New aperture photometry technique for fast moving fly-by NEOs: detection of the 2.58s rotation period of 2024 BX1.
Maxime Devogèle, Peter Jenniskens(Ames Research Center), Z. Benkhaldoun(Center for Astrophysics Harvard & Smithsonian), Dóra Föhring(North Atlantic Treaty Organization), M. Micheli, Juan Luis Cano(Planetary Science Institute), Charlie Drury, Luca Buzi, Marin Ferrais(University of Central Florida), Francisco Ocaña, Emmanuël Jehin(European Southern Observatory)
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