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Molecules in ULIRGS, and high density tracers PowerPoint PPT Presentation
Molecules in ULIRGS, and high density tracers - The H2 gas is also more concentrated. In average, the H2 ... Vertical filament: SiO chimney. coincident with radio cm emission. Gas ejected by the starburst ...
The H2 gas is also more concentrated. In average, the H2 ... Vertical filament: SiO chimney. coincident with radio cm emission. Gas ejected by the starburst ...
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ULIRGs in hard Xray: From XMM to Simbol X PowerPoint PPT Presentation
ULIRGs in hard Xray: From XMM to Simbol X - Open questions: relative contribution SB and AGN. Need of observation above 10 keV ... To calibrate a SFR IR-X ray indicator is fundamental a direct measure of the ...
Open questions: relative contribution SB and AGN. Need of observation above 10 keV ... To calibrate a SFR IR-X ray indicator is fundamental a direct measure of the ...
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PILOT Survey for Supernovae in Starbursts PowerPoint PPT Presentation
PILOT Survey for Supernovae in Starbursts - VLT+NACO monitoring of 14 ULIRGs out to D ~ 300 Mpc. Historical SN in NGC 7714 Found in archival UKIRT K image from Sep 1998. Optimal Image Subtraction Allard ...
VLT+NACO monitoring of 14 ULIRGs out to D ~ 300 Mpc. Historical SN in NGC 7714 Found in archival UKIRT K image from Sep 1998. Optimal Image Subtraction Allard ...
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Galaxy Evolution and Star Formation Efficiency in the Last Half of the Universe PowerPoint PPT Presentation
Galaxy Evolution and Star Formation Efficiency in the Last Half of the Universe - About half of the galaxy formation and evolution gets out ... Dole et al 2006. Compilation by Hopkins 2004. ULIRGs. L 1011 Lo. L 1011 Lo. total ...
About half of the galaxy formation and evolution gets out ... Dole et al 2006. Compilation by Hopkins 2004. ULIRGs. L 1011 Lo. L 1011 Lo. total ...
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Gas Dynamics in Galactic Nuclei: PowerPoint PPT Presentation
Gas Dynamics in Galactic Nuclei: - Ultraluminous Infrared Galaxies (ULIRGs) Discovered by IRAS in mid 80's ... Key Phase in Growth of Elliptical Galaxies and Massive BHs? Chapman et al. 2004 ...
Ultraluminous Infrared Galaxies (ULIRGs) Discovered by IRAS in mid 80's ... Key Phase in Growth of Elliptical Galaxies and Massive BHs? Chapman et al. 2004 ...
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Line detections in IC 860: (Top) HCN v2=1, J=4 and PowerPoint PPT Presentation
Line detections in IC 860: (Top) HCN v2=1, J=4 and - (Bottom) H2CO and CH2NH emission lines, Pre-Biotic and Other Molecules in ULIRGs (a) Arp 220 ... The 6-cm lines of excited-OH in ULIRG, III Zw35. ...
(Bottom) H2CO and CH2NH emission lines, Pre-Biotic and Other Molecules in ULIRGs (a) Arp 220 ... The 6-cm lines of excited-OH in ULIRG, III Zw35. ...
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Diapositive 1 PowerPoint PPT Presentation
Diapositive 1 - The SWIRE Spitzer survey has detected by far the largest set of Sub-Millimeter ... Chapman, Blain, Smail, Ivison 2005. SCUBA(-MAMBO) census of high-z ULIRGs ...
The SWIRE Spitzer survey has detected by far the largest set of Sub-Millimeter ... Chapman, Blain, Smail, Ivison 2005. SCUBA(-MAMBO) census of high-z ULIRGs ...
