MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on angular scales of 10 arcminutes to 5 degrees

Abstract

We present a map and an angular power spectrum of the anisotropy of the cosmic microwave background (CMB) from the first flight of MAXIMA. MAXIMA is a balloon-borne experiment with an array of 16 bolometric photometers operated at 100 mK. MAXIMA observed a 124 square degrees region of the sky with 10 arcminute resolution at frequencies of 150, 240 and 410 GHz. The data were calibrated using in-flight measurements of the CMB dipole anisotropy. A map of the CMB anisotropy was produced from three 150 and one 240 GHz photometer without need for foreground subtractions. Analysis of this CMB map yields a power spectrum for the CMB anisotropy over the range 36 < l < 785. The spectrum shows a peak with an amplitude of 78 +/- 6 micro-Kelvin at l ~ 220 and an amplitude varying between ~40 micro-Kelvin and ~50 micro-Kelvin for 400 < l < 785.

Reflects version accepted for publication in Ap J Letters

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• Non-Gaussianity, Isocurvature Perturbation, Gravitational Waves and a No-Go Theorem for Isocurvaton
• Constraints on the non-linear coupling parameter fnl with the Archeops data
• Observational evidence for a correlation between peak-luminosities and beaming in GRBs
• Cosmic strings, loops, and linear growth of matter perturbations
• Evidence for a Significant Blazar Contamination in CMB Anisotropy Maps
• Lecture Notes on CMB Theory: From Nucleosynthesis to Recombination
• Observational Constraints on Dynamical Dark Energy Models
• Interacting Two-Fluid Viscous Dark Energy Models In Non-Flat Universe
• A Cyclic Universe With Varying Cosmological Constant in $f(R,T)$ gravity
• Infinity in string cosmology: A review through open problems
• Quintessence with two energy scales
• Early and Late Transient Cosmic Acceleration due to Curvature Inspired Dark Energy
• How dominant is the vacuum?
• Particle decay in the early universe: predictions for 21 cm
• Measuring the geometry of the Universe in the presence of isocurvature modes
• The Cosmological Constant Problem, an Inspiration for New Physics
• SNLS data are consistent with acceleration at z=3
• Plane waves in a general Robertson-Walker background
• Complex Visibilities of Cosmic Microwave Background Anisotropies
• Geometrical estimators as a test of Gaussianity in the CMB
• Full-sky correlations of peaks in the microwave background
• Two-Fluid Dark Energy Models in Bianchi Type-III Universe with Variable Deceleration Parameter
• Direct Dark Matter Detection - A spin 3/2 WIMP candidate
• Geodesic Structure of the Quantum-Corrected Schwarzschild Black Hole Surrounded by Quintessence
• Galactosynthesis: Halo Histories, Star Formation, and Disks
• Theoretical direct WIMP detection rates for transitions to excited states
• Graviton Mass, Quintessence and Oscillatory Character of the Universe Evolution
• Harmonic analysis of cosmic microwave background data II: from ring-sets to the sky
• Constraints in Cosmological Parameter Space from the Sunyaev-Zel'dovich Effect and Thermal Bremsstrahlung
• Fast and precise map-making for massively multi-detector CMB experiments
• CMB power spectrum estimation using noncircular beams
• CMB Constraints on a Baryonic Dark Matter-Dominated Universe
• The Cosmic Baryon Fraction and the Extragalactic Ionizing Background
• A Braneworld Dark Energy Model with Induced Gravity and the Gauss-Bonnet Effect
• Physics of the cosmic microwave background anisotropy
• The Influence of Free Quintessence on Gravitational Frequency Shift and Deflection of Light with 4D momentum
• FRW Cosmology From Five Dimensional Vacuum Brans-Dicke Theory
• Model-independent study for a quintessence model of dark energy: Analysis and Observational constraints
• Mass of Galactic Lenses in Modified Newtonian Dynamics
• Stable Charged Gravastar model in Cylindrically Symmetric Space-time
• Foreground separation using a flexible maximum-entropy algorithm: an application to COBE data
• How is the Reionization Epoch Defined?
