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In this Letter, we propose a model-independent method to determine the Hubble constant and curvature simultaneously taking advantage of the possibilities of future space-borne gravitational wave (GW) detector DECIGO in combination with the…

宇宙学与河外天体物理 · 物理学 2024-04-12 Tonghua Liu , Shuo Cao , Marek Biesiada , Yilong Zhang , Jieci Wang

We propose a method to determine the galactic constants R_0 (distance to the Galactic Center) and V_0 (rotation velocity of the Sun) from measurements of distances, radial velocities and proper motions of objects near the solar circle. This…

星系天体物理 · 物理学 2015-05-28 Y. Sofue , T. Nagayama , M. Matsui , A. Nakagawa

The Gaia celestial reference frame (Gaia-CRF) will benefit from a close assessment with independent methods, such as Very Long Baseline Interferometry (VLBI) measurements of radio stars at bright magnitudes. However, obtaining full…

Lorentz symmetry violations can be described by an effective field theory framework that contains both General Relativity and the Standard Model of particle physics called the Standard-Model extension (SME). Recently, post-fit analysis of…

广义相对论与量子宇宙学 · 物理学 2017-01-04 C. Le Poncin-Lafitte , A. Hees , S. lambert

Galaxy cluster peculiar velocities can be inferred from high-sensitivity, high-resolution multiple-frequency observations in the 30 to 400 GHz range. While galaxy cluster counts and power spectra are sensitive to the growth factor, peculiar…

天体物理学 · 物理学 2009-11-07 A. Peel , L. Knox

Spatially-resolved X-ray observations are the key to understanding electron acceleration in solar flares. Currently, the underlying processes that efficiently energize solar flare particles are poorly constrained. Abundant flare…

太阳与恒星天体物理 · 物理学 2026-03-09 Morgan Stores , Natasha Jeffrey , Ewan Dickson , James McLaughlin , Eduard Kontar

We present a novel approach to disentangle two key contributions to the largest-scale anisotropy of the galaxy distribution: (i) the intrinsic dipole due to clustering and anisotropic geometry, and (ii) the kinematic dipole due to our…

宇宙学与河外天体物理 · 物理学 2021-11-09 Tobias Nadolny , Ruth Durrer , Martin Kunz , Hamsa Padmanabhan

Stellar activity is a potential important limitation to the detection of low mass extrasolar planets with indirect methods (RV, photometry, astrometry). In previous papers, using the Sun as a proxy, we investigated the impact of stellar…

太阳与恒星天体物理 · 物理学 2015-05-27 A. -M. Lagrange , N. Meunier , M. Desort , F. Malbet

Astrometric monitoring of stars provides a promising method for discovery of low-mass planets around nearby Sun-like stars. The astronomical community has proposed several telescopes designed to perform high-precision astrometric…

太阳与恒星天体物理 · 物理学 2026-05-20 Conaire Deagan , Benjamin T. Montet , P. Tuthill , M. Ferraro , R. Lyu , E. Sheehan

In the framework of focused transport theory, adiabatic deceleration arises from adiabatic focusing in the solar wind frame and from differential solar wind convection. An explicit formula is given for the deceleration of individual…

天体物理学 · 物理学 2009-10-22 D. Ruffolo

The motion of the solar system against an isotropic radiation background, such as the cosmic microwave background, induces a dipole anisotropy in the background due to the Doppler effect. Flux-limited observation of the continuum radiation…

宇宙学与河外天体物理 · 物理学 2025-01-20 Kyungjin Ahn

Doppler imaging spectroscopy is the most reliable way to directly measure wind speeds of planetary atmospheres of the Solar system. However, most knowledge about atmospheric dynamics has been obtained with cloud-tracking technique, which…

地球与行星天体物理 · 物理学 2019-06-14 Patrick Gaulme , Francois-Xavier Schmider , Ivan Goncalves

Published analyses of very long baseline interferometry (VLBI) data for the sources included in the third International Celestial Reference Frame (ICRF3) catalog have revealed object-specific, excess astrometric variability and…

The next generation of galaxy surveys will provide highly accurate measurements of the large-scale structure of the Universe, allowing for more stringent tests of gravity on cosmological scales. Higher order statistics are a valuable tool…

宇宙学与河外天体物理 · 物理学 2023-03-29 Alejandro Aviles , Gustavo Niz

We observed the pair of radio sources 1150+812 and 1803+784 in November 1993 with a VLBI array, simultaneously recording at 8.4 and 2.3 GHz. We determined the angular separation between the two sources with submilliarcsecond accuracy by…

天体物理学 · 物理学 2009-10-31 M. A. Perez-Torres , J. M. Marcaide , J. C. Guirado , E. Ros

HI absorption systems are great targets for direct measurement of the Sandage-Loeb (SL) effect throughout a wide range of redshift for ground-based radio telescopes. We demonstrate the significance of improving the accuracy of SL effect…

宇宙学与河外天体物理 · 物理学 2020-02-05 Kang Jiao , Jian-Chen Zhang , Tong-Jie Zhang , Hao-Ran Yu , Ming Zhu , Di Li

In order to establish the position of the center of mass of the Earth in the International Celestial Reference Frame, observations of the Global Positioning Satellite (GPS) constellation using the IVS network are important. With a good…

天体物理仪器与方法 · 物理学 2010-08-30 John M. Dickey

Here we explore the possibility of extending to the Solar System scenario the combined residual approach employed for the deterination of the Lense-Thirring effect in the Earth-LAGEOS satellites system. After calculating the secular…

广义相对论与量子宇宙学 · 物理学 2013-11-04 Lorenzo Iorio

Imaging systems based on a narrow-band tunable filter are used to obtain Doppler velocity maps of solar features. These velocity maps are created by taking the difference between the blue- and red-wing intensity images of a chosen spectral…

太阳与恒星天体物理 · 物理学 2010-09-16 Sreejith Padinhatteeri , R. Sridharan , K. Sankarasubramanian

General relativistic deflection of light by mass, dipole, and quadrupole moments of gravitational field of a moving massive planet in the Solar system is derived. All terms of order 1 microarcsecond are taken into account, parametrized, and…

天体物理学 · 物理学 2008-11-26 Sergei Kopeikin , Valeri Makarov