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AGN Unification Viewed in the mid-IR PowerPoint PPT Presentation
AGN Unification Viewed in the mid-IR - But the dust structure in AGN is more complicated. ... Active Galactic Nuclei Population in SDSS Author: Lei Hao Last modified by: Lei Hao Created Date:
But the dust structure in AGN is more complicated. ... Active Galactic Nuclei Population in SDSS Author: Lei Hao Last modified by: Lei Hao Created Date:
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IR%20properties%20of%20distant%20IR%20galaxies PowerPoint PPT Presentation
IR%20properties%20of%20distant%20IR%20galaxies - Delphine Marcillac. Moriond 2005 When UV meets IR ... 1. IR properties ... Faint Objects = long time exposure. it needs a good correction for the attenuation. ...
Delphine Marcillac. Moriond 2005 When UV meets IR ... 1. IR properties ... Faint Objects = long time exposure. it needs a good correction for the attenuation. ...
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PILOT Survey for Supernovae in Starbursts PowerPoint PPT Presentation
PILOT Survey for Supernovae in Starbursts - Core-collapse SNe (CCSNe) generate/liberate the bulk of the ... Can serve as probes of extinction and ISM. CCSNe blast wave probes progenitor mass-loss history. ...
Core-collapse SNe (CCSNe) generate/liberate the bulk of the ... Can serve as probes of extinction and ISM. CCSNe blast wave probes progenitor mass-loss history. ...
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Molecular Gas, Dense Molecular Gas and the Star Formation Rate in Galaxies (near and far) P. Solomon PowerPoint PPT Presentation
Molecular Gas, Dense Molecular Gas and the Star Formation Rate in Galaxies (near and far) P. Solomon - Molecular Gas, Dense Molecular Gas and the Star Formation Rate in Galaxies (near and far) P. Solomon Molecular Gas Mass as traced by CO emission and the star ...
Molecular Gas, Dense Molecular Gas and the Star Formation Rate in Galaxies (near and far) P. Solomon Molecular Gas Mass as traced by CO emission and the star ...
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Hunt for Molecules in Local Universe Galaxies PowerPoint PPT Presentation
Hunt for Molecules in Local Universe Galaxies - Hunt for Molecules in Local Universe Galaxies Santiago GARCIA-BURILLO Observatorio Astron mico Nacional (OAN)-Spain Hunt for Molecules, November 19-20, 2005, Paris ...
Hunt for Molecules in Local Universe Galaxies Santiago GARCIA-BURILLO Observatorio Astron mico Nacional (OAN)-Spain Hunt for Molecules, November 19-20, 2005, Paris ...
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The Coeval Growth of Black Holes and their host Spheriods PowerPoint PPT Presentation
The Coeval Growth of Black Holes and their host Spheriods - Title: PowerPoint Presentation Last modified by: Xia Xiaoyang Created Date: 1/1/1601 12:00:00 AM Document presentation format: Other titles
Title: PowerPoint Presentation Last modified by: Xia Xiaoyang Created Date: 1/1/1601 12:00:00 AM Document presentation format: Other titles
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GRB Host Galaxies S. R.Kulkarni, E. J. Berger PowerPoint PPT Presentation
GRB Host Galaxies S. R.Kulkarni, E. J. Berger - GRB Host Galaxies S. R.Kulkarni, E. J. Berger & Caltech GRB group
GRB Host Galaxies S. R.Kulkarni, E. J. Berger & Caltech GRB group
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16 micron Imaging in the GOODS fields with the Spitzer IRS PowerPoint PPT Presentation
16 micron Imaging in the GOODS fields with the Spitzer IRS - 16 micron Imaging in the GOODS fields with the Spitzer IRS. Harry Teplitz ... Pilot Study: GTO 16 mm in GOODS-N ... GOODS South. Data obtained in Feb 05. Some ...
16 micron Imaging in the GOODS fields with the Spitzer IRS. Harry Teplitz ... Pilot Study: GTO 16 mm in GOODS-N ... GOODS South. Data obtained in Feb 05. Some ...
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Feedback from Momentum-Driven Winds PowerPoint PPT Presentation
Feedback from Momentum-Driven Winds - Dust absorbs the radiation produced by starbursts or AGN ... sufficient to blow away. all of the gas in a galaxy ... If L LM, AGN can blow dusty gas out of. its ...
Dust absorbs the radiation produced by starbursts or AGN ... sufficient to blow away. all of the gas in a galaxy ... If L LM, AGN can blow dusty gas out of. its ...
