Zero-polarization candidate regions for the calibration of wide-field optical polarimeters
Artikel i vetenskaplig tidskrift, 2024
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.
catalogs
methods: observational
polarization
ISM: general
techniques: polarimetric
Författare
N. Mandarakas
Panepistimio Kritis
Idryma Technologias kai Erevnas (FORTH)
Georgia Virginia Panopoulou
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
V. Pelgrims
Université libre de Bruxelles (ULB)
S. B. Potter
South African Astronomical Observatory
University of Johannesburg
V. Pavlidou
Panepistimio Kritis
Idryma Technologias kai Erevnas (FORTH)
A. N. Ramaprakash
Inter-University Centre for Astronomy and Astrophysics
Idryma Technologias kai Erevnas (FORTH)
California Institute of Technology (Caltech)
Konstantinos Tassis
Idryma Technologias kai Erevnas (FORTH)
Panepistimio Kritis
D. Blinov
Idryma Technologias kai Erevnas (FORTH)
S. Kiehlmann
Idryma Technologias kai Erevnas (FORTH)
E. Koutsiona
Panepistimio Kritis
S. Maharana
South African Astronomical Observatory
S. Romanopoulos
Idryma Technologias kai Erevnas (FORTH)
Panepistimio Kritis
R. Skalidis
California Institute of Technology (Caltech)
A. Vervelaki
Panepistimio Kritis
S. E. Clark
Stanford University
Kavli Institute for Particle Astrophysics and Cosmology
J. A. Kypriotakis
Panepistimio Kritis
Idryma Technologias kai Erevnas (FORTH)
A. C.S. Readhead
California Institute of Technology (Caltech)
Idryma Technologias kai Erevnas (FORTH)
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 684 A132Ämneskategorier (SSIF 2011)
Astronomi, astrofysik och kosmologi
Atom- och molekylfysik och optik
DOI
10.1051/0004-6361/202348099