostly hydrogen) in the accretion disk, obtained from the companion star, may fall into the white dwarf, ...

White dwarf in X-ray from ROSAT The gas (mostly hydrogen) in the accretion disk, obtained from the companion star, may fall into the white dwarf, ...

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Texas in Florence PowerPoint PPT Presentation

Texas in Florence - Radio - X ray comparison. Connection between the existence of ... in hard X ray ... IC emission in soft X ray band possibly detected from ROSAT in A85 ...

Radio - X ray comparison. Connection between the existence of ... in hard X ray ... IC emission in soft X ray band possibly detected from ROSAT in A85 ...

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The 6dF Galaxy Redshift Survey: Status Report and Data Release 2 PowerPoint PPT Presentation

The 6dF Galaxy Redshift Survey: Status Report and Data Release 2 - The 6dF Galaxy Redshift Survey: Status Report and Data Release 2. Heath ... Galaxy ... SuperCosmos galaxy catalogs. ROSAT All-Sky Survey (RASS) HI Parkes Sky ...

The 6dF Galaxy Redshift Survey: Status Report and Data Release 2. Heath ... Galaxy ... SuperCosmos galaxy catalogs. ROSAT All-Sky Survey (RASS) HI Parkes Sky ...

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A Review of Magnetic Activity in Sunlike stars PowerPoint PPT Presentation

A Review of Magnetic Activity in Sunlike stars - (from Patten and Simon 1996) Pobs=0.527 d. Photometric ... (from Patten and Simon 1996) Stars in open cluster 2391 (30My old) RX from ROSAT observations ...

(from Patten and Simon 1996) Pobs=0.527 d. Photometric ... (from Patten and Simon 1996) Stars in open cluster 2391 (30My old) RX from ROSAT observations ...

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P1252428529vaeWs PowerPoint PPT Presentation

P1252428529vaeWs - ... energies from X-ray to radio, and including images, object lists, and ... Chandra X-ray image (SAO/CXC) USC/ISI. ROSAT image (GSFC/HEASARC) UW-Madison/NCSA ...

... energies from X-ray to radio, and including images, object lists, and ... Chandra X-ray image (SAO/CXC) USC/ISI. ROSAT image (GSFC/HEASARC) UW-Madison/NCSA ...

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Why is the BAT survey for AGN Important? PowerPoint PPT Presentation

Why is the BAT survey for AGN Important? - BAT survey should be unbiased wrt obscuration ... The Rosat and BAT fluxes are not correlated. The follow-up to the BAT data shows us why: in many objects the ...

BAT survey should be unbiased wrt obscuration ... The Rosat and BAT fluxes are not correlated. The follow-up to the BAT data shows us why: in many objects the ...

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An XMMNewton observation of the variable Seyfert 1 galaxy 1H 0419577 PowerPoint PPT Presentation

An XMMNewton observation of the variable Seyfert 1 galaxy 1H 0419577 - ... observed by ASCA, ROSAT, BeppoSAX and XMM-Newton over recent years) and is one ... XMM-Newton observed 1H 0419-577 in December 2000. ...

... observed by ASCA, ROSAT, BeppoSAX and XMM-Newton over recent years) and is one ... XMM-Newton observed 1H 0419-577 in December 2000. ...

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XMM-Newton slew sources A quick analysis PowerPoint PPT Presentation

XMM-Newton slew sources A quick analysis - Median exposure time: ~6.2 seconds (min ~ 1s, max~12s) Images roughly 1 degree by 0.5 degree ... eslewchain (create images, exposure maps) emask (area for ...

Median exposure time: ~6.2 seconds (min ~ 1s, max~12s) Images roughly 1 degree by 0.5 degree ... eslewchain (create images, exposure maps) emask (area for ...

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A Multiwavelength Study of the Supernova Remnant W28 PowerPoint PPT Presentation

A Multiwavelength Study of the Supernova Remnant W28 - A Multiwavelength Study of the Supernova Remnant W28. Jonathan Keohane ... Tom Pannuti (SSC) Kazik Borkowski (NC State) Frank Winkler (Middlebury) H alpha. S II ...

A Multiwavelength Study of the Supernova Remnant W28. Jonathan Keohane ... Tom Pannuti (SSC) Kazik Borkowski (NC State) Frank Winkler (Middlebury) H alpha. S II ...

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Persistent%20and%20Transient%20Blank%20Field%20Sources PowerPoint PPT Presentation

Persistent%20and%20Transient%20Blank%20Field%20Sources - Persistent and Transient Blank Field Sources A. Treves Insubria University, Italy S. Campana Brera Observatory, Italy M. Chieregato Insubria University, Italy ...