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Richard Davies, Eckhard Sturm PowerPoint PPT Presentation
Richard Davies, Eckhard Sturm - Black Hole Feeding & Feedback: what can we learn from nearby AGN? Richard Davies, Eckhard Sturm Max Planck Institute for Extraterrestrial Physics, Germany
Black Hole Feeding & Feedback: what can we learn from nearby AGN? Richard Davies, Eckhard Sturm Max Planck Institute for Extraterrestrial Physics, Germany
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Extragalactic Foreground Sources PowerPoint PPT Presentation
Extragalactic Foreground Sources - Cosmic Microwave Background (CMB) is an 'echo' of the Big Bang. ... Has same spectral behavior as CMB anisotropy. Difficult to correct for, but relatively minor. ...
Cosmic Microwave Background (CMB) is an 'echo' of the Big Bang. ... Has same spectral behavior as CMB anisotropy. Difficult to correct for, but relatively minor. ...
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X-ray clues on the nature of sub-mm galaxies PowerPoint PPT Presentation
X-ray clues on the nature of sub-mm galaxies - SMG: an Introduction SCUBA detector (850micron) on JCMT gave a boost to sub-mm Cosmology The negative K-correction plays a major role making high-redshift ...
SMG: an Introduction SCUBA detector (850micron) on JCMT gave a boost to sub-mm Cosmology The negative K-correction plays a major role making high-redshift ...
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????1m??????????ANIR??? ??LIRG?Paa?? PowerPoint PPT Presentation
????1m??????????ANIR??? ??LIRG?Paa?? - Title: 1m ANIR LIRG Pa Author: toshikawa Last modified by: toshikawa Created Date
Title: 1m ANIR LIRG Pa Author: toshikawa Last modified by: toshikawa Created Date
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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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The VLA-COSMOS survey: Tracing star-forming and AGN galaxies through cosmic time PowerPoint PPT Presentation
The VLA-COSMOS survey: Tracing star-forming and AGN galaxies through cosmic time - Thermal (free-free) emission (radio) Thermal dust emission (FIR) ... probing thermal (free-free) radio emission for z 3.5. VLA-COSMOS Large Project limits ...
Thermal (free-free) emission (radio) Thermal dust emission (FIR) ... probing thermal (free-free) radio emission for z 3.5. VLA-COSMOS Large Project limits ...
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The Discovery of Extragalactic Magnetic Fields in OH Megamasers PowerPoint PPT Presentation
The Discovery of Extragalactic Magnetic Fields in OH Megamasers - The Discovery of Extragalactic Magnetic Fields in OH Megamasers
The Discovery of Extragalactic Magnetic Fields in OH Megamasers
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Nessun titolo diapositiva PowerPoint PPT Presentation
Nessun titolo diapositiva - INTEGRAL IBIS Survey (Bassani et al., 2006) sensitivity ... INTEGRAL IBIS Survey (Sazonov et al., 2006) ... INTEGRAL IBIS AGN Survey (Beckmann et al., 2006) ...
INTEGRAL IBIS Survey (Bassani et al., 2006) sensitivity ... INTEGRAL IBIS Survey (Sazonov et al., 2006) ... INTEGRAL IBIS AGN Survey (Beckmann et al., 2006) ...
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A close relationship at z2: SMGs and BzKs PowerPoint PPT Presentation
A close relationship at z2: SMGs and BzKs - ... galaxies. A simple two color selection for culling galaxies ... Classify galaxies as star-forming or passive systems. The selection is independent of reddening ...
... galaxies. A simple two color selection for culling galaxies ... Classify galaxies as star-forming or passive systems. The selection is independent of reddening ...
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FLAMES/GIRAFFE:%20%20%20Euro3D,%20kickoff%20meeting,%20science PowerPoint PPT Presentation
FLAMES/GIRAFFE:%20%20%20Euro3D,%20kickoff%20meeting,%20science - I. Kinematics & Dynamics of nearby galaxies (in tight ... absorption lines (Kelson et al. 2000) Long-slit spectroscopy (Keck Telescope) Low spectral res. ...
