Figure 3.1 from Witnessing the Differential Evolution of Disk Galaxies in Luminosity and Size via Gravitational Lensing (Image 1 of 5) Kaushala Bandara.

Slides:

Advertisements

Similar presentations

Figure 4 from The Hubble Space Telescope Cluster Supernova Survey. II. The Type Ia Supernova Rate in High-redshift Galaxy Clusters (Image 1 of 3) K. Barbary.

Advertisements

Figure 7 from Effects of Circumnuclear Disk Gas Evolution on the Spin of Central Black Holes (Image 1 of 7) Umberto Maio et al ApJ doi: / X/767/1/37.

Figure 6 from HST/WFC3 Near-infrared Spectroscopy of Quenched Galaxies at z ~ 1.5 from the WISP Survey: Stellar Population Properties (Image 1 of 8) A.

Figure 14 from MUSCLE W49: A Multi-Scale Continuum and Line Exploration of the Most Luminous Star Formation Region in the Milky Way. I. Data and the Mass.

Figure 4 from Power Spectrum Analysis of Polarized Emission from the Canadian Galactic Plane Survey (Image 1 of 6) R. A. Stutz et al ApJ doi: / X/787/1/34.

Figure 14 from The Compositional Diversity of Extrasolar Terrestrial Planets. I. In Situ Simulations (Image 1 of 4) Jade C. Bond et al ApJ

Figure 4 from The Australia Telescope Compact Array H I Survey of the Galactic Center (Image 1 of 9) N. M. McClure-Griffiths et al ApJS doi: / /199/1/12.

Figure 15 from Spectral Energy Distributions of QSOs at z > 5: Common Active Galactic Nucleus-heated Dust and Occasionally Strong Star-formation (Image.

Figure 15 from Star Formation in the Central 400 pc of the Milky Way: Evidence for a Population of Massive Young Stellar Objects (Image 1 of 2) F. Yusef-Zadeh.

Figure 5 from The Australia Telescope Compact Array H I Survey of the Galactic Center (Image 1 of 5) N. M. McClure-Griffiths et al ApJS doi: / /199/1/12.

Figure 3 from Multiple Component Outflows in an Active Region Observed with the EUV Imaging Spectrometer on Hinode (Image 1 of 11) P. Bryans et al

K. Decker French et al ApJ doi: / X/801/1/1 Information:

Figure 15 from Cloud–Cloud Collision as a Trigger of the High-mass Star Formation: a Molecular Line Study in RCW120 (Image 1 of 5) K. Torii et al

Figure 7 from The Evolution of Dwarf Galaxy Satellites with Different Dark Matter Density Profiles in the ErisMod Simulations. I. The Early Infalls Mihai.

Figure 9 from A Direct Measurement of the Forward Shock Speed in Supernova Remnant : Constraints on the Age, Ambient Density, Shock Compression.

Figure 2 from The Role of Active Region Loop Geometry. II

Figure 5 from The ACS LCID Project. II

Qing-Wen Tang et al ApJ doi: / X/806/2/194 Information:

Figure 8 from Dust Reddened Quasars in FIRST and UKIDSS: Beyond the Tip of the Iceberg (Image 1 of 5) Eilat Glikman et al ApJ doi: / X/778/2/127.

Figure 4 from Electron Heating by the Ion Cyclotron Instability in Collisionless Accretion Flows. II. Electron Heating Efficiency as a Function of Flow.

Figure 27 from Embedded Protostars in the Dust, Ice, and Gas In Time (DIGIT) Herschel Key Program: Continuum SEDs, and an Inventory of Characteristic Far-infrared.

Y. Q. Xue et al ApJS doi: / /195/1/10 Information:

A. A. Abdo et al ApJ doi: / X/722/1/520 Information:

John R. Dickel et al AJ doi: / /140/5/1511 Information:

Figure 22 from Stellar Disks of Collisional Ring Galaxies. I

Figure 1 from Characterizing the Cool KOIs. VI

Gregory D. Fleishman et al ApJ doi: / X/802/2/122 Information:

Figure 5 from The Cool Component and the Dichotomy, Lateral Expansion, and Axial Rotation of Solar X-Ray Jets (Image 1 of 2) Ronald L. Moore et al

Figure 3 from The Cool Component and the Dichotomy, Lateral Expansion, and Axial Rotation of Solar X-Ray Jets (Image 1 of 2) Ronald L. Moore et al

Figure 3 from The Detectability of Transit Depth Variations Due to Exoplanetary Oblateness and Spin Precession Joshua A. Carter and Joshua N. Winn 2010.

