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HIFI: Submm Workshop, PowerPoint PPT Presentation
HIFI: Submm Workshop, - HIFI Heterodyne Instrument for the Far Infrared (The high resolution spectrometer for Herschel) Michel Fich
HIFI Heterodyne Instrument for the Far Infrared (The high resolution spectrometer for Herschel) Michel Fich
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High Resolution Submm Observations of Massive Protostars PowerPoint PPT Presentation
High Resolution Submm Observations of Massive Protostars - High Resolution Submm Observations of Massive Protostars Crystal Brogan (NRAO/NAASC) T. R. Hunter (NRAO), R. Indebetouw (UVa), Y. L. Shirley (U. of Arizona), C. J ...
High Resolution Submm Observations of Massive Protostars Crystal Brogan (NRAO/NAASC) T. R. Hunter (NRAO), R. Indebetouw (UVa), Y. L. Shirley (U. of Arizona), C. J ...
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Galaxy formation: radio through submm view PowerPoint PPT Presentation
Galaxy formation: radio through submm view - Galaxy formation: radio through submm view
Galaxy formation: radio through submm view
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HIFI: Submm Workshop, PowerPoint PPT Presentation
HIFI: Submm Workshop, - Formation and evolution of galaxies and clusters in the early universe ... studies of nearby resolvable galaxies. Cometary, planetary, and satellite atmospheres ...
Formation and evolution of galaxies and clusters in the early universe ... studies of nearby resolvable galaxies. Cometary, planetary, and satellite atmospheres ...
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Theoretical Motivation for Submm-VLBI of Sgr A* PowerPoint PPT Presentation
Theoretical Motivation for Submm-VLBI of Sgr A* - Dark matter particles: weakly interacting bosons and scalar fields may ... Can one form a central dark ... no solid surface ('boson sponge') and no horizon ...
Dark matter particles: weakly interacting bosons and scalar fields may ... Can one form a central dark ... no solid surface ('boson sponge') and no horizon ...
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AST 443: Submm PowerPoint PPT Presentation
AST 443: Submm - Visible, radio, & mm radiation reach the ground. Mm (1-3 mm) and submm ( 1 mm) ... In the Rayleigh-Jeans limit, hn / kT 1, the flux density is given by, ...
Visible, radio, & mm radiation reach the ground. Mm (1-3 mm) and submm ( 1 mm) ... In the Rayleigh-Jeans limit, hn / kT 1, the flux density is given by, ...
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Integrated Submm Receivers based on tunnel nanostructures PowerPoint PPT Presentation
Integrated Submm Receivers based on tunnel nanostructures - Kotel'nikov Institute of Radio Engineering and Electronics RAS ... TErahertz Limb Sounder (TELIS) TELIS Objectives: Measure many species for. atmospheric science ...
Kotel'nikov Institute of Radio Engineering and Electronics RAS ... TErahertz Limb Sounder (TELIS) TELIS Objectives: Measure many species for. atmospheric science ...
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New Astronomy Highlights from the Submm Spectroscopy Satellite Odin - PowerPoint PPT Presentation
New Astronomy Highlights from the Submm Spectroscopy Satellite Odin - - Orion KL spectral scan (Henrik Olofsson et al., Carina Persson et al., two A&A papers 2006) ... Pagani et al. 2006: 'First detection of molecular oxygen in ...
Orion KL spectral scan (Henrik Olofsson et al., Carina Persson et al., two A&A papers 2006) ... Pagani et al. 2006: 'First detection of molecular oxygen in ...
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ALMA Early Science: Submm Galaxies PowerPoint PPT Presentation
ALMA Early Science: Submm Galaxies - There are only ~200 SMGs in ALMA-accessible fields... Mix of detailed investigation of well-studied SMGs, detection of fainter pops ...
There are only ~200 SMGs in ALMA-accessible fields... Mix of detailed investigation of well-studied SMGs, detection of fainter pops ...
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AMI-LA radio continuum observations of low mass young stars: target sample for e-MERLIN legacy project PowerPoint PPT Presentation
AMI-LA radio continuum observations of low mass young stars: target sample for e-MERLIN legacy project - ... Class I: 70 3000 Ratio of Spitzer IRAC to submm emission F3.6/F850 0.003 A form of thermal ...