I. Kinematics & Dynamics of nearby galaxies (in tight ... absorption lines (Kelson et al. 2000) Long-slit spectroscopy (Keck Telescope) Low spectral res. ...
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High energy emission from supernova remnants and regions of star formation PowerPoint PPT Presentation
High energy emission from supernova remnants and regions of star formation - ... radio map of the nearby star LS 5039 obtained with VLBA and VLA in ... No WR or Of massive stars in the field, no X-ray binaries or black hole candidates ...
... radio map of the nearby star LS 5039 obtained with VLBA and VLA in ... No WR or Of massive stars in the field, no X-ray binaries or black hole candidates ...
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Pulsar Powerhouse: The Center of the Crab Nebula PowerPoint PPT Presentation
Pulsar Powerhouse: The Center of the Crab Nebula - Title: Pulsar Powerhouse: The Center of the Crab Nebula Author: M Bietenholz Last modified by: michael Created Date: 1/4/1980 12:41:10 AM Document presentation format
Title: Pulsar Powerhouse: The Center of the Crab Nebula Author: M Bietenholz Last modified by: michael Created Date: 1/4/1980 12:41:10 AM Document presentation format
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AGN Unification Viewed in the midIR PowerPoint PPT Presentation
AGN Unification Viewed in the midIR - The probability of Seyfert 1s showing SA is larger than the probabilities of ... Emission vs. absorption for Type I and Type II are clearer for high-luminosity AGN. ...
The probability of Seyfert 1s showing SA is larger than the probabilities of ... Emission vs. absorption for Type I and Type II are clearer for high-luminosity AGN. ...
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The Star Formation Law in Atomic and Molecular Gas PowerPoint PPT Presentation
The Star Formation Law in Atomic and Molecular Gas - The free-fall time in molecular clouds tff determined by SF feedback in low ... The star formation rate per free-fall time ff this is always ~1% due to the ...
The free-fall time in molecular clouds tff determined by SF feedback in low ... The star formation rate per free-fall time ff this is always ~1% due to the ...
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X-RAY NATURE of the LINER nuclear sources Isabel M PowerPoint PPT Presentation
X-RAY NATURE of the LINER nuclear sources Isabel M - Title: CURRICULUM VITAE Isabel M rquez P rez Author: Isabel M rquez P rez Last modified by: zhangfan Created Date: 1/24/2001 10:15:49 PM
Title: CURRICULUM VITAE Isabel M rquez P rez Author: Isabel M rquez P rez Last modified by: zhangfan Created Date: 1/24/2001 10:15:49 PM
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Coevolution of black holes and galaxies at high redshift PowerPoint PPT Presentation
Coevolution of black holes and galaxies at high redshift - Coevolution of black holes and galaxies at high redshift David M Alexander (Durham)
Coevolution of black holes and galaxies at high redshift David M Alexander (Durham)
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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 obscured quasars PowerPoint PPT Presentation
High-redshift obscured quasars - S 3.6 m 45 Jy : rejects type-1s and low-z type-2s (z phot 1.4) ... z phot = 1.90. z spec = 2.08. Av 35. Mid-IR radio reveals z 2 obscured quasars ...
S 3.6 m 45 Jy : rejects type-1s and low-z type-2s (z phot 1.4) ... z phot = 1.90. z spec = 2.08. Av 35. Mid-IR radio reveals z 2 obscured quasars ...
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New Astronomy in a Virtual Observatory PowerPoint PPT Presentation
New Astronomy in a Virtual Observatory - New Astronomy in a Virtual Observatory S. G. Djorgovski (Caltech) Presentation at the NSF Symposium on Knowledge Environments for Science, Arlington, 26 Nov 02
New Astronomy in a Virtual Observatory S. G. Djorgovski (Caltech) Presentation at the NSF Symposium on Knowledge Environments for Science, Arlington, 26 Nov 02
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Starbursts and the triggering of the activity in low redshift radio galaxies PowerPoint PPT Presentation
Starbursts and the triggering of the activity in low redshift radio galaxies - 3C Radio Galaxies at 60mm with IRAS. Only ~30% of 3CR radio galaxies at z 0.5. were detected by IRAS at 60mm. Spitzer/MIPS observations of complete samples of ...
