Max Tegmark

Q: What Schools Are Affiliated With Max Tegmark

Max Tegmark is affiliated with the following schools: KTH Royal Institute of Technology, University of California, Berkeley, Stockholm School of Economics, Massachusetts Institute of Technology

Q: What Are Max Tegmark's Academic Contributions?

Max Tegmark has made the following academic contributions: Our Mathematical Universe, Life 3.0

Why Is Max Tegmark Influential?

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By Erik J. Larson, PhD

Max Tegmark was born in Stockholm, Sweden in 1967. He received a BA in economics from the Stockholm School of Economics and completed a BSc degree in physics a year later at the KTH Royal Institute of Technology. He then ventured to the University of California, Berkeley where he earned an MA and PhD studying physics. He is a professor at the Massachusetts Institute of Technology and the Scientific Director of the Foundational Questions Institute. He is also a co-founder along with Skype founder Jaan Tallinn of the Future of Life Institute, which examines issues of existential risk, particularly the some think we face by the advance of artificial intelligence leading to superintelligent machines.

Tegmark’s primary work has been in the area of cosmology. Along with physicists Daniel Eisenstein and Wayne Hu, he introduced the idea of using “baryon acoustic oscillations” as a so-called “standard ruler” in cosmology—a known physical length used to measure cosmological phenomena. Baryon acoustic oscillations are fluctuations in the density of visible baryons in the universe. He has also helped develop the theory of the cosmological interpretation of quantum mechanics, where quantum mechanics describes not possibilities by infinite sequences of actual phenomena.

Tegmark’s books include Our Mathematical Universe and Life 3.0: Being Human in the Age of Artificial Intelligence. He was elected Fellow of the American Physical Society in 2012.

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Featured in Top Influential Physicists Today

According to Wikipedia, Max Erik Tegmark is a Swedish-American physicist, cosmologist and machine learning researcher. He is a professor at the Massachusetts Institute of Technology and the president of the Future of Life Institute. He is also a scientific director at the Foundational Questions Institute and a supporter of the effective altruism movement.

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Max Tegmark's Published Works

Number of citations in a given year to any of this author's works

Total number of citations to an author for the works they published in a given year. This highlights publication of the most important work(s) by the author

