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Mock Catalogs for DEEP2 PowerPoint PPT Presentation
Mock Catalogs for DEEP2 - Constraining evolution in the Halo Model using galaxy redshift surveys (astro-ph ... Halo Model N-body simulation provides a practical way of building ...
Constraining evolution in the Halo Model using galaxy redshift surveys (astro-ph ... Halo Model N-body simulation provides a practical way of building ...
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DEEP2 Galaxy Redshift Survey and Post-Starburst galaxies at z~1 PowerPoint PPT Presentation
DEEP2 Galaxy Redshift Survey and Post-Starburst galaxies at z~1 - ... Redshift Survey, which uses the DEIMOS spectrograph on the Keck II telescope, is ... DEEP2 is similar to LCRS in sample size but at z=1 - with a very ...
... Redshift Survey, which uses the DEIMOS spectrograph on the Keck II telescope, is ... DEEP2 is similar to LCRS in sample size but at z=1 - with a very ...
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IRACselected EROs with DEEP2 zs PowerPoint PPT Presentation
IRACselected EROs with DEEP2 zs - IRAC-selected EROs (with DEEP2 z's) Gillian Wilson (Spitzer Science Center) ... at those with DEEP2 spectroscopy == ~ 89 EROs. Early-type? Dusty Star-forming? ...
IRAC-selected EROs (with DEEP2 z's) Gillian Wilson (Spitzer Science Center) ... at those with DEEP2 spectroscopy == ~ 89 EROs. Early-type? Dusty Star-forming? ...
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Results from the DEEP2 Redshift Survey PowerPoint PPT Presentation
Results from the DEEP2 Redshift Survey - Resolved kinematics of galaxies (Cooper et al., in prep) The dependence of galaxy properties on environment (Cooper/Gerke/Madgwick et al., in prep) ...
Resolved kinematics of galaxies (Cooper et al., in prep) The dependence of galaxy properties on environment (Cooper/Gerke/Madgwick et al., in prep) ...
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The DEEP2 Galaxy Redshift Survey First Results on Groups and Clusters PowerPoint PPT Presentation
The DEEP2 Galaxy Redshift Survey First Results on Groups and Clusters - Study galaxy properties and formation history especially in extreme environments ... Improve simulations (how do galaxies populate DM halos? ...
Study galaxy properties and formation history especially in extreme environments ... Improve simulations (how do galaxies populate DM halos? ...
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From Fine Structure to LargeScale Structure with the DEEP2 Redshift Survey PowerPoint PPT Presentation
From Fine Structure to LargeScale Structure with the DEEP2 Redshift Survey - From Fine Structure to LargeScale Structure with the DEEP2 Redshift Survey
From Fine Structure to LargeScale Structure with the DEEP2 Redshift Survey
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The DEEP2 Redshift Survey: Summary and Status PowerPoint PPT Presentation
The DEEP2 Redshift Survey: Summary and Status - ... P. Guhathakurta, D. Phillips, C. Willmer, B. Weiner, ... U. Hawaii: N. Kaiser, G. Luppino. Lawrence Berkeley National Laboratory: J. Newman, D. Madgwick ...
... P. Guhathakurta, D. Phillips, C. Willmer, B. Weiner, ... U. Hawaii: N. Kaiser, G. Luppino. Lawrence Berkeley National Laboratory: J. Newman, D. Madgwick ...
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Target Selection for the DEEP2 Redshift Survey PowerPoint PPT Presentation
Target Selection for the DEEP2 Redshift Survey - We will need to investigate what types of objects we miss in more detail (mostly just mag. ... By comparing the universe at high redshift to what is seen ...
We will need to investigate what types of objects we miss in more detail (mostly just mag. ... By comparing the universe at high redshift to what is seen ...
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Early Results from the DEEP2 Redshift Survey PowerPoint PPT Presentation
Early Results from the DEEP2 Redshift Survey - Early Results from the DEEP2 Redshift Survey. Jeffrey Newman. and the DEEP2 Team ... relative velocities of faint neighbors of bright galaxies (ala Prada et al. 2003) ...
