Short timescale evolution of the polarized radio jet during V404 Cygni's 2015 outburst

Accepted/In Press date: 5 January 2023

Published date: 2 March 2023

Additional Information: Funding Information: The authors extend their sincere thanks to all of the NRAO staff involved in the scheduling and execution of these observations. The authors offer a special thanks to Frank Schnitzel for sharing his expertise of polarization observation, and calibration, and data reduction with the VLA and CASA. The authors thank Cameron Van Eck for helpful discussions regarding Galactic magnetic field models and the Canadian Initiative for Radio Astronomy Data Analysis (CIRADA) RM synthesis routine. Finally, the authors thank the referee for their insightful and helpful comments. This research has made use of software provided by CIRADA. CIRADA is funded by a grant from the Canada Foundation for Innovation 2017 Innovation Fund (Project 35999), as well as by the Provinces of Ontario, British Columbia, Alberta, Manitoba, and Quebec, in collaboration with the National Research Council of Canada, the US National Radio Astronomy Observatory and Australia’s Commonwealth Scientific and Industrial Research Organisation. AKH and GRS are supported by NSERC Discovery Grants RGPIN-2016-06569 and RGPIN-2021-0400. Support for this work of AJT was provided by NASA through the NASA Hubble Fellowship grant #HST–HF2–51494.001 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5–26555. TDR acknowledges financial contribution from the agreement ASI-INAF n.2017-14-H.0. GEA is the recipient of an Australian Research Council Discovery Early Career Researcher Award (project number DE180100346). SM is thankful for support from an NWO (Dutch Research Council) VICI award, grant Nr. 639.043.513. TMB acknowledges the financial contribution from grant PRIN-INAF 2019 N.15. RS acknowledges support from grant number 12073029 from the National Natural Science Foundation of China (NSFC). AKH and GRS respectfully acknowledge that they perform the majority of their research from Treaty 6 territory, a traditional gathering place for diverse Indigenous peoples including the Cree, Blackfoot, Métis, Nakota Sioux, Iroquois, Dene, Ojibway/ Saulteaux/Anishinaabe, Inuit, and many others whose histories, languages, and cultures continue to influence our vibrant community. The authors also wish to recognize and acknowledge the significant cultural role and reverence that the summit of Maunakea has always had within the indigenous Hawaiian community. The authors are most fortunate to have the opportunity to conduct VLBA observations from this mountain. Funding Information: AKH and GRS are supported by NSERC Discovery Grants RGPIN-2016-06569 and RGPIN-2021-0400. Support for this work of AJT was provided by NASA through the NASA Hubble Fellowship grant #HST–HF2–51494.001 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5–26555. TDR acknowledges financial contribution from the agreement ASI-INAF n.2017-14-H.0. GEA is the recipient of an Australian Research Council Discovery Early Career Researcher Award (project number DE180100346). SM is thankful for support from an NWO (Dutch Research Council) VICI award, grant Nr. 639.043.513. TMB acknowledges the financial contribution from grant PRIN-INAF 2019 N.15. RS acknowledges support from grant number 12073029 from the National Natural Science Foundation of China (NSFC). Funding Information: This research has made use of software provided by CIRADA. CIRADA is funded by a grant from the Canada Foundation for Innovation 2017 Innovation Fund (Project 35999), as well as by the Provinces of Ontario, British Columbia, Alberta, Manitoba, and Quebec, in collaboration with the National Research Council of Canada, the US National Radio Astronomy Observatory and Australia’s Commonwealth Scientific and Industrial Research Organisation. Publisher Copyright: © 2023 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.

Keywords: astro-ph.GA, astro-ph.HE, astro-ph.SR, ISM: jets and outflows, radio continuum: stars, black hole physics, X-rays: binaries, polarization, stars: individual: V404 Cygni, GS 2023 + 338

Local EPrints ID: 477787

URI: http://eprints.soton.ac.uk/id/eprint/477787

DOI: doi:10.1093/mnras/stad396

ISSN: 1365-2966

PURE UUID: d2b1bf14-aa44-4262-8bd9-f6ae2323e685

ORCID for Diego Altamirano: orcid.org/0000-0002-3422-0074

Date deposited: 14 Jun 2023 16:46

Last modified: 12 Nov 2024 02:49