Sentences with word «polarimetry»

Here we present new J - band imaging polarimetry of LkC... ▽ More LkCa 15 hosts a pre-transitional disk as well as at least one accreting protoplanet orbiting in its gap.

Here we present new J - band imaging polarimetry of LkCa 15 with SPHERE IRDIS, yielding the most accurate and detailed scattered - light images of the disk to date down to the planet - hosting inner regions.

An ad hoc subgroup was formed to produce a stand - alone report on the advantages and requirements for polarimetry for atmospheric correction, aerosol characterization, and oceanic retrievals.

ALMA observed a bright source 3C 286 for the verifications of polarimetry observations.

Peralta, R.J., C. Nardell, B. Cairns, E.E. Russell, L.D. Travis, M.I. Mishchenko, and B.A. Fafaul, 2007: Aerosol polarimetry sensor for the Glory Mission.

Researchers have demonstrated ALMA's unprecedented capability for polarimetry in millimeter wavebands.

Glory's Aerosol Polarimetry Sensor aims to change that.

«This is the very first step in the research on dust evolution with polarimetry, and I believe the future progress will be full of excitement.»

GPI's high contrast imaging and polarimetry capabilities together were essential for this new synthesis.

Lovell Telescope] in Cycle - 7) imaging at cm wavelengths as well as polarimetry, spectroscopy and astrometry.

Both the high CP and its extended size a... ▽ More We present results from deep imaging linear and circular polarimetry of the massive star - forming region NGC 6334 - V.

Rapid development of anisotropic ice.crystal - alignment fabrics inferred from englacial radar polarimetry, central West Antarctica.

The enhanced X-Ray Timing and Polarimetry mission, planned for launch around 2025, would probe x-rays from violent, fast - changing cosmic events.

Only 55 million lightyears away, SN 2017cbv was one of the closest supernovae discovered in recent years, found by the DLT40 survey using the Panchromatic Robotic Optical Monitoring and Polarimetry Telescope (PROMPT) in Chile, which monitors galaxies nightly at distances less than 40 megaparsecs (120 million light - years).

In this talk, and as part of our goal to provide tools for the characterization of ultra-cool atmospheres, I will present an on - going effort to obtain the linear polarimetry indices at optical and near infrared wavelengths for a sample of field ultra-cool dwarfs at different ages.

«Linear polarimetry as a tool to characterize ultra-cool atmospheres» by Paulo Miles Paez, postdoc, Western University

We find that the near - side gap edge revealed by polarimetry matches the sharp crescent seen in previous ADI imaging very well.

These observation results were published by Nagai et al. as «ALMA Science Verification Data: Millimeter Continuum Polarimetry of the Bright Radio Quasar 3C 286» in the Astrophysical Journal issued on 20 June 2016.

ALMA is designed to perform sensitive polarimetry observations.

See also: ALMA News as of July 19, 2016 «ALMA Achieved Highest Sensitivity Polarimetry in Millimeter Wavelength»

The removal of the membrane is due to the high demand for sub-mm polarimetry.

High sensitivity is essential for the precise polarimetry, and ALMA is suitable for it.

Using novel instrumentation SON has a network of telescopes that, while of modest aperture, now have unique capabilities to do 1e - 5 broadband polarimetry.

HBOI researchers and colleagues collected more than 1,500 video - polarimetry measurements from live fish from distinct habitats under a variety of viewing conditions, and have revealed for the first time that fish have an «omnidirectional» solution they use to camouflage themselves, demonstrating a new form of camouflage in nature — light polarization matching.

Investigation of optical birefringence at ferroelectric domain wall in LiNbO3 by phase - shift polarimetry M. Paturzo, L. Aiello, F. Pignatiello, P. Ferraro, P. De Natale, M. de Angelis, and S. De Nicola Applied Physics Letters 88, 151918 - 151920 (2006).

