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Radio Interferometric Planet Search II: Constraints on sub-Jupiter-Mass Companions to GJ 896A
Interferometric Planet Constraints sub-Jupit
2011/10/10
We present results from the Radio Interferometric Planet (RIPL) search for compan- ions to the nearby star GJ 896A. We present 11 observations over 4.9 years. Fitting astrometric parameters to the dat...
Prospects for Direct Detection of Inflationary Gravitational Waves by Next Generation Interferometric Detectors
Direct Detection Inflationary Gravitational Waves Next Generation Interferometric Detectors
2011/1/11
We study the potential impact of detecting the inflationary gravitational wave background by the future space-based gravitational wave detectors, such as DECIGO and BBO. The signal-to-noise ratio of e...
Millimeter and submillimeter high angular resolution interferometric observations: dust in the heart of IRAS 18162-2048
circumstellar matter — ISM individual (GGD27, HH 80-81 IRAS 18162-2048)— stars
2010/11/12
The GGD27 complex includes the HH 80-81-80N system, which is one of the most powerful molecular outflows associated with a high mass star-forming region observed up to now. This outflow is powered by ...
Compressed sensing for wide-field radio interferometric imaging
Instrumentation and Methods for Astrophysics (astro-ph.IM)
2011/1/7
For the next generation of radio interferometric telescopes it is of paramount importance to incorporate wide field-of-view (WFOV) considerations in interferometric imaging, otherwise the fidelity of ...
Interferometric imaging with the 32 element Murchison Wide-field Array
Instrumentation and Methods for Astrophysics (astro-ph.IM)
2010/12/28
The Murchison Wide-field Array (MWA) is a low frequency radio telescope, currently under construction, intended to search for the spectral signature of the epoch of re-ionisation (EOR) and to probe th...
Primary Beam Shape Calibration from Mosaicked, Interferometric Observations
Instrumentation and Methods for Astrophysics (astro-ph.IM)
2010/12/24
Image quality in mosaicked observations from interferometric radio telescopes is strongly dependent on the accuracy with which the antenna primary beam is calibrated. The next generation of radio tele...
Conclusions of the workshop on the interferometric mode of OSIRIS
interferometric mode OSIRIS Conclusions of the workshop
2009/6/25
Conclusions of the workshop on the interferometric mode of OSIRIS。
NEW ORBITAL ELEMENTS OF 5 INTERFEROMETRIC DOUBLE STARS
ORBITAL ELEMENTS 5 INTERFEROMETRIC DOUBLE STARS
2009/3/19
In this paper, for the first time, are presented elliptical and Thiel-
Innes orbitatal elements for the following interferometric pairs: WDS 00416+2438
= WRH, WDS 03271+1845 = CHARA 10, WDS 04044+24...