• Ionization history of the Universe as a test for Super Heavy Dark Matter particles
• A note on interacting holographic dark energy with a Hubble-scale cutoff
• Crossing of the Phantom Divided Barrier with Lorentz Invariance Violating Fields
• Curvature Inspired Cosmological Scenario
• Role of Modified Chaplygin Gas as a Dark Energy Model in Collapsing Spherically Symmetric Cloud
• Comparison of Frames: Jordan vs Einstein Frame for a Non-minimal Dark Energy Model
• Cosmological Evolution of Global Monopoles
• Limits Due to Instrumental Polarisation in CMB Experiments at Microwave Wavelengths
• Cosmological anisotropy from non-comoving dark matter and dark energy
• Direct dark matter searches - Test of the Big Bounce Cosmology
• Anisotropic f(Q) gravity model with bulk viscosity
• Parameterizing and Measuring Dark Energy Trajectories from Late-Inflatons
• Global fits for the spectral index of the cosmological curvature perturbation
• A Singular Conformal Spacetime
• Late reionizations of the Universe and their manifestation in the CMB data
• Constraint on Cosmological Model with Matter Creation Using Complementary Astronomical Observations
• Cosmological evolution of interacting dark energy in Lorentz violation
• Best values of parameters for interacting HDE with GO IR-cutoff in Brans-Dicke cosmology
• Holographic dark energy with the sign-changeable interaction term
• Reconstruction of $f(R,T)$ gravity model via the Raychaudhuri equation
• Partial rip scenario - a cosmology with a growing cosmological term
• Euler-Heisenberg black hole surrounded by quintessence in the background of perfect fluid dark matter: Thermodynamics, Shadows and Quasinormal modes
• An exact model of conformal quintessence
• TASI Lectures: Cosmology for String Theorists
• Bayesian joint estimation of non-Gaussianity and the power spectrum
• MAXIMA: A Balloon-Borne Cosmic Microwave Background Anisotropy Experiment
• Friedmann Equation for Brans Dicke Cosmology
• Gravitationally induced matter creation in scalar-tensor $f(R,T_{\mu \nu }{T}^{\mu \nu })$ gravity
• Mirage: a new iterative Map-Making code for CMB experiments
• Measuring ${\sigma }_8$ using DESI Legacy Imaging Surveys Emission-Line Galaxies and Planck CMB Lensing and the Impact of Dust on Parameter Inference
• Constraints on Omega_B, Omega_m and h from MAXIMA and BOOMERANG
• Blind component separation for polarized observations of the CMB
• Einstein's Biggest Blunder? High-Redshift Supernovae and the Accelerating Universe
• Direct Wimp Detection in Directional Experiments
• Current constraints on Cosmological Parameters from Microwave Background Anisotropies
• Direct Detection Rates of Dark Matter Coupled to Dark Energy
• A tensor theory of space-time as a strained material continuum
• Charged gravastar model in Rastall theory of gravity
• The Confining Heterotic Brane Gas: A Non-Inflationary Solution to the Entropy and Horizon Problems of Standard Cosmology
• Holographic Dark Energy Model and Scalar-Tensor Theories
• Implications of the WMAP Age Measurement for Stellar Evolution and Dark Energy
• Dark Energy: The Observational Challenge
• Bumpy Power Spectra and dT/T
• Dark Energy and the Hubble Age
• Observational constraints on the interacting dark energy - dark matter (IDM) cosmological models
• Comparing and combining the Saskatoon, QMAP and COBE CMB maps
• Clustering of SZ clusters on a past light-cone: acoustic oscillations and constraints on dark energy
• Tracing the Nature of Dark Energy with Galaxy Distribution
• Bremsstrahlung in the gravitational field of a global monopole
• Inhomogeneous Big Bang Nucleosynthesis and the High Baryon Density Suggested by Boomerang and MAXIMA
• MAXIPOL: A Balloon-borne Experiment for Measuring the Polarization Anisotropy of the Cosmic Microwave Background Radiation
• Scaling property and peculiar velocity of global monopoles
• Small Second Acoustic Peak from Interacting Cold Dark Matter?