Published Papers

THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY (2008) (3973)
Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies (2005) (3546)
Cosmological parameters from SDSS and WMAP (2003) (3123)
Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample (2009) (1394)
The Three-Dimensional Power Spectrum of Galaxies from the Sloan Digital Sky Survey (2004) (1237)
The Sixth Data Release of the Sloan Digital Sky Survey (2007) (1219)
Cosmological constraints from the SDSS luminous red galaxies (2006) (1204)
The 3D power spectrum of galaxies from the SDSS (2003) (1000)
New York University Value-Added Galaxy Catalog: A Galaxy Catalog Based on New Public Surveys (2005) (924)
The Galaxy Luminosity Function and Luminosity Density at Redshift z = 0.1 (2002) (868)
Cosmological parameter analysis including SDSS Lyα forest and galaxy bias: Constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy (2004) (858)
The First Data Release of the Sloan Digital Sky Survey (2003) (768)
Karhunen-Loève Eigenvalue Problems in Cosmology: How Should We Tackle Large Data Sets? (1996) (742)
The Fifth Data Release of the Sloan Digital Sky Survey (2007) (631)
The Luminosity and Color Dependence of the Galaxy Correlation Function (2004) (622)
How Small Were the First Cosmological Objects? (1996) (619)
NYU-VAGC: a galaxy catalog based on new public surveys (2004) (576)
GALAXY CLUSTERING IN THE COMPLETED SDSS REDSHIFT SURVEY: THE DEPENDENCE ON COLOR AND LUMINOSITY (2010) (563)
The role of artificial intelligence in achieving the Sustainable Development Goals (2019) (531)
The Second Data Release of the Sloan Digital Sky Survey (2004) (528)
Research Priorities for Robust and Beneficial Artificial Intelligence (2015) (504)
Why Does Deep and Cheap Learning Work So Well? (2016) (503)
Cosmological constraints from the clustering of the Sloan Digital Sky Survey DR7 luminous red galaxies (vol 404, pg 60, 2010) (2009) (494)
Galaxy Clustering in Early Sloan Digital Sky Survey Redshift Data (2002) (488)
Significance of the largest scale CMB fluctuations in WMAP (2003) (485)
Nanophotonic particle simulation and inverse design using artificial neural networks (2017) (474)
High resolution foreground cleaned CMB map from WMAP (2003) (469)
The Fourth Data Release of the Sloan Digital Sky Survey (2005) (461)
The importance of quantum decoherence in brain processes (1999) (425)
The Mathematical Universe (2007) (393)
A Map of the Universe (2003) (376)
Hydrogen Epoch of Reionization Array (HERA) (2015) (371)
A model of diffuse Galactic radio emission from 10 MHz to 100 GHz (2008) (336)
The Third Data Release of the Sloan Digital Sky Survey (2004) (329)
Measuring Cosmological Parameters with Galaxy Surveys (1997) (328)
Limits on non-Gaussianities from WMAP data (2005) (325)
The end of unified dark matter (2002) (321)
AI Feynman: A physics-inspired method for symbolic regression (2019) (315)
Weighing Neutrinos with Galaxy Surveys (1997) (311)
Dimensionless constants, cosmology and other dark matters (2005) (306)
Constraining f ( R ) gravity as a scalar-tensor theory (2006) (302)
The clustering of luminous red galaxies in the Sloan Digital Sky Survey imaging data (2006) (297)
How to measure CMB power spectra without losing information (1996) (285)
A method for subtracting foregrounds from multifrequency CMB sky maps (1995) (274)
A Measurement of the CMB ⟨EE⟩ Spectrum from the 2003 Flight of BOOMERANG (2005) (259)
On Departures from a Power Law in the Galaxy Correlation Function (2003) (254)
Foregrounds and Forecasts for the Cosmic Microwave Background (1999) (247)
Cosmic Complementarity: Joint Parameter Estimation from Cosmic Microwave Background Experiments and Redshift Surveys (1998) (238)
Cosmological Parameters from Eigenmode Analysis of Sloan Digital Sky Survey Galaxy Redshifts (2004) (227)
A Measurement of the Angular Power Spectrum of the CMB Temperature Anisotropy from the 2003 Flight of BOOMERANG (2005) (223)
Forecasting cosmic parameter errors from microwave background anisotropy experiments (1997) (221)
Is “the Theory of Everything” Merely the Ultimate Ensemble Theory? (1997) (221)
Inflationary Constraints on Type IIA String Theory (2007) (219)
The Shape of the Sloan Digital Sky Survey Data Release 5 Galaxy Power Spectrum (2007) (218)
Our Mathematical Universe: My Quest for the Ultimate Nature of Reality (2014) (215)
New dark energy constraints from supernovae, microwave background, and galaxy clustering. (2004) (211)
WHAT NEXT-GENERATION 21 cm POWER SPECTRUM MEASUREMENTS CAN TEACH US ABOUT THE EPOCH OF REIONIZATION (2013) (209)
