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, University of Pennsylvania

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?

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, a supporter of the effective altruism movement, and has received research grants from Elon Musk to investigate existential risk from advanced artificial intelligence.

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

Detection of the baryon acoustic peak in the large-scale correlation function of SDSS luminous red galaxies (2005) (3234)
Cosmological parameters from SDSS and WMAP (2004) (2913)
Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample (2010) (1251)
THE THREE-DIMENSIONAL POWER SPECTRUM OF GALAXIES FROM THE SLOAN DIGITAL SKY SURVEY (2004) (1209)
Cosmological constraints from the SDSS luminous red galaxies (2006) (1102)
The 3D power spectrum of galaxies from the SDSS (2003) (948)
NEW YORK UNIVERSITY VALUE-ADDED GALAXY CATALOG: A GALAXY CATALOG BASED ON NEW PUBLIC SURVEYS (2005) (925)
The Galaxy Luminosity Function and Luminosity Density at Redshift z = 0.1* (2002) (860)
Cosmological parameter analysis including SDSS Lyα forest and galaxy bias: Constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy (2005) (797)
Karhunen-Loève Eigenvalue Problems in Cosmology: How Should We Tackle Large Data Sets? (1996) (688)
The Luminosity and Color Dependence of the Galaxy Correlation Function (2005) (613)
How small were the first cosmological objects (1997) (602)
Galaxy Clustering in the Completed SDSS Redshift Survey: The Dependence on Color and Luminosity (2011) (549)
The Second Data Release of the Sloan Digital Sky Survey (2004) (531)
NYU-VAGC: a galaxy catalog based on new public surveys (2004) (527)
Galaxy clustering in early sloan digital sky survey redshift data (2002) (491)
The fourth data release of the Sloan Digital Sky Survey (2005) (476)
The importance of quantum decoherence in brain processes (2000) (465)
Why Does Deep and Cheap Learning Work So Well? (2016) (455)
Significance of the largest scale CMB fluctuations in WMAP (2004) (448)
High resolution foreground cleaned CMB map from WMAP (2003) (444)
Cosmological Constraints from the Clustering of the Sloan Digital Sky Survey DR7 Luminous Red Galaxies (2010) (438)
Research Priorities for Robust and Beneficial Artificial Intelligence (2015) (434)
Nanophotonic particle simulation and inverse design using artificial neural networks (2018) (361)
The Mathematical Universe (2008) (361)
A map of the universe (2003) (359)
The role of artificial intelligence in achieving the Sustainable Development Goals (2020) (338)
The Third Data Release of the Sloan Digital Sky Survey (2004) (336)
A model of diffuse Galactic radio emission from 10 MHz to 100 GHz (2008) (310)
Measuring Cosmological Parameters with Galaxy Surveys (1997) (303)
The end of unified dark matter (2004) (293)
Weighing Neutrinos with Galaxy Surveys (1998) (282)
Limits on non-Gaussianities from WMAP data (2006) (281)
The clustering of luminous red galaxies in the Sloan Digital Sky Survey imaging data (2006) (281)
Dimensionless constants, cosmology and other dark matters (2006) (280)
Constraining f ( R ) gravity as a scalar-tensor theory (2007) (271)
How to measure CMB power spectra without losing information (1997) (271)
A method for subtracting foregrounds from multifrequency CMB sky maps (1996) (271)
On Departures from a Power Law in the Galaxy Correlation Function (2003) (253)
A Measurement of the CMB EE Spectrum from the 2003 Flight of BOOMERANG (2006) (246)
Foregrounds and Forecasts for the Cosmic Microwave Background (2000) (244)
Cosmic Complementarity: Joint Parameter Estimation from Cosmic Microwave Background Experiments and Redshift Surveys (1998) (239)
The shape of the sloan digital sky survey data release 5 galaxy power spectrum (2007) (220)
