Latest view of CTA 1 with VERITAS

dc.contributor.authorChromey, Alisha
dc.contributor.authorValverde, Janeth
dc.contributor.authorVERITAS Collaboration
dc.contributor.authoret al
dc.date.accessioned2025-11-21T00:30:04Z
dc.date.issued2025-10-06
dc.description39th International Cosmic Ray Conference (ICRC2025),July 15-24,2025,Geneva, Switzerland
dc.descriptionAuthors: VERITAS Collaboration, A. Archer , P. Bangale , J. T. Bartkoske , W. Benbow , Y. Chen , J. L. Christiansen , A. J. Chromey , A. Duerr , M. Errando , M. Escobar Godoy , J. Escudero Pedrosa , Q. Feng , S. Filbert , L. Fortson , A. Furniss , W. Hanlon , O. Hervet , C. E. Hinrichs, , J. Holder, T. B. Humensky, M. Iskakova , W. Jin , M. N. Johnson , E. Joshi, M. Kertzman , M. Kherlakian, D. Kieda , T. K. Kleiner, N. Korzoun, S. Kumar, M. J. Lang, M. Lundy, G. Maier, C. E McGrath, P. Moriarty, R. Mukherjee , W. Ning , R. A. Ong , A. Pandey , M. Pohl, E. Pueschel, J. Quinn, P. L. Rabinowitz , K. Ragan, P. T. Reynolds, D. Ribeiro , E. Roache , I. Sadeh, L. Saha , H. Salzmann , M. Santander, G. H. Sembroski, B. Shen, M. Splettstoesser , A. K. Talluri , S. Tandon, J. V. Tucci, J. Valverde, V. V. Vassiliev , D. A. Williams , S. L. Wong, T. Yoshikoshi
dc.description.abstractCTA 1 is a shell-type supernova remnant (SNR) with a central pulsar wind nebula (PWN), visible at very-high-energy (VHE) from 50 GeV to 100 TeV from a moderately extended emission region. While general consensus concludes the VHE emission originates from relativistic leptons accelerated by the PWN and undergoing inverse Compton scattering, questions remain about electron escape and propagation, as well as the evolutionary stage of this particular PWN. CTA 1 is on the cusp of middle age (~13 kyr) and spatially resolvable at energies visible to imaging atmospheric Cherenkov telescopes (IACTs), such as the Very Energetic Radiation Imaging Telescope Array System (VERITAS) (PSF < 0.1 deg). Therefore, this remnant is an excellent candidate to study lepton propagation and escape between different PWN evolutionary stages. Since the initial VERITAS publication on CTA 1 in 2013, VERITAS has performed new observations, adding to a total exposure of about 120 hours. We have analyzed the entire VERITAS CTA 1 dataset to date and report results.
dc.description.sponsorshipThis research is supported by grants from the U.S. Department of Energy Office of Science, the U.S. National Science Foundation and the Smithsonian Institution, by NSERC in Canada, and by the Helmholtz Association in Germany. This research used resources provided by the Open Science Grid, which is supported by the National Science Foundation and the U.S. Department of Energy’s Office of Science, and resources of the National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility operated under Contract No. DE-AC02-05CH11231. We acknowledge the excellent work of the technical support staff at the Fred Lawrence Whipple Observatory and at the collaborating institutions in the construction and operation of the instrument.
dc.description.urihttp://arxiv.org/abs/2510.04414
dc.format.extent6 pages
dc.genreconference papers and proceedings
dc.genrepreprints
dc.identifierdoi:10.13016/m2awug-5iuo
dc.identifier.urihttps://doi.org/10.48550/arXiv.2510.04414
dc.identifier.urihttp://hdl.handle.net/11603/40832
dc.language.isoen
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology (CSST) / Center for Research and Exploration in Space Sciences & Technology II (CRSST II)
dc.relation.ispartofUMBC Faculty Collection
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/deed.en
dc.subjectAstrophysics - High Energy Astrophysical Phenomena
dc.titleLatest view of CTA 1 with VERITAS
dc.typeText

Files

Original bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
251004414v1.pdf
Size:
1.12 MB
Format:
Adobe Portable Document Format