SwePub
Sök i LIBRIS databas

  Extended search

onr:"swepub:oai:research.chalmers.se:a232227b-c18d-459e-b33f-5b72d69891de"
 

Search: onr:"swepub:oai:research.chalmers.se:a232227b-c18d-459e-b33f-5b72d69891de" > Zero-polarization c...

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

Zero-polarization candidate regions for the calibration of wide-field optical polarimeters

Mandarakas, N. (author)
Panepistimio Kritis,University of Crete
Panopoulou, Georgia Virginia, 1989 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Pelgrims, V. (author)
Université libre de Bruxelles (ULB)
show more...
Potter, S. B. (author)
South African Astronomical Observatory,University of Johannesburg
Pavlidou, V. (author)
Panepistimio Kritis,University of Crete
Ramaprakash, A. N. (author)
California Institute of Technology (Caltech),Inter-University Centre for Astronomy and Astrophysics (IUCAA)
Tassis, Konstantinos (author)
Panepistimio Kritis,University of Crete
Blinov, D. (author)
Kiehlmann, S. (author)
Koutsiona, E. (author)
Panepistimio Kritis,University of Crete
Maharana, S. (author)
South African Astronomical Observatory
Romanopoulos, S. (author)
Panepistimio Kritis,University of Crete
Skalidis, R. (author)
California Institute of Technology (Caltech)
Vervelaki, A. (author)
Panepistimio Kritis,University of Crete
Clark, S. E. (author)
Stanford University
Kypriotakis, J. A. (author)
Panepistimio Kritis,University of Crete
Readhead, A. C.S. (author)
California Institute of Technology (Caltech)
show less...
 (creator_code:org_t)
2024
2024
English.
In: Astronomy and Astrophysics. - 0004-6361 .- 1432-0746. ; 684
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • Context. The calibration of optical polarimeters relies on the use of stars with negligible polarization (i.e., unpolarized standard stars) for determining the instrumental polarization zero point. For wide-field polarimeters, calibration is often done by imaging the same star over multiple positions in the field of view (FoV), which is a time-consuming process. A more effective technique is to target fields containing multiple standard stars. While this method has been used for fields with highly polarized stars, there are no such sky regions with well measured unpolarized standard stars. Aims. We aim to identify sky regions with tens of stars exhibiting negligible polarization that are suitable for a zero-point calibration of wide-field polarimeters. Methods. We selected stars in regions with extremely low reddening, located at high Galactic latitudes. We targeted four ∼40′ × 40′ fields in the northern and eight in the southern equatorial hemispheres. Observations were carried out at the Skinakas Observatory and the South African Astronomical Observatory. Results. We found two fields in the north and seven in the south characterized by a mean polarization lower than p < 0.1%. Conclusions. At least 9 out of the 12 fields can be used for a zero-point calibration of wide-field polarimeters.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Atom- och molekylfysik och optik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Atom and Molecular Physics and Optics (hsv//eng)

Keyword

polarization
ISM: general
methods: observational
catalogs
techniques: polarimetric

Publication and Content Type

art (subject category)
ref (subject category)

Find in a library

To the university's database

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Close

Copy and save the link in order to return to this view