Is “the Theory of Everything” Merely the Ultimate Ensemble Theory?☆ (1997) (213)
A Measurement of the Angular Power Spectrum of the CMB Temperature Anisotropy from the 2003 Flight of BOOMERANG (2006) (210)
Analysis of Systematic Effects and Statistical Uncertainties in Angular Clustering of Galaxies from Early Sloan Digital Sky Survey Data (2001) (205)
New dark energy constraints from supernovae, microwave background, and galaxy clustering. (2004) (201)
WHAT NEXT-GENERATION 21 cm POWER SPECTRUM MEASUREMENTS CAN TEACH US ABOUT THE EPOCH OF REIONIZATION (2014) (196)
Cosmological Parameters from Eigenmode Analysis of Sloan Digital Sky Survey Galaxy Redshifts (2004) (191)
The Time evolution of bias (1998) (184)
The Intermediate-Scale Clustering of Luminous Red Galaxies (2005) (183)
How accurately can 21cm tomography constrain cosmology (2008) (182)
Our Mathematical Universe: My Quest for the Ultimate Nature of Reality (2014) (181)
Cosmological Parameters from the 2003 Flight of BOOMERANG (2006) (176)
What does inflation really predict (2005) (174)
Cosmic Microwave Background Observables and Their Cosmological Implications (2001) (172)
Inflationary Constraints on Type IIA String Theory (2007) (171)
The shape of the SDSS DR5 galaxy power spectrum (2006) (170)
Axion cosmology and the energy scale of inflation (2008) (168)
AI Feynman: A physics-inspired method for symbolic regression (2020) (166)
Life 3.0: Being Human in the Age of Artificial Intelligence (2017) (165)
Forecasting cosmic parameter errors from microwave background anisotropy experiments (1997) (165)
Measuring the galaxy power spectrum with future redshift surveys (1998) (164)
Methods for rapidly processing angular masks of next-generation galaxy surveys (2008) (153)
CMB Observables and Their Cosmological Implications (2000) (150)
Using the kinematic Sunyaev-Zeldovich effect to determine the peculiar velocities of clusters of galaxies (1995) (147)
An Icosahedron-based Method for Pixelizing the Celestial Sphere (1996) (147)
The Interpretation of Quantum Mechanics: Many Worlds or Many Words? (1998) (142)
Uncorrelated measurements of the cosmic expansion history and dark energy from supernovae (2005) (141)
A Measurement of the Polarization-Temperature Angular Cross-Power Spectrum of the Cosmic Microwave Background from the 2003 Flight of BOOMERANG (2006) (135)
Is cosmology consistent (2002) (134)
The power spectrum of galaxies in the 2dF 100k redshift survey (2002) (134)
Overcoming real-world obstacles in 21 cm power spectrum estimation: A method demonstration and results from early Murchison Widefield Array data (2014) (133)
Tunable Efficient Unitary Neural Networks (EUNN) and their application to RNNs (2017) (133)
SDSS galaxy bias from halo mass-bias relation and its cosmological implications (2005) (129)
The power of deeper networks for expressing natural functions (2018) (128)
Weak Lensing: Prospects for Measuring Cosmological Parameters (1998) (127)
21 cm Tomography with Foregrounds (2006) (125)
First Season MWA EoR Power Spectrum Results at Redshift 7 (2016) (120)
A method for 21 cm power spectrum estimation in the presence of foregrounds (2011) (118)
Consciousness as a state of matter (2015) (118)
Constraints from the Lyα Forest Power Spectrum (2000) (118)
Angular Clustering with Photometric Redshifts in the Sloan Digital Sky Survey: Bimodality in the Clustering Properties of Galaxies (2003) (115)
CMB mapping experiments: a designer's guide (1997) (114)
A Brute Force Analysis of the COBE DMR Data (1995) (114)
How to Make Maps from Cosmic Microwave Background Data without Losing Information (1996) (113)
Fast Fourier transform telescope (2009) (111)
How to measure CMB polarization power spectra without losing information (2001) (109)
Why Is the Cosmic Microwave Background Fluctuation Level 10?5? (1998) (108)
