Abstract is: Tod R. Lauer (born 1957) is an American astronomer on the research staff of the National Optical Astronomy Observatory. He was a member of the Hubble Space Telescope Wide Field and Planetary Camera team, and is a founding member of the Nuker Team. His research interests includes observational searches for massive black holes in the centers of galaxies, the structure of elliptical galaxies, stellar populations, large-scale structure of the universe, and astronomical image processing. He was the Principal Investigator of the Destiny JDEM concept study, one of the precursors to the Nancy Grace Roman Space Telescope mission. Asteroid 3135 Lauer is named for him. He appears in an episode of the documentary series Naked Science. He joined the New Horizons Pluto team in order to apply his extensive experience with deep space imaging to the New Horizons data, yielding significantly clearer and mathematically accurate images of Pluto and Charon.
human | Q5 |
P6178 | Dimensions author ID | 016121745601.24 |
P646 | Freebase ID | /m/026z8xj |
P1960 | Google Scholar author ID | 1bg9b1kAAAAJ |
P2930 | INSPIRE-HEP author ID | T.R.Lauer.1 |
P213 | ISNI | 0000000109551739 |
P244 | Library of Congress authority ID | no95058593 |
P496 | ORCID iD | 0000-0003-3234-7247 |
P3987 | SHARE Catalogue author ID | 15840 |
P10861 | Springer Nature person ID | 016121745601.24 |
P214 | VIAF ID | 11894352 |
P166 | award received | NASA Exceptional Scientific Achievement Medal | Q17091138 |
P27 | country of citizenship | United States of America | Q30 |
P69 | educated at | University of California, Santa Cruz | Q1047293 |
California Institute of Technology | Q161562 | ||
P108 | employer | Princeton University | Q21578 |
National Optical Astronomy Observatory | Q1315390 | ||
P734 | family name | Lauer | Q28150821 |
Lauer | Q28150821 | ||
Lauer | Q28150821 | ||
P735 | given name | Tod | Q18697527 |
Tod | Q18697527 | ||
P106 | occupation | astronomer | Q11063 |
P551 | residence | Arizona | Q816 |
P21 | sex or gender | male | Q6581097 |
Q59981081 | A Hubble Space Telescope survey for novae in M87 – III. Are novae good standard candles 15 d after maximum brightness? |
Q58330364 | A Hubble Space Telescope survey for novae in M87. I. Light and color curves, spatial distributions, and the nova rate |
Q58330348 | A Radio Relic and a Search for the Central Black Hole in the Abell 2261 Brightest Cluster Galaxy |
Q29030846 | A Relationship between Nuclear Black Hole Mass and Galaxy Velocity Dispersion |
Q116213961 | A Universal Power-law Prescription for Variability from Synthetic Images of Black Hole Accretion Flows |
Q56502135 | A brightest cluster galaxy with an extremely large flat core |
Q58330639 | A candidate sub-parsec supermassive binary black hole system |
Q58330831 | A family of models for spherical stellar systems |
Q34300921 | A magnified young galaxy from about 500 million years after the Big Bang |
Q58330624 | A quintet of black hole mass determinations |
Q58330634 | A stellar dynamical measurement of the black hole mass in the maser galaxy NGC 4258 |
Q58330362 | AHubble Space TelescopeSurvey for Novae in M87. II. Snuffing out the Maximum Magnitude–Rate of Decline Relation for Novae as a Non-standard Candle, and a Prediction of the Existence of Ultrafast Novae |
Q58330581 | Adaptive Optics-Based Measurements of the Black Hole in Abell 2162–BCG |
Q56934589 | An Erupting Classical Nova in a Globular Cluster of M87 |
Q58330437 | An ancient metal-poor population in M32, and halo satellite accretion in M31, identified by RR Lyrae stars |