Early Results from the DEEP2 Redshift Survey. Jeffrey Newman. and the DEEP2 Team ... relative velocities of faint neighbors of bright galaxies (ala Prada et al. 2003) ...
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Early Galaxy Clustering Results from The DEEP2 Redshift Survey PowerPoint PPT Presentation
Early Galaxy Clustering Results from The DEEP2 Redshift Survey - ... Survey, which uses the DEIMOS spectrograph on the Keck II telescope, will ... From the projected function wp(rp) we can recover the real-space correlation ...
... Survey, which uses the DEIMOS spectrograph on the Keck II telescope, will ... From the projected function wp(rp) we can recover the real-space correlation ...
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Software: PowerPoint PPT Presentation
Software: - Software: Steve Allen Will Deich De Clarke Bob Kibrick Carmen Kunz Dean Tucker UC Berkeley DEEP2 Team Scientists: Michael Bolte Harland Epps Raja Guhathakurta
Software: Steve Allen Will Deich De Clarke Bob Kibrick Carmen Kunz Dean Tucker UC Berkeley DEEP2 Team Scientists: Michael Bolte Harland Epps Raja Guhathakurta
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Zheng Zheng PowerPoint PPT Presentation
Zheng Zheng - Halo Occupation Distribution (HOD) Breaking the Degeneracies between ... Zheng, Tinker, Weinberg, & Berlind. 2002. Changing m with 8, ns, and Fixed. Cosmology ...
Halo Occupation Distribution (HOD) Breaking the Degeneracies between ... Zheng, Tinker, Weinberg, & Berlind. 2002. Changing m with 8, ns, and Fixed. Cosmology ...
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Lyman Break Galaxies in Large Quasar Groups at z~1 PowerPoint PPT Presentation
Lyman Break Galaxies in Large Quasar Groups at z~1 - Lyman Break Galaxies in Large Quasar Groups at z~1 G Williger (Louisville/JHU), R Clowes (Central Lancashire), L Campusano (U de Chile), L Haberzettl & J Lauroesch ...
Lyman Break Galaxies in Large Quasar Groups at z~1 G Williger (Louisville/JHU), R Clowes (Central Lancashire), L Campusano (U de Chile), L Haberzettl & J Lauroesch ...
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Early%20Results%20from%20the%20DEEP2%20Redshift%20Survey PowerPoint PPT Presentation
Early%20Results%20from%20the%20DEEP2%20Redshift%20Survey - Red galaxies are the ones with bulges. DEEP 1 galaxies with HST imaging (fits by L. Simard) ... brighter bulges. COMBO- 17 photometric survey. Large area, 17 ...
Red galaxies are the ones with bulges. DEEP 1 galaxies with HST imaging (fits by L. Simard) ... brighter bulges. COMBO- 17 photometric survey. Large area, 17 ...
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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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The Deep Imaging Multi-Object Spectrograph for Keck II by S. M. Faber and the DEIMOS Team PowerPoint PPT Presentation
The Deep Imaging Multi-Object Spectrograph for Keck II by S. M. Faber and the DEIMOS Team - Fast readout time: 50 sec. Rapid slitmask alignment: 5 min (goal) ... Below: test analysis of one tilted slitlet. ... limit of the survey) ...
Fast readout time: 50 sec. Rapid slitmask alignment: 5 min (goal) ... Below: test analysis of one tilted slitlet. ... limit of the survey) ...
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The Evolution of Galaxies over the Last Half of Cosmic Time by S' M' Faber and the DEEP PowerPoint PPT Presentation
The Evolution of Galaxies over the Last Half of Cosmic Time by S' M' Faber and the DEEP - The Evolution of Galaxies over the Last Half of Cosmic Time by S' M' Faber and the DEEP
The Evolution of Galaxies over the Last Half of Cosmic Time by S' M' Faber and the DEEP
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The Role of Galaxy Mergers in Forming the Red-Sequence Galaxies PowerPoint PPT Presentation
The Role of Galaxy Mergers in Forming the Red-Sequence Galaxies - 35% of bulge-dominated galaxies experienced a merger with mass ratio 1:4 in the ... For both field and cluster galaxies, the merger events are dominated by Sp-Sp ...