Figure 2 from New Constraints on Cosmic Polarization Rotation from B-Mode Polarization in the Cosmic Microwave Background Sperello di Serego Alighieri.

Figure 1 from Ab Initio Free Energy Calculations of the Solubility of Silica in Metallic Hydrogen and Application to Giant Planet Cores F. González-Cataldo.

Figure 2 from Ab Initio Free Energy Calculations of the Solubility of Silica in Metallic Hydrogen and Application to Giant Planet Cores F. González-Cataldo.

Figure 3 from Ab Initio Free Energy Calculations of the Solubility of Silica in Metallic Hydrogen and Application to Giant Planet Cores F. González-Cataldo.

Figure 1 from Direct Evidence for Ammonium Ion Formation in Ice through Ultraviolet-induced Acid-Base Reaction of NH3 with H3O+ Eui-Seong Moon et al

Figure 6 from Classification and Ranking of Fermi LAT Gamma-ray Sources from the 3FGL Catalog using Machine Learning Techniques P. M. Saz Parkinson et.

Figure 3 from Spectral Line Survey toward the Young Massive Protostar NGC 2264 CMM3 in the 4 mm, 3 mm, and 0.8 mm Bands (Image 1 of 12) Yoshimasa Watanabe.

Figure 8 from Lateral Offset of the Coronal Mass Ejections from the X-flare of 2006 December 13 and Its Two Precursor Eruptions Alphonse C. Sterling et.

Figure 3 from The ACS Nearby Galaxy Survey Treasury. VIII

Figure 3 from On the Formation of Silacyclopropenylidene (c-SiC2H2) and its Role in the Organosilicon Chemistry in the Interstellar Medium Dorian S. N.

Figure 2 from An X-ray Imaging Survey of Quasar Jets: Testing the Inverse Compton Model (Image 1 of 4) H. L. Marshall et al ApJS doi: / /193/1/15.

Figure 4 from Spectroscopic Properties of Star-forming Host Galaxies and Type Ia Supernova Hubble Residuals in a nearly Unbiased Sample Chris B. D'Andrea.

Figure 1 from Spectroscopic Properties of Star-forming Host Galaxies and Type Ia Supernova Hubble Residuals in a nearly Unbiased Sample Chris B. D'Andrea.

P. M. Fry et al AJ doi: / /143/6/150 Information:

Figure 3 from On the Incorporation of Metallicity Data into Measurements of Star Formation History from Resolved Stellar Populations Andrew E. Dolphin.

Figure 5 from Circumstellar 12C/13C Isotope Ratios from Millimeter Observations of CN and CO: Mixing in Carbon- and Oxygen-Rich Stars (Image 1 of 18) S.

Danielle A. Berg et al ApJ doi: / X/754/2/98 Information:

Figure 2 from A Statistical Survey of Peculiar L and T Dwarfs in SDSS, 2MASS, and WISE (Image 1 of 5) Kendra Kellogg et al AJ doi: / /aa83b0.

Catherine Walsh et al ApJ doi: / X/722/2/1607 Information:

Figure 15 from The Carnegie-Irvine Galaxy Survey. II

Figure 3 from Spectral Line Survey toward the Spiral Arm of M51 in the 3 and 2 mm Bands (Image 1 of 6) Yoshimasa Watanabe et al ApJ doi: / X/788/1/4.

Figure 1 from Hubble Space Telescope Combined Strong and Weak Lensing Analysis of the CLASH Sample: Mass and Magnification Models and Systematic Uncertainties.

Figure 2 from Large-scale Kinematics, Astrochemistry, and Magnetic Field Studies of Massive Star-forming Regions through HC3N, HNC, and C2H Mappings (Image.