Q58330761 | AnI-Band-selected Sample of Radio-emitting Quasars: Evidence for a Large Population of Red Quasars |
Q58330764 | Axisymmetric Dynamical Models of the Central Regions of Galaxies |
Q58330787 | Axisymmetric, Three-Integral Models of Galaxies: A Massive Black Hole in NGC 3379 |
Q57310504 | Basins, fractures and volcanoes: Global cartography and topography of Pluto from New Horizons |
Q58330783 | Black Hole Mass Estimates from Reverberation Mapping and from Spatially Resolved Kinematics |
Q58330596 | Boroson and Lauer reply |
Q57310507 | Breaking up is hard to do: Global cartography and topography of Pluto's mid-sized icy Moon Charon from New Horizons |
Q58330812 | Brightest Cluster Galaxy Profile Shapes |
Q58330826 | Brightest cluster galaxies as standard candles |
Q58330390 | Brightest cluster galaxies at the present epoch |
Q115593414 | Broadband Multi-wavelength Properties of M87 during the 2017 Event Horizon Telescope Campaign |
Q56442928 | Calibration of the Surface Brightness Fluctution Method for use with the Hubble Space Telescope |
Q58330824 | Can standard cosmological models explain the observed Abell cluster bulk flow? |
Q116213960 | Characterizing and Mitigating Intraday Variability: Reconstructing Source Structure in Accreting Black Holes with mm-VLBI |
Q41040015 | Charon tectonics |
Q110248431 | Charon’s Far Side Geomorphology |
Q58330355 | Climate zones on Pluto and Charon |
Q58330795 | Clustering at High Redshift: Precise Constraints from a Deep, Wide‐Area Survey |
Q58330644 | Color bimodality in M87 globular clusters |
Q58330792 | Combining Undersampled Dithered Images |
Q58330604 | Compact high-redshift galaxies are the cores of the most massive present-day spheroids |
Q116213970 | Constraints on black-hole charges with the 2017 EHT observations of M87* |
Q58330865 | Core expansion in young star clusters in the Large Magellanic Cloud |
Q58330416 | Cores and the kinematics of early-type galaxies |
Q58330357 | Craters of the Pluto-Charon system |
Q58330713 | DESTINY: The dark energy space telescope |
Q58330683 | DESTINY: the dark energy space telescope |
Q58330766 | Deconvolution with a spatially-variant PSF |
Q58330706 | Destiny: a candidate architecture for the Joint Dark Energy Mission |
Q58330791 | Detailed Surface Photometry of Dwarf Elliptical and Dwarf S0 Galaxies in the Virgo Cluster |
Q58330803 | Detection of the Tip of the Red Giant Branch in NGC 3379 (M105) in the Leo I Group Using the Hubble Space Telescope |
Q58330649 | Dissipation and extra light in galactic nuclei. II. "Cusp" ellipticals |
Q58330630 | Dissipation and extra light in galactic nuclei. III. "Core" ellipticals and "missing" light |
Q56081078 | Dunes on Pluto |
Q56005245 | Dynamical measurements of black hole masses in four brightest cluster galaxies at 100 mpc |
Q58330748 | E+A Galaxies and the Formation of Early‐Type Galaxies atz ∼ 0 |
Q58330796 | Erratum: “The Nuclear Region of M51 Imaged with the [ITAL]HST[/ITAL] Planetary Camera” [Astron. J. [BF]113[/BF], 225 (1997)] |
Q116213954 | Event Horizon Telescope imaging of the archetypal blazar 3C 279 at an extreme 20 microarcsecond resolution |
Q116213944 | Event Horizon Telescope observations of the jet launching and collimation in Centaurus A |
Q58330577 | Exploring the spectral space of low redshift QSOs |
Q63087930 | First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole |
Q63087935 | First M87 Event Horizon Telescope Results. II. Array and Instrumentation |