... Class I: 70 3000 Ratio of Spitzer IRAC to submm emission F3.6/F850 0.003 A form of thermal ...
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The use of PN precursors to study DIBs PowerPoint PPT Presentation
The use of PN precursors to study DIBs - ... the chemical composition of the dust grains (ISO, mm/submm, radio) ... ISO data in most cases; also from submm and/or radio observations) ... HD 183143. Pedro ...
... the chemical composition of the dust grains (ISO, mm/submm, radio) ... ISO data in most cases; also from submm and/or radio observations) ... HD 183143. Pedro ...
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Planetary Atmosphere With ALMA PowerPoint PPT Presentation
Planetary Atmosphere With ALMA - 3D mapping and monitoring: seasonal variations ... JCMT- Marten etal 04. Titan. Dense and cold : N2/CH4. mm/submm : CO and HCN ...
3D mapping and monitoring: seasonal variations ... JCMT- Marten etal 04. Titan. Dense and cold : N2/CH4. mm/submm : CO and HCN ...
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Overview of the 2 Ms CDF-N survey PowerPoint PPT Presentation
Overview of the 2 Ms CDF-N survey - Chandra Deep Field-North data. Source Redshifts. Diversity of X-ray selected sources ... Moderately deep Chandra surveys reported little overlap with the submm source ...
Chandra Deep Field-North data. Source Redshifts. Diversity of X-ray selected sources ... Moderately deep Chandra surveys reported little overlap with the submm source ...
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Radio Science and PILOT PowerPoint PPT Presentation
Radio Science and PILOT - Radio-IR Astrometry ... Radio/submm observations of the ISM can complement PILOT's capabilities, ... Large FOV facilitates astrometry with radio maps. ...
Radio-IR Astrometry ... Radio/submm observations of the ISM can complement PILOT's capabilities, ... Large FOV facilitates astrometry with radio maps. ...
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Superconducting THz Transmission Spectrometer Comprising Josephson Oscillator and Cold-Electron Bolometer PowerPoint PPT Presentation
Superconducting THz Transmission Spectrometer Comprising Josephson Oscillator and Cold-Electron Bolometer - Combination of a Terahertz-band Josephson junction and a hot electron bolometer brings a possibility to develop a quasioptical ... quasioptical submm wave grid ...
Combination of a Terahertz-band Josephson junction and a hot electron bolometer brings a possibility to develop a quasioptical ... quasioptical submm wave grid ...
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Magic%20of%20(sub)mm PowerPoint PPT Presentation
Magic%20of%20(sub)mm - Comparable SFR at high z in dusty starbursts ('submm gal') as ... Optical phot z. Radio phot z: (1 z) propto T_D. 20K. 60K. Z_rad, Z_opt(2) Z_opt (1) COSBO 7 ...
Comparable SFR at high z in dusty starbursts ('submm gal') as ... Optical phot z. Radio phot z: (1 z) propto T_D. 20K. 60K. Z_rad, Z_opt(2) Z_opt (1) COSBO 7 ...
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Radio multiobject spectrograph C. Carilli, NRAO, GBT new instrumentation workshop, Sept 06 PowerPoint PPT Presentation
Radio multiobject spectrograph C. Carilli, NRAO, GBT new instrumentation workshop, Sept 06 - 10's 100's galaxies per night. Slit positions pre-set based on optical/submm/radio/Xray imaging ... Selection with 1.4 GHz imaging gets 50% to 75% at 10's ...
10's 100's galaxies per night. Slit positions pre-set based on optical/submm/radio/Xray imaging ... Selection with 1.4 GHz imaging gets 50% to 75% at 10's ...
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Radio multiobject spectrograph C. Carilli, NRAO, GBT new instrumentation workshop, Sept 06 PowerPoint PPT Presentation
Radio multiobject spectrograph C. Carilli, NRAO, GBT new instrumentation workshop, Sept 06 - Need multiobject spectrograph for unbiased search for CO, other molecules in ... Submm gals: Dz_phot ~ 0.2 = ~2 GHz/source. Potentially trade-off of slits' for ...
Need multiobject spectrograph for unbiased search for CO, other molecules in ... Submm gals: Dz_phot ~ 0.2 = ~2 GHz/source. Potentially trade-off of slits' for ...