Separating the early universe from the late universe: Cosmological parameter estimation beyond the black box (2002) (107)
Instrument, Method, Brightness and Polarization Maps from the 2003 flight of BOOMERanG (2005) (107)
Testing two-field inflation (2011) (107)
100 years of the quantum (2001) (105)
An improved method for 21‐cm foreground removal (2009) (101)
Foregrounds in Wide-Field Redshifted 21 cm Power Spectra (2015) (100)
Improved Measures of Integrated Information (2016) (98)
Towards a refined cosmic concordance model: Joint 11-parameter constraints from the cosmic microwave background and large-scale structure (2001) (95)
Precision calibration of radio interferometers using redundant baselines (2010) (94)
A scheme to deal accurately and efficiently with complex angular masks in galaxy surveys (2004) (92)
Cmb multipole measurements in the presence of foregrounds (2006) (90)
Gated Orthogonal Recurrent Units: On Learning to Forget (2019) (90)
Cross-Correlation of Tenerife Data with Galactic Templates-Evidence for Spinning Dust? (1999) (89)
SDSS galaxy clustering: luminosity and colour dependence and stochasticity (2008) (88)
Constraining Torsion with Gravity Probe B (2007) (87)
Task force on cosmic microwave background research (2006) (86)
Apparent wave function collapse caused by scattering (1993) (86)
Cosmology and the Halo Occupation Distribution from Small-Scale Galaxy Clustering in the Sloan Digital Sky Survey (2004) (85)
Why is the CMB fluctuation level 10^{-5}? (1997) (83)
Empirical covariance modeling for 21 cm power spectrum estimation: A method demonstration and new limits from early Murchison Widefield Array 128-tile data (2015) (83)
The Low-Frequency Environment of the Murchison Widefield Array: Radio-Frequency Interference Analysis and Mitigation (2015) (82)
The Three-dimensional Power Spectrum from Angular Clustering of Galaxies in Early Sloan Digital Sky Survey Data (2002) (81)
The Quest for Microwave Foreground X (2004) (80)
The angular correlation function of galaxies from early sloan digital sky survey data (2001) (79)
Combined reconstruction of weak and strong lensing data with wslap (2005) (78)
CHIPS: The COSMOLOGICAL H i POWER SPECTRUM ESTIMATOR (2016) (77)
Current Cosmological Constraints from a 10 Parameter Cosmic Microwave Background Analysis (2000) (77)
How well can we measure and understand foregrounds with 21-cm experiments? (2011) (76)
Non-parametric inversion of strong lensing systems (2005) (75)
Time Evolution of Galaxy Formation and Bias in Cosmological Simulations (2000) (72)
The Angular Power Spectrum of Galaxies from Early Sloan Digital Sky Survey Data (2001) (71)
Late reionization by supernova-driven winds (1993) (71)
Removing Point Sources from Cosmic Microwave Background Maps (1998) (70)
MITEoR: a scalable interferometer for precision 21 cm cosmology (2014) (68)
Will point sources spoil 21-cm tomography? (2009) (68)
Why Is the Fraction of Four-Image Radio Lens Systems So High? (2001) (68)
Twenty-one centimeter tomography with foregrounds (2005) (68)
A New Spin on Galactic Dust (2002) (67)
The real-space power spectrum of the PSCz survey from 0.01 to 300 h Mpc−1 (2002) (67)
Limits on fNL parameters from Wilkinson Microwave Anisotropy Probe three-year data (2007) (67)
An Improved Model of Diffuse Galactic Radio Emission from 10 MHz to 5 THz (2017) (66)
Multiple universes, cosmic coincidences, and other dark matters (2004) (66)
Investigating Inflation in Type IIA (2007) (65)
Measuring the metric: A parametrized post-Friedmannian approach to the cosmic dark energy problem (2002) (64)
LARGE-SCALE SUNYAEV-ZELDOVICH EFFECT: MEASURING STATISTICAL PROPERTIES WITH MULTIFREQUENCY MAPS (2000) (64)
Stephen Hawking: \'Transcendence looks at the implications of artificial intelligence - but are we taking AI seriously enough?\' (2014) (64)
