BibTex format
@inproceedings{McBride:2025:10.22323/1.501.1120,
author = {McBride, K and Abarr, Q and Allison, P and Alvarez-Muñiz, J and Yebra, JA and Anderson, T and Basharina-Freshville, A and Beatty, JJ and Beaufore, L and Besson, DZ and Bose, R and Braun, D and Chamanbahar, B and Chen, P and Chen, Y and Clem, JM and Coakley, T and Connolly, A and Cremonesi, L and Cummings, A and Dasgupta, P and Deaconu, C and Flaherty, J and Gorham, PW and Hornhuber, C and Hoffman, J and Hughes, K and Hynous, A and Jung, A and Kofman, A and Ku, Y and Kuo, CY and Linton, P and Lisalda, L and Liu, TC and Luszczak, W and Mackey, SC and Martin, Z and McBride, K and Miki, C and Nam, J and Nichol, RJ and Novikov, A and Nozdrina, A and Oberla, E and Prohira, S and Pumphrey, H and Radomski, D and Rauch, BF and Scrandis, R and Seckel, D and Seikh, MFH and Shiao, J and Simburger, G and Vieregg, AG and Wang, SH and Welling, C and Wissel, SA and Xie, C and Yao, J and Young, R and Zas, E and Zeolla, A},
doi = {10.22323/1.501.1120},
title = {Design of the Payload for Ultrahigh Energy Observations},
url = {http://dx.doi.org/10.22323/1.501.1120},
year = {2025}
}
RIS format (EndNote, RefMan)
TY - CPAPER
AB - Ultrahigh-energy cosmic rays (UHECR) should produce ultrahigh-energy neutrinos (UHEN) as byproducts of their propagation. Many candidate UHECR source models also predict an emission of UHEN local to their acceleration sites. The Payload for Ultrahigh Energy Observations (PUEO) is a balloon-borne observatory that will scan the Antarctic ice for these UHEN through their Askaryan emission and is the successor to the ANtarctic Impulsive Transient Antenna (ANITA). The payload design is optimized to detect these Askaryan signals with wide bandwidth measurements of dual-polarized antennas. The challenge in reaching high neutrino sensitivity includes outfitting many low-noise channels with linear polarization measurements and efficient filtering of backgrounds with size, power, and weight constraints to fit on a balloon-borne instrument. This poster will present the antennas, filtering, and data acquisition system in the context of meeting the science requirements of the PUEO mission.
AU - McBride,K
AU - Abarr,Q
AU - Allison,P
AU - Alvarez-Muñiz,J
AU - Yebra,JA
AU - Anderson,T
AU - Basharina-Freshville,A
AU - Beatty,JJ
AU - Beaufore,L
AU - Besson,DZ
AU - Bose,R
AU - Braun,D
AU - Chamanbahar,B
AU - Chen,P
AU - Chen,Y
AU - Clem,JM
AU - Coakley,T
AU - Connolly,A
AU - Cremonesi,L
AU - Cummings,A
AU - Dasgupta,P
AU - Deaconu,C
AU - Flaherty,J
AU - Gorham,PW
AU - Hornhuber,C
AU - Hoffman,J
AU - Hughes,K
AU - Hynous,A
AU - Jung,A
AU - Kofman,A
AU - Ku,Y
AU - Kuo,CY
AU - Linton,P
AU - Lisalda,L
AU - Liu,TC
AU - Luszczak,W
AU - Mackey,SC
AU - Martin,Z
AU - McBride,K
AU - Miki,C
AU - Nam,J
AU - Nichol,RJ
AU - Novikov,A
AU - Nozdrina,A
AU - Oberla,E
AU - Prohira,S
AU - Pumphrey,H
AU - Radomski,D
AU - Rauch,BF
AU - Scrandis,R
AU - Seckel,D
AU - Seikh,MFH
AU - Shiao,J
AU - Simburger,G
AU - Vieregg,AG
AU - Wang,SH
AU - Welling,C
AU - Wissel,SA
AU - Xie,C
AU - Yao,J
AU - Young,R
AU - Zas,E
AU - Zeolla,A
DO - 10.22323/1.501.1120
PY - 2025///
TI - Design of the Payload for Ultrahigh Energy Observations
UR - http://dx.doi.org/10.22323/1.501.1120
ER -