RoboPol: a four-channel optical imaging polarimeter

dc.contributor.authorA. N. Ramaprakash
dc.contributor.authorC. V. Rajarshi
dc.contributor.authorH. K. Das
dc.contributor.authorP. Khodade
dc.contributor.authorD. Modi
dc.contributor.authorG. Panopoulou
dc.contributor.authorS. Maharana
dc.contributor.authorD. Blinov
dc.contributor.authorE. Angelakis
dc.contributor.authorC. Casadio
dc.contributor.authorL. Fuhrmann
dc.contributor.authorT. Hovatta
dc.contributor.authorS. Kiehlmann
dc.contributor.authorO. G. King
dc.contributor.authorN. Kylafis
dc.contributor.authorA. Kougentakis
dc.contributor.authorA. Kus
dc.contributor.authorA. Mahabal
dc.contributor.authorA. Marecki
dc.contributor.authorI. Myserlis
dc.contributor.authorG. Paterakis
dc.contributor.authorE. Paleologou
dc.contributor.authorI. Liodakis
dc.contributor.authorI. Papadakis
dc.contributor.authorI. Papamastorakis
dc.contributor.authorV. Pavlidou
dc.contributor.authorE. Pazderski
dc.contributor.authorT. J. Pearson
dc.contributor.authorA. C. S. Readhead
dc.contributor.authorP. Reig
dc.contributor.authorA. Słowikowska
dc.contributor.authorK. Tassis
dc.contributor.authorJ. A. Zensus
dc.contributor.organizationfi=Suomen ESO-keskus|en=Finnish Centre for Astronomy with ESO|
dc.contributor.organization-code1.2.246.10.2458963.20.54954054844
dc.converis.publication-id41438532
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/41438532
dc.date.accessioned2022-10-28T13:17:29Z
dc.date.available2022-10-28T13:17:29Z
dc.description.abstractWe present the design and performance of RoboPol, a four-channel optical polarimeter operating at the Skinakas Observatory in Crete, Greece. RoboPol is capable of measuring both relative linear Stokes parameters q and u (and the total intensity I) in one sky exposure. Though primarily used to measure the polarization of point sources in the R band, the instrument features additional filters (B, V, and I), enabling multiwavelength imaging polarimetry over a large field of view (13.6' x 13.6'). We demonstrate the accuracy and stability of the instrument throughout its 5 yr of operation. Best performance is achieved within the central region of the field of view and in the R band. For such measurements the systematic uncertainty is below 0.1 per cent in fractional linear polarization, p (0.05 per cent maximum likelihood). Throughout all observing seasons the instrumental polarization varies within 0.1 per cent in p and within similar to 1 degrees in polarization angle.
dc.format.pagerange2355
dc.format.pagerange2366
dc.identifier.eissn1365-2966
dc.identifier.jour-issn0035-8711
dc.identifier.olddbid181080
dc.identifier.oldhandle10024/164174
dc.identifier.urihttps://www.utupub.fi/handle/11111/36963
dc.identifier.urnURN:NBN:fi-fe2021042822263
dc.language.isoen
dc.okm.affiliatedauthorHovatta, Talvikki
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeA1 ScientificArticle
dc.publisherOXFORD UNIV PRESS
dc.publisher.countryUnited Kingdomen_GB
dc.publisher.countryBritanniafi_FI
dc.publisher.country-codeGB
dc.relation.doi10.1093/mnras/stz557
dc.relation.ispartofjournalMonthly Notices of the Royal Astronomical Society
dc.relation.issue2
dc.relation.volume485
dc.source.identifierhttps://www.utupub.fi/handle/10024/164174
dc.titleRoboPol: a four-channel optical imaging polarimeter
dc.year.issued2019

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