Q63087934 | First M87 Event Horizon Telescope Results. III. Data Processing and Calibration |
Q63087932 | First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole |
Q63087931 | First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring |
Q63088081 | First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole |
Q116213953 | First M87 Event Horizon Telescope Results. VII. Polarization of the Ring |
Q116213951 | First M87 Event Horizon Telescope Results. VIII. Magnetic Field Structure near The Event Horizon |
Q116213969 | First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way |
Q116213971 | First Sagittarius A* Event Horizon Telescope Results. II. EHT and Multiwavelength Observations, Data Processing, and Calibration |
Q116213959 | First Sagittarius A* Event Horizon Telescope Results. III. Imaging of the Galactic Center Supermassive Black Hole |
Q116213972 | First Sagittarius A* Event Horizon Telescope Results. IV. Variability, Morphology, and Black Hole Mass |
Q116213966 | First Sagittarius A* Event Horizon Telescope Results. V. Testing Astrophysical Models of the Galactic Center Black Hole |
Q116213973 | First Sagittarius A* Event Horizon Telescope Results. VI. Testing the Black Hole Metric |
Q58330774 | Galaxies with a Central Minimum in Stellar Luminosity Density |
Q69820026 | Geologic Landforms and Chronostratigraphic History of Charon as Revealed by a Hemispheric Geologic Map |
Q57308277 | Geological mapping of Sputnik Planitia on Pluto |
Q58330874 | Global Stellar Populations of Elliptical Galaxies: B. Ultraviolet Energy Distributions |
Q100676658 | Gravitational Test beyond the First Post-Newtonian Order with the Shadow of the M87 Black Hole |
Q59751236 | Great Expectations: Plans and Predictions for New Horizons Encounter With Kuiper Belt Object 2014 MU69 (“Ultima Thule”) |
Q53952308 | HSTSTIS Spectroscopy of the Triple Nucleus of M31: Two Nested Disks in Keplerian Rotation around a Supermassive Black Hole |
Q58330367 | High-resolution mapping of dust via extinction in the M31 bulge |
Q56603866 | Hubble Space Telescope Planetary Camera images of R136 |
Q58330853 | Hubble Space Telescope imaging of Eta Carinae |
Q58330606 | Hubble space telescope images and KPNO spectroscopy of the binary black hole candidate SDSS J153636.22+044127.0 |
Q58330658 | Hubble's unsung heroes |
Q124851253 | Imaging Lunar Craters with the Lucy Long Range Reconnaissance Imager (L’LORRI): A Resolution Test for NASA's Lucy Mission |
Q92022941 | Impact craters on Pluto and Charon indicate a deficit of small Kuiper belt objects |
Q63918383 | Initial results from the New Horizons exploration of 2014 MU69, a small Kuiper Belt object |
Q58330857 | Ionization fronts and shocked flows - The structure of the Orion Nebula at 0.1 arcsec |
Q56032065 | Is there a black hole in NGC 4382? |
Q58330759 | Kinematics of 10 Early‐Type Galaxies fromHubble Space Telescopeand Ground‐based Spectroscopy |
Q56934437 | Luminosity Function of Faint Globular Clusters in M87 |
Q58330793 | M32+/-1 |
Q58330585 | M32: Is there an Ancient and Metal-poor Stellar Population? |
Q58330777 | M33: A Galaxy with No Supermassive Black Hole |
Q55923525 | Mean radius and shape of Pluto and Charon from New Horizons images |
Q56934653 | Microlensing Candidates in M87 and the Virgo Cluster with the Hubble Space Telescope |
Q116213957 | Millimeter Light Curves of Sagittarius A* Observed during the 2017 Event Horizon Telescope Campaign |
Q116213937 | Monitoring the Morphology of M87* in 2009–2017 with the Event Horizon Telescope |
Q58330769 | NOAO Science Archive |
