Skip to content
DraconiticResearch
Search Sources API
203,203 studies31 sourcesUpdated 14 min ago
PreprintCC BY 4.0arXiv

Progress in quantum telescopes

Abstract

Classically, the angular resolution of a telescope is limited by its diffraction limit: the ratio of its observing wavelength to its diameter. Developments in quantum information theory over the past decade have uncovered quantum-optimal measurement methods that enable super-resolution imaging beyond the diffraction limit, and many laboratory-scale demonstrations of these methods have been performed over the past decade, culminating in the recent first on-sky demonstration of quantum-enhanced astronomical imaging. In this Review, we detail the current progress and achievements of these theoretical and experimental results, discuss the astronomical science cases motivating the development of higher resolution telescopes, summarise the technological challenges facing the practical application of quantum imaging technologies to astronomy, and present a vision for the realization of \emph{quantum telescopes} with imaging resolutions orders of magnitude better than current observatories.

Related

  1. Early Optical Follow-up of Gamma-Ray Bursts: The Critical Role of Robotic Telescopes
    Rahul Gupta, Judith Racusin, Gor Oganesyan +26
    HALPreprintLicence not statedGeneral astronomyGeneral physicsHAL
  2. A New Probe of Strongly-Interacting Dark Sector using Neutrino Telescopes
    Jose A. Macias Cruz, Christopher V. Cappiello, P. S. Bhupal Dev +1
    arXivPreprintCC BY 4.0Full textHigh-energy astrophysicsHigh-energy & particle physicsarXiv
  3. CURTAIN: Towards a Foundation Model for Neutrino Telescopes
    Severin Magel, Felix J. Yu, Carlos A. Argüelles
    arXivPreprintarXiv licenceFull textInstrumentation & methodsHigh-energy & particle physicsarXiv
  4. A Differentiable Neural Surrogate for Photon Propagation in Neutrino Telescopes
    Felix J. Yu, Berthy T. Feng, Nicholas Kamp +1
    arXivPreprintCC BY 4.0Full textHigh-energy astrophysicsHigh-energy & particle physicsarXiv
  5. The Effect of Large Apertures on Atmospheric Noise Spectra for Millimeter-wave Telescopes
    Thomas W. Morris, Neelima Sehgal
    arXivPreprintCC BY 4.0Full textCosmologyInstrumentation & methodsarXiv
BibTeX
@misc{gozzard2026progress,
  title = {{Progress in quantum telescopes}},
  author = {David R. Gozzard and Fiona H. Panther and Andrew G. White},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2609.18079},
  eprint = {2609.18079},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.18079},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Progress in quantum telescopes
AU  - David R. Gozzard
AU  - Fiona H. Panther
AU  - Andrew G. White
PY  - 2026
DA  - 2026/09/16
PB  - arXiv
DO  - 10.48550/arxiv.2609.18079
UR  - https://arxiv.org/abs/2609.18079
AB  - Classically, the angular resolution of a telescope is limited by its diffraction limit: the ratio of its observing wavelength to its diameter. Developments in quantum information theory over the past decade have uncovered quantum-optimal measurement methods that enable super-resolution imaging beyond the diffraction limit, and many laboratory-scale demonstrations of these methods have been performed over the past decade, culminating in the recent first on-sky demonstration of quantum-enhanced astronomical imaging. In this Review, we detail the current progress and achievements of these theoretical and experimental results, discuss the astronomical science cases motivating the development of higher resolution telescopes, summarise the technological challenges facing the practical application of quantum imaging technologies to astronomy, and present a vision for the realization of \emph{quantum telescopes} with imaging resolutions orders of magnitude better than current observatories.
ER  -