Skip to content
DraconiticResearch
Search Sources API
201,642 studies31 sourcesUpdated 14 min ago
PreprintCC0arXiv

ALMA - CTAO synergies

  • Paola Andreani
  • Maria Diaz-Trigo
Open at sourcePDFDOICite

Abstract

This article aims to raise awareness within the ESO astronomical community of the scientific opportunities offered by the upcoming Cherenkov Telescope Array, CTAO, highlighting cases where combining millimetre/submillimetre capabilities of the Atacama Large Millimeter / submillimeter Array, ALMA with the CTAO's very high energy, TeV, observations enables new avenues for discovery. Many astrophysical sources and environments exhibit emission processes detectable in both regimes; however, the synergies extend beyond shared emission mechanisms and include broader physical processes and observational connections linking millimetre, submillimetre and TeV energies.

Related

  1. Unsupervised domain adaptation for multitask image analysis in realistic context with extreme label shift; Application to the CTAO first large sized telescope
    Michael Dell'Aiera, Thomas Vuillaume, Alexandre Benoit
    Astron.Comput.Peer-reviewedCC BYGeneral astronomyGeneral physicsHAL
  2. Pair echo model of CTAO/LST-1 signal from GRB 221009A
    Andrii Neronov, Ievgen Vovk, Teneman Keita +1
    HALPreprintarXiv licenceFull textCosmologyHigh-energy astrophysicsHALarXiv
  3. Geminga and Monogem in the CTAO Era: Probing TeV Halos and Cosmic-Ray Transport
    Youyou Li, Oscar Macias, Manuela Vecchi +1
    arXivPreprintarXiv licenceFull textHigh-energy astrophysicsarXiv
  4. Square Kilometer Array Synergies for the Epoch of Reionization and Cosmic Dawn
    Anirban Chakraborty, Tirthankar R Choudhury, Kanan K Datta +15
    HALPreprintLicence not statedGeneral astronomyGeneral physicsHAL
  5. Study of blazar variability through their flux distribution for CTAO long-term monitoring
    A. Mikhno, J. Biteau, J. -P. Lenain on behalf of the CTAO collaboration
    arXivPreprintCC BY-NC-SA 4.0Full textHigh-energy astrophysicsarXiv

Cite

BibTeXRIS
BibTeX
@misc{andreani2026alma,
  title = {{ALMA - CTAO synergies}},
  author = {Paola Andreani and Maria Diaz-Trigo},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2609.37797},
  eprint = {2609.37797},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.37797},
  note = {CC0},
}
RIS
TY  - UNPB
TI  - ALMA - CTAO synergies
AU  - Paola Andreani
AU  - Maria Diaz-Trigo
PY  - 2026
DA  - 2026/09/29
PB  - arXiv
DO  - 10.48550/arxiv.2609.37797
UR  - https://arxiv.org/abs/2609.37797
AB  - This article aims to raise awareness within the ESO astronomical community of the scientific opportunities offered by the upcoming Cherenkov Telescope Array, CTAO, highlighting cases where combining millimetre/submillimetre capabilities of the Atacama Large Millimeter / submillimeter Array, ALMA with the CTAO's very high energy, TeV, observations enables new avenues for discovery. Many astrophysical sources and environments exhibit emission processes detectable in both regimes; however, the synergies extend beyond shared emission mechanisms and include broader physical processes and observational connections linking millimetre, submillimetre and TeV energies.
ER  -