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Mm-Wave Interferometry Claire Chandler PowerPoint PPT Presentation
Mm-Wave Interferometry Claire Chandler - some of the problems are unique to the mm/submm, and affect the way ... In the Rayleigh-Jeans regime, hn ' kT, Sn = 2kTn2tnW Wm-2Hz-1. c2. dust opacity n2 ...
some of the problems are unique to the mm/submm, and affect the way ... In the Rayleigh-Jeans regime, hn ' kT, Sn = 2kTn2tnW Wm-2Hz-1. c2. dust opacity n2 ...
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Studying Protostellar and Debris Disks with BLISS PowerPoint PPT Presentation
Studying Protostellar and Debris Disks with BLISS - Dust continuum emission peaks in FIR/submm out to z 5 ... BICE Galactic maps of CII at very low spectral resolution (top) and dust emission (bottom) ...
Dust continuum emission peaks in FIR/submm out to z 5 ... BICE Galactic maps of CII at very low spectral resolution (top) and dust emission (bottom) ...
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Large grains in 7 classical RV Tauri stars PowerPoint PPT Presentation
Large grains in 7 classical RV Tauri stars - SCUBA 850 micron observations. TIMMI2 10 micron observations. Conclusions ... JCMT SCUBA 850 micron observations. To extend the SED to submm continuum emission ...
SCUBA 850 micron observations. TIMMI2 10 micron observations. Conclusions ... JCMT SCUBA 850 micron observations. To extend the SED to submm continuum emission ...
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The Obscured Growth Phase of Black Holes in Distant Massive Galaxies PowerPoint PPT Presentation
The Obscured Growth Phase of Black Holes in Distant Massive Galaxies - ... selection of the most bolometrically luminous far-IR galaxies in Universe ... Before SCUBA2, submm will miss hot ultraluminous sources. Hughes et al. (1998) ...
... selection of the most bolometrically luminous far-IR galaxies in Universe ... Before SCUBA2, submm will miss hot ultraluminous sources. Hughes et al. (1998) ...
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Atmospheric Transmission at DomeC between 0 and 10 THz PowerPoint PPT Presentation
Atmospheric Transmission at DomeC between 0 and 10 THz - Accurate modeling of terrestrial atmosphere is needed ... Many atmospheric models for mm- and submm exist, the most recent used. in ... ODIN satellite ...
Accurate modeling of terrestrial atmosphere is needed ... Many atmospheric models for mm- and submm exist, the most recent used. in ... ODIN satellite ...
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Herschel: An Introduction PowerPoint PPT Presentation
Herschel: An Introduction - Far-infrared and submm observatory in space. Much more sensitive than ground or airborne observatories ... Grating spectrograph disperses the light ...
Far-infrared and submm observatory in space. Much more sensitive than ground or airborne observatories ... Grating spectrograph disperses the light ...
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From PreStellar Cores to Protostars: The Initial Conditions of Star Formation PowerPoint PPT Presentation
From PreStellar Cores to Protostars: The Initial Conditions of Star Formation - Andre P., Ward-Thompson D., Barsony M., 2000, in Protostars and Planets IV, ... Introduction: Stages of low-mass ... SCUBA on JCMT (submm) IRAM (mm) 10/18/09 ...
Andre P., Ward-Thompson D., Barsony M., 2000, in Protostars and Planets IV, ... Introduction: Stages of low-mass ... SCUBA on JCMT (submm) IRAM (mm) 10/18/09 ...
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Probing the Highz Universe with GRB Multiwavelength Emission PowerPoint PPT Presentation
Probing the Highz Universe with GRB Multiwavelength Emission - From radio, submm, IR to GeV gamma-rays. 1. radio dispersion and ... Haddock & Sciama 65, Weinberg 72. Ginzburg 73, Palmer 93. H I. H II. zGRB. zreion. z= 0 ...
From radio, submm, IR to GeV gamma-rays. 1. radio dispersion and ... Haddock & Sciama 65, Weinberg 72. Ginzburg 73, Palmer 93. H I. H II. zGRB. zreion. z= 0 ...