3C Radio Galaxies at 60mm with IRAS. Only ~30% of 3CR radio galaxies at z 0.5. were detected by IRAS at 60mm. Spitzer/MIPS observations of complete samples of ...
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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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Twenty years ago IRAS gave us what is still our best view of the midinfrared sky' PowerPoint PPT Presentation
Twenty years ago IRAS gave us what is still our best view of the midinfrared sky' - Twenty years ago IRAS gave us what is still our best view of the midinfrared sky'
Twenty years ago IRAS gave us what is still our best view of the midinfrared sky'
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ALMA: Resolving (optically) obscured galaxy formation PowerPoint PPT Presentation
ALMA: Resolving (optically) obscured galaxy formation - Obscured galaxy formation: high redshift (Downes et al 2002; Dunlop et al 2003) Single Scuba galaxy dominates SFR at z 2 in HDF over 10000 optical galaxies! ...
Obscured galaxy formation: high redshift (Downes et al 2002; Dunlop et al 2003) Single Scuba galaxy dominates SFR at z 2 in HDF over 10000 optical galaxies! ...
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Diapositiva 1 PowerPoint PPT Presentation
Diapositiva 1 - To understand the differential properties and observational biases of UV and FIR selections. ... 2 1010 L, all of them FIR selected and 3 also NUV selected. ...
To understand the differential properties and observational biases of UV and FIR selections. ... 2 1010 L, all of them FIR selected and 3 also NUV selected. ...
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The sources of the CIRB have been identified... PowerPoint PPT Presentation
The sources of the CIRB have been identified... - COBE - 240 mm. LIRGs dominate the CSFR above z=0.6. At z=1: 70 % CSFR. LIRGs ... Red line: Spitzer-MIPS 24 mm galaxies. No excess correlation for GOODS sources. ...
COBE - 240 mm. LIRGs dominate the CSFR above z=0.6. At z=1: 70 % CSFR. LIRGs ... Red line: Spitzer-MIPS 24 mm galaxies. No excess correlation for GOODS sources. ...
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(Some of the possible) Astrophysical origins of high energy cosmic rays PowerPoint PPT Presentation
(Some of the possible) Astrophysical origins of high energy cosmic rays - To accelerate a particle efficiently it must cross the shocks ... Observational panorama: composition. Arrival directions & clustering. H.E.S.S.. 17 h data ...
To accelerate a particle efficiently it must cross the shocks ... Observational panorama: composition. Arrival directions & clustering. H.E.S.S.. 17 h data ...
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WISE General Presentation PowerPoint PPT Presentation
WISE General Presentation - Constellation Orion. Trifid Nebula. Visible. Light. NOAO. Infrared ... WISE will map the sky in infrared light, searching for the nearest and coolest stars, ...
Constellation Orion. Trifid Nebula. Visible. Light. NOAO. Infrared ... WISE will map the sky in infrared light, searching for the nearest and coolest stars, ...
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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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The Cosmic X-ray Background Facts: a Nobel prize Fictions: The AGN synthesis models (?) PowerPoint PPT Presentation
The Cosmic X-ray Background Facts: a Nobel prize Fictions: The AGN synthesis models (?) - 8/5/09. GH2003 Workshop. The Cosmic X-ray Background. Facts: a Nobel prize ... Some 'Facts' ... Gandhi & Fabian 2003. Franceschini et al. 2002 link with IR? ...
8/5/09. GH2003 Workshop. The Cosmic X-ray Background. Facts: a Nobel prize ... Some 'Facts' ... Gandhi & Fabian 2003. Franceschini et al. 2002 link with IR? ...
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The EVN PowerPoint PPT Presentation
The EVN - The EVN
The EVN
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Presentazione di PowerPoint PowerPoint PPT Presentation
Presentazione di PowerPoint - ... Herschel probes the rest-frame bolometric emission from galaxies as they formed most of their stars Wedding Cake Survey GOODS-S 0.04 deg^2 GOODS-N 0.04 ...