New microwave background constraints on the cosmic matter budget: trouble for nucleosynthesis? (2000) (62)
Omniscopes: Large area telescope arrays with only NlogN computational cost (2010) (61)
The Murchison Widefield Array 21 cm Power Spectrum Analysis Methodology (2016) (61)
Karhunen-Loève Estimation of the Power Spectrum Parameters from the Angular Distribution of Galaxies in Early Sloan Digital Sky Survey Data (2001) (61)
ON THE INEVITABILITY OF REIONIZATION : IMPLICATIONS FOR COSMIC MICROWAVE BACKGROUND FLUCTUATIONS (1994) (60)
Confirmation of wide-field signatures in redshifted 21 cm power spectra (2015) (59)
Testing Multi-Field Inflation: A Geometric Approach (2011) (58)
Removing Real-World Foregrounds from Cosmic Microwave Background Maps (1998) (58)
Decorrelating the power spectrum of galaxies (1999) (58)
Observational evidence for stochastic biasing (1999) (57)
Physical evidence for dark energy (2003) (57)
Observationally determining the properties of dark matter (1998) (57)
Non-Gaussianity in Two-Field Inflation (2011) (57)
Is the Cosmic Microwave Background Really Non-Gaussian? (1999) (57)
Born in an Infinite Universe: A Cosmological Interpretation of Quantum Mechanics (2011) (55)
First limits on the 21 cm power spectrum during the Epoch of X-ray heating (2016) (55)
Toward an artificial intelligence physicist for unsupervised learning. (2019) (54)
The Multiverse Hierarchy (2007) (51)
The Importance of Wide-field Foreground Removal for 21 cm Cosmology: A Demonstration With Early MWA Epoch of Reionization Observations (2016) (51)
The Hydrogen Epoch of Reionization Array Dish. I. Beam Pattern Measurements and Science Implications (2016) (50)
A fast method for power spectrum and foreground analysis for 21 cm cosmology (2013) (50)
Criticality in Formal Languages and Statistical Physics (2016) (49)
Parametrizing Epoch of Reionization foregrounds: a deep survey of low-frequency point-source spectra with the Murchison Widefield Array (2016) (48)
Low frequency observations of linearly polarized structures in the interstellar medium near the south Galactic pole (2016) (47)
A Limit on the Large Angular Scale Polarization of the Cosmic Microwave Background (2001) (45)
Limits on f_NL parameters from WMAP 3yr data (2006) (45)
Critical Behavior in Physics and Probabilistic Formal Languages (2017) (45)
Two-dimensional Topology of the Sloan Digital Sky Survey (2002) (44)
Last stand before WMAP: Cosmological parameters from lensing, CMB, and galaxy clustering (2003) (44)
Global 21 cm signal experiments: A designer’s guide (2013) (44)
Parallel universes? (2006) (44)
Cosmic complementarity: H(0) and Omega(m) from combining CMB experiments and redshift surveys (1998) (42)
An Elementary Proof That the Biharmonic Green Function of an Eccentric Ellipse Changes Sign (1994) (42)
Searching for Inflation in Simple String Theory Models: An Astrophysical Perspective (2007) (42)
How unitary cosmology generalizes thermodynamics and solves the inflationary entropy problem (2012) (39)
Anthropic predictions for neutrino masses (2005) (38)
The Hydrogen Epoch of Reionization Array Dish. II. Characterization of Spectral Structure with Electromagnetic Simulations and Its Science Implications. (2016) (37)
Does the universe in fact contain almost no information? (1996) (37)
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) (36)
A method for extracting maximum resolution power spectra from microwave sky maps (1996) (35)
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)
Many lives in many worlds (2007) (34)
Mapping the Cosmic Microwave Background Anisotropy:The First Flight of the QMAP Experiment (1998) (33)
AI Feynman 2.0: Pareto-optimal symbolic regression exploiting graph modularity (2020) (33)
Decoherence produces coherent states: An explicit proof for harmonic chains. (1994) (32)