Figure 7 from The Hubble Space Telescope/Advanced Camera for Surveys Atlas of Protoplanetary Disks in the Great Orion Nebula (Image 1 of 4) L. Ricci et.

Figure 3 from Ultraviolet Light Curves of Supernovae with the Swift Ultraviolet/Optical Telescope (Image 1 of 25) Peter J. Brown et al AJ

Figure 2 from Search for Interstellar Methoxyacetonitrile and Cyanoethanol: Insights Into Coupling of Cyano- to Methanol and Ammonia Chemistry (Image 1.

Figure 2 from High-Resolution Submillimeter Multiline Observations of G19.61 – 0.23: Small-Scale Chemistry (Image 1 of 2) Sheng-Li Qin et al ApJ.

Figure 4 from Time Evolution of a Viscous Protoplanetary Disk with a Free Geometry: Toward a More Self-consistent Picture Kévin Baillié and Sébastien Charnoz.

Figure 1 from Subaru Adaptive-optics High-spatial-resolution Infrared K- and L'-band Imaging Search for Deeply Buried Dual AGNs in Merging Galaxies (Image.

Figure 17 from The SCUBA-2 Cosmology Legacy Survey: Multiwavelength Counterparts to 103 Submillimeter Galaxies in the UKIDSS-UDS Field (Image 1 of 7) Chian-Chou.

Figure 10 from The Change of the Orbital Periods across Eruptions and the Ejected Mass for Recurrent Novae CI Aquilae and U Scorpii Bradley E. Schaefer.

Figure 2 from Thermodynamics of the Solar Corona and Evolution of the Solar Magnetic Field as Inferred from the Total Solar Eclipse Observations of 2010.

Figure from Validating Time-Distance Helioseismology with Realistic Quiet-Sun Simulations (Image 1 of 9) K. DeGrave et al ApJ doi: / X/788/2/127.

Figure 8 from A New Tool for Image Analysis Based on Chebyshev Rational Functions: CHEF Functions (Image 1 of 2) Y. Jiménez-Teja and N. Benítez 2012 ApJ.

Figure 1 from The EMPIRE Survey: Systematic Variations in the Dense Gas Fraction and Star Formation Efficiency from Full-disk Mapping of M51 Frank Bigiel.

Figure 6 from Detailed Compositional Analysis of the Heavily Polluted DBZ White Dwarf SDSS J : A Window on Planet Formation? (Image 1.

Tomoharu Oka et al ApJS doi: / /201/2/14 Information:

Figure 2 from The Physical Characterization of the Potentially Hazardous Asteroid 2004 BL86: A Fragment of a Differentiated Asteroid Vishnu Reddy et al.

Figure 2 from Mid-Infrared Properties of OH Megamaser Host Galaxies. I

Figure 11 from The Galactic O-Star Spectroscopic Survey (GOSSS). II

Presentation transcript:

Figure 3.1 from Witnessing the Differential Evolution of Disk Galaxies in Luminosity and Size via Gravitational Lensing (Image 1 of 5) Kaushala Bandara et al. 2013 ApJ 777 1 doi:10.1088/0004-637X/777/1/1 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

Figure 3.1 from Witnessing the Differential Evolution of Disk Galaxies in Luminosity and Size via Gravitational Lensing (Image 2 of 5) Kaushala Bandara et al. 2013 ApJ 777 1 doi:10.1088/0004-637X/777/1/1 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

Figure 3.1 from Witnessing the Differential Evolution of Disk Galaxies in Luminosity and Size via Gravitational Lensing (Image 3 of 5) Kaushala Bandara et al. 2013 ApJ 777 1 doi:10.1088/0004-637X/777/1/1 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

Figure 3.1 from Witnessing the Differential Evolution of Disk Galaxies in Luminosity and Size via Gravitational Lensing (Image 4 of 5) Kaushala Bandara et al. 2013 ApJ 777 1 doi:10.1088/0004-637X/777/1/1 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

Figure 3.1 from Witnessing the Differential Evolution of Disk Galaxies in Luminosity and Size via Gravitational Lensing (Image 5 of 5) Kaushala Bandara et al. 2013 ApJ 777 1 doi:10.1088/0004-637X/777/1/1 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.