Analysis of Systematic Effects and Statistical Uncertainties in Angular Clustering of Galaxies from Early Sloan Digital Sky Survey Data (2001) (206)
How accurately can 21cm tomography constrain cosmology (2008) (202)
What does inflation really predict? (2004) (199)
Axion cosmology and the energy scale of inflation (2008) (196)
Cosmological Parameters from the 2003 Flight of BOOMERANG (2005) (193)
The shape of the SDSS DR5 galaxy power spectrum (2006) (193)
The Intermediate-Scale Clustering of Luminous Red Galaxies (2004) (186)
The Time Evolution of Bias (1998) (186)
Cosmic Microwave Background Observables and Their Cosmological Implications (2001) (177)
Measuring the Galaxy Power Spectrum with Future Redshift Surveys (1997) (173)
Life 3.0: Being Human in the Age of Artificial Intelligence (2017) (173)
CMB Observables and Their Cosmological Implications (2000) (171)
The Interpretation of Quantum Mechanics: Many Worlds or Many Words? (1997) (163)
Tunable Efficient Unitary Neural Networks (EUNN) and their application to RNNs (2016) (161)
Methods for rapidly processing angular masks of next-generation galaxy surveys (2007) (159)
An Icosahedron-based Method for Pixelizing the Celestial Sphere (1996) (154)
Uncorrelated measurements of the cosmic expansion history and dark energy from supernovae (2005) (153)
Using the kinematic Sunyaev-Zeldovich effect to determine the peculiar velocities of clusters of galaxies (1995) (153)
The power of deeper networks for expressing natural functions (2017) (147)
A Measurement of the Polarization-Temperature Angular Cross-Power Spectrum of the Cosmic Microwave Background from the 2003 Flight of BOOMERANG (2005) (142)
The power spectrum of galaxies in the 2dF 100k redshift survey (2001) (142)
Overcoming real-world obstacles in 21 cm power spectrum estimation: A method demonstration and results from early Murchison Widefield Array data (2013) (137)
FIRST SEASON MWA EOR POWER SPECTRUM RESULTS AT REDSHIFT 7 (2016) (137)
Consciousness as a state of matter (2014) (136)
SDSS galaxy bias from halo mass-bias relation and its cosmological implications (2004) (135)
Is cosmology consistent (2001) (135)
Testing two-field inflation (2010) (133)
Weak Lensing: Prospects for Measuring Cosmological Parameters (1998) (130)
Fast Fourier transform telescope (2008) (128)
21 cm Tomography with Foregrounds (2006) (126)
A method for 21 cm power spectrum estimation in the presence of foregrounds (2011) (125)
How to Make Maps from Cosmic Microwave Background Data without Losing Information (1996) (122)
Constraints from the Lyα Forest Power Spectrum (2000) (120)
CMB mapping experiments: a designer's guide (1997) (117)
Separating the early universe from the late universe: Cosmological parameter estimation beyond the black box (2002) (117)
A Brute Force Analysis of the COBE DMR Data (1994) (115)
How to measure CMB polarization power spectra without losing information (2000) (115)
Angular Clustering with Photometric Redshifts in the Sloan Digital Sky Survey: Bimodality in the Clustering Properties of Galaxies (2003) (115)
Why Is the Cosmic Microwave Background Fluctuation Level 10−5? (1998) (113)
Instrument, Method, Brightness and Polarization Maps from the 2003 flight of BOOMERanG (2005) (110)
Gated Orthogonal Recurrent Units: On Learning to Forget (2017) (108)
100 years of the quantum (2001) (103)
Improved Measures of Integrated Information (2016) (102)
CMB multipole measurements in the presence of foregrounds (2006) (102)
An improved method for 21‐cm foreground removal (2009) (102)
Precision calibration of radio interferometers using redundant baselines (2010) (101)
FOREGROUNDS IN WIDE-FIELD REDSHIFTED 21 cm POWER SPECTRA (2015) (101)
A scheme to deal accurately and efficiently with complex angular masks in galaxy surveys (2003) (97)
Why is the CMB fluctuation level 10^{-5}? (1997) (97)
Towards a refined cosmic concordance model: Joint 11-parameter constraints from the cosmic microwave background and large-scale structure (2000) (94)
Task force on cosmic microwave background research (2006) (93)
Constraining Torsion with Gravity Probe B (2006) (92)
SDSS galaxy clustering: luminosity and colour dependence and stochasticity (2007) (92)
Cross-Correlation of Tenerife Data with Galactic Templates—Evidence for Spinning Dust? (1999) (92)
The Low-Frequency Environment of the Murchison Widefield Array: Radio-Frequency Interference Analysis and Mitigation (2015) (89)
Apparent wave function collapse caused by scattering (1993) (86)
