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SUMMARY:Robust Inference of the Binary Black Hole Spin Population Using Gr
 avitational-Wave Data
DTSTART;VALUE=DATE-TIME:20260715T090000Z
DTEND;VALUE=DATE-TIME:20260715T092000Z
DTSTAMP;VALUE=DATE-TIME:20260718T163621Z
UID:indico-contribution-8970@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Kazuya Kobayashi ()\nThe spin population of binary b
 lack holes (BBHs) provides key insights into their formation channels. Rec
 ent gravitational-wave (GW) observations have suggested the presence of sp
 in subpopulations and correlations between spin and other BBH parameters. 
 However\, the limited measurability of spins in certain regions of the par
 ameter space can bias the inference of the underlying spin population. We 
 propose a new inference method to mitigate this limitation\, demonstrate i
 ts performance using simulations\, and apply it to real GW data to infer t
 he underlying BBH spin population.\n\nhttps://indico.icrr.u-tokyo.ac.jp/ev
 ent/1254/contributions/8970/
LOCATION:Kashiwa Large Seminar Room 601 (Kashiwa)
URL:https://indico.icrr.u-tokyo.ac.jp/event/1254/contributions/8970/
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