• Anisotropic bulk viscous string cosmological models of the Universe under a time-dependent deceleration parameter
• Peaks in the CMBR power spectrum. II. Physical interpretation for any cosmological scenario
• RHDE models in FRW Universe with two IR cut-offs with redshift parametrization
• Residual noise covariance for Planck low-resolution data analysis
• A heuristic wave equation parameterizing BEC dark matter halos with a quantum core and an isothermal atmosphere
• The CMB power spectrum at l=30-200 from QMASK
• Detectability of Cosmic Topology in Flat Universes
• The Central Mass and Phase-Space Densities of Dark Matter Halos: Cosmological Implications
• A Two-field Dilaton Model of Dark Energy
• Supernovae as a probe of particle physics and cosmology
• CMB anisotropies from pre-big bang cosmology
• Kaluza-Klein Type Robertson Walker Cosmological Model With Dynamical Cosmological Term $\Lambda$
• Neutrino Dark Energy and Moduli Stabilization in a BPS Braneworld Scenario
• Reproducing the observed Cosmic microwave background anisotropies with causal scaling seeds
• Leptogenesis in a Realistic Supersymmetric Model of Inflation with a Low Reheat Temperature
• Direct Dark Matter Detection with Velocity Distribution in the Eddington approach
• Optimized in-flight absolute calibration for extended CMB surveys
• Small-Scale Cosmic Microwave Background Polarization from Reionization
• The lepton asymmetry: the last chance for a critical-density cosmology?
• Phantom Cosmology with Non-minimally Coupled Real Scalar Field
• The Angular Power Spectrum of the First-Year WMAP Data Reanalysed
• Interacting Holographic Dark Energy, the Present Accelerated Expansion and Black Holes
• The primordial baryonic clouds and their contribution to the CMB anisotropy and polarization formation
• Cosmological parameters from complementary observations of the Universe
• Future Island Universes in a Background Universe Accelerated by Cosmological Constant and by Quintessence
• Reheating and particle creation in unimodular f(R, T) gravity
• A Sober Assessment of Cosmology at the New Millennium
• Scalar field-perfect fluid correspondence and nonlinear perturbation equations
• Asymfast, a method for convolving maps with asymmetric main beams
• Precision Primordial ${}^4$He Measurement with CMB Experiments
• Is Noncommutative Eternal Inflation Possible?
• Dark Energy From Fifth Dimensional Brans-Dicke Theory
• Concerning Parameter Estimation Using the Cosmic Microwave Background
• Dynamical-Screening and the Phantom-Like Effects in a DGP-Inspired $F(R,\varphi )$ Model
• Correlated Component Analysis for diffuse component separation with error estimation on simulated Planck polarization data
• Tomography of the Reionization Epoch with Multifrequency CMB Observations
• Generalized Self-similar Scalar-Tensor Theories
• Observations of the High Redshift Universe
• Non-linear Preheating with Scalar Metric Perturbations
• Gravitational Collapse in Higher Dimensional Husain Space-Time
• Ricci Dark Energy of Amended FRW Universe in Chern-Simon Modified Gravity
• Correlations Between the WMAP and MAXIMA Cosmic Microwave Background Anisotropy Maps
• Fast Parameter Estimation from the CMB Power Spectrum
• The mass function of the Las Campanas loose groups of galaxies
• Quantum driven Bounce of the future Universe
• Testing Gaussianity on Archeops Data
• Knotlike Cosmic Strings in The Early Universe
• Map-making methods for Cosmic Microwave Background experiments
• An FLRW interacting dark energy model of the Universe
• Reconstruction of $5D$ Cosmological Models From Equation of State of Dark Energy
• A flat FRW model with dynamical $\Lambda$ as function of matter and geometry
• Quintessence Model and Observational Constraints
• Light WIMP searches involving electron scattering
• Relic gravitational waves and the generalized second law
• Vacuum Bubbles Nucleation and Dark Matter Production through Gauge Symmetry Rearrangement
• Cosmology from Cosmic Microwave Background and Galaxy Clusters
• Clusters of galaxies: setting the stage
• Power-law solutions and accelerated expansion in scalar-tensor theories
• Theoretical direct WIMP detection rates for transitions to nuclear excited states
• Self-Dual Cosmic Strings and Gravitating Vortices in Gauged Sigma Models
• Determining Foreground Contamination in CMB Observations: Diffuse Galactic Emission in the MAXIMA-I Field
• Omega_m - Different Ways to Determine the Matter Density of the Universe
• FRW dark energy cosmological model with hybrid expansion law
• Graviton mass and total relative density of mass Omega_tot in Universe
• Is Physics Asking for a New Kinematics?
