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The Cassiopeia A Supernova remnant and its Central Compact Object in X-rays

The Cassiopeia A Supernova remnant and its Central Compact Object as seen by the Chandra X-ray telescope

Credit: NASA/CXC/SAO

Dr. Bettina Posselt

Research Scientist / Affiliate Associate Research Professor (PSU)

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • MeerKAT
  • Pulsars, transients and relativistic astrophysics
  • The Square Kilometre Array (SKA)
bettina.posselt@physics.ox.ac.uk
  • About
  • Publications

The MeerKAT telescope as a pulsar facility: System verification and early science results from MeerTime

Publications of the Astronomical Society of Australia Cambridge University Press 37 (2020) e028

Authors:

M Bailes, A Jameson, F Abbate, Ed Barr, Ndr Bhat, L Bondonneau, M Burgay, Sj Buchner, F Camilo, Dj Champion, I Cognard, Pb Demorest, Pcc Freire, T Gautam, M Geyer, Jm Griessmeier, L Guillemot, H Hu, F Jankowski, S Johnston, A Karastergiou, R Karuppusamy, D Kaur, Mj Keith, M Kramer, J Van Leeuwen, Me Lower, Y Maan, Ma McLaughlin, Bw Meyers, S Osłowski, Ls Oswald, A Parthasarathy, T Pennucci, B Posselt, A Possenti, Sm Ransom, Dj Reardon, A Ridolfi, Ctg Schollar, M Serylak, G Shaifullah, M Shamohammadi, Rm Shannon, C Sobey, X Song, R Spiewak, Ih Stairs, Bw Stappers, W Van Straten

Abstract:

We describe system verification tests and early science results from the pulsar processor (PTUSE) developed for the newly commissioned 64-dish SARAO MeerKAT radio telescope in South Africa. MeerKAT is a high-gain low-system temperature radio array that currently operates at 580-1 670 MHz and can produce tied-array beams suitable for pulsar observations. This paper presents results from the MeerTime Large Survey Project and commissioning tests with PTUSE. Highlights include observations of the double pulsar, pulse profiles from 34 millisecond pulsars (MSPs) from a single 2.5-h observation of the Globular cluster Terzan 5, the rotation measure of Ter5O, a 420-sigma giant pulse from the Large Magellanic Cloud pulsar PSR , and nulling identified in the slow pulsar PSR J0633-2015. One of the key design specifications for MeerKAT was absolute timing errors of less than 5 ns using their novel precise time system. Our timing of two bright MSPs confirm that MeerKAT delivers exceptional timing. PSR exhibits a jitter limit of whilst timing of PSR over almost 11 months yields an rms residual of 66 ns with only 4 min integrations. Our results confirm that the MeerKAT is an exceptional pulsar telescope. The array can be split into four separate sub-arrays to time over 1 000 pulsars per day and the future deployment of S-band (1 750-3 500 MHz) receivers will further enhance its capabilities.
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Details from ORA

Possible Phase-dependent Absorption Feature in the X-Ray Spectrum of the Middle-aged PSR J0659+1414

The Astrophysical Journal American Astronomical Society 869:2 (2018) 97

Authors:

Prakash Arumugasamy, Oleg Kargaltsev, Bettina Posselt, George G Pavlov, Jeremy Hare
More details from the publisher

The Variable Pulsar Wind Nebula of PSR J1809–1917

The Astrophysical Journal American Astronomical Society 868:2 (2018) 119

Authors:

Noel Klingler, Oleg Kargaltsev, George G Pavlov, Bettina Posselt
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Discovery of Extended Infrared Emission around the Neutron Star RXJ0806.4–4123* * Based on observations made with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with program GO-14745. † † Based on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), Ministerio de Ciencia, Tecnología e Innovación Productiva (Argentina), and Ministério da Ciência, Tecnologia e Inovação (Brazil).

The Astrophysical Journal American Astronomical Society 865:1 (2018) 1

Authors:

B Posselt, GG Pavlov, Ü Ertan, S Çalışkan, KL Luhman, CC Williams
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Discovery of extended infrared emission around the neutron star RX J0806.4-4123

(2018)

Authors:

B Posselt, GG Pavlov, Ü Ertan, S Çalışkan, KL Luhman, CC Williams
More details from the publisher
Details from ArXiV

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