Q58330782 | Observational Constraints on Higher Order Clustering up toz≃ 1 |
Q58330524 | Orbit-based dynamical models of the Sombrero galaxy (NGC 4594) |
Q104739849 | Origins of pits and troughs and degradation on a small primitive planetesimal in the Kuiper Belt: high-resolution topography of (486958) Arrokoth (aka 2014 MU69) from New Horizons |
Q64166801 | Overview of the DESI Legacy Imaging Surveys |
Q58330879 | Photometric decomposition of the multiple-nucleus galaxy NGC 6166 |
Q58330380 | Photometric evidence of an intermediate-age stellar population in the inner bulge of M31 |
Q58330850 | Planetary Camera observations of the M87 stellar cusp |
Q56031842 | Planetary camera observations of the central parsec of M32 |
Q113950528 | Polarimetric Properties of Event Horizon Telescope Targets from ALMA |
Q58330662 | Precision attitude determination for an infrared space telescope |
Q58330347 | Principal Component Analysis as a Tool for Characterizing Black Hole Images and Variability |
Q59784610 | RR Lyrae variables in M32 and the disk of M31 |
Q58330614 | RR Lyrae variables in two fields in the spheroid of M31 |
Q58330757 | Red Galaxy Clustering in the NOAO Deep Wide‐Field Survey |
Q114023005 | Resolving the Inner Parsec of the Blazar J1924–2914 with the Event Horizon Telescope |
Q58330677 | Selection Bias in Observing the Cosmological Evolution of theM•‐σ andM•‐LRelationships |
Q116213965 | Selective Dynamical Imaging of Interferometric Data |
Q58330668 | Simulations of sample-up-the-ramp for space-based observations of faint sources |
Q58330800 | Spectroscopic Evidence for a Supermassive Black Hole in NGC 4486B |
Q58330558 | Stardust-NExT, Deep Impact, and the accelerating spin of 9P/Tempel 1 |
Q58330858 | Stellar photometry with the Hubble Space Telescope Wide-field/Planetary camera - A progress report |
Q58330360 | Sublimation as a landform-shaping process on Pluto |
Q56169483 | THEM-σ ANDM-LRELATIONS IN GALACTIC BULGES, AND DETERMINATIONS OF THEIR INTRINSIC SCATTER |
Q58330734 | Technical implementation of the DESTINY mission concept |
Q56005266 | The Black Hole Mass and Extreme Orbital Structure in NGC 1399 |
Q58330813 | The Centers of Early-Type Galaxies With HST. III. Non-Parametric Recovery of Stellar Luminosity Distribution |
Q57406844 | The Centers of Early-Type Galaxies with HST. IV. Central Parameter Relations |
Q58330726 | The Centers of Early-Type Galaxies withHubble Space Telescope. V. New WFPC2 Photometry |
Q58330692 | The Centers of Early‐Type Galaxies withHubble Space Telescope. VI. Bimodal Central Surface Brightness Profiles |
Q58330739 | The DESTINY concept for the Joint Dark Energy Mission (JDEM) |
Q110248626 | The Dark Side of Pluto |
Q55879578 | The Demography of Massive Dark Objects in Galaxy Centers |
Q116213946 | The Event Horizon General Relativistic Magnetohydrodynamic Code Comparison Project |
Q58330798 | The Far‐Field Hubble Constant |
Q56943282 | The Galactic Exoplanet Survey Telescope (GEST) |
Q58330844 | The Hubble flow from brightest cluster galaxies |
Q58330780 | The Infrared Surface Brightness Fluctuation Hubble Constant |
Q58330773 | The KPNO/Deeprange Distant Cluster Survey. I. The Catalog and the Space Density of Intermediate‐Redshift Clusters |
Q58330696 | The Masses of Nuclear Black Holes in Luminous Elliptical Galaxies and Implications for the Space Density of the Most Massive Black Holes |
Q58330841 | The Motion of the Local Group with Respect to the 15,000 km/s Abell Cluster Frame |
Q58330805 | The Nuclear Region of M51 Imaged with the HST Planetary Camera |