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Exploring structure around submillimetre-bright QSOs PowerPoint PPT Presentation
Exploring structure around submillimetre-bright QSOs - Exploring structure around submillimetre-bright QSOs Francisco J. Carrera (IFCA, CSIC-UC, Spain/Imperial, UK) Mathew J. Page (MSSL-UCL, UK) Jason Stevens (CAR, U ...
Exploring structure around submillimetre-bright QSOs Francisco J. Carrera (IFCA, CSIC-UC, Spain/Imperial, UK) Mathew J. Page (MSSL-UCL, UK) Jason Stevens (CAR, U ...
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High Redshift Galaxies PowerPoint PPT Presentation
High Redshift Galaxies - High Redshift Galaxies
High Redshift Galaxies
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Continuum Observing PowerPoint PPT Presentation
Continuum Observing - Continuum Observing
Continuum Observing
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Blank PowerPoint PPT Presentation
Blank - Blank
Blank
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The Transient Radio Sky Astrophysical and Artificial PowerPoint PPT Presentation
The Transient Radio Sky Astrophysical and Artificial - ... disk surrounding a SMBH = coeval SMBH galaxy formation? ... M-s relation coeval SMBH and galaxy formation? QSO dust heating: star formation or AGN? ...
... disk surrounding a SMBH = coeval SMBH galaxy formation? ... M-s relation coeval SMBH and galaxy formation? QSO dust heating: star formation or AGN? ...
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MRI Molecular Imaging | MR Upgrade | In Vivo Imaging PowerPoint PPT Presentation
MRI Molecular Imaging | MR Upgrade | In Vivo Imaging - Mediso USA is a leading supplier of MRI Molecular Imaging. All Preclinical Imaging systems include the MultiCell small-animal handling systemsensuring efficient animal preparation, consistent anesthesia delivery, temperature control, and physiology monitoring. Contact us now at medisousa.com or call on +1.571.970.0738!
Mediso USA is a leading supplier of MRI Molecular Imaging. All Preclinical Imaging systems include the MultiCell small-animal handling systemsensuring efficient animal preparation, consistent anesthesia delivery, temperature control, and physiology monitoring. Contact us now at medisousa.com or call on +1.571.970.0738!
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The chemistry and stability of PowerPoint PPT Presentation
The chemistry and stability of - photosphere chromosphere. Vertical density. structure in a. flaring T Tauri disk ... scaled solar chromosphere IUE data stellar atmosphere model [Kamp ...
photosphere chromosphere. Vertical density. structure in a. flaring T Tauri disk ... scaled solar chromosphere IUE data stellar atmosphere model [Kamp ...
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The%20other%20side%20of%20galaxy%20formation:%20radio%20deep%20fields PowerPoint PPT Presentation
The%20other%20side%20of%20galaxy%20formation:%20radio%20deep%20fields - The other side of galaxy formation: radio deep fields
The other side of galaxy formation: radio deep fields
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Galaxy Formation and Evolution PowerPoint PPT Presentation
Galaxy Formation and Evolution - Galaxy Formation and Evolution
Galaxy Formation and Evolution
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EVIDENCE FOR A POPULATION OF HIGH REDSHIFT SUBMILLIMETER GALAXIES PowerPoint PPT Presentation
EVIDENCE FOR A POPULATION OF HIGH REDSHIFT SUBMILLIMETER GALAXIES - M. L. N. Ashby, M. A. Gurwell, K. Lai, A. B. Peck, G. Petitpas, D. Wilner (CfA) ... Younger, Dunlop, Peck, Ivison et al. [in prep.] MULTIWAVELENGTH COUNTERPARTS ...
M. L. N. Ashby, M. A. Gurwell, K. Lai, A. B. Peck, G. Petitpas, D. Wilner (CfA) ... Younger, Dunlop, Peck, Ivison et al. [in prep.] MULTIWAVELENGTH COUNTERPARTS ...
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1.4 GHz Source Counts (Hopkins 2000) PowerPoint PPT Presentation
1.4 GHz Source Counts (Hopkins 2000) - Relation to (sub)mm galaxies (Barger, Chapman, Blain, Dannerbauer, ... Temperature redshift degeneracy: measure (1 z)/T_D (Blain 1999) ...
Relation to (sub)mm galaxies (Barger, Chapman, Blain, Dannerbauer, ... Temperature redshift degeneracy: measure (1 z)/T_D (Blain 1999) ...
