Does transparent hidden matter generate optical scintillation?
Open accessAbstract
Stars twinkle because their light goes through the atmosphere. The same phenomenon is expected when the light of extra-galactic stars goes through a Galactic – disk or halo – refractive medium. Because of the large distances involved here, the length and time scales of the optical intensity fluctuations resulting from the wave distortions are accessible to current technology. In this paper, we discuss the different possible scintillation regimes and we focus on the so-called strong diffractive regime that is likely to produce large intensity contrasts. The critical relationship between the source angular size and the intensity contrast in optical wavelengths is also discussed in detail. We propose to monitor small extra-galactic stars every ~10 s to search for intensity scintillation produced by molecular hydrogen clouds. We discuss means to discriminate such hidden matter signals from the foreground effects on light propagation. Appropriate observation of the scintillation process described here should allow one to detect column density stochastic variations in Galactic molecular clouds of the order of ~, that is per ~ transverse distance.
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
The individual sequences would be sensitive to 1% variability on subminute timescales, allowing discovery of planetary eclipses and interstellar scintillation effects.
“The individual sequences would be sensitive to 1% variability on subminute timescales, allowing discovery of planetary eclipses and of interstellar scintillation effects, expected when the light of a background star propagates through a turbulent gas medium ( Moniez 2003; Habibi et al. 2011 ) .”
From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Moniez 2003
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Cites
Born, M., Wolf, E., Bhatia, A. B., Clemmow, P. C., Gabor, D., Stokes, A. R., Taylor, A. M., Wayman, P. A., & Wilcock, W. L. (1999) · Cambridge University Press eBooks · doi:10.1017/9781108769914 · Cited by 26,627 · see citing works
Bennett, C. L., Halpern, M., Hinshaw, G., Jarosik, N., Kogut, A., Limon, M., Meyer, S. S., Page, L., Spergel, D. N., Tucker, G. S., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377253 · Cited by 4,860 · see citing works
Allen's Astrophysical Quantities
Cox, A. N., & Pilachowski, C. A. (2000) · Physics Today · doi:10.1063/1.1325201 · Cited by 2,287 · see citing works
Filippenko, A. V. (1997) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.35.1.309 · Cited by 1,824 · see citing works
The MACHO Project: Microlensing Results from 5.7 Years of Large Magellanic Cloud Observations
Alcock, C. R., Allsman, R. A., Alves, D. R., Axelrod, T. S., Becker, A. C., Bennett, D. P., Cook, K. H., Dalal, N., Drake, A. J., Freeman, K. C., et al. (2000) · The Astrophysical Journal · doi:10.1086/309512 · Cited by 1,008 · see citing works
Primordial nucleosynthesis: theory and observations
Olive, K. A., Steigman, G., & Walker, T. P. (2000) · Physics Reports · doi:10.1016/s0370-1573(00)00031-4 · Cited by 448 · see citing works
Detection of Cosmic Dark Matter
Primack, J. R., Seckel, D., & Sadoulet, B. (1988) · Annual Review of Nuclear and Particle Science · doi:10.1146/annurev.ns.38.120188.003535 · Cited by 439 · see citing works
3D mapping of the dense interstellar gas around the Local Bubble
Lallement, R., Welsh, B. Y., Vergely, J., Crifo, F., & Sfeir, D. M. (2003) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20031214 · Cited by 386 · see citing works
The physics of pulsar scintillation
Narayan, R. (1992) · Philosophical Transactions of the Royal Society of London Series A Physical and Engineering Sciences · doi:10.1098/rsta.1992.0090 · Cited by 261 · see citing works
Limits on Galactic dark matter with 5 years of EROS SMC data
Afonso, C., Albert, J. N., Andersen, J., Ansari, R., Aubourg, É., Bareyre, P., Beaulieu, J., Blanc, G., Charlot, X., Couchot, F., et al. (2003) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20030087 · Cited by 166 · see citing works