Astrophysics: Is a doomsday catastrophe likely? (2005) (32)
Galactic Emission at 19 GHz (1998) (32)
Baryon acoustic oscillations in the Sloan Digital Sky Survey Data Release 7 galaxy sample (vol 401, pg 2148, 2010) (2011) (32)
The Angular Power Spectrum of BATSE 3B Gamma-Ray Bursts (1996) (32)
Anthropic predictions for vacuum energy and neutrino masses (2004) (31)
Comparing Redundant and Sky-model-based Interferometric Calibration: A First Look with Phase II of the MWA (2018) (31)
A High-Resolution Map of the Cosmic Microwave Background around the North Celestial Pole (1997) (29)
A method for extracting maximum resolution power spectra from galaxy surveys (1995) (29)
Morphological Measures of Non-Gaussianity in Cosmic Microwave Background Maps (2002) (29)
Mapmaking for precision 21 cm cosmology (2015) (29)
On Math, Matter and Mind (2006) (28)
The Angular Power Spectrum of the Four-Year COBE Data (1996) (26)
Cosmology from the Highly-Redshifted 21 cm Line (2009) (26)
BOOMERanG constraints on primordial non-Gaussianity from analytical Minkowski functionals (2009) (26)
Cosmological neutrino bounds for non-cosmologists (2005) (26)
Many Worlds in Context (2010) (25)
Measuring Spacetime: From the Big Bang to Black Holes (2002) (25)
Non-Gaussianity as a Probe of the Physics of the Primordial Universe and the Astrophysics of the Low Redshift Universe (2009) (24)
Likely values of the Higgs vev (2009) (22)
Learnability for the Information Bottleneck (2019) (21)
Reionization in an open CDM universe: implications for cosmic microwave background fluctuations (1994) (21)
CMBFIT: Rapid WMAP likelihood calculations with normal parameters (2004) (21)
A high reliability survey of discrete Epoch of Reionization foreground sources in the MWA EoR0 field (2016) (21)
Large-scale polarization of the microwave background and foreground (2003) (20)
Likely values of the Higgs vacuum expectation value (2010) (20)
Science and Ultimate Reality: Parallel universes (2004) (19)
Cosmological Parameters and Beyond (2004) (19)
Cosmological constraints from the clustering of the Sloan Digital Sky Survey DR7 luminous red galaxies (vol 404, pg 60, 2010) (2011) (18)
Brute-force mapmaking with compact interferometers: a MITEoR northern sky map from 128 to 175 MHz (2017) (18)
Searching for non-Gaussian signals in the BOOMERANG 2003 CMB maps (2007) (18)
Mapping the CMB II: the second flight of the QMAP experiment (1998) (18)
Shut up and calculate (2007) (18)
Doppler peaks and all that: CMB anisotropies and what they can tell us (1995) (18)
Galactic Contamination in the QMAP Experiment (2000) (18)
Measuring CMB polarization with Boomerang (2003) (17)
Parallel universes. Not just a staple of science fiction, other universes are a direct implication of cosmological observations. (2003) (17)
Spectral Energy Distribution and Radio Halo of NGC 253 at Low Radio Frequencies (2017) (17)
The Power Spectrum of the CfA/SSRS UZC Galaxy Redshift Survey (2001) (17)
On the dimensionality of space-time (1997) (17)
The hydrogen epoch of reionization array dish III: measuring chromaticity of prototype element with reflectometry (2018) (16)
Removing real-world foregrounds from CMB maps (1997) (16)
Toward an AI Physicist for Unsupervised Learning (2018) (16)
THE 3D POWER SPECTRUM FROM ANGULAR CLUSTERING OF GALAXIES IN EARLY SDSS DATA 1 (2001) (16)
Cosmological Constraints from Current Cosmic Microwave Background and Type Ia Supernova Data: A Brute Force, Eight-Parameter Analysis (1999) (16)
Meta-learning autoencoders for few-shot prediction (2018) (15)
Redundant-baseline calibration of the hydrogen epoch of reionization array (2020) (15)
Improved Limits on Gamma-Ray Burst Repetition from BATSE (1996) (15)
Assessing whether artificial intelligence is an enabler or an inhibitor of sustainability at indicator level (2021) (15)