... Herschel probes the rest-frame bolometric emission from galaxies as they formed most of their stars Wedding Cake Survey GOODS-S 0.04 deg^2 GOODS-N 0.04 ...
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Molecules in Starbursts and PowerPoint PPT Presentation
Molecules in Starbursts and - Habing 1968 BAN 19, 421; Draine 1978 ApJS 36, 595. photon energy (eV) ... Draine 2002. Cesarsky et al. 1996 AA 315 L305. Infrared Space Observatory ...
Habing 1968 BAN 19, 421; Draine 1978 ApJS 36, 595. photon energy (eV) ... Draine 2002. Cesarsky et al. 1996 AA 315 L305. Infrared Space Observatory ...
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H2 in external galaxies and baryonic dark matter PowerPoint PPT Presentation
H2 in external galaxies and baryonic dark matter - Or cold gas in the vicinity of galaxies and cosmic. filaments (Pfenniger & Combes 94) ... Mass profiles for dwarf Irr galaxies dominated by DM ...
Or cold gas in the vicinity of galaxies and cosmic. filaments (Pfenniger & Combes 94) ... Mass profiles for dwarf Irr galaxies dominated by DM ...
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Star formation histories PowerPoint PPT Presentation
Star formation histories - Star formation histories and environment Bianca M. Poggianti INAF Osservatorio Astronomico di Padova WE ARE ALL AFTER THE BIG PICTURE: To what extent, environment
Star formation histories and environment Bianca M. Poggianti INAF Osservatorio Astronomico di Padova WE ARE ALL AFTER THE BIG PICTURE: To what extent, environment
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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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Molecular tracers in the Galaxy and beyond PowerPoint PPT Presentation
Molecular tracers in the Galaxy and beyond - Galactic Molecular Survey (in progress)? Objectives: ... (3) bootstrap = Galactic properties = nearby extragalactic = distant galaxies ...
Galactic Molecular Survey (in progress)? Objectives: ... (3) bootstrap = Galactic properties = nearby extragalactic = distant galaxies ...
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Quasars PowerPoint PPT Presentation
Quasars - Quasars & AGN Some supplemental reading: GREAT compilation of review articles at http://nedwww.ipac.caltech.edu/level5/active_galaxies.html Ties to Host Galaxy ...
Quasars & AGN Some supplemental reading: GREAT compilation of review articles at http://nedwww.ipac.caltech.edu/level5/active_galaxies.html Ties to Host Galaxy ...
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The Formation and Evolution of Galaxies PowerPoint PPT Presentation
The Formation and Evolution of Galaxies - What is the relationship between active galactic nuclei and their ... Supernovae as probes of chemical evolution and star-formation The DRM programs in The ...
What is the relationship between active galactic nuclei and their ... Supernovae as probes of chemical evolution and star-formation The DRM programs in The ...
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Herschel followup of SCUBA2 and ASTROF AllSky Surveys PowerPoint PPT Presentation
Herschel followup of SCUBA2 and ASTROF AllSky Surveys - 5 150mJy at 850 m, triple scanning redundancy ... Strong synergy with ASTRO-F for high-z drop-outs & photo-z ... luminosities, dust masses, better photo-z ...
5 150mJy at 850 m, triple scanning redundancy ... Strong synergy with ASTRO-F for high-z drop-outs & photo-z ... luminosities, dust masses, better photo-z ...
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A Cm-Wavelength Search for Pre-Biotic Molecules PowerPoint PPT Presentation
A Cm-Wavelength Search for Pre-Biotic Molecules - Title: PowerPoint Presentation Author: Zaphod Document presentation format: Custom Other titles: Times New Roman Tahoma Monotype Corsiva Symbol Default Design Slide 1
Title: PowerPoint Presentation Author: Zaphod Document presentation format: Custom Other titles: Times New Roman Tahoma Monotype Corsiva Symbol Default Design Slide 1
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