Self-citationThe geometry and distance of the Magellanic Clouds from Cepheid variables
Caldwell, J. A. R., & Coulson, I. M. (1986) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/218.2.223 · Cited by 143 · see citing works
Refractive interstellar scintillation in pulsar dynamic spectra
Gupta, Y., Rickett, B. J., & Lyne, A. G. (1994) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/269.4.1035 · Cited by 134 · see citing works
Far Ultraviolet Spectroscopic ExplorerSurvey of the Local Interstellar Medium within 200 Parsecs
Lehner, N., Jenkins, E. B., Gry, C., Moos, H. W., Chayer, P., & Lacour, S. (2003) · The Astrophysical Journal · doi:10.1086/377493 · Cited by 113 · see citing works
Light Curves of Variable Stars
(1996) · Cambridge University Press eBooks · doi:10.1017/cbo9780511564796 · Cited by 75 · see citing works
Radio wave scattering in the interstellar medium
Cordes, J. M., Rickett, B. J., & Backer, D. C. (1988) · OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) · Cited by 66 · see citing works
A Case for a Baryonic Dark Halo
Paolis, F. D., INGROSSO, G., Jetzer, P., & Roncadelli, M. (1995) · Physical Review Letters · doi:10.1103/physrevlett.74.14 · Cited by 62 · see citing works
Evidence for a Source Size of Less than 2000 AU in Quasar 2237+0305
Yonehara, A. (2001) · The Astrophysical Journal · doi:10.1086/319090 · Cited by 59 · see citing works
Lensing of Stars by Spherical Gas Clouds
Draine, B. T. (1998) · The Astrophysical Journal · doi:10.1086/311751 · Cited by 58 · see citing works
A gravitational microlensing determination of continuum source size in Q2237+0305
Wyithe, J. S. B., Webster, R. L., Turner, E. L., & Mortlock, D. J. (2000) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2000.03361.x · Cited by 57 · see citing works
HST observations of the field star population in the Large Magellanic Cloud
Elson, R. A. W., Gilmore, G. F., & Santiago, B. X. (1997) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/289.1.157 · Cited by 50 · see citing works
Comparison of filters for detecting gravitational wave bursts in interferometric detectors
Arnaud, N., Barsuglia, M., Bizouard, M. A., Brisson, V., Cavalier, F., Michel Davier, A., Hello, P., Kreckelbergh, S., Porter, E. K., & Pradier, T. (2003) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.67.062004 · Cited by 34 · see citing works
Ferlet, R. (1999) · The Astronomy and Astrophysics Review · doi:10.1007/s001590050016 · Cited by 33 · see citing works
Halo Dark Clusters of Brown Dwarfs and Molecular Clouds
Paolis, F. D., Ingrosso, G., Jetzer, P., & Roncadelli, M. (1998) · The Astrophysical Journal · doi:10.1086/305692 · Cited by 22 · see citing works
Constraints on Cold H2Clouds from Gravitational Microlensing Searches
Rafikov, R. R., & Draine, B. T. (2001) · The Astrophysical Journal · doi:10.1086/318355 · Cited by 18 · see citing works
Some integrated photometric properties of the Large Magellanic Cloud
Hardy, E. (1978) · Publications of the Astronomical Society of the Pacific · doi:10.1086/130294 · Cited by 8 · see citing works
The Space Stellar Photometry Mission COROT: Asteroseismology and Search for Extrasolar Planets
Baglin, A., Vauclair, G., & the COROT team (2000) · International Astronomical Union Colloquium · doi:10.1017/s0252921100064757 · Cited by 2 · see citing works
Possible use of the dedicated MARLY one meter telescope for intensive supernovae studiesPreprint
Moniez, M., & Perdereau, O. (2001) · arXiv (Cornell University) · doi:10.48550/arxiv.astro-ph/0110448
Self-citation
Flagged first, then by citations
Research works printed but not linked: 5
- Elson, R. A. W., Gilmore, G. F., & Santiago, B. X. 1997 [astro-ph/9705149] · arXiv
- O. R. Frisch (Pergamon Press)
- Lyne, A. G., & Graham-Smith., F. 1998, Pulsar Astronomy (Cambridge University Press)
- Narayan, R. 1992, Phil. Trans. R. Soc. Lond. A, 341, 151
- Sommerfeld, A. 1954, Optics (New York Academic Press Inc.)