35% of bulge-dominated galaxies experienced a merger with mass ratio 1:4 in the ... For both field and cluster galaxies, the merger events are dominated by Sp-Sp ...
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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 Evolution and WFMOS PowerPoint PPT Presentation
Galaxy Evolution and WFMOS - Galaxy Evolution and WFMOS History of Galaxies Present-day Universe: SDSS WFMOS Survey of z1 Universe K. Shimasaku (University of Tokyo) galaxy morphology galaxy ...
Galaxy Evolution and WFMOS History of Galaxies Present-day Universe: SDSS WFMOS Survey of z1 Universe K. Shimasaku (University of Tokyo) galaxy morphology galaxy ...
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FMOS Workshop, Jan. 2004 PowerPoint PPT Presentation
FMOS Workshop, Jan. 2004 - ... Jan. 2004. The Decline in Cosmic Star Formation: is Environment to ... Mapping the interaction of galaxies with their environment as a function of cosmic time. ...
... Jan. 2004. The Decline in Cosmic Star Formation: is Environment to ... Mapping the interaction of galaxies with their environment as a function of cosmic time. ...
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GALAXY EVOLUTION OPTICAL AND IR SURVEYS PowerPoint PPT Presentation
GALAXY EVOLUTION OPTICAL AND IR SURVEYS - GALAXY EVOLUTION OPTICAL AND IR SURVEYS Lucia Pozzetti INAF Osservatorio Astronomico di Bologna PEOPLE INVOLVED IN BOLOGNA INAF-OAB: Bardelli, Cappi, Ciliegi ...
GALAXY EVOLUTION OPTICAL AND IR SURVEYS Lucia Pozzetti INAF Osservatorio Astronomico di Bologna PEOPLE INVOLVED IN BOLOGNA INAF-OAB: Bardelli, Cappi, Ciliegi ...
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Star%20Formation%20Downsizing:%20Testing%20the%20Role%20of%20Mergers%20and%20AGN PowerPoint PPT Presentation
Star%20Formation%20Downsizing:%20Testing%20the%20Role%20of%20Mergers%20and%20AGN - Star Formation Downsizing: Testing the Role of Mergers and AGN
Star Formation Downsizing: Testing the Role of Mergers and AGN
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COSMOS clusters as tracers of LSS PowerPoint PPT Presentation
COSMOS clusters as tracers of LSS - Berian James, John Peacock, Gigi Guzzo, Nico Cappelluti, ... Hans Boehringer, Stefania Giodini, Mara Salvato, Nick Scoville, Olivier Ilbert, ...
Berian James, John Peacock, Gigi Guzzo, Nico Cappelluti, ... Hans Boehringer, Stefania Giodini, Mara Salvato, Nick Scoville, Olivier Ilbert, ...
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The Void Probability function and related statistics PowerPoint PPT Presentation
The Void Probability function and related statistics - Count probability PN(V): probability of finding N galaxies in a randomly chosen ... Skewness and kurtosis (2D) for the Deeprange and SDSS. From Szapudi et al. 2002 ...
Count probability PN(V): probability of finding N galaxies in a randomly chosen ... Skewness and kurtosis (2D) for the Deeprange and SDSS. From Szapudi et al. 2002 ...
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2006 Work Plan PowerPoint PPT Presentation
2006 Work Plan - 16/32 ch Amp-CDS-ADC with 0.635 mm pitch. System noise 50 electrons (depends on CCD) ... KEK Annual budget 'A' Electronics. Fine Pixel. Standard size. G ...
16/32 ch Amp-CDS-ADC with 0.635 mm pitch. System noise 50 electrons (depends on CCD) ... KEK Annual budget 'A' Electronics. Fine Pixel. Standard size. G ...