Empirical covariance modeling for 21 cm power spectrum estimation: A method demonstration and new limits from early Murchison Widefield Array 128-tile data (2015) (85)
Cosmology and the Halo Occupation Distribution from Small-Scale Galaxy Clustering in the Sloan Digital Sky Survey (2004) (85)
How well can we measure and understand foregrounds with 21-cm experiments? (2011) (83)
The Three-dimensional Power Spectrum from Angular Clustering of Galaxies in Early Sloan Digital Sky Survey Data (2002) (82)
The Quest for Microwave Foreground X (2003) (82)
Combined reconstruction of weak and strong lensing data with WSLAP (2005) (81)
CHIPS: THE COSMOLOGICAL H i POWER SPECTRUM ESTIMATOR (2016) (80)
The Angular Correlation Function of Galaxies from Early Sloan Digital Sky Survey Data (2001) (79)
Current Cosmological Constraints from a 10 Parameter Cosmic Microwave Background Analysis (2000) (77)
Non-parametric inversion of strong lensing systems (2004) (77)
Non-Gaussianity in Two-Field Inflation (2010) (76)
Sloan Digital Sky Survey Imaging of Low Galactic Latitude Fields: Technical Summary and Data Release (2004) (75)
MITEoR: a scalable interferometer for precision 21 cm cosmology (2014) (75)
Removing Point Sources from Cosmic Microwave Background Maps (1998) (75)
Time Evolution of Galaxy Formation and Bias in Cosmological Simulations (1999) (74)
An Improved Model of Diffuse Galactic Radio Emission from 10 MHz to 5 THz (2016) (73)
Twenty-one centimeter tomography with foregrounds (2005) (73)
Late reionization by supernova-driven winds (1993) (72)
Multiple universes, cosmic coincidences, and other dark matters (2004) (72)
The real-space power spectrum of the PSCz survey from 0.01 to 300 h Mpc−1 (2000) (71)
Large-Scale Sunyaev-Zeldovich Effect: Measuring Statistical Properties with Multifrequency Maps (2000) (70)
Testing Multi-Field Inflation: A Geometric Approach (2011) (70)
Will point sources spoil 21-cm tomography? (2008) (70)
The Angular Power Spectrum of Galaxies from Early Sloan Digital Sky Survey Data (2001) (69)
Stephen Hawking: \'Transcendence looks at the implications of artificial intelligence - but are we taking AI seriously enough?\' (2014) (68)
A New Spin on Galactic Dust (2000) (68)
Why Is the Fraction of Four-Image Radio Lens Systems So High? (2000) (67)
Limits on f_NL parameters from WMAP 3yr data (2006) (67)
Physical evidence for dark energy (2003) (67)
Toward an artificial intelligence physicist for unsupervised learning. (2019) (66)
Measuring the metric: A parametrized post-Friedmannian approach to the cosmic dark energy problem (2001) (66)
Omniscopes: Large area telescope arrays with only NlogN computational cost (2009) (64)
AI Feynman 2.0: Pareto-optimal symbolic regression exploiting graph modularity (2020) (63)
Observationally determining the properties of dark matter (1998) (63)
Limits on fNL parameters from Wilkinson Microwave Anisotropy Probe three-year data (2007) (63)
First limits on the 21 cm power spectrum during the Epoch of X-ray heating (2016) (62)
Karhunen-Loève Estimation of the Power Spectrum Parameters from the Angular Distribution of Galaxies in Early Sloan Digital Sky Survey Data (2001) (62)
Decorrelating the power spectrum of galaxies (1999) (62)
THE MURCHISON WIDEFIELD ARRAY 21 cm POWER SPECTRUM ANALYSIS METHODOLOGY (2016) (62)
New microwave background constraints on the cosmic matter budget: trouble for nucleosynthesis? (2000) (61)
ON THE INEVITABILITY OF REIONIZATION : IMPLICATIONS FOR COSMIC MICROWAVE BACKGROUND FLUCTUATIONS (1993) (60)
CONFIRMATION OF WIDE-FIELD SIGNATURES IN REDSHIFTED 21 cm POWER SPECTRA (2015) (59)
Observational Evidence for Stochastic Biasing (1998) (59)
The Multiverse Hierarchy (2009) (58)
Born in an Infinite Universe: A Cosmological Interpretation of Quantum Mechanics (2010) (58)
Removing Real-World Foregrounds from Cosmic Microwave Background Maps (1998) (57)
Is the Cosmic Microwave Background Really Non-Gaussian? (1999) (56)
THE HYDROGEN EPOCH OF REIONIZATION ARRAY DISH. I. BEAM PATTERN MEASUREMENTS AND SCIENCE IMPLICATIONS (2016) (53)
THE IMPORTANCE OF WIDE-FIELD FOREGROUND REMOVAL FOR 21 cm COSMOLOGY: A DEMONSTRATION WITH EARLY MWA EPOCH OF REIONIZATION OBSERVATIONS (2016) (53)
Cosmic Complementarity: H0 and Ωm from Combining Cosmic Microwave Background Experiments and Redshift Surveys (1998) (52)
A fast method for power spectrum and foreground analysis for 21 cm cosmology (2012) (52)
On the dimensionality of spacetime (1997) (51)
Critical Behavior in Physics and Probabilistic Formal Languages (2017) (50)