Why the brain is probably not a quantum computer (2000) (15)
AI Poincaré: Machine Learning Conservation Laws from Trajectories (2021) (15)
Mapping the CMB III: combined analysis of QMAP flights (1998) (15)
Comparing and Combining Cosmic Microwave Background Data Sets (1999) (14)
COSMIC COMPLEMENTARITY: PROBING THE ACCELERATION OF THE UNIVERSE (1998) (13)
Assessment of Ionospheric Activity Tolerances for Epoch of Reionization Science with the Murchison Widefield Array (2018) (13)
CMB power spectrum at l = 30 – 200 from QMASK (2002) (13)
Pareto-Optimal Data Compression for Binary Classification Tasks (2020) (12)
Mapping the Cosmic Microwave Background Anisotropy:Combined Analysis of QMAP Flights (1998) (12)
How Unlikely is a Doomsday Catastrophe (2005) (12)
Astrophysics from the Highly-Redshifted 21 cm Line (2009) (12)
DELAY SPECTRUM WITH PHASE-TRACKING ARRAYS: EXTRACTING THE H i POWER SPECTRUM FROM THE EPOCH OF REIONIZATION (2016) (12)
Nanophotonic Inverse Design Using Artificial Neural Network (2017) (12)
Non-parametric mass reconstruction of A1689 from strong lensing data with the Strong Lensing Analysis Package: Mass reconstruction of A1689 (2005) (12)
First attempt at measuring the CMB cross-polarization (2003) (11)
Removing point sources from CMB maps (1998) (11)
Symbolic Pregression: Discovering Physical Laws from Raw Distorted Video (2021) (11)
Linear Redshift Distortions and Power in the PSCz Survey (2000) (10)
Automated in vivo patch-clamp evaluation of extracellular multielectrode array spike recording capability. (2018) (10)
Solving the Corner-Turning Problem for Large Interferometers (2009) (10)
Measuring spacetime: from the big bang to black holes. (2002) (10)
SUBDEGREE SUNYAEV-ZEL'DOVICH SIGNAL FROM MULTIFREQUENCY BOOMERANG OBSERVATIONS (2009) (10)
Cosmology from Large Scale Structure (2002) (10)
Comparing and combining the Saskatoon, QMAP, and COBE CMB maps (2001) (9)
Observations of the temperature and polarization anisotropies with Boomerang 2003 (2006) (9)
Joint Efficient Dark-energy Investigation (JEDI): a Candidate Implementation of the NASA-DOE Joint Dark Energy Mission (JDEM) (2005) (9)
The HERA-19 Commissioning Array: Direction-dependent Effects (2019) (9)
Friendly Artificial Intelligence: The Physics Challenge (2015) (9)
Cosmic Complementarity: H 0 and Ω M from Combining Cmb Experiments and Redshift Surveys (8)
Measuring space-time: From big bang to black holes (2002) (8)
CMB Polarization at Large Angular Scales: Data Analysis of the POLAR Experiment (2003) (8)
Sharpening the second law of thermodynamics with the quantum Bayes theorem. (2014) (8)
Measuring quantum states: Experimental setup for measuring the spatial density matrix. (1996) (8)
Cosmological constraints from current CMB and SN 1a data: A Brute force 9 parameter analysis (1998) (7)
DID THE UNIVERSE RECOMBINE ? NEW SPECTRAL CONSTRAINTS ON REHEATING (1994) (7)
Ensemble inhibition and excitation in the human cortex: An Ising-model analysis with uncertainties. (2019) (7)
Real-space cosmic fields from redshift-space distributions: a Green function approach (1994) (7)
Cosmological Parameter Estimation (2020) (7)
Years of the Quantum (6)
Observing the Evolution of the Universe (2009) (6)
Is lensing of point sources a problem for future CMB experiments (1997) (6)
Power-Spectrum--independent Constraints on Cosmological Models (1994) (6)
CMB polarization with Boomerang 2003 (2007) (6)
Polarized Foreground Power Spectra from the HERA-19 Commissioning Array (2018) (6)
The HERA Dish II: Electromagnetic Simulations and Science Implications (2016) (6)
Mapping our universe in 3D with MITEoR (2013) (6)
A Spin-Modulated Telescope to Make Two-Dimensional Cosmic Microwave Background Maps (2000) (5)
Foreground modelling via Gaussian process regression: an application to HERA data (2020) (5)