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Virtual Deep Field Surveys PowerPoint PPT Presentation
Virtual Deep Field Surveys - GOODS goals (evolution of normal galaxies to z 6, numbers, luminosity, size, ... They are indispensable tool in interpreting a wide range of observational data ...
GOODS goals (evolution of normal galaxies to z 6, numbers, luminosity, size, ... They are indispensable tool in interpreting a wide range of observational data ...
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FPCCD Vertex Detector R PowerPoint PPT Presentation
FPCCD Vertex Detector R - FPCCD Vertex Detector R&D for ILC Yasuhiro Sugimoto KEK @Vertex Detector Review
FPCCD Vertex Detector R&D for ILC Yasuhiro Sugimoto KEK @Vertex Detector Review
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SURVEY CHALLENGES PowerPoint PPT Presentation
SURVEY CHALLENGES - HST, Spitzer, VLA, GALEX, CFHT LS blah blah blah 'AEGIS' ApJL special issue (~20 ... AGN contribution to the total luminosity of the universe (c.f. stars) ...
HST, Spitzer, VLA, GALEX, CFHT LS blah blah blah 'AEGIS' ApJL special issue (~20 ... AGN contribution to the total luminosity of the universe (c.f. stars) ...
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Intrinsic ellipticity correlation of luminous red galaxies and misalignment with their host dark matter halos PowerPoint PPT Presentation
Intrinsic ellipticity correlation of luminous red galaxies and misalignment with their host dark matter halos - ... of luminous red galaxies and misalignment with their host dark matter halos ... Directly probe the matter distribution. es. Observable. Ellipticity of ...
... of luminous red galaxies and misalignment with their host dark matter halos ... Directly probe the matter distribution. es. Observable. Ellipticity of ...
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Quasar Heating in Structure Formation PowerPoint PPT Presentation
Quasar Heating in Structure Formation - OpenMP version of the Hydra' SPH code (Pearce & Couchman 1997, Thacker et al ... (Hydra) Entropy evolution (slice from simulation) Rendered on 13403. grid. ...
OpenMP version of the Hydra' SPH code (Pearce & Couchman 1997, Thacker et al ... (Hydra) Entropy evolution (slice from simulation) Rendered on 13403. grid. ...
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FPCCD Vertex Detector for ILC PowerPoint PPT Presentation
FPCCD Vertex Detector for ILC - Fine pixel of ~5mm (x20 more pixels than 'standard' pixels) to keep low pixel occupancy ... Fine Pixel CCD. Z. f. Low Pt. b.g. High Pt. Signal. B.G. rejection ...
Fine pixel of ~5mm (x20 more pixels than 'standard' pixels) to keep low pixel occupancy ... Fine Pixel CCD. Z. f. Low Pt. b.g. High Pt. Signal. B.G. rejection ...
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Astronomical spectroscopy and the Virtual Observatory: a user-oriented perspective PowerPoint PPT Presentation
Astronomical spectroscopy and the Virtual Observatory: a user-oriented perspective - Astronomical spectroscopy and the Virtual Observatory: a user-oriented perspective ... Virtual data generation: cut-out, reprojection, dynamic extraction etc. ...
Astronomical spectroscopy and the Virtual Observatory: a user-oriented perspective ... Virtual data generation: cut-out, reprojection, dynamic extraction etc. ...
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Stellar populations, star formation and their evolution over the last 8 billion years PowerPoint PPT Presentation
Stellar populations, star formation and their evolution over the last 8 billion years - Stellar populations, star formation and their evolution over ... galaxies (Garching-MPA, Stephane Charlot, Jarle Brichmann, Simon White, Guinevere Kauffmann) ...
Stellar populations, star formation and their evolution over ... galaxies (Garching-MPA, Stephane Charlot, Jarle Brichmann, Simon White, Guinevere Kauffmann) ...
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The coordinated growth of stars, haloes and largescale structure since z1 PowerPoint PPT Presentation
The coordinated growth of stars, haloes and largescale structure since z1 - Models too efficient at shutting off gas supply? Weinmann et al. 2006. Local environment ... Hypothesis that cooling is shut off in haloes above a critical mass ...