Parametrizing Epoch of Reionization foregrounds: a deep survey of low-frequency point-source spectra with the Murchison Widefield Array (2016) (49)
LOW-FREQUENCY OBSERVATIONS OF LINEARLY POLARIZED STRUCTURES IN THE INTERSTELLAR MEDIUM NEAR THE SOUTH GALACTIC POLE (2016) (48)
A Limit on the Large Angular Scale Polarization of the Cosmic Microwave Background (2001) (47)
An Elementary Proof That the Biharmonic Green Function of an Eccentric Ellipse Changes Sign (1994) (47)
Criticality in Formal Languages and Statistical Physics (2016) (46)
Two-dimensional Topology of the Sloan Digital Sky Survey (2002) (45)
Global 21 cm signal experiments: A designer’s guide (2012) (45)
Searching for Inflation in Simple String Theory Models: An Astrophysical Perspective (2007) (44)
Last stand before WMAP: Cosmological parameters from lensing, CMB, and galaxy clustering (2002) (43)
How unitary cosmology generalizes thermodynamics and solves the inflationary entropy problem (2011) (43)
Comparing Redundant and Sky-model-based Interferometric Calibration: A First Look with Phase II of the MWA (2018) (41)
THE HYDROGEN EPOCH OF REIONIZATION ARRAY DISH. II. CHARACTERIZATION OF SPECTRAL STRUCTURE WITH ELECTROMAGNETIC SIMULATIONS AND ITS SCIENCE IMPLICATIONS (2016) (40)
Many lives in many worlds (2007) (38)
Anthropic predictions for neutrino masses (2003) (38)
Does the universe in fact contain almost no information? (1996) (38)
LETTER TO THE EDITOR: On the dimensionality of spacetime (1997) (37)
Linear redshift distortions and power in the IRAS Point Source Catalog Redshift Survey (2000) (37)
Cosmic Complementarity: [ITAL]H[/ITAL][TINF]0[/TINF] and Ω[TINF][CLC][ITAL]m[/ITAL][/CLC][/TINF] from Combining Cosmic Microwave Background Experiments and Redshift Surveys (1998) (35)
A method for extracting maximum resolution power spectra from microwave sky maps (1994) (34)
The Angular Power Spectrum of BATSE 3B Gamma-Ray Bursts (1995) (34)
Decoherence produces coherent states: An explicit proof for harmonic chains. (1994) (34)
Mapping the Cosmic Microwave Background Anisotropy:The First Flight of the QMAP Experiment (1998) (34)
Measuring Spacetime: From the Big Bang to Black Holes (2002) (34)
Critical Behavior from Deep Dynamics: A Hidden Dimension in Natural Language (2016) (32)
Galactic Emission at 19 GHz (1998) (32)
Astrophysics: Is a doomsday catastrophe likely? (2005) (32)
AI Poincaré: Machine Learning Conservation Laws from Trajectories (2020) (31)
On Math, Matter and Mind (2005) (30)
Mapmaking for precision 21 cm cosmology (2014) (30)
Morphological Measures of Non-Gaussianity in Cosmic Microwave Background Maps (2002) (30)
A method for extracting maximum resolution power spectra from galaxy surveys (1995) (29)
A High-Resolution Map of the Cosmic Microwave Background around the North Celestial Pole (1996) (29)
Cosmology from the Highly-Redshifted 21 cm Line (2009) (29)
Learnability for the Information Bottleneck (2019) (29)
Baryon acoustic oscillations in the Sloan Digital Sky Survey Data Release 7 galaxy sample (vol 401, pg 2148, 2010) (2011) (29)
Cosmological neutrino bounds for non-cosmologists (2005) (28)
Assessing whether artificial intelligence is an enabler or an inhibitor of sustainability at indicator level (2021) (27)
Many Worlds in Context (2009) (27)
BOOMERanG constraints on primordial non-Gaussianity from analytical Minkowski functionals (2009) (27)
The Angular Power Spectrum of the Four-Year COBE Data (1996) (27)
Cosmic Complementarity: H 0 and Ω M from Combining Cmb Experiments and Redshift Surveys (26)
Toward an AI Physicist for Unsupervised Learning (2018) (24)
A high reliability survey of discrete Epoch of Reionization foreground sources in the MWA EoR0 field (2016) (23)
CMBFIT: Rapid WMAP likelihood calculations with normal parameters (2003) (22)
Likely values of the Higgs vev (2009) (22)
Symbolic Pregression: Discovering Physical Laws from Raw Distorted Video (2020) (21)
Reionization in an open CDM universe: implications for cosmic microwave background fluctuations (1994) (21)
Searching for Non-Gaussian Signals in the BOOMERANG 2003 CMB Maps (2007) (20)
Brute-force mapmaking with compact interferometers: a MITEoR northern sky map from 128 to 175 MHz (2016) (20)
Likely values of the Higgs vacuum expectation value (2010) (20)
Large-scale polarization of the microwave background and foreground (2002) (20)
Parallel universes. Not just a staple of science fiction, other universes are a direct implication of cosmological observations. (2003) (19)
Parallel universes? (2003) (19)
Meta-learning autoencoders for few-shot prediction (2018) (19)