Cosmic complementarity: combining CMB and supernova observations (1998) (5)
Mapping the CMB I: the first flight of the QMAP experiment (1998) (5)
The millimeter sky as seen with BOOMERanG (2007) (5)
Consciousness is a state of matter, like a solid or gas (2014) (5)
16p11.2 deletion is associated with hyperactivation of human iPSC-derived dopaminergic neuron networks and is rescued by RHOA inhibition in vitro (2021) (5)
The unification of physics: the quest for a theory of everything (2015) (4)
How accurately can suborbital experiments measure the CMB (2005) (4)
A Measurement of the CMB Spectrum from the 2003 Flight (2006) (4)
COSMIC MICROWAVE BACKGROUND MAPS FROM THE HACME EXPERIMENT (1997) (4)
Searching for non-Gaussian signals in the BOOMERanG 2003 CMB map: Preliminary results (2007) (4)
Uncorrelated Measurements of the CMB Power Spectrum (1997) (4)
Nanophotonic particle simulation and inverse design using artificial neural networks (2018) (4)
ERRATUM: “WHAT NEXT-GENERATION 21 cm POWER SPECTRUM MEASUREMENTS CAN TEACH US ABOUT THE EPOCH OF REIONIZATION” (2014, ApJ, 782, 66) (2014) (4)
Reality by numbers What is the universe really made of (2007) (3)
The large-scale polarization of the microwave foreground (2003) (3)
Weighing neutrinos with microwave background and galaxy data (2001) (3)
On the Impossibility of Supersized Machines (2017) (3)
Beyond Cosmological Parameters (2003) (3)
How Small Were the First Cosmological Objects? 1 (1996) (3)
Optimal Latent Representations: Distilling Mutual Information into Principal Pairs (2019) (3)
Machine-Learning Non-Conservative Dynamics for New-Physics Detection (2021) (3)
Machine-learning hidden symmetries (2021) (2)
Probing primordial non Gaussianity in the BOOMERanG CMB maps: an analysis based on analytical Minkowski functionals (2009) (2)
Latent Representations of Dynamical Systems: When Two is Better Than One (2019) (2)
Quantum money and scalable 21-cm cosmology (2011) (2)
Physics-Augmented Learning: A New Paradigm Beyond Physics-Informed Learning (2021) (2)
Mathematical cosmos: why numbers rule (2007) (2)
Overview of Foregrounds and their Impact (1999) (2)
The quantum brain (1999) (1)
Latest cosmological constraints on the densities of hot and cold dark matter (2000) (1)
How to make CMB maps without losing information (1996) (1)
Gaussianity of the QMASK Map (2001) (1)
decomposition of finite pixelized CMB maps (2003) (1)
Extragalactic astronomy: Cosmic censorship (2002) (1)
It's all just mathematics (2014) (1)
Maps of the millimetre sky from the BOOMERanG experiment (2003) (1)
Cosmological lessons from MAP and SDSS (2003) (1)
Priorities for Robust and Bene fi cial (2016) (1)
Probes of the Early Universe (1994) (1)
Keynote speaker: Putting the radio into software defined radio ∼ and the meaning for arrays (2013) (1)
Toward a More Accurate 3D Atlas of C. elegans Neurons (2021) (1)
Friendly Artificial Intelligence (2018) (1)
The MIT Survey on Science , Religion and Origins : the Belief Gap (2013) (1)
00 Years of the Quantum (1)
The Second Law and Cosmology (2008) (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)
Constraints from the Lyman Α Forest Power Spectrum (2000) (1)
Bias and beyond (1998) (1)
Closing in on the Cosmological Parameters (2000) (0)
Inflation and Parallel Universes: Science or Fiction? (2015) (0)
Mapping our universe in 3 D with MITEoR Citation (2013) (0)
0 Ju l 2 00 2 Two-Dimensional Topology of the Sloan Digital Sky Survey (2002) (0)
Title Mapmaking for precision 21 cm cosmology MAPMAKING for PRECISION 21 CM COSMOLOGY (2015) (0)
Galactic microwave emission at 19 GHz (1998) (0)
02 12 55 2 v 1 2 7 D ec 2 00 2 1 Cosmology from Large Scale Structure (2002) (0)
Material to “ How Unlikely is a Doomsday Catastrophe ? ” (2007) (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)
Nuclear War from a Cosmic Perspective (2015) (0)