Models too efficient at shutting off gas supply? Weinmann et al. 2006. Local environment ... Hypothesis that cooling is shut off in haloes above a critical mass ...
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Lens Galaxy Environments PowerPoint PPT Presentation
Lens Galaxy Environments - This constrains the galaxy-mass correlation function and ... We ran FOF to find halos, and populated the halos with lens galaxies using our best-fitting HOD. ...
This constrains the galaxy-mass correlation function and ... We ran FOF to find halos, and populated the halos with lens galaxies using our best-fitting HOD. ...
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Large Scale Structure and Galaxy Properties PowerPoint PPT Presentation
Large Scale Structure and Galaxy Properties - Korea Institute for Advanced Study (KIAS) A Proposal for LAMOST & AS2. Dark matter halos surrounding galaxies, ... [Prada et al. 03; Brainerd 04] - [SDSS & 2dF] ...
Korea Institute for Advanced Study (KIAS) A Proposal for LAMOST & AS2. Dark matter halos surrounding galaxies, ... [Prada et al. 03; Brainerd 04] - [SDSS & 2dF] ...
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Galaxy Formation and Evolution in Clusters PowerPoint PPT Presentation
Galaxy Formation and Evolution in Clusters - ... mechanism for ellipticals and bulges, which are collections of old ... Big question: what's the best way to constrain the baryonic physics of galaxy ...
... mechanism for ellipticals and bulges, which are collections of old ... Big question: what's the best way to constrain the baryonic physics of galaxy ...
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Stars introduction and brief overview of properties PowerPoint PPT Presentation
Stars introduction and brief overview of properties - Andrey Kravtsov. Kavli Institute for Cosmological Physics (KICP) The University of Chicago ... The sexiest simulation? http://www.this-wonderful-life.com. SDSS survey ...
Andrey Kravtsov. Kavli Institute for Cosmological Physics (KICP) The University of Chicago ... The sexiest simulation? http://www.this-wonderful-life.com. SDSS survey ...
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R PowerPoint PPT Presentation
R - ... CCD. Design of small. Prototype of FPCCD. FPCCD. fabrication. Sample test ... LOI: Letter of Intent (?) FPCCD VTX. Short term plan. Study of fully depleted CCD ...
... CCD. Design of small. Prototype of FPCCD. FPCCD. fabrication. Sample test ... LOI: Letter of Intent (?) FPCCD VTX. Short term plan. Study of fully depleted CCD ...
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FPCCD Vertex detector PowerPoint PPT Presentation
FPCCD Vertex detector - LOI: Letter of Intent (?) FPCCD VTX. Short term plan. Study of fully depleted CCD ... The 1st test sample of FPCCD is expected to be made by Hamamatsu in FY2007 ...
LOI: Letter of Intent (?) FPCCD VTX. Short term plan. Study of fully depleted CCD ... The 1st test sample of FPCCD is expected to be made by Hamamatsu in FY2007 ...
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The Dark Energy Survey PowerPoint PPT Presentation
The Dark Energy Survey - The Dark Energy Survey
The Dark Energy Survey
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Cosmic evolution of galaxy clustering PowerPoint PPT Presentation
Cosmic evolution of galaxy clustering - Search for a statistical description of the dark matter / galaxy distribution ... Based on GIF/VIRGO N-body. simulations by Jenkins et al. (1998) At z=3: r0~1 ...
Search for a statistical description of the dark matter / galaxy distribution ... Based on GIF/VIRGO N-body. simulations by Jenkins et al. (1998) At z=3: r0~1 ...
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The LBNL Supernova Cosmology Program PowerPoint PPT Presentation
The LBNL Supernova Cosmology Program - These observations add to the Subaru search in building up a sample of highest ... Discoveries of 29 high redshift SNe with Subaru. HST ACS follow ups of 5 SNe ...
These observations add to the Subaru search in building up a sample of highest ... Discoveries of 29 high redshift SNe with Subaru. HST ACS follow ups of 5 SNe ...