• Thermal fluctuations in viscous cosmology
• ARCRAIDER II: Arc search in a sample of non-Abell clusters
• Analytic Spectra of CMB Anisotropies and Polarization Generated by Scalar Perturbations in Synchronous Gauge
• Consistency of nonlinear interacting ghost dark energy with recent observations
• Comparing teh holographic principle inspired dark energy models
• COSMOSOMAS: A Circular Scanning Instrument to Map the Sky at Centimetric Wavelengths
• Interacting holographic dark energy models: A general approach
• Determining cosmic microwave background structure from its peak distribution
• Galaxy-QSO Correlation induced by Weak Gravitational Lensing arising from Large-Scale Structure
• Constraining Cosmological Models by the Cluster Mass Function
• Warm inflation with non-comoving scalar field and radiation fluid
• Noncommutative wormhole in de Rham-Gabadadze-Tolley like massive gravity
• UHECR as Decay Products of Heavy Relics? The Lifetime Problem
• F(R) cosmology via Noether symmetry and lambda-Chaplygin Gas like model
• The supercluster-void network V. Alternative evidence for its regularity
• Dense gas clouds and the Unidentified EGRET sources
• Stable phantom-divide crossing in two scalar models with matter
• Gravitational Origin of Phantom Dark Energy and Late Cosmic Acceleration
• Constraints from the damping tail
• Cosmological models of generalized ghost pilgrim dark energy (GGPDE) in the gravitation theory of Saez-Ballester
• Simulating the formation of cosmic structure
• Recent Results from the MAXIMA Experiment
• Numerical computation of Maass waveforms and an application to cosmology
• Local Constraints on the Oscillating G Model
• Thermal non-Gaussianity in holographic cosmology
• Brane gas-driven bulk expansion as a precursor stage to brane inflation
• Gauge Theories on de Sitter space and Killing Vectors
• A Comparison of Quintessence and Nonlinear Born-Infeld Scalar Field Using Gold Supernova data
• Dissipative quintessence, and its cosmological implications
• Quantum Statistical Entropy and Minimal Length of 5D Ricci-flat Black String with Generalized Uncertainty Principle
• WMAP Constraints on Quintessence
• Suppression of Gravitational Structure Formation by Cosmological Accretion Heating
• X-ray Clusters of Galaxies as Cosmological Tools
• Effect of component separation on the temperature distribution of the CMB
• Cosmological constraints on dark energy
• Predictions of mixed non-Gaussian cosmological density fields for the cosmic microwave background radiation
• On primordial trispectrum from exchanging scalar modes in general multiple field inflationary models
• Particle Creation in Pre-Big-Bang Cosmology: theory and observational consequences
• Strong lensing, cosmology and lensing halos
• Weak gravitational lensing by compact objects in fourth order gravity
• Gaussianity of the CMB: Smooth Goodness of Fit Tests Applied to Interferometric Data
• Amplitude-Phase Analysis of Cosmic Microwave Background maps
• Rapid onset of the 21-cm signal suggests a preferred mass range for dark matter particle
• Recent CMB Observations and the Ionization History of the Universe
• Scalar Field as Dark Energy Accelerating Expansion of the Universe
• Viscous Dark Energy and Phantom Field in An Anisotropic Universe
• Spectral Indications of thermal Sunyaev-Zel'dovich Effect in Archeops and WMAP Data
• Ghost dark energy with sign-changeable interaction term
• Barrow holographic dark energy models in $f\left(Q\right)$ symmetric teleparallel gravity with Lambert function distribution
• CMB Telescopes and Optical Systems
• Topology of the Las Campanas Redshift Survey
• Mixed fluid cosmological model in $f(R,T)$ gravity
• Accelerating Cosmic Microwave Background map-making procedure through preconditioning
• On the primordial helium content: CMB and stellar constraints
• Comments on Scalar-Tensor Representation of $f(R)$ Theories
• Non-singular inflation with vacuum decay
• Inelastic WIMP-nucleus scattering to the first excited state in ${}^{125}$Te
• Posing Constraints on the Free Parameters of a New Model of Dark Energy EoS : Responses Through Cosmological Behaviours
• CMB Polarization as complementary information to anisotropies
• Nonlinear Behavior of Baryon Acoustic Oscillations in Redshift Space from the Zel'dovich Approximation
• Primordial Feature at the Scale of Superclusters of Galaxies
• The Sunyaev-Zel'dovich Effect: Results and Future Prospects
• Voids and overdensities of coupled Dark Energy
• Aspects of Some New Versions of Pilgrim Dark Energy in DGP Braneworld
• Inflationary scenarios with scale-invariant spectral tensorial index
• Probing large-scale structure with large samples of X-ray selected AGN: I Baryonic acoustic oscillations
• What have we learned from observational cosmology ?