The study of planet surfaces using polarimetry was significantly advanced by the French astronomer Bernard Ferdinand Lyot.

Braak, C.J., J.F. de Haan, J.W. Hovenier, and L.D. Travis, 2002: Spatial and temporal variations of Venus haze properties obtained from Pioneer Venus Orbiter polarimetry.

This is GPI imaging polarimetry of the circumstellar disk around HR 4796A, a ring of dust and planetesimals similar in some ways to a scaled up version of the solar system's Kuiper Belt.

Abstract: We present results from deep imaging linear and circular polarimetry of the massive star - forming region NGC 6334 - V.

«Toward Exploring the Synergy Between Cloud Radar Polarimetry and Doppler Spectral Analysis in Deep Cold Precipitating Systems in the Arctic.»

Chowdhary, J., 1999: Multiple Scattering of Polarized Light in Atmosphere - Ocean Systems: Application to Sensitivity Analyses of Aerosol Polarimetry.

GPI imaging polarimetry of the circumstellar disk around HR 4796A, a ring of dust and planetesimals similar in some ways to a scaled up version of the solar system's Kuiper Belt.

AMiBA, a millimeter interferometer like ALMA, was constructed by ASIAA (Academia Sinica Institute of Astronomy and Astrophysics) and National Taiwan University for polarimetry of microwave background radiation and detection of distant clusters of galaxies using the Sunyaev Zeldovich effect.

The enhanced X-Ray Timing and Polarimetry (eXTP) mission would be China's most ambitious space science satellite yet — and its most expensive, with an estimated price tag of $ 473 million.

Polarimetry of the fast radio burst source FRB121102.

One source of excitement is a $ 440 - million X-ray telescope led by the CNSA, called Enhanced X-ray Timing and Polarimetry (eXTP).

A dedicated instrument for the direct detection of planets, SPHERE, is composed of a polametric camera in visible light, the Zurich IMager POLarimeter (ZIMPOL), and two near - infrared sub-systems: the Infra - Red Dual - beam Imager and Spectrograph (IRDIS), a multi-purpose camera for imaging, polarimetry, and long - slit spectroscopy, and the integral field spectrograph (IFS), an integral field spectrograph.

«This observation has certainly verified the high capability of the polarimetry observation with ALMA,» said Hiroshi Nagai at the National Astronomical Observatory of Japan and the leader of the verification team.

The Near Infrared Camera and Multi-Object Spectrometer (NICMOS) provides imaging capabilities in broad, medium, and narrow band filters, broad - band imaging polarimetry, coronographic imaging, and slitless grism spectroscopy, in the wavelength range 0.8 - 2.5 microns.

Polarimetry is one of the handful methods to investigate magnetic fields in the Universe.

Polarimetry is an important method to investigate magnetic fields in the Universe and astronomers eager to use ALMA for unveiling magnetic mysteries, such as the launching mechanism of high energy jets from supermassive black holes.

The science verification activities for polarimetry is introduced in an article «Polarization observations with ALMA» in the serial column Bienvenido a ALMA!»

The polarimetry and signal modulation are achieved using an achromatic half wave plate (AHWP) rotating on a superconducting magnetic bearing and a fixed wire grid polarizer.

The main techniques will be high - dynamic range imaging, imaging polarimetry, aperture polarimetry, spectropolarimetry,

By using a low - scattered light telescope with the contrast enhancement techniques of coronagraphy and polarimetry, regions around extremely bright sources can be seen.

By combining expertise from various fields — coronagraphy and high contrast imaging from solar physics, polishing, polarimetry and adaptive optics from astronomical communities and the experience of each institutional partner, this telescope will make significant advances in several fields.

They used a single 360 degree camera around the horizontal plane of the targets and used both light microscopy and full - body video - polarimetry.

The main techniques will be high - dynamic range imaging, imaging polarimetry, aperture polarimetry, spectropolarimetry, coronagraphy, and adaptive optics assistance for many of these techniques.