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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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High Redshift Galaxies PowerPoint PPT Presentation
High Redshift Galaxies - High Redshift Galaxies
High Redshift Galaxies
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Calibrating Photometric Redshifts beyond Spectroscopic Limits PowerPoint PPT Presentation
Calibrating Photometric Redshifts beyond Spectroscopic Limits - We want to measure p(z) for a sample of galaxies in one photometric redshift bin ... Generally, we measure the autocorrelation of some sort of object with other ...
We want to measure p(z) for a sample of galaxies in one photometric redshift bin ... Generally, we measure the autocorrelation of some sort of object with other ...
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The Dark Energy Survey - DES PowerPoint PPT Presentation
The Dark Energy Survey - DES - The Dark Energy Survey DES
The Dark Energy Survey DES
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Dark Energy and Cosmic Sound PowerPoint PPT Presentation
Dark Energy and Cosmic Sound - Sound Waves ... Sound speed plummets. Wave stalls at a radius of 150 Mpc. ... A crest launches a planar sound wave, which at recombination may or may not be in phase ...
Sound Waves ... Sound speed plummets. Wave stalls at a radius of 150 Mpc. ... A crest launches a planar sound wave, which at recombination may or may not be in phase ...
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Albert Stebbins PowerPoint PPT Presentation
Albert Stebbins - Theoretical Astrophysics Group @ Fermilab Albert Stebbins Theoretical Astrophysics Group Fermi National Laboratory stebbins@fnal.gov Annual DOE Review
Theoretical Astrophysics Group @ Fermilab Albert Stebbins Theoretical Astrophysics Group Fermi National Laboratory stebbins@fnal.gov Annual DOE Review
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DES Photoz WG discussion topics PowerPoint PPT Presentation
DES Photoz WG discussion topics - Compare/optimize photo-z codes from interested groups. Finally test neural network photo-z module (from DC1) ... Data Challenge 4 (DC4) and Photo-z WG. 2 ...
Compare/optimize photo-z codes from interested groups. Finally test neural network photo-z module (from DC1) ... Data Challenge 4 (DC4) and Photo-z WG. 2 ...
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The Coevolution of Galaxies and Dark Matter Halos PowerPoint PPT Presentation
The Coevolution of Galaxies and Dark Matter Halos - The 2-pt auto-correlation of halos in this model does not depend on ... Appropriate for the most massive galaxies where zform,stars 2 ... Validated by hydro-sims. ...
The 2-pt auto-correlation of halos in this model does not depend on ... Appropriate for the most massive galaxies where zform,stars 2 ... Validated by hydro-sims. ...
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Multivariate Properties of Galaxies at Low Redshift PowerPoint PPT Presentation
Multivariate Properties of Galaxies at Low Redshift - Multivariate Properties of Galaxies at Low Redshift. Galaxy Properties from Imaging ... From Mara Salvato's web page. Where is the stellar mass? ...
Multivariate Properties of Galaxies at Low Redshift. Galaxy Properties from Imaging ... From Mara Salvato's web page. Where is the stellar mass? ...
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Astro 105: Our Place in the Universe PowerPoint PPT Presentation
Astro 105: Our Place in the Universe - Nearby clusters include the Virgo Cluster (hundreds, maybe thousands of galaxies) ... slice with CfA2 slice (find stick man!) SDSS Great Wall 300 Mpc long ...
Nearby clusters include the Virgo Cluster (hundreds, maybe thousands of galaxies) ... slice with CfA2 slice (find stick man!) SDSS Great Wall 300 Mpc long ...
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EUCLID spectroscopy : overview and synergies with WFXT PowerPoint PPT Presentation
EUCLID spectroscopy : overview and synergies with WFXT - These predictions have been verified using some recent 'real' data at 0.6 z 1.0 ... Currently only one object with spectroscopic confirmation at z ~ 7 ...
These predictions have been verified using some recent 'real' data at 0.6 z 1.0 ... Currently only one object with spectroscopic confirmation at z ~ 7 ...
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