Redundant-baseline calibration of the hydrogen epoch of reionization array (2020) (19)
Why the brain is probably not a quantum computer (2000) (19)
Galactic Contamination in the QMAP Experiment (2000) (18)
Anthropic predictions for vacuum energy and neutrino masses (2004) (18)
Removing real-world foregrounds from CMB maps (1997) (17)
The hydrogen epoch of reionization array dish III: measuring chromaticity of prototype element with reflectometry (2017) (17)
16p11.2 deletion is associated with hyperactivation of human iPSC-derived dopaminergic neuron networks and is rescued by RHOA inhibition in vitro (2021) (17)
Doppler peaks and all that: CMB anisotropies and what they can tell us (1995) (17)
Polarized Foreground Power Spectra from the HERA-19 Commissioning Array (2018) (17)
Spectral Energy Distribution and Radio Halo of NGC 253 at Low Radio Frequencies (2017) (17)
Mapping the CMB II: the second flight of the QMAP experiment (1998) (17)
The Power Spectrum of the CfA/SSRS UZC Galaxy Redshift Survey (1999) (17)
Measuring CMB polarization with Boomerang (2003) (17)
Shut up and calculate (2007) (17)
Pareto-Optimal Data Compression for Binary Classification Tasks (2019) (16)
On the dimensionality of space-time (1997) (16)
Improved Limits on Gamma-Ray Burst Repetition from BATSE (1995) (15)
Comparing and Combining Cosmic Microwave Background Data Sets (1999) (15)
THE 3D POWER SPECTRUM FROM ANGULAR CLUSTERING OF GALAXIES IN EARLY SDSS DATA 1 (2001) (15)
Assessment of Ionospheric Activity Tolerances for Epoch of Reionization Science with the Murchison Widefield Array (2018) (15)
Cosmological Constraints from Current Cosmic Microwave Background and Type Ia Supernova Data: A Brute Force, Eight-Parameter Analysis (1999) (15)
Mapping the Cosmic Microwave Background Anisotropy:Combined Analysis of QMAP Flights (1998) (15)
Machine-learning hidden symmetries (2021) (15)
COSMIC COMPLEMENTARITY: PROBING THE ACCELERATION OF THE UNIVERSE (1998) (15)
Mapping the CMB III: combined analysis of QMAP flights (1998) (15)
Removing point sources from CMB maps (1998) (14)
Cosmology from Large Scale Structure (2002) (14)
Science and Ultimate Reality: Parallel universes (2004) (14)
Automated in vivo patch-clamp evaluation of extracellular multielectrode array spike recording capability. (2018) (13)
Astrophysics from the Highly-Redshifted 21 cm Line (2009) (13)
DELAY SPECTRUM WITH PHASE-TRACKING ARRAYS: EXTRACTING THE H i POWER SPECTRUM FROM THE EPOCH OF REIONIZATION (2016) (13)
Non-Gaussianity as a Probe of the Physics of the Primordial Universe and the Astrophysics of the Low Redshift Universe (2009) (13)
Linear Redshift Distortions and Power in the PSCz Survey (2000) (13)
CMB power spectrum at l = 30 – 200 from QMASK (2001) (13)
Joint Efficient Dark-energy Investigation (JEDI): a Candidate Implementation of the NASA-DOE Joint Dark Energy Mission (JDEM) (2005) (12)
How Unlikely is a Doomsday Catastrophe (2005) (12)
Nanophotonic Inverse Design Using Artificial Neural Network (2017) (12)
First attempt at measuring the CMB cross-polarization (2002) (11)
Observations of the temperature and polarization anisotropies with Boomerang 2003 (2006) (11)
SUBDEGREE SUNYAEV–ZEL'DOVICH SIGNAL FROM MULTIFREQUENCY BOOMERanG OBSERVATIONS (2009) (10)
Solving the Corner-Turning Problem for Large Interferometers (2009) (10)
Friendly Artificial Intelligence: The Physics Challenge (2014) (10)
The HERA-19 Commissioning Array: Direction-dependent Effects (2018) (9)
Physics-Augmented Learning: A New Paradigm Beyond Physics-Informed Learning (2021) (9)
Comparing and combining the Saskatoon, QMAP, and COBE CMB maps (2000) (9)
Ensemble inhibition and excitation in the human cortex: An Ising-model analysis with uncertainties. (2018) (9)
Measuring quantum states: Experimental setup for measuring the spatial density matrix. (1996) (8)
Machine-Learning Non-Conservative Dynamics for New-Physics Detection (2021) (8)
Measuring space-time: From big bang to black holes (2002) (8)
Sharpening the second law of thermodynamics with the quantum Bayes theorem. (2013) (8)
CMB Polarization at Large Angular Scales: Data Analysis of the POLAR Experiment (2002) (8)
Foreground modelling via Gaussian process regression: an application to HERA data (2020) (7)
Real-space cosmic fields from redshift-space distributions: a Green function approach (1994) (7)
DID THE UNIVERSE RECOMBINE ? NEW SPECTRAL CONSTRAINTS ON REHEATING (1993) (7)
Observing the Evolution of the Universe (2009) (7)
Mapping our universe in 3D with MITEoR (2013) (6)
Power-Spectrum--independent Constraints on Cosmological Models (1993) (6)