• Implications of the BOOMERANG and MAXIMA-I results for the Baryon Mass Fraction in Clusters of galaxies
• Astrophysical and electromagnetic emissivity properties of black holes surrounded by a quintessence type exotic fluid in the Scalar-Vector-Tensor Modified Gravity
• Status of CMB Polarization Measurements from DASI and Other Experiments
• Causal perturbation theory in general FRW cosmologies I: energy momentum conservation and matching conditions
• The shape of a small universe: signatures in the cosmic microwave background
• Goodness-of-fit tests of Gaussianity: constraints on the cumulants of the MAXIMA data
• A cosmological model describing the early inflation, the intermediate decelerating expansion, and the late accelerating expansion by a quadratic equation of state
• Reconstruction of Five-dimensional Bounce cosmological Models From Deceleration Factor
• Geometrical measures of non-Gaussianity generated from single field Inflationary models
• Observational Matter Power Spectrum and the Height of the Second Acoustic Peak
• Acceptable Inverse Power Law Potential Quintessence with n=18/7
• Curvature of the universe and the dark energy potential
• Tsallis holographic inflation in $f(R,T)$ gravity: CMB constraints, reheating, and swampland implications
• Validation of Emission-Line Galaxies Target Selection Algorithms for the Dark Energy Spectroscopic Instrument Using the MMT Binospec
• Constraining the reionization history with large angle CMB polarization
• Crossing of the Cosmological Constant Boundary - an Equation of State Description
• Gauge Theories on A(dS) space and Killing Vectors
• Structure formation and CMBR anisotropy spectrum in the inflessence model
• Constraining $f(R)$ Theories with Temporal Variation of Fine Structure Constant
• Tests of Gaussianity
• Transient Accelerating Scalar Models with Exponential Potential
• Cosmological models based on a complex scalar field with a power-law potential associated with a polytropic equation of state
• Cosmic opacity to CMB photons and polarization measurements
• Cosmic String Signatures in the Cosmic Microwave Background Anisotropies
• Beyond the Standard Model of Physics with Astronomical Observations
• Bouncing Universe with a Nonminimally Coupled Scalar Field on a Moving Domain Wall
• Cosmic Evolution with Early and Late Acceleration Inspired by Dual Nature of the Ricci Scalar Curvature
• Inhomogenous Primordial Baryon Distributions on Sub-Galactic Scales: High-z Galaxy Formation with WDM
• Have Acoustic Oscillations been Detected in the Current Cosmic Microwave Background Data?
• Interacting Induced Dark Energy Model
• Dynamics of Multi-Component, Multi-Field Quintessence
• Polarization experiments
• Non-Linearly Interacting Ghost Dark Energy in Brans-Dicke Cosmology
• Far infrared polarimeter with very low instrumental polarization
• Constraining Dynamical Dark Energy Models through the Abundance of High-Redshift Supermassive Black Holes
• Can inflationary models of cosmic perturbations evade the secondary oscillation test?
• 20+ years of Inflation
• Considering Late-Time Acceleration in some Cosmological Models
• How accurately can suborbital experiments measure the CMB?
• Defect Formation Rates in Cosmological First-Order Phase Transitions
• Lensing-induced Non-Gaussian Signatures in the Cosmic Microwave Background
• Predictions of Dynamically Emerging Brane Inflation Models
• Halo Density Profiles Consistent with Asymmetric M-B Velocity Distributions-Implications on Direct Dark Matter Searches
• On Inflation and Variation of the Strong Coupling Constant
• Viscous Cardassian universe
• Primordial Gaussian Fluctuations from Cosmic Defects
• Gauss-Bonnet Braneworld Cosmology with Modified Induced Gravity on the Brane
• Predicted modulated differential rates for direct WIMP searches at low energy transfers
• A Newtonian Model for the Quantum Gravitational Back-Reaction on Inflation
• About the connection between the $C_{\ell }$ power spectrum of the Cosmic Microwave Background and the ${\Gamma }_m$ Fourier spectrum of rings on the sky
• Anisotropic background for two fluids: matter and holographic dark energy
• Phantom Mimicry on the Normal Branch of a DGP-inspired Braneworld Scenario with Curvature Effect
• Dark Matter phenomenology : from simplified WIMP models to refined alternative solutions
• Cosmic Equation of State and Advanced LIGO Type Gravity Wave Experiments
• CMB and Cosmological Parameters: Current Status and Prospects
• Phase structure of the $O(2)$ ghost model with higher-order gradient term