Persistent and Transient Blank Field Sources A. Treves Insubria University, Italy S. Campana Brera Observatory, Italy M. Chieregato Insubria University, Italy ...

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Extending aOX Studies to Include the Numerous Low-to-Moderate Luminosity AGNs PowerPoint PPT Presentation

Extending aOX Studies to Include the Numerous Low-to-Moderate Luminosity AGNs - Extending aOX Studies to Include the Numerous Low-to-Moderate Luminosity ... inverse-Compton scattering off of energetic electrons in optically thin corona. ...

Extending aOX Studies to Include the Numerous Low-to-Moderate Luminosity ... inverse-Compton scattering off of energetic electrons in optically thin corona. ...

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This image shows the plane of our Galaxy in infrared light. The thin disk of our home spiral galaxy is clearly apparent, with stars appearing white and interstellar dust appearing red. - This image shows the plane of our Galaxy in infrared light' The thin disk of our home spiral galaxy

This image shows the plane of our Galaxy in infrared light' The thin disk of our home spiral galaxy

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Holger Stiele - Holger Stiele

Holger Stiele

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Gamma Ray Antimatter PowerPoint PPT Presentation

Gamma Ray Antimatter - It is probably about 4,000 light-years across and extends nearly 3,500 light ... Credit: W. Purcell (NWU) et al. The Search for Dark Matter ...

It is probably about 4,000 light-years across and extends nearly 3,500 light ... Credit: W. Purcell (NWU) et al. The Search for Dark Matter ...

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The Hot ISM - The Hot ISM K.D.Kuntz The Henry Rowland Dept. of Physics The Johns Hopkins University and NASA/LHEA

The Hot ISM K.D.Kuntz The Henry Rowland Dept. of Physics The Johns Hopkins University and NASA/LHEA

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X-rays from Elliptical Galaxies PowerPoint PPT Presentation

X-rays from Elliptical Galaxies - X-rays from Elliptical Galaxies. Ross Collins. with. Ewan O'Sullivan (CfA) ... Virgocentric flow corrected recession velocity vrec 10,500 km s-1 ...

X-rays from Elliptical Galaxies. Ross Collins. with. Ewan O'Sullivan (CfA) ... Virgocentric flow corrected recession velocity vrec 10,500 km s-1 ...

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XMM-NEWTON scientific instruments PowerPoint PPT Presentation

XMM-NEWTON scientific instruments - EPIC - imaging and spectroscopy at 0.2 - 10 keV. ERMS - particle detector. OM - optical/UV imaging at 1.9 ... Largest X-ray ccd detector ever built (36 cm^2) ...

EPIC - imaging and spectroscopy at 0.2 - 10 keV. ERMS - particle detector. OM - optical/UV imaging at 1.9 ... Largest X-ray ccd detector ever built (36 cm^2) ...

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Supersoft X-ray Sources in M31 in Be binaries? An astronomical game of PowerPoint PPT Presentation

Supersoft X-ray Sources in M31 in Be binaries? An astronomical game of - Characterized by very soft emission - no flux at energies 1 keV ... Unerstanding whether they are the 'single degenerate' progenitors of type Ia SN is crucial ...

Characterized by very soft emission - no flux at energies 1 keV ... Unerstanding whether they are the 'single degenerate' progenitors of type Ia SN is crucial ...

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Cosmology: The Sunyaev-Zeldovich effect and large-scale structure of the Universe from the perspective of the CMB - Cosmology: The SunyaevZeldovich effect and largescale structure of the Universe from the perspective

Cosmology: The SunyaevZeldovich effect and largescale structure of the Universe from the perspective

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The%20Fainting%20of%20Alpha%20Centauri%20A,%20Resolved!%20T.%20R.%20Ayres%20(CASA),%20and%20friends PowerPoint PPT Presentation

The%20Fainting%20of%20Alpha%20Centauri%20A,%20Resolved!%20T.%20R.%20Ayres%20(CASA),%20and%20friends - The Alpha Centauri triple system has two solar-like stars separated by about Sun ... and divided by reference traces-- WD at longer wavelengths, AGN at shorter ...

The Alpha Centauri triple system has two solar-like stars separated by about Sun ... and divided by reference traces-- WD at longer wavelengths, AGN at shorter ...

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1927?,???, - Title: Author: quasar Last modified by: sunych Created Date: 9/30/2003 2:18:25 AM Document presentation format:

Title: Author: quasar Last modified by: sunych Created Date: 9/30/2003 2:18:25 AM Document presentation format:

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An Introduction to X-ray Astronomy PowerPoint PPT Presentation

An Introduction to X-ray Astronomy - Produces highest spatial resolution images. Also best time resolution (but be careful) ... High resolution spectroscopy on extended objects that are larger than 10 ...