Is lensing of point sources a problem for future CMB experiments? (1996) (6)
Towards Understanding Grokking: An Effective Theory of Representation Learning (2022) (6)
CMB polarization with Boomerang 2003 (2007) (6)
Years of the Quantum (6)
The HERA Dish II: Electromagnetic Simulations and Science Implications (2016) (6)
Cosmological constraints from current CMB and SN 1a data: A Brute force 9 parameter analysis (1998) (6)
The millimeter sky as seen with BOOMERanG (2007) (5)
A Spin-Modulated Telescope to Make Two-Dimensional Cosmic Microwave Background Maps (1999) (5)
Cosmic complementarity: combining CMB and supernova observations (1998) (5)
Mapping the CMB I: the first flight of the QMAP experiment (1998) (5)
Consciousness is a state of matter, like a solid or gas (2014) (5)
Uncorrelated Measurements of the CMB Power Spectrum (1997) (4)
Cosmic Microwave Background Maps from the HACME Experiment (1997) (4)
How accurately can suborbital experiments measure the CMB (2004) (4)
A Measurement of the CMB Spectrum from the 2003 Flight (2006) (4)
How Small Were the First Cosmological Objects? 1 (1996) (4)
On the Impossibility of Supersized Machines (2017) (4)
The unification of physics: the quest for a theory of everything (2015) (4)
Reality by numbers What is the universe really made of (2007) (3)
Constraints from the Lyman Α Forest Power Spectrum (2000) (3)
Overview of Foregrounds and their Impact (1999) (3)
Optimal Latent Representations: Distilling Mutual Information into Principal Pairs (2019) (3)
ERRATUM: “WHAT NEXT-GENERATION 21 cm POWER SPECTRUM MEASUREMENTS CAN TEACH US ABOUT THE EPOCH OF REIONIZATION” (2014, ApJ, 782, 66) (2014) (3)
The large-scale polarization of the microwave foreground (2003) (3)
Weighing neutrinos with microwave background and galaxy data (2001) (3)
Beyond Cosmological Parameters (2003) (3)
decomposition of finite pixelized CMB maps (2003) (2)
Mathematical cosmos: why numbers rule (2007) (2)
Latent Representations of Dynamical Systems: When Two is Better Than One (2019) (2)
Probing primordial non Gaussianity in the BOOMERanG CMB maps: an analysis based on analytical Minkowski functionals (2009) (2)
Cosmological Parameters and Beyond (2004) (2)
Quantum money and scalable 21-cm cosmology (2011) (2)
Poisson Flow Generative Models (2022) (2)
AI Poincaré 2.0: Machine Learning Conservation Laws from Differential Equations (2022) (2)
Bias and beyond (1998) (1)
New constraints on reionization from the Compton y-parameter (1994) (1)
Friendly Artificial Intelligence (2018) (1)
Gaussianity of the QMASK Map (2001) (1)
The Second Law and Cosmology (2008) (1)
Latest cosmological constraints on the densities of hot and cold dark matter (2000) (1)
Nuclear War from a Cosmic Perspective (2015) (1)
Extragalactic astronomy: Cosmic censorship (2002) (1)
Toward a more accurate 3D atlas of C. elegans neurons (2021) (1)
Omnigrok: Grokking Beyond Algorithmic Data (2022) (1)
Machine-learning media bias (2021) (1)
Maps of the millimetre sky from the BOOMERanG experiment (2003) (1)
Mapping the Cosmic Microwave Background Anisotropy:The Second Flight of the QMAP Experiment (1998) (1)
The quantum brain (1999) (1)
Precision Machine Learning (2022) (1)
Keynote speaker: Putting the radio into software defined radio ∼ and the meaning for arrays (2013) (1)
The MIT Survey on Science , Religion and Origins : the Belief Gap (2013) (1)
Cosmological lessons from MAP and SDSS (2003) (1)
Microwave foregrounds : "this volume was produced as a part of the Sloan Summit on Origins held at the Institute for Advanced Study in Princeton 1998-99" Princeton, New Jersey, USA 14-15 November, 1998 (1999) (1)
00 Years of the Quantum (1)
How to make CMB maps without losing information (1996) (1)
It's all just mathematics (2014) (1)
ICOSAHEDRON: A package for pixelizing the sphere (1999) (1)
Probes of the Early Universe (1994) (1)
On the Inevitability of Reionization : Implications forCosmic Microwave Background Fluctuations yMax (1996) (0)
MITEoR: A prototype highly scalable interferometer for 21 cm cosmology (2014) (0)
Bias is Complicated (2000) (0)
Uphold the nuclear weapons test moratorium (2020) (0)
HERA: Chasing Our Cosmic Dawn (2014) (0)
Solid. Liquid. Consciousness (2014) (0)
A New Method for Calibrating Radio Interferometers (2010) (0)
A bright future for dark energy (2003) (0)
Inflation and Parallel Universes: Science or Fiction? (2015) (0)
J un 2 00 2 Morphological Measures of nonGaussianity in CMB Maps (2002) (0)
Why Does Deep and Cheap Learning Work So Well? (2017) (0)
