%D8%A2%D8%AF%D9%85_%D8%B1%D9%8A%D8%B3%D8%A2%D8%AF%D9%85_%D8%B1%D9%8A%D8%B3%D8%A2%D8%AF%D9%85_%D8%B1%DB%8C%D8%B3%D0%90%D0%B4%D0%B0%D0%BC_%D0%A0%D1%8B%D1%81%D0%90%D0%B4%D0%B0%D0%BC_%D0%A0%D0%B8%D0%B9%D1%81%E0%A6%85%E0%A7%8D%E0%A6%AF%E0%A6%BE%E0%A6%A1%E0%A6%BE%E0%A6%AE_%E0%A6%9C%E0%A6%BF._%E0%A6%B0%E0%A7%87%E0%A6%87%E0%A6%B8Adam_RiessCategory:Adam_RiessAdam_RiessAdam_RiessAdam_RiessAdam_RiessAdam_RiessAdam_RiessAdam_Riess%D8%A2%D8%AF%D9%85_%D8%B1%DB%8C%D8%B3Adam_RiessAdam_RiessAdam_Riess%D7%90%D7%93%D7%9D_%D7%A8%D7%99%D7%A1%E0%A4%8F%E0%A4%A1%E0%A4%AE_%E0%A4%B0%E0%A5%80%E0%A4%B8Adam_RiessAdam_Riess%D4%B1%D5%A4%D5%A1%D5%B4_%D5%8C%D5%AB%D5%BDAdam_G._RiessAdam_Guy_RiessAdam_RiessAdam_Riess%E3%82%A2%E3%83%80%E3%83%A0%E3%83%BB%E3%83%AA%E3%83%BC%E3%82%B9_(%E5%A4%A9%E4%BD%93%E7%89%A9%E7%90%86%E5%AD%A6%E8%80%85)%E0%B2%86%E0%B2%A6%E0%B2%AE%E0%B3%8D_%E0%B2%9C%E0%B2%BF._%E0%B2%B0%E0%B3%80%E0%B2%B8%E0%B3%8D%EC%95%A0%EB%8D%A4_%EB%A6%AC%EC%8A%A4Adam_Riess%C4%80dams_R%C4%ABss%D0%90%D0%B4%D0%B0%D0%BC_%D0%A0%D0%B8%D1%81Adam_RiessAdam_Guy_RiessAdam_RiessAdam_G._RiessAdam_G._RiessAdam_Riess
about
P185
P3373
Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samplesThe Sloan Digital Sky Survey-II supernova survey: technical summaryFirst-year spectroscopy for the Sloan Digital Sky Survey-II supernova surveyCosmological Results from High‐zSupernovaeThe Puzzle of Dark Energy.A luminous, blue progenitor system for the type Iax supernova 2012Z.Astrophysics. Multiple images of a highly magnified supernova formed by an early-type cluster galaxy lens.A 3% solution: determination of the Hubble constant with the Hubble Space Telescope and Wide Field Camera 3Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological ConstantExtreme magnification of an individual star at redshift 1.5 by a galaxy-cluster lensParallax beyond a kiloparsec from spatially scanning the wide field camera 3 on the Hubble Space TelescopeMeasuring the Hubble constantA geometric distance to the galaxy NGC4258 from orbital motions in a nuclear gas diskThe seventh data release of the Sloan Digital Sky SurveyPS1-10afx ATz= 1.388: PAN-STARRS1 DISCOVERY OF A NEW TYPE OF SUPERLUMINOUS SUPERNOVACepheid Calibrations from the Hubble Space Telescope of the Luminosity of Two Recent Type Ia Supernovae and a Redetermination of the Hubble ConstantDid LIGO Detect Dark Matter?The rise and fall of type Ia supernova light curves in the SDSS-II supernova surveyMilky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble ConstantA 2.4% determination of the local value of the Hubble constantThe SH0ES Project: Observations of Cepheids in NGC 4258 and Type Ia SN HostsThe superluminous supernova PS1-11ap: bridging the gap between low and high redshiftObservational probes of cosmic accelerationThe Sloan Digital Sky Survey-II supernova survey: search algorithm and follow-up observationsLight curves of 213 type Ia supernovae from the ESSENCE surveyThe spectroscopic diversity of type Ia supernovaeEvidence for type Ia supernova diversity from ultraviolet observations with the Hubble space telescopeSpectroscopy of high-redshift supernovae from the ESSENCE project: the first four yearsConstraining Cosmic Evolution of Type Ia SupernovaeTime Dilation in Type Ia Supernova Spectra at High RedshiftExploring the Outer Solar System with the ESSENCE Supernova SurveyObservational Constraints on the Nature of Dark Energy: First Cosmological Results from the ESSENCE Supernova SurveyScrutinizing Exotic Cosmological Models Using ESSENCE Supernova Data Combined with Other Cosmological ProbesThe ESSENCE Supernova Survey: Survey Optimization, Observations, and Supernova PhotometryA Light Echo from Type Ia SN 1995E?Hubble Space Telescopeand Ground‐based Observations of Type Ia Supernovae at Redshift 0.5: Cosmological ImplicationsUsing Line Profiles to Test the Fraternity of Type Ia Supernovae at High and Low RedshiftsHubble Space TelescopeObservations of Nine High-Redshift ESSENCE SupernovaeSpectroscopy of High-Redshift Supernovae from the ESSENCE Project: The First 2 YearsImaging and Demography of the Host Galaxies of High-Redshift Type Ia Supernovae
P50
description
American Nobel laureate
@en
Amerikaans astrofysicus, Nobelprijswinnaar
@nl
US-amerikanischer Astronophysiker
@de
americký astrofyzik
@sk
americký astrofyzik, nositel Nobelovy ceny
@cs
amerikansk astrofysiker
@sv
amerikansk astronom
@da
amerikansk astronom
@nb
amerikansk astronom
@nn
amerykański astrofizyk, noblista
@pl
name
Adam G. Riess
@id
Adam G. Riess
@nb
Adam G. Riess
@nn
Adam G. Riess
@ro
Adam Guy Riess
@io
Adam Guy Riess
@nds
Adam Riess
@ast
Adam Riess
@ca
Adam Riess
@cs
Adam Riess
@cy
type
label
Adam G. Riess
@id
Adam G. Riess
@nb
Adam G. Riess
@nn
Adam G. Riess
@ro
Adam Guy Riess
@io
Adam Guy Riess
@nds
Adam Riess
@ast
Adam Riess
@ca
Adam Riess
@cs
Adam Riess
@cy
altLabel
A. G. Riess
@fr
A. Riess
@fr
Adam G. Riess
@cs
Adam G. Riess
@de
Adam G. Riess
@eo
Adam G. Riess
@es
Adam G. Riess
@fr
Adam G. Riess
@pl
Adam G. Riess
@sv
Adam G. Riess
@tr
prefLabel
Adam G. Riess
@id
Adam G. Riess
@nb
Adam G. Riess
@nn
Adam G. Riess
@ro
Adam Guy Riess
@io
Adam Guy Riess
@nds
Adam Riess
@ast
Adam Riess
@ca
Adam Riess
@cs
Adam Riess
@cy