Produces highest spatial resolution images. Also best time resolution (but be careful) ... High resolution spectroscopy on extended objects that are larger than 10 ...

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G - Gnther Hasinger, MPE Garching

Gnther Hasinger, MPE Garching

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PowerPoint Presentation - Presentaci PowerPoint PPT Presentation

PowerPoint Presentation - Presentaci - Title: PowerPoint Presentation - Presentaci n de PowerPoint Author: Margarida Hernanz Last modified by: Margarita Hernanz Carb Created Date

Title: PowerPoint Presentation - Presentaci n de PowerPoint Author: Margarida Hernanz Last modified by: Margarita Hernanz Carb Created Date

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CBI Observations of the Sunyaev-Zeldovich Effect PowerPoint PPT Presentation

CBI Observations of the Sunyaev-Zeldovich Effect - National Radio Astronomy Observatory. Socorro, NM. Patricia Udomprasert, and the CBI Team ... Discovered 1965 (Penzias & Wilson) 2.7 K blackbody. Isotropic ...

National Radio Astronomy Observatory. Socorro, NM. Patricia Udomprasert, and the CBI Team ... Discovered 1965 (Penzias & Wilson) 2.7 K blackbody. Isotropic ...

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M. Dadina: XMM-Newton PowerPoint PPT Presentation

M. Dadina: XMM-Newton - Highlights: The first large X-ray telescope with mirrors. Einstein made the first X-ray images of shock waves in supernova remnants, hot ...

Highlights: The first large X-ray telescope with mirrors. Einstein made the first X-ray images of shock waves in supernova remnants, hot ...

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Young active star research with SONG and mini-SONG PowerPoint PPT Presentation

Young active star research with SONG and mini-SONG - Young active star research with SONG and mini-SONG Huijuan Wang National Astronomical Observatories Chinese Academy of Sciences @ Charleston *

Young active star research with SONG and mini-SONG Huijuan Wang National Astronomical Observatories Chinese Academy of Sciences @ Charleston *

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An Introduction to X-ray Astronomy - An Introduction to X-ray Astronomy Keith Arnaud NASA Goddard University of Maryland X-ray Astronomy X-ray Processes X-rays from the Sun X-ray Binaries All-Sky Surveys ...

An Introduction to X-ray Astronomy Keith Arnaud NASA Goddard University of Maryland X-ray Astronomy X-ray Processes X-rays from the Sun X-ray Binaries All-Sky Surveys ...

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Soft X-ray emission in Parkes Quasars. PowerPoint PPT Presentation

Soft X-ray emission in Parkes Quasars. - M.Whiting1, R.Webster1, P.Francis2. ... Parkes quasars are known to be reddened. (Webster et al. 1995, Nature,375, 469 ; Francis et al. 1999, PASA, in prep. ...

M.Whiting1, R.Webster1, P.Francis2. ... Parkes quasars are known to be reddened. (Webster et al. 1995, Nature,375, 469 ; Francis et al. 1999, PASA, in prep. ...

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Multiwavelength spectroscopy of high accretion rate polars PowerPoint PPT Presentation

Multiwavelength spectroscopy of high accretion rate polars - Multiwavelength spectroscopy of high accretion rate polars. Axel Schwope ... NONE of the 'classical bright polars was observed in a high accretion state ...

Multiwavelength spectroscopy of high accretion rate polars. Axel Schwope ... NONE of the 'classical bright polars was observed in a high accretion state ...

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An Introduction to X-ray Astronomy - High resolution spectroscopy by two gratings that can be placed in the optical ... highest spatial resolution images. Also best time resolution (but be careful) ...

High resolution spectroscopy by two gratings that can be placed in the optical ... highest spatial resolution images. Also best time resolution (but be careful) ...

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High Energy Astronomy PowerPoint PPT Presentation

High Energy Astronomy - The Sun Makes History ... If it wasn't for the Sun, the Norse would probably have colonised America 500 ... energy processes in the Sun are best studied using ...

The Sun Makes History ... If it wasn't for the Sun, the Norse would probably have colonised America 500 ... energy processes in the Sun are best studied using ...

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Astronomy 496: Xray Astronomy PowerPoint PPT Presentation

Astronomy 496: Xray Astronomy - ... History of the X-ray Sky. Herbert Gursky (AS&E) detected Cyg ... Survey the sky for more sources. Sco X-1 was not understood, although its optical counterpart ...

... History of the X-ray Sky. Herbert Gursky (AS&E) detected Cyg ... Survey the sky for more sources. Sco X-1 was not understood, although its optical counterpart ...

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Collisional ISM Heating in PowerPoint PPT Presentation

Collisional ISM Heating in - M86 has very weak radio source, so AGN heating of ISM unlikely at present. Although extreme case, ISM easy to study in M86: should teach us about general ...

