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Autor:
Simha, Sunil, Lee, Khee-Gan, Prochaska, J. Xavier, Khrykin, Ilya S., Huang, Yuxin, Tejos, Nicolas, Marnoch, Lachlan, Ata, Metin, Bernales, Lucas, Bhandari, Shivani, Cooke, Jeff, Deller, Adam T., Ryder, Suart, Zhang, Jielai
The FLIMFLAM survey is collecting spectroscopic data of field galaxies near fast radio burst (FRB) sightlines to constrain key parameters describing the distribution of matter in the Universe. In this work, we leverage the survey data to determine th
Externí odkaz:
http://arxiv.org/abs/2303.07387