Title The hydrogen epoch of reionization array dish III : measuring chromaticity of prototype element with reflectometry Permalink (2017) (0)
New constraints on reionization from the Compton y-parameter (1994) (0)
03 10 72 3 v 1 27 O ct 2 00 3 Cosmological parameters from SDSS and WMAP (2003) (0)
Ju n 20 02 Two-Dimensional Topology of the Sloan Digital Sky Survey (2002) (0)
Comparing and combining CMB datasets (1998) (0)
Lethal autonomous weapons (2019) (0)
Uphold the nuclear weapons test moratorium (2020) (0)
OBSERVABLES AND THEIR COSMOLOGICAL IMPLICATIONS (2008) (0)
How did it all begin (2005) (0)
A ug 2 00 6 Constraining Torsion with Gravity Probe (2006) (0)
Using Cosmology to Teach Physics (2011) (0)
0 Ju l 2 00 2 Measuring Spacetime : from Big Bang to Black Holes (2004) (0)
Effects of model incompleteness on the drift-scan calibration of radio telescopes (2021) (0)
Realistic Galaxy Models for Lensing Statistics (2005) (0)
Estimating Microwave Power Spectra (1995) (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)
Trouble with physics: Time to rethink cosmic inflation? (2013) (0)
Mangle: Angular Mask Software (2012) (0)
The Hydrogen Epoch of Reionization Array (HERA) (2015) (0)
HERA: Illuminating our early universe (2014) (0)
Steady states of harmonic oscillator chains and shortcomings of harmonic heat baths (2002) (0)
A bright future for dark energy (2003) (0)
05 12 20 4 v 2 2 1 D ec 2 00 5 How Unlikely is a Doomsday Catastrophe ? (2007) (0)
O ct 2 00 5 A Map of the Universe (2021) (0)
BOOMERanG-B03 observations of CMB anisotropy and polarization (2006) (0)
MITEoR: A prototype highly scalable interferometer for 21 cm cosmology (2014) (0)
Machine-Learning media bias (2021) (0)
A map of the universe - eScholarship (2003) (0)
03 10 72 3 v 2 15 J an 2 00 4 Cosmological parameters from SDSS and WMAP (2004) (0)
Reconstructing cosmic fields from redshift data: An explicit solution for the linear regime (1995) (0)
New Techniques for Making CMB Maps (1998) (0)
Solid. Liquid. Consciousness (2014) (0)
Priorities for Robust and Beneficial Artificial Intelligence (2015) (0)
Cosmology: The dark side of distortion (2000) (0)
Estimating power spectra from 3D galaxy surveys (1995) (0)
Morphological Measures of nonGaussianity in CMB Maps (2001) (0)
VizieR Online Data Catalog: KGS EoR0 Catalogue (Carroll+, 2016) (2018) (0)
Weak Lensing: Prospects for Parameter Estimation (2008) (0)
HERA: Chasing Our Cosmic Dawn (2014) (0)
HERA: Illuminating our early universe (2014) (0)
ICOSAHEDRON: A package for pixelizing the sphere (1999) (0)
0 Ju n 20 02 Two-Dimensional Topology of the Sloan Digital Sky Survey (2002) (0)
Bias is Complicated (2000) (0)
Fast Power Spectrum Analysis and Foreground Subtraction for 21 cm Cosmology (2011) (0)
A New Method for Calibrating Radio Interferometers (2010) (0)
03 10 72 3 v 2 1 5 Ja n 20 04 Cosmological parameters from SDSS and WMAP (2019) (0)
On the Inevitability of Reionization : Implications forCosmic Microwave Background Fluctuations yMax (1996) (0)
Analyzing Redshift Surveys to Measure the Power Spectrum on Large Scales (1998) (0)
The power spectrum of the UZC galaxy redshift survey (1999) (0)
POLAR: Instrument and results (2002) (0)
as tr oph / 9 71 20 57 v 2 2 6 M ay 1 99 8 Weighing Neutrinos with Galaxy Surveys (1998) (0)
Relativity Revisited (2008) (0)
Spherical harmonic analysis of the angular distribution of GRBs (2008) (0)
Quantum Decoherence: From Technology to Cosmology (2001) (0)
LATE REIONIZATION BY SUPERNOVA DRIVEN WINDS1 (1992) (0)
Statistical lensing constraints on the shape of galaxy halos (2000) (0)
Lawrence Berkeley National Laboratory Recent Work Title Measuring CMB polarization with Boomerang Permalink (2008) (0)
J un 2 00 2 Morphological Measures of nonGaussianity in CMB Maps (2002) (0)

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