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ALMA: Imaging the cold Universe PowerPoint PPT Presentation
ALMA: Imaging the cold Universe - Coeval formation of SMBH/Galaxy? Dust formation by massive stars? ... coeval formation of SMBH/Galaxy? Break-down of M- relation at high z? ...
Coeval formation of SMBH/Galaxy? Dust formation by massive stars? ... coeval formation of SMBH/Galaxy? Break-down of M- relation at high z? ...
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Accretion onto the Supermassive Black Hole in our Galactic Center PowerPoint PPT Presentation
Accretion onto the Supermassive Black Hole in our Galactic Center - ... ambient conditions around BH Feeding the monster Stellar dynamics & star formation in Galactic Nuclei Useful laboratory for other ... Presentation Last ...
... ambient conditions around BH Feeding the monster Stellar dynamics & star formation in Galactic Nuclei Useful laboratory for other ... Presentation Last ...
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Physics 1A, Section 6 PowerPoint PPT Presentation
Physics 1A, Section 6 - OM Problem 9-69. Section Business. Final is 4 hour long. ... OM, Problem 3-62. Quiz Problem 33. Quiz Problem 33. Answer: a) = v/R. b) sin = kv/(mgR2) ...
OM Problem 9-69. Section Business. Final is 4 hour long. ... OM, Problem 3-62. Quiz Problem 33. Quiz Problem 33. Answer: a) = v/R. b) sin = kv/(mgR2) ...
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ATACAMA PowerPoint PPT Presentation
ATACAMA - ATACAMA CCAT : The Cornell-Caltech Atacama Telescope A joint project of Cornell University, the California Institute of Technology and the Jet Propulsion Laboratory
ATACAMA CCAT : The Cornell-Caltech Atacama Telescope A joint project of Cornell University, the California Institute of Technology and the Jet Propulsion Laboratory
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Introduction to mm-wave astronomy PowerPoint PPT Presentation
Introduction to mm-wave astronomy - Introduction to mmwave astronomy
Introduction to mmwave astronomy
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Scientific requirements of ALMA, and its capabilities for key-projects: extragalactic PowerPoint PPT Presentation
Scientific requirements of ALMA, and its capabilities for key-projects: extragalactic - Current millimeter interferometers have collecting areas between 500 and 1000 m2. ... plateau at 5000m altitude is superior to all existing mm observatories. ...
Current millimeter interferometers have collecting areas between 500 and 1000 m2. ... plateau at 5000m altitude is superior to all existing mm observatories. ...
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ALMA and distant galaxies PowerPoint PPT Presentation
ALMA and distant galaxies - ALMA and distant galaxies
ALMA and distant galaxies
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Massive galaxy (and black hole) formation in the early Universe PowerPoint PPT Presentation
Massive galaxy (and black hole) formation in the early Universe - Fine structure lines: dominant ISM gas coolant ... Index = 1. FIR -- HCN = linear relation from GMCs to HyLIRGs ... Rapid enrichment of metals, dust in ISM (z 8) ...
Fine structure lines: dominant ISM gas coolant ... Index = 1. FIR -- HCN = linear relation from GMCs to HyLIRGs ... Rapid enrichment of metals, dust in ISM (z 8) ...
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Herschel Galaxy Counts and High Redshift Luminosity Functions: The Formation of Massive Early Type Galaxies PowerPoint PPT Presentation
Herschel Galaxy Counts and High Redshift Luminosity Functions: The Formation of Massive Early Type Galaxies - Title: PowerPoint Presentation Last modified by: Thinkpad User Created Date: 1/1/1601 12:00:00 AM Document presentation format:
Title: PowerPoint Presentation Last modified by: Thinkpad User Created Date: 1/1/1601 12:00:00 AM Document presentation format:
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ULTRAVIOLET, VISIBLE, AND GRAVITATIONAL ASTROPHYSICS PROGRAM PowerPoint PPT Presentation
ULTRAVIOLET, VISIBLE, AND GRAVITATIONAL ASTROPHYSICS PROGRAM - ULTRAVIOLET, VISIBLE, AND GRAVITATIONAL ASTROPHYSICS PROGRAM. Philippe Crane. October 26, 2000 ... Discipline Scientist for Fundamental Physics and Gravity ...