M ay 2 00 3 The First Data Release of the Sloan Digital Sky Survey (2014) (0)
Ju l 2 00 2 Two-Dimensional Topology of the Sloan Digital Sky Survey (2002) (0)
A ug 2 00 6 Constraining Torsion with Gravity Probe (2006) (0)
Estimating power spectra from 3D galaxy surveys (1995) (0)
Galactic microwave emission at 19 GHz (1998) (0)
Steady states of harmonic oscillator chains and shortcomings of harmonic heat baths (2002) (0)
03 10 72 3 v 2 15 J an 2 00 4 Cosmological parameters from SDSS and WMAP (2004) (0)
Analyzing Redshift Surveys to Measure the Power Spectrum on Large Scales (1997) (0)
Trouble with physics: Time to rethink cosmic inflation? (2013) (0)
Mangle: Angular Mask Software (2012) (0)
Biological error correction codes generate fault-tolerant neural networks (2022) (0)
Material to “ How Unlikely is a Doomsday Catastrophe ? ” (2007) (0)
VizieR Online Data Catalog: KGS EoR0 Catalogue (Carroll+, 2016) (2018) (0)
0 Ju l 2 00 2 Measuring Spacetime : from Big Bang to Black Holes (2004) (0)
New Techniques for Making CMB Maps (1998) (0)
Relativity Revisited (2008) (0)
Reconstructing cosmic fields from redshift data: An explicit solution for the linear regime (1995) (0)
Machine learning conservation laws from differential equations. (2022) (0)
Parametrising Epoch of Reionization foregrounds: A deep survey of low-frequency point-source spectra with the MWA (2016) (0)
The hydrogen epoch of reionization array dish III: measuring chromaticity of prototype element with reflectometry (2018) (0)
Mapping our universe in 3 D with MITEoR Citation (2013) (0)
Using Cosmology to Teach Physics (2011) (0)
Lawrence Berkeley National Laboratory Recent Work Title Measuring CMB polarization with Boomerang Permalink (2008) (0)
Fast Power Spectrum Analysis and Foreground Subtraction for 21 cm Cosmology (2011) (0)
02 12 55 2 v 1 2 7 D ec 2 00 2 1 Cosmology from Large Scale Structure (2002) (0)
Statistical lensing constraints on the shape of galaxy halos (2000) (0)
HERA: Illuminating our early universe (2014) (0)
Effects of model incompleteness on the drift-scan calibration of radio telescopes (2021) (0)
Morphological Measures of nonGaussianity in CMB Maps (2001) (0)
0 Ju n 20 02 Two-Dimensional Topology of the Sloan Digital Sky Survey (2002) (0)
Weak Lensing: Prospects for Parameter Estimation (2008) (0)
Cosmology: The dark side of distortion (2000) (0)
Ju n 20 02 Two-Dimensional Topology of the Sloan Digital Sky Survey (2002) (0)
02 12 41 7 v 2 2 0 D ec 2 00 2 The last stand before MAP : cosmological parameters from lensing , CMB and galaxy clustering (2018) (0)
Closing in on the Cosmological Parameters (2000) (0)
The power spectrum of the UZC galaxy redshift survey (1999) (0)
EIGENVALUE PROBLEMS IN COSMOLOGY: HOW SHOULD WE KARHUNEN-LOE‹VE TACKLE LARGE DATA SETS? (1997) (0)
A map of the universe - eScholarship (2003) (0)
BOOMERanG-B03 observations of CMB anisotropy and polarization (2006) (0)
as tr oph / 9 71 20 57 v 2 2 6 M ay 1 99 8 Weighing Neutrinos with Galaxy Surveys (1998) (0)
Lethal autonomous weapons (2019) (0)
0 Ju l 2 00 2 Two-Dimensional Topology of the Sloan Digital Sky Survey (2002) (0)
O ct 2 00 3 Draft v 3 . 0 A Map of the Universe (2004) (0)
Realistic Galaxy Models for Lensing Statistics (2005) (0)
Estimating Microwave Power Spectra (1995) (0)
01 04 41 9 v 2 1 8 Ja n 20 02 The CMB power spectrum at l = 30 − 200 from QMASK (2021) (0)
Cosmological Neutrino Bounds for Non-Cosmologists (2005) (0)
Cosmological Parameter Estimation (1997) (0)
How did it all begin (2005) (0)
05 12 20 4 v 2 2 1 D ec 2 00 5 How Unlikely is a Doomsday Catastrophe ? (2007) (0)
Pareto-Optimal Clustering with the Primal Deterministic Information Bottleneck (2022) (0)
03 10 72 3 v 2 1 5 Ja n 20 04 Cosmological parameters from SDSS and WMAP (2019) (0)
Mapmaking for precision 21 cm cosmology MAPMAKING for PRECISION 21 CM COSMOLOGY (2015) (0)
OBSERVABLES AND THEIR COSMOLOGICAL IMPLICATIONS (2008) (0)
O ct 2 00 5 A Map of the Universe (2021) (0)
Title The hydrogen epoch of reionization array dish III : measuring chromaticity of prototype element with reflectometry Permalink (2017) (0)
Spherical harmonic analysis of the angular distribution of GRBs (1996) (0)
Polar: Instrument and results (2002) (0)
Comparing and combining CMB datasets (1998) (0)
Quantum Decoherence: From Technology to Cosmology (2001) (0)
Priorities for Robust and Beneficial Artificial Intelligence (2015) (0)
03 10 72 3 v 1 27 O ct 2 00 3 Cosmological parameters from SDSS and WMAP (2003) (0)
LATE REIONIZATION BY SUPERNOVA DRIVEN WINDS1 (1992) (0)

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