• The picture of our universe: A view from modern cosmology
• Overconstrained dynamics in galaxy redshift surveys
• Kaluza-Klein Higher Derivative Induced Gravity
• Reconstruction of a Deceleration Parameter from the Latest Type Ia Supernovae Gold Dataset
• Vacuum Decay Constraints on a Cosmological Scalar Field
• The Standard Model, Dark Matter, and Dark Energy: From the Sublime to the Ridiculous
• In Support of Inflation
• Periodic distribution of galaxies in generalized scalar tensor theory
• A theoretically-explained new-variant of Modified-Newtonian-Dynamics (MOND)
• Scattering of scalar perturbations with cosmological constant in low-energy and high-energy regimes
• The Fourth Gravity Test and Quintessence Matter Field
• Red Density Perturbations and Inflationary Gravitational Waves
• On the cosmological viability of the Hu-Sawicki type modified induced gravity
• Cosmological constraints from galaxy clustering
• Inflation
• Statistical evaluation of the observational information on ${\Omega }_m$ and ${\Omega }_{\Lambda }$
• Power-law solutions for TeVeS
• The ${\Omega }_{DE}-{\Omega }_M$ Plane in Dark Energy Cosmology
• Inhomogeneous structure formation may alleviate need for accelerating universe
• An overview of the current status of CMB observations
• FLRW Cosmology of Induced Dark Energy Model and Open Universe
• Observational constraints in late time for an axially symmetric transitioning model with bulk viscous fluid
• Classical and quantum quintessence cosmology
• The Cosmic Microwave Background anisotropies: open problems
• Likelihood distribution for models with cosmological constant from COBE data
• Cosmology Rounding the Cape
• Multi-component power spectra estimation method for multi-detector observations of the Cosmic Microwave Background
• Cosmic Time Transformations in Cosmological Relativity
• Acceleration and Deceleration in Curvature Induced Phantom Model of the Late and Future Universe, Cosmic Collapse as Well as its Quantum Escape
• Searching for light WIMPS in view of neutron decay to dark matter
• Solar neutrinos as background in dark matter searches involving electron detection
• On the Cross-Correlation between Dark Matter Distribution and Secondary CMB Anisotropies by Ionized Intergalactic Medium
• Physics of Cosmic Microwave Background anisotropies and primordial fluctuations
• Reply to "On scaling solutions with a dissipative fluid"
• Constraining Lambda using cluster quadrupoles
• Holographic F(Q,T) Gravity with Lambert Solution
• Predicted rates for direct WIMP searches
• Testing CMB polarization data using position angles
• An Inflationary Scenario Taking into Account of Possible Dark Energy Effects in the Early Universe
• Direct dark matter detection: The diurnal variation in directional experiments
• On Local Approximations to the Nonlinear Evolution of Large-Scale Structure
• Excessive shift of the CMB acoustic peaks of the Cold Spot area
• Goodness--of--fit Statistics and CMB Data Sets
• Testing the CMB Data for Systematic Effects
• Stability of HDE model with sign-changeable interaction in Brans-Dicke theory
• Cosmic Microwave Background anisotropies: the power spectrum and beyond
• Fluids in cosmology
• A comparison of designs of off-axis Gregorian telescopes for mm-wave large focal plane arrays
• Determination of cosmology and evolution from K-band magnitude-redshift and number count observations
• Multiple Peaks in the CMB
• How much will we learn from the CMB ?
• Revisiting Agegraphic Dark Energy in Brans-Dicke Cosmology
• Cosmological Parameter Estimation: Method
• Can hyperbolic phase of Brans-Dicke field account for Dark Matter?
• Pico: Parameters for the Impatient Cosmologist
• The BaR-SPOrt Experiment
• Extended black hole cosmologies in de Sitter space
• Quintessence and the first Doppler peak
• Non-linear effects in early Universe cosmology
• Bianchi type-III THDE quintessence model with hybrid expansion law
• Forecasting isocurvature models with CMB lensing information: axion and curvaton scenarios
• Cosmological predictions from the Misner brane
• Evolution of entropic dark energy and its phantom nature
• Inflationary study of non-Gaussianity using two-dimensional geometrical measures of CMB temperature maps
• Seeable universe and its accelerated expansion: an observational test
• On the accelerated expansion of the cosmos
• Archeops, mapping the CMB sky from large to small angular scales
• $\Lambda$CDM, $\Lambda$DGP and extended phantom-like cosmologies
• Maps of the Cosmos: The Cosmic Microwave Background