ULTRAVIOLET, VISIBLE, AND GRAVITATIONAL ASTROPHYSICS PROGRAM. Philippe Crane. October 26, 2000 ... Discipline Scientist for Fundamental Physics and Gravity ...
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Extragalactic science with the Herschel Space Observatory PowerPoint PPT Presentation
Extragalactic science with the Herschel Space Observatory - Extragalactic science with the Herschel Space Observatory Marc Sauvage CEA/DSM/DAPNIA Service d'Astrophysique UMR AIM
Extragalactic science with the Herschel Space Observatory Marc Sauvage CEA/DSM/DAPNIA Service d'Astrophysique UMR AIM
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ATACAMA PowerPoint PPT Presentation
ATACAMA - (trough the European Southern Observatory). It will consist of an array ... At distances of 40-50 AU, KBOs have temperatures near 45 K, ...
(trough the European Southern Observatory). It will consist of an array ... At distances of 40-50 AU, KBOs have temperatures near 45 K, ...
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AGN/GALAXY COEVOLUTION PowerPoint PPT Presentation
AGN/GALAXY COEVOLUTION - WHIM Backlight Scaling relation fudge factor Point source contaminant Cooling problem get-out clause AGN/GALAXY COEVOLUTION Kirpal Nandra Imperial College London
WHIM Backlight Scaling relation fudge factor Point source contaminant Cooling problem get-out clause AGN/GALAXY COEVOLUTION Kirpal Nandra Imperial College London
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ESO PowerPoint PPT Presentation
ESO - The other side of galaxy formation: radio line and continuum ... Extreme gas rich galaxies without extreme starbursts. Gas depletion timescales 5 x108 yrs ...
The other side of galaxy formation: radio line and continuum ... Extreme gas rich galaxies without extreme starbursts. Gas depletion timescales 5 x108 yrs ...
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ALMA and The North America ALMA Science Center (NAASC) PowerPoint PPT Presentation
ALMA and The North America ALMA Science Center (NAASC) - ALMA and The North America ALMA Science Center NAASC
ALMA and The North America ALMA Science Center NAASC
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Fundamental Sensitivity Limits for Coherent and Direct Detection PowerPoint PPT Presentation
Fundamental Sensitivity Limits for Coherent and Direct Detection - Fundamental Sensitivity Limits for Coherent and Direct Detection Jonas Zmuidzinas Caltech Coherent vs. Direct Detection 7/20/08 KISS MMIC Array Workshop - Zmuidzinas ...
Fundamental Sensitivity Limits for Coherent and Direct Detection Jonas Zmuidzinas Caltech Coherent vs. Direct Detection 7/20/08 KISS MMIC Array Workshop - Zmuidzinas ...
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Galaxy Formation and Evolution in Clusters PowerPoint PPT Presentation
Galaxy Formation and Evolution in Clusters - 0. Introductory remarks about galaxy formation & evolution and why clusters ... for overdensities in galaxies (Miley, Rottgering, de Breuck, Kurk, Overzier) ...
0. Introductory remarks about galaxy formation & evolution and why clusters ... for overdensities in galaxies (Miley, Rottgering, de Breuck, Kurk, Overzier) ...
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Galaxies and cosmology: the promise of ALMA PowerPoint PPT Presentation
Galaxies and cosmology: the promise of ALMA - ALMA will see CO structure in detail. ALMA ... May not see most important region in the optical ... Heterodyne R 106 and 8-GHz bandwidth: ALMA can see details ...
ALMA will see CO structure in detail. ALMA ... May not see most important region in the optical ... Heterodyne R 106 and 8-GHz bandwidth: ALMA can see details ...
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From Pre-Stellar Cores to Protostars: The Initial Conditions of Star Formation PowerPoint PPT Presentation
From Pre-Stellar Cores to Protostars: The Initial Conditions of Star Formation - From Pre-Stellar Cores to Protostars: The Initial Conditions of Star Formation Andre P., Ward-Thompson D., Barsony M., 2000, in Protostars and Planets IV, ed. V ...
From Pre-Stellar Cores to Protostars: The Initial Conditions of Star Formation Andre P., Ward-Thompson D., Barsony M., 2000, in Protostars and Planets IV, ed. V ...
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