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A search for weak distortion of distant galaxy images by large-scale structure

Mould, Jeremy and Blandford, Roger and Villumsen, Jens and Brainerd, Tereasa and Smail, Ian and Small, Todd and Kells, William (1994) A search for weak distortion of distant galaxy images by large-scale structure. Monthly Notices of the Royal Astronomical Society, 271 (1). pp. 31-38. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20190523-125439677

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Abstract

We have completed a feasibility study for the measurement of weak distortion of distant galaxy images by intervening large-scale structure by using the 5-m Hale reflector to acquire a very deep, r ~ 26, exposure of a single field. The error budget of our observations is dominated by the effects of atmospheric seeing (which strongly degrades this signal because the faintest images are under-resolved) and telescope effects. After performing a correction for telescope aberrations and possible guiding errors, the observed mean ‘polarization’ of the images of 4363 galaxies with magnitudes 23 ≤ r ≤ 26 within a circle of radius 4.8 arcmin was found to be p̄ =0.01 ± 0.01⁠. The associated two-point polarization correlation function has a constant value of C_(pp) = (1.4 ± 3.0) x 10^(−5) over the angular range 1 to 6 arcmin. It is predicted that the cosmological polarization should be in the range p = 0.03 ± 0.01 for a standard CDM universe normalized by a bias parameter, b, of unity (p scales inversely with b and approximately linearly with Ω_0). For the atmospheric seeing and sky noise conditions associated with our data, Monte Carlo simulations suggest that the efficiency of measuring the mean cosmological polarization is on the order of 40 ± 10 per cent. Thus our preliminary analysis suggests an upper limit on the cosmological mean polarization in the field of p̄_(max) ∼ 0.04⁠. Deep wide-field imaging in 0.5 arcsec seeing to study this polarization signal should provide limits that constrain current cosmological models.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/271.1.31DOIArticle
http://adsabs.harvard.edu/abs/1994MNRAS.271...31MADSArticle
ORCID:
AuthorORCID
Mould, Jeremy0000-0003-3820-1740
Blandford, Roger0000-0002-1854-5506
Smail, Ian0000-0003-3037-257X
Additional Information:© 1994 Royal Astronomical Society. Provided by the NASA Astrophysics Data System. Accepted 1994 May 24. Received 1994 May 12; in original form 1993 November 22. We thank Alan Dressler for leading the construction of the COSMIC camera and Simon Lilly, Nick Kaiser and Tony Tyson for advice and encouragement. Support under NSF grants AST-89-17765 (RDB, TGB), AST 92-23370 (RDB, TGB), AST-89-13664 (TGB), AST-89-21001 (NV), the Ohio Supercomputer Center (NV), a NATO Postdoctoral Fellowship (IRS), and an NSF Graduate Fellowship (TAS) is gratefully acknowledged.
Group:TAPIR
Funders:
Funding AgencyGrant Number
NSFAST 89-17765
NSFAST 92-23370
NSFAST 89-13664
NSFAST 89-21001
Ohio Supercomputer CenterUNSPECIFIED
North Atlantic Treaty Organization (NATO)UNSPECIFIED
NSF Graduate Research FellowshipUNSPECIFIED
Subject Keywords:polarization - galaxies: photometry - cosmology: observations - gravitational lensing - large-scale structure of Universe
Issue or Number:1
Record Number:CaltechAUTHORS:20190523-125439677
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190523-125439677
Official Citation:Jeremy Mould, Roger Blandford, Jens Villumsen, Tereasa Brainerd, Ian Smail, Todd Small, William Kells, A search for weak distortion of distant galaxy images by large-scale structure, Monthly Notices of the Royal Astronomical Society, Volume 271, Issue 1, 1 November 1994, Pages 31–38, https://doi.org/10.1093/mnras/271.1.31
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:95758
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:23 May 2019 21:14
Last Modified:03 Oct 2019 21:16

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