Zobrazeno 1 - 10
of 16
pro vyhledávání: '"Farnes, Jamie"'
Autor:
Anderson, Craig S., Heald, George, O'Sullivan, Shane P., Bunton, John D., Carretti, Ettore, Chippendale, Aaron P., Collier, Jordan D., Farnes, Jamie S., Gaensler, Bryan M., Harvey-Smith, Lisa, Koribalski, Bärbel S., Landecker, Tom L., Lenc, Emil, McClure-Griffiths, Naomi M., Mitchell, Daniel, Rudnick, Lawrence, West, Jennifer
We present observations of linear polarisation in the southern radio lobe of Centaurus A, conducted during commissioning of the Australian Square Kilometre Array Pathfinder (ASKAP) telescope. We used 16 antennas to observe a 30 square degree region i
Externí odkaz:
http://arxiv.org/abs/1811.11760
Publikováno v:
Galaxies 2018, 6(4), 120
The Square Kilometre Array (SKA) will be both the largest radio telescope ever constructed and the largest Big Data project in the known Universe. The first phase of the project will generate on the order of 5 zettabytes of data per year. A critical
Externí odkaz:
http://arxiv.org/abs/1811.08272
Autor:
Sakemi, Haruka, Machida, Mami, Akahori, Takuya, Nakanishi, Hiroyuki, Akamatsu, Hiroki, Kurahara, Kohei, Farnes, Jamie
We report a polarization analysis of the eastern region of W50, observed with the Australia Telescope Compact Array (ATCA) at 1.4 - 3.0 GHz. In order to study the physical structures in the region where the SS433 jet and W50 interact, we obtain an in
Externí odkaz:
http://arxiv.org/abs/1802.05829
Autor:
Vernstrom, Tessa, Gaensler, Bryan, Vacca, Valentina, Farnes, Jamie, Haverkorn, Marijke, O'Sullivan, Shane
We present the largest ever sample of radio polarization properties for $z>4$ sources, with 14 sources having significant polarization detections. Using wideband data from the Karl G. Jansky Very Large Array, we obtained the rest-frame total intensit
Externí odkaz:
http://arxiv.org/abs/1712.01909
Autor:
Lamee, Mehdi, Rudnick, Lawrence, Farnes, Jamie S., Carretti, Ettore, Gaensler, B. M., Haverkorn, Marijke, Poppi, Sergio
We present a polarization catalog of 533 extragalactic radio sources with 2.3 GHz total intensity above 420 mJy from the S-band Polarization All Sky Survey, S-PASS, with corresponding 1.4 GHz polarization information from the NRAO VLA Sky Survey, NVS
Externí odkaz:
http://arxiv.org/abs/1607.04914
Autor:
Farnes, Jamie Stephen
Magnetic fields play a fundamental role in the evolution of astrophysical systems. These fields can be studied through wide-field spectropolarimetry, which allows for faint polarised signals to be detected at relatively low radio frequencies. An inte
Externí odkaz:
http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.610653
Autor:
Gaensler, B. M., Agudo, Iván, Akahori, Takuya, Banfield, Julie, Beck, Rainer, Carretti, Ettore, Farnes, Jamie, Haverkorn, Marijke, Heald, George, Jones, David, Landecker, Thomas, Mao, Sui Ann, Norris, Ray, O'Sullivan, Shane, Rudnick, Lawrence, Schnitzeler, Dominic, Seymour, Nicholas, Sun, Xiaohui
Faraday rotation of polarised background sources is a unique probe of astrophysical magnetic fields in a diverse range of foreground objects. However, to understand the properties of the polarised sources themselves and of depolarising phenomena alon
Externí odkaz:
http://arxiv.org/abs/1501.00626
Autor:
Mao, Sui Ann, Banfield, Julie, Gaensler, Bryan, Rudnick, Lawrence, Stil, Jeroen, Purcell, Cormac, Beck, Rainer, Farnes, Jamie, O'Sullivan, Shane, Schnitzeler, Dominic, Willis, Tony, Sun, Xiaohui, Carretti, Ettore, Dolag, Klaus, Sokoloff, Dmitry, Kothes, Roland, Wolleben, Maik, Heald, George, Geisbuesch, Joern, Robishaw, Tim, Afonso, Jose, Magalhães, Antonio Mario, Lundgren, Britt, Haverkorn, Marijke, Oppermann, Niels, Taylor, Russ
A VLA Sky Survey of the extragalactic sky at S band (2-4 GHz) with polarization information can uniquely probe the magneto-ionic medium in a wide range of astrophysical environments over cosmic time. For a shallow all-sky survey, we expect to detect
Externí odkaz:
http://arxiv.org/abs/1401.1875
Autor:
Farnes, Jamie S.
Magnetic fields play a fundamental role in the evolution of astrophysical systems. These fields can be studied through wide-field spectropolarimetry, which allows for faint polarised signals to be detected at relatively low radio frequencies. An inte
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3a49a94f52bdaa4658269fc895ff98fe
Autor:
Sakemi, Haruka, Machida, Mami, Ohmura, Takumi, Ideguchi, Shinsuke, Miyashita, Yoshimitsu, Takahashi, Keitaro, Akahori, Takuya, Akamatsu, Hiroki, Nakanishi, Hiroyuki, Kurahara, Kohei, Farnes, Jamie
Publikováno v:
Galaxies (2075-4434); Dec2018, Vol. 6 Issue 4, p137, 1p
