Recovery of the X-ray polarisation of Swift J1727.8-1613 after the soft-to-hard spectral transition (Corrigendum) (Astronomy and Astrophysics (2024) 686 (L12) DOI: 10.1051/0004-6361/202450566)

Authors

J. Podgorný, Academy of Sciences of the Czech Republic
J. Svoboda, Academy of Sciences of the Czech Republic
M. Dovčiak, Academy of Sciences of the Czech Republic
A. Veledina, Turun yliopisto
J. Poutanen, Turun yliopisto
P. Kaaret, NASA Marshall Space Flight Center
S. Bianchi, Università degli Studi Roma Tre
A. Ingram, Newcastle University
F. Capitanio, Istituto Nazionale Di Astrofisica, Rome
S. R. Datta, Academy of Sciences of the Czech Republic
E. Egron, Osservatorio Astronomico di Cagliari
H. Krawczynski, McDonnell Center for the Space Sciences
G. Matt, Università degli Studi Roma Tre
F. Muleri, Istituto Nazionale Di Astrofisica, Rome
P. O. Petrucci, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG)
T. D. Russell, INAF Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo
J. F. Steiner, Harvard-Smithsonian Center for Astrophysics
N. Bollemeijer, Anton Pannekoek Instituut voor Sterrenkunde
M. Brigitte, Academy of Sciences of the Czech Republic
N. Castro Segura, Faculty of Science, Engineering and Medicine
R. Emami, Harvard-Smithsonian Center for Astrophysics
J. A. García, NASA Goddard Space Flight Center
K. Hu, McDonnell Center for the Space Sciences
M. N. Iacolina, Agenzia Spaziale Italiana
V. Kravtsov, Turun yliopisto
L. Marra, Università degli Studi Roma Tre
G. Mastroserio, Università degli Studi di Milano
T. Muñoz-Darias, Instituto Astrofisico de Canarias
E. Nathan, California Institute of Technology
M. Negro, Louisiana State University
A. Ratheesh, Istituto Nazionale Di Astrofisica, Rome
N. Rodriguez Cavero, McDonnell Center for the Space Sciences
R. Taverna, Università degli Studi di Padova

Document Type

Article

Publication Date

9-1-2025

Abstract

(Figure presented) In Fig. 4, the X-ray hardness value for observation 8 was plotted using a count-based ratio instead of the energy-flux-based ratio used for other points in the figure. The correction of the position of this point in Fig. 4 does not affect any other figures, results, or conclusions in the paper.

Publication Source (Journal or Book title)

Astronomy and Astrophysics

Recommended Citation

Podgorný, J., Svoboda, J., Dovčiak, M., Veledina, A., Poutanen, J., Kaaret, P., Bianchi, S., Ingram, A., Capitanio, F., Datta, S., Egron, E., Krawczynski, H., Matt, G., Muleri, F., Petrucci, P., Russell, T., Steiner, J., Bollemeijer, N., Brigitte, M., Castro Segura, N., Emami, R., García, J., Hu, K., Iacolina, M., Kravtsov, V., Marra, L., Mastroserio, G., Muñoz-Darias, T., Nathan, E., Negro, M., Ratheesh, A., Rodriguez Cavero, N., & Taverna, R. (2025). Recovery of the X-ray polarisation of Swift J1727.8-1613 after the soft-to-hard spectral transition (Corrigendum) (Astronomy and Astrophysics (2024) 686 (L12) DOI: 10.1051/0004-6361/202450566). Astronomy and Astrophysics, 701 https://doi.org/10.1051/0004-6361/202557075e