M86 has very weak radio source, so AGN heating of ISM unlikely at present. Although extreme case, ISM easy to study in M86: should teach us about general ...

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GSC2 Science Projects @ ESO PowerPoint PPT Presentation

GSC2 Science Projects @ ESO - GSC2 Science Projects @ ESO 7th GSC2 Meeting 2001 R.Mignani ESO

GSC2 Science Projects @ ESO 7th GSC2 Meeting 2001 R.Mignani ESO

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The Chandra Multi-wavelength Project (ChaMP) PowerPoint PPT Presentation

The Chandra Multi-wavelength Project (ChaMP) - The Chandra Multi-wavelength Project (ChaMP) PIs: Paul Green & Belinda Wilkes X-ray: Dong-Woo Kim Imaging: Rob Cameron, Wayne Barkhouse Spectroscopy: John Silverman

The Chandra Multi-wavelength Project (ChaMP) PIs: Paul Green & Belinda Wilkes X-ray: Dong-Woo Kim Imaging: Rob Cameron, Wayne Barkhouse Spectroscopy: John Silverman

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PowerPoint-Pr PowerPoint PPT Presentation

PowerPoint-Pr - Max-Planck-Institut f r ... The XMM-Newton/Chandra Era The XMM-Newton ... PowerPoint-Pr sentation Simulation of line profiles for ionized discs PowerPoint ...

Max-Planck-Institut f r ... The XMM-Newton/Chandra Era The XMM-Newton ... PowerPoint-Pr sentation Simulation of line profiles for ionized discs PowerPoint ...

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An Aqueye view of the Crab Pulsar PowerPoint PPT Presentation

An Aqueye view of the Crab Pulsar - X-ray: NASA/CXC/ASU/J.Hester et al.; Optical: NASA/ESA/ASU/J.Hester & A.Loll; ... orthogonal rotator. 6. Parameters of the Crab pulsar ...

X-ray: NASA/CXC/ASU/J.Hester et al.; Optical: NASA/ESA/ASU/J.Hester & A.Loll; ... orthogonal rotator. 6. Parameters of the Crab pulsar ...

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Group Evolution Multi-wavelength Survey (GEMS) PowerPoint PPT Presentation

Group Evolution Multi-wavelength Survey (GEMS) - Colour-Magnitude Relation and Fundamental Plane studies constrain the formation ... richness: = 4 galaxies within 3 magnitudes of the brightest galaxy ...

Colour-Magnitude Relation and Fundamental Plane studies constrain the formation ... richness: = 4 galaxies within 3 magnitudes of the brightest galaxy ...

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Joachim Tr - Radiation radius of the radio-quiet isolated. neutron star RX J1856-3754 ... HZ 43 Her, and Sirius B in the. wavelength band marked by the. dotted lines: ...

Radiation radius of the radio-quiet isolated. neutron star RX J1856-3754 ... HZ 43 Her, and Sirius B in the. wavelength band marked by the. dotted lines: ...

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J. E. Hibbard (NRAO), with: PowerPoint PPT Presentation

J. E. Hibbard (NRAO), with: - HCG 07 (N=4) VLA Archive. Vilchez & Iglesias-Paramo 1998. DefHI=0.64 ... HCG 16 (N=4 2) R-band. Halpha. IRAC. Optical HI. 24um. XMM. Verdes-Montenegro 2001 ...

HCG 07 (N=4) VLA Archive. Vilchez & Iglesias-Paramo 1998. DefHI=0.64 ... HCG 16 (N=4 2) R-band. Halpha. IRAC. Optical HI. 24um. XMM. Verdes-Montenegro 2001 ...

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The%20Sunyaev-Zeldovich%20Effect%20with%20ALMA%20Band%201 PowerPoint PPT Presentation

The%20Sunyaev-Zeldovich%20Effect%20with%20ALMA%20Band%201 - single dishes with bolometer camers. SPT, APEX, ACT, etc. or small interferometers ... fast bolometer array or interferometer. e.g. SPT,APEX,SZA,AMI. 23 ...

single dishes with bolometer camers. SPT, APEX, ACT, etc. or small interferometers ... fast bolometer array or interferometer. e.g. SPT,APEX,SZA,AMI. 23 ...

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The Xray LHB PowerPoint PPT Presentation

The Xray LHB - Transitions in O 7 produces lines labeled OVIII ... Bowyer et al.(1968), Henry et al.(1968), Bunner et al.(1968) The fundamental surveys: Wisconsin ...

Transitions in O 7 produces lines labeled OVIII ... Bowyer et al.(1968), Henry et al.(1968), Bunner et al.(1968) The fundamental surveys: Wisconsin ...

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