Measurements of Ω and Λ from 42 High‐Redshift Supernovae
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Constraints on the Dark Side of the Universe and Observational Hubble Parameter DataAxions and the strong C P problemTheoretical aspects of massive gravityExperimental astrophysics with high power lasers and Z pinchesThe cosmological constant and dark energyMore on ghosts in the Dvali-Gabadaze-Porrati modelMechanics and Newton-Cartan-like gravity on the Newton-Hooke space-timede Sitter vacua in string theoryImportance of supernovae at z > 1.5 to probe dark energyLong-term future of extragalactic astronomyLong γ-ray bursts and core-collapse supernovae have different environmentsPeculiar motions, accelerated expansion, and the cosmological axisQuark masses: An environmental impact statementA guided tour through the wild nuclear landscapeProbing violation of the Copernican principle via the integrated Sachs-Wolfe effectBehavior of varying-alpha cosmologiesHolography and the large number hypothesisEvidence for Dark Energy from the Cosmic Microwave Background Alone Using the Atacama Cosmology Telescope Lensing MeasurementsMeasurement of the Casimir Force between Parallel Metallic SurfacesConfirmation of the Copernican Principle at Gpc Radial Scale and above from the Kinetic Sunyaev-Zel’dovich Effect Power SpectrumReconstructing the Cosmic Equation of State from Supernova DistancesChameleon cosmologyA Test of the Copernican PrincipleWhy the universe is just soTesting general relativity with 21-cm intensity mappingConservation laws in theories with universal gravity/matter couplingIs cosmic speed-up due to new gravitational physics?Detecting dark energy in orbit: The cosmological chameleonLate-time cosmology of a scalar-tensor theory with a universal multiplicative coupling between the scalar field and the matter LagrangianBlack-Hole No-Hair Theorems for a Positive Cosmological ConstantObservational constraints on dark energy and cosmic curvatureCoexistence of Black Holes and a Long-Range Scalar Field in CosmologySupermassive boson star at the galactic center?Quintessence as a runaway dilatonUncorrelated measurements of the cosmic expansion history and dark energy from supernovaeDark energy or apparent acceleration due to a relativistic cosmological model more complex than the Friedmann-Lemaitre-Robertson-Walker model?Living in a Void: Testing the Copernican Principle with Distant SupernovaeNew Dark Energy Constraints from Supernovae, Microwave Background, and Galaxy ClusteringCosmology from start to finishSupernova SN 2011fe from an exploding carbon-oxygen white dwarf star
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Measurements of Ω and Λ from 42 High‐Redshift Supernovae
description
article publié dans la revue scientifique Astrophysical Journal
@fr
im Juni 1999 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in the Astrophysical Journal
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована в червні 1999
@uk
name
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
@en
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
@nl
type
label
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
@en
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
@nl
prefLabel
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
@en
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
@nl
P2093
P50
P356
P1476
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
@en
P2093
A. S. Fruchter
A. V. Filippenko
B. J. Boyle
B. Schaefer
C. R. Pennypacker
D. E. Groom
G. Goldhaber
P304
P356
10.1086/307221
P407
P577
1999-06-01T00:00:00Z
P5875
P818
astro-ph/9812133
P819
1999ApJ...517..565P