TY - JOUR
T1 - Search for Gravitational Waves Emitted from SN2023ixf
AU - LIGO Scientific Collaboration
AU - Virgo Collaboration
AU - The KAGRA Collaboration
AU - Abac, A. G.
AU - Abbott, R.
AU - Abouelfettouh, I.
AU - Acernese, F.
AU - Ackley, K.
AU - Adhicary, S.
AU - Adhikari, N.
AU - Adhikari, R. X.
AU - Adkins, V. K.
AU - Agarwal, D.
AU - Agathos, M.
AU - Aghaei Abchouyeh, M.
AU - Aguiar, O. D.
AU - Aguilar, I.
AU - Aiello, L.
AU - Ain, A.
AU - Akutsu, T.
AU - Albanesi, S.
AU - Alfaidi, R. A.
AU - Al-Jodah, A.
AU - Alléné, C.
AU - Allocca, A.
AU - Al-Shammari, S.
AU - Altin, P. A.
AU - Alvarez-Lopez, S.
AU - Amato, A.
AU - Amez-Droz, L.
AU - Amorosi, A.
AU - Amra, C.
AU - Ananyeva, A.
AU - Anderson, S. B.
AU - Anderson, W. G.
AU - Andia, M.
AU - Ando, M.
AU - Andrade, T.
AU - Andres, N.
AU - Andrés-Carcasona, M.
AU - Andrić, T.
AU - Anglin, J.
AU - Ansoldi, S.
AU - Caudill, S.
AU - Dietrich, T.
AU - Gupta, P.
AU - Hannuksela, O. A.
AU - Kuijer, P.
AU - Miller, A. L.
AU - Pang, P. T.H.
AU - Phukon, K. S.
AU - Puecher, A.
AU - Van Den Broeck, C.
N1 - Publisher Copyright:
© 2025. The Author(s).
PY - 2025/6/1
Y1 - 2025/6/1
N2 - We present the results of a search for gravitational-wave transients associated with core-collapse supernova SN 2023ixf, which was observed in the galaxy Messier 101 via optical emission on 2023 May 19, during the LIGO–Virgo–KAGRA 15th Engineering Run. We define a five-day on-source window during which an accompanying gravitational-wave signal may have occurred. No gravitational waves have been identified in data when at least two gravitational-wave observatories were operating, which covered ∼14% of this five-day window. We report the search detection efficiency for various possible gravitational-wave emission models. Considering the distance to M101 (6.7 Mpc), we derive constraints on the gravitational-wave emission mechanism of core-collapse supernovae across a broad frequency spectrum, ranging from 50 Hz to 2 kHz, where we assume the gravitational-wave emission occurred when coincident data are available in the on-source window. Considering an ellipsoid model for a rotating proto-neutron star, our search is sensitive to gravitational-wave energy 1 × 10−4 M⊙c2 and luminosity 2.6 × 10−4 M⊙c2 s−1 for a source emitting at 82 Hz. These constraints are around an order of magnitude more stringent than those obtained so far with gravitational-wave data. The constraint on the ellipticity of the proto-neutron star that is formed is as low as 1.08, at frequencies above 1200 Hz, surpassing past results.
AB - We present the results of a search for gravitational-wave transients associated with core-collapse supernova SN 2023ixf, which was observed in the galaxy Messier 101 via optical emission on 2023 May 19, during the LIGO–Virgo–KAGRA 15th Engineering Run. We define a five-day on-source window during which an accompanying gravitational-wave signal may have occurred. No gravitational waves have been identified in data when at least two gravitational-wave observatories were operating, which covered ∼14% of this five-day window. We report the search detection efficiency for various possible gravitational-wave emission models. Considering the distance to M101 (6.7 Mpc), we derive constraints on the gravitational-wave emission mechanism of core-collapse supernovae across a broad frequency spectrum, ranging from 50 Hz to 2 kHz, where we assume the gravitational-wave emission occurred when coincident data are available in the on-source window. Considering an ellipsoid model for a rotating proto-neutron star, our search is sensitive to gravitational-wave energy 1 × 10−4 M⊙c2 and luminosity 2.6 × 10−4 M⊙c2 s−1 for a source emitting at 82 Hz. These constraints are around an order of magnitude more stringent than those obtained so far with gravitational-wave data. The constraint on the ellipticity of the proto-neutron star that is formed is as low as 1.08, at frequencies above 1200 Hz, surpassing past results.
UR - http://www.scopus.com/inward/record.url?scp=105006750730&partnerID=8YFLogxK
U2 - 10.3847/1538-4357/adc681
DO - 10.3847/1538-4357/adc681
M3 - Article
AN - SCOPUS:105006750730
SN - 0004-637X
VL - 985
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 183
ER -