Q57524274 | The Panchromatic Hubble Andromeda Treasury. X. Ultraviolet to infrared photometry of 117 million equidistant stars |
Q58330790 | The Photometry of Undersampled Point‐Spread Functions |
Q27011937 | The Pluto system: Initial results from its exploration by New Horizons |
Q116213938 | The Polarized Image of a Synchrotron-emitting Ring of Gas Orbiting a Black Hole |
Q58330776 | The Slope of the Black Hole Mass versus Velocity Dispersion Correlation |
Q58330591 | The Stellar Populations of M32: Resolving the nearest elliptical with HST ACS/HRC |
Q116213941 | The Variability of the Black Hole Image in M87 at the Dynamical Timescale |
Q58330398 | The black hole mass and the stellar ring in NGC 3706 |
Q53952639 | The black hole mass in M87 from Gemini/NIFS adaptive optics observations |
Q58330564 | The black hole mass in the brightest cluster galaxy NGC 6086 |
Q58330487 | The cluster of blue stars surrounding the M31 nuclear black hole |
Q58330859 | The core of the nearby S0 galaxy NGC 7457 imaged with the HST planetary camera |
Q58330571 | The deepest Hubble space telescope color-magnitude diagram of M32. Evidence for intermediate-age populations |
Q58330400 | The effect of spatial gradients in stellar mass-to-light ratio on black hole mass measurements |
Q58330871 | The far-ultraviolet spectra of early-type galaxies |
Q30277136 | The geology of Pluto and Charon through the eyes of New Horizons |
Q58330872 | The morphology of multiple-nucleus brightest cluster galaxies |
Q58330828 | The motion of the Local Group with respect to the 15,000 kilometer per second Abell cluster inertial frame |
Q56601248 | The nuclear regions of NGC 3311 and NGC 7768 imaged with the Hubble Space Telescope Planetary Camera |
Q58330846 | The nucleus of M32 at 0.2 arcsec resolution |
Q57524297 | The panchromatic Hubble Andromeda treasury |
Q57524291 | The panchromatic Hubble Andromeda treasury. I. Bright UV stars in the bulge of M31 |
Q58330426 | The panchromatic Hubble Andromeda treasury. II. Tracing the inner M31 halo with blue horizontal branch stars |
Q58330395 | The panchromatic Hubble Andromeda treasury. VII. The steep mid-ultraviolet to near-infrared extinction curve in the central 200 pc of the M31 bulge |
Q58330372 | The panchromatic Hubble Andromeda treasury. VIII. A wide-area, high-resolution map of dust extinction in M31 |
Q58330861 | The postcollapse core of M15 imaged with the HST planetary camera |
Q58330868 | The reduction of wide field/planetary camera images |
Q58330835 | The shapes of brightest cluster galaxies |
Q58330501 | The star formation history of M32 |
Q58330386 | Tracing the metal-poor M31 stellar halo with blue horizontal branch stars |
Q34029756 | Two ten-billion-solar-mass black holes at the centres of giant elliptical galaxies |
Q116213936 | Verification of Radiative Transfer Schemes for the EHT |
Q58330762 | [ITAL]Hubble Space Telescope[/ITAL] Imaging of Brightest Cluster Galaxies |
Q58330810 | [ITAL]Hubble Space Telescope[/ITAL] Observations of the Double Nucleus of NGC 4486B |
Q53952732 | [ITAL]Hubble Space Telescope[/ITAL] Spectroscopic Evidence for a 1 × 10[TSUP]9[/TSUP] [ITAL]M[/ITAL][TINF]⊙[/TINF] Black Hole in NGC 4594 |
Q748227 | 3135 Lauer | named after | P138 |
Egyptian Arabic (arz / Q29919) | تود ر | wikipedia |
Tod R. Lauer | wikipedia | |
Esperanto (eo / Q143) | Tod R. Lauer | wikipedia |
Թոդ Լաուեր | wikipedia | |
Tod R. Lauer | wikipedia | |
ta | தோடு ஆர். இலவுவேர் | wikipedia |
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