搜索结果: 1-13 共查到“天文学 interferometric”相关记录13条 . 查询时间(0.102 秒)
Interferometric 890 mu m images of high-redshift submillimeter galaxies
high redshift submillimeter
font style='font-size:12px;'>
2014/12/23
We present high-resolution 890 μm images of two 20 mJy submillimeter galaxies, SMM J123711+622212 and MIPS J142824.0+352619, obtained using the Submillimeter Array (SMA). Using submillimeter interfero...
Evidence for a population of high-redshift submillimeter galaxies from interferometric imaging
submillimeter formation
font style='font-size:12px;'>
2014/12/23
We have used the Submillimeter Array to image a flux-limited sample of seven submillimeter galaxies, selected by the AzTEC camera on the JCMT at 1.1 mm, in the COSMOS field at 890 μ m with ~2'' resolu...
THE AzTEC/SMA INTERFEROMETRIC IMAGING SURVEY OF SUBMILLIMETER-SELECTED HIGH-REDSHIFT GALAXIES
observations evolution
font style='font-size:12px;'>
2014/12/23
We present results from a continuing interferometric survey of high-redshift submillimeter galaxies (SMGs) with the Submillimeter Array, including high-resolution (beam size ~2 arcsec) imaging of eigh...
Radio Interferometric Planet Search II: Constraints on sub-Jupiter-Mass Companions to GJ 896A
Interferometric Planet Constraints sub-Jupit
font style='font-size:12px;'>
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...
Mid-infrared interferometric monitoring of evolved stars - The dust shell around the Mira variable RR Aql at 13 epochs
Techniques:interferometric – Stars:AGB – Stars:atmospheres – Stars:mass loss – Stars:individual:RR Aql
font style='font-size:12px;'>
2011/9/28
We obtained 13 epochs of mid-infrared interferometry with the MIDI instrument at the VLTI between April 2004 and July 2007, covering pulsation phases 0.45-0.85 within four cycles. The data are modeled...
Prospects for Direct Detection of Inflationary Gravitational Waves by Next Generation Interferometric Detectors
Direct Detection Inflationary Gravitational Waves Next Generation Interferometric Detectors
font style='font-size:12px;'>
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
font style='font-size:12px;'>
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)
font style='font-size:12px;'>
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)
font style='font-size:12px;'>
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)
font style='font-size:12px;'>
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
font style='font-size:12px;'>
2009/6/25
Conclusions of the workshop on the interferometric mode of OSIRIS。
ORBITS OF TWO INTERFEROMETRIC AND ONE VISUAL BINARY STARS
ORBITS OF TWO INTERFEROMETRIC BINARY STARS
font style='font-size:12px;'>
2009/4/22
ORBITS OF TWO INTERFEROMETRIC AND ONE VISUAL BINARY STARS。
NEW ORBITAL ELEMENTS OF 5 INTERFEROMETRIC DOUBLE STARS
ORBITAL ELEMENTS 5 INTERFEROMETRIC DOUBLE STARS
font style='font-size:12px;'>
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...