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)

J. Podgorný; J. Svoboda; M. Dovčiak; A. Veledina; J. Poutanen; P. Kaaret; S. Bianchi; A. Ingram; F. Capitanio; S. R. Datta; E. Egron; H. Krawczynski; G. Matt; F. Muleri; P. O. Petrucci; T. D. Russell; J. F. Steiner; N. Bollemeijer; M. Brigitte; N. Castro Segura; R. Emami; J. A. García; K. Hu; M. N. Iacolina; V. Kravtsov; L. Marra; G. Mastroserio; T. Muñoz-Darias; E. Nathan; M. Negro; A. Ratheesh; N. Rodriguez Cavero; R. Taverna; F. Tombesi; Y. J. Yang; W. Zhang; Y. Zhang

doi:10.1051/0004-6361/202557075e

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)

J. Podgorný
, J. Svoboda
, M. Dovčiak
, A. Veledina
, J. Poutanen
, P. Kaaret
, S. Bianchi
, A. Ingram
, F. Capitanio
, S. R. Datta
, E. Egron
, H. Krawczynski
, G. Matt
, F. Muleri
, P. O. Petrucci
, T. D. Russell
, J. F. Steiner
, N. Bollemeijer
, M. Brigitte
, N. Castro Segura

R. Emami, J. A. García, K. Hu, M. N. Iacolina, V. Kravtsov, L. Marra, G. Mastroserio, T. Muñoz-Darias, E. Nathan, M. Negro, A. Ratheesh, N. Rodriguez Cavero, R. Taverna, F. Tombesi, Y. J. Yang, W. Zhang, Y. Zhang

Research output: Contribution to journal › Comment/debate

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.

Original language	English
Article number	C2
Journal	Astronomy and Astrophysics
Volume	701
DOIs	https://doi.org/10.1051/0004-6361/202557075e
State	Published - Sep 1 2025

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Podgorný, J., Svoboda, J., Dovčiak, M., Veledina, A., Poutanen, J., Kaaret, P., Bianchi, S., Ingram, A., Capitanio, F., Datta, S. R., Egron, E., Krawczynski, H., Matt, G., Muleri, F., Petrucci, P. O., Russell, T. D., Steiner, J. F., Bollemeijer, N., Brigitte, M., ... Zhang, Y. (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, Article C2. https://doi.org/10.1051/0004-6361/202557075e

@article{802a321d4fbc48bdb54bb824f1da7185,

title = "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)",

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.",

author = "J. Podgorn{\'y} and J. Svoboda and M. Dov{\v c}iak and A. Veledina and J. Poutanen and P. Kaaret and S. Bianchi and A. Ingram and F. Capitanio and Datta, \{S. R.\} and E. Egron and H. Krawczynski and G. Matt and F. Muleri and Petrucci, \{P. O.\} and Russell, \{T. D.\} and Steiner, \{J. F.\} and N. Bollemeijer and M. Brigitte and \{Castro Segura\}, N. and R. Emami and Garc{\'i}a, \{J. A.\} and K. Hu and Iacolina, \{M. N.\} and V. Kravtsov and L. Marra and G. Mastroserio and T. Mu{\~n}oz-Darias and E. Nathan and M. Negro and A. Ratheesh and \{Rodriguez Cavero\}, N. and R. Taverna and F. Tombesi and Yang, \{Y. J.\} and W. Zhang and Y. Zhang",

note = "Publisher Copyright: {\textcopyright} The Authors 2025.",

year = "2025",

month = sep,

day = "1",

doi = "10.1051/0004-6361/202557075e",

language = "English",

volume = "701",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

}

Podgorný, J, Svoboda, J, Dovčiak, M, Veledina, A, Poutanen, J, Kaaret, P, Bianchi, S, Ingram, A, Capitanio, F, Datta, SR, Egron, E, Krawczynski, H, Matt, G, Muleri, F, Petrucci, PO, Russell, TD, Steiner, JF, Bollemeijer, N, Brigitte, M, Castro Segura, N, Emami, R, García, JA, Hu, K, Iacolina, MN, Kravtsov, V, Marra, L, Mastroserio, G, Muñoz-Darias, T, Nathan, E, Negro, M, Ratheesh, A, Rodriguez Cavero, N, Taverna, R, Tombesi, F, Yang, YJ, Zhang, W & Zhang, Y 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, vol. 701, C2. https://doi.org/10.1051/0004-6361/202557075e

TY - JOUR

T1 - 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)

AU - Podgorný, J.

AU - Svoboda, J.

AU - Dovčiak, M.

AU - Veledina, A.

AU - Poutanen, J.

AU - Kaaret, P.

AU - Bianchi, S.

AU - Ingram, A.

AU - Capitanio, F.

AU - Datta, S. R.

AU - Egron, E.

AU - Krawczynski, H.

AU - Matt, G.

AU - Muleri, F.

AU - Petrucci, P. O.

AU - Russell, T. D.

AU - Steiner, J. F.

AU - Bollemeijer, N.

AU - Brigitte, M.

AU - Castro Segura, N.

AU - Emami, R.

AU - García, J. A.

AU - Hu, K.

AU - Iacolina, M. N.

AU - Kravtsov, V.

AU - Marra, L.

AU - Mastroserio, G.

AU - Muñoz-Darias, T.

AU - Nathan, E.

AU - Negro, M.

AU - Ratheesh, A.

AU - Rodriguez Cavero, N.

AU - Taverna, R.

AU - Tombesi, F.

AU - Yang, Y. J.

AU - Zhang, W.

AU - Zhang, Y.

PY - 2025/9/1

Y1 - 2025/9/1

N2 - (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.

AB - (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.

UR - https://www.scopus.com/pages/publications/105017874568

U2 - 10.1051/0004-6361/202557075e

DO - 10.1051/0004-6361/202557075e

M3 - Comment/debate

AN - SCOPUS:105017874568

SN - 0004-6361

VL - 701

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - C2

ER -

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)

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