Paul, K., Maurya, A., Henry, Q., Sharma, K., Satheesh, P., Divyajyoti, . . . Mishra, C. K. (2024). ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes.
Citazione stile Chigago Style (17a edizione)Paul, Kaushik, Akash Maurya, Quentin Henry, Kartikey Sharma, Pranav Satheesh, Divyajyoti, Prayush Kumar, e Chandra Kant Mishra. ESIGMAHM: An Eccentric, Spinning Inspiral-merger-ringdown Waveform Model with Higher Modes for the Detection and Characterization of Binary Black Holes. 2024.
Citatione MLA (9a ed.)Paul, Kaushik, et al. ESIGMAHM: An Eccentric, Spinning Inspiral-merger-ringdown Waveform Model with Higher Modes for the Detection and Characterization of Binary Black Holes. 2024.