Cited by
Sorted by citations
LSST: From Science Drivers to Reference Design and Anticipated Data Products
Ivezić, Ž., Kahn, S. M., Tyson, J. A., Abel, B., Acosta, E., Allsman, R., Alonso, D., AlSayyad, Y., Anderson, S. F., Andrew, J., et al. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab042c · Cited by 4,357 · see citing works
Rubin Observatory LSST Transients and Variable Stars Roadmap
Hambleton, K., Bianco, F. B., Street, R. A., Bell, K. J., Buckley, D. A. H., Graham, M. L., Hernitschek, N., Lund, M. B., Mason, E., Pepper, J. A., et al. (2023) · Publications of the Astronomical Society of the Pacific · doi:10.1088/1538-3873/acdb9a · Cited by 56 · see citing works
Self-citationLooking for MACHOs in the spectra of fast radio bursts
Andrey Katz, A., Kopp, J., Sibiryakov, S. M., & Wei Xue, B. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa1497 · Cited by 38 · see citing works
Imaging dark objects with intensity interferometry
Strekalov, D., Kulikov, I. K., & Yu, N. (2014) · Optics Express · doi:10.1364/oe.22.012339 · Cited by 32 · see citing works
Possible detection of the M 31 rotation in WMAP data
Paolis, F. D., Gurzadyan, V. G., INGROSSO, G., Jetzer, P., Nucita, A., Qadir, A., Vetrugno, D., Кашин, А. Л., Khachatryan, H. G., & Mirzoyan, S. (2011) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201117846 · Cited by 23 · see citing works
Binary microlensing with plasma environment – star and planet
Sun, J., Er, X., & Tsupko, O. Y. (2023) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stad200 · Cited by 12 · see citing works
CMB as a possible new tool to study the dark baryons in galaxies
Paolis, F. D., Ingrosso, G., Nucita, A., Vetrugno, D., Gurzadyan, V. G., Kashin, A. L., Khachatryan, H. G., Mirzoyan, S., Jetzer, P., & Qadir, A. (2012) · Journal of Physics Conference Series · doi:10.1088/1742-6596/354/1/012004 · Cited by 11 · see citing works
Habibi, F., Moniez, M., Ansari, R., & Rahvar, S. (2011) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201015260 · Cited by 13 · see citing works
Self-citationTrimble, V., & Aschwanden, M. J. (2005) · Publications of the Astronomical Society of the Pacific · doi:10.1086/429117 · Cited by 6 · see citing works
Simulation of optical interstellar scintillation
Habibi, F., Moniez, M., Ansari, R., & Rahvar, S. (2013) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201220172 · Cited by 5 · see citing works
Self-citationCMB as a possible new tool to study the dark baryons in galaxies
Paolis, F. D., INGROSSO, G., Nucita, A., Vetrugno, D., Gurzadyan, V. G., Кашин, А. Л., Khachatryan, H. G., Mirzoyan, S., Jetzer, P., & Qadir, A. (2012) · Zurich Open Repository and Archive (University of Zurich) · doi:10.5167/uzh-70229 · Cited by 3 · see citing works
Search for Turbulent Gas Through Interstellar Scintillation
Moniez, M., Ansari, R., Habibi, F., & Rahvar, S. (2013) · Springer proceedings in physics · doi:10.1007/978-94-007-7241-0_6
Self-citationIvezić, Ž. (2016) · Zenodo (CERN European Organization for Nuclear Research) · doi:10.5281/zenodo.44697
Large Synoptic Survey Telescope Town Hall
Willman, B. (2016) · Zenodo (CERN European Organization for Nuclear Research) · doi:10.5281/zenodo.44768
The Lsst Data Processing Software Stack
Jenness, T. (2016) · American Astronomical Society Meeting Abstracts #227 · doi:10.5281/zenodo.44634
Searching for missing baryons through scintillation
Habibi, F. (2011) · HAL · doi:10.70675/c49e43cez784cz4ca6zb87az7660ea2b90c5
- Authors
- Moniez, M.
- Affiliations
- Université Paris-Sud (FR)
- Corresponding author
- Moniez, M.
- ORCID
- Moniez, M.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2003-11-25
- Volume
- 412
- Issue
- 1
- Pages
- 105-120
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W2122779161
- Cited by
- 17
- References
- 27
- Citations by year
- 2023: 2 · 2020: 1 · 2019: 1 · 2016: 3 · 2014: 1 · 2013: 2 · 2012: 2
- FWCI
- 0.17
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Astronomy and Astrophysics (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- Springer Link (Chiba Institute of Technology) (submittedVersion)
- HAL (submittedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Atomic and Molecular Physics, and Optics › Adaptive optics and wavefront sensing
- Keywords
- optical scintillation, stellar scintillation, Galactic halo, Galactic disk, intensity contrast, interstellar medium, wavefront distortion
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
