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PlanetPol

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The William Herschel Telescope building

PlanetPol was a ground-based, high sensitivitypolarimeter based at theWilliam Herschel Telescope[1] on the island ofLa Palma in theCanary Islands,Spain that has now been decommissioned. It was the most sensitive astronomical visual polarimeter ever built in fractional polarisation, a mantle that since its decommissioning now belongs toHIPPI. Although the device could be used for a wide range of astronomy, its primary use was thedetection of extrasolar planets.[1]

Results

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PlanetPol did not discover any extrasolar planets, however it was used to provide upper limits to planetary albedos in the known55 Cnc andτ Boo planetary systems.[2] Observations with the polarimeter in the Canary Islands, which are affected by dust from the Sahara, also identified airborne dust as a source of polarization within our atmosphere.[3] Additionally, PlanetPol provided measurements of the polarization of a few dozen nearby stars,[4] which were later combined with southern hemisphere measurements from PlanetPol's successor, HIPPI,[5] to provide information about the nature of those stars and the distribution of the interstellar medium.[6]

References

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  1. ^abHough, J. H.; Lucas, P. W.; Bailey, J. A.; Tamura, M.; et al. (2006-09-01)."PlanetPol: A Very High Sensitivity Polarimeter".The Publications of the Astronomical Society of the Pacific.118 (847):1302–1318.Bibcode:2006PASP..118.1302H.doi:10.1086/507955. Retrieved2012-01-22.
  2. ^Lucas, P. W.; Hough, J. H.; Bailey, J. A.; Tamura, M.; Hirst, E.; Harrison, D. (2009-02-11)."Planetpol polarimetry of the exoplanet systems 55 Cnc and τ Boo".Monthly Notices of the Royal Astronomical Society.393 (1):229–244.arXiv:0807.2568.Bibcode:2009MNRAS.393..229L.doi:10.1111/j.1365-2966.2008.14182.x.ISSN 0035-8711.
  3. ^Bailey, Jeremy; Ulanowski, Z.; Lucas, P. W.; Hough, J. H.; Hirst, E.; Tamura, M. (May 2008)."The effect of airborne dust on astronomical polarization measurements".Monthly Notices of the Royal Astronomical Society.386 (2):1016–1022.Bibcode:2008MNRAS.386.1016B.doi:10.1111/j.1365-2966.2008.13088.x.ISSN 0035-8711.
  4. ^Bailey, Jeremy; Lucas, P. W.; Hough, J. H. (April 2010)."The linear polarization of nearby bright stars measured at the parts per million level".Monthly Notices of the Royal Astronomical Society.405 (4): 2570.arXiv:1003.1753.Bibcode:2010MNRAS.405.2570B.doi:10.1111/j.1365-2966.2010.16634.x.ISSN 0035-8711.S2CID 16710999.
  5. ^Bailey, Jeremy; Kedziora-Chudczer, Lucyna; Cotton, Daniel V.; Bott, Kimberly; Hough, J. H.; Lucas, P. W. (2015-04-08)."A high-sensitivity polarimeter using a ferro-electric liquid crystal modulator".Monthly Notices of the Royal Astronomical Society.449 (3):3064–3073.arXiv:1503.02236.Bibcode:2015MNRAS.449.3064B.doi:10.1093/mnras/stv519.ISSN 1365-2966.
  6. ^Cotton, Daniel V.; Bailey, Jeremy; Kedziora-Chudczer, Lucyna; Bott, Kimberly; Lucas, P. W.; Hough, J. H.; Marshall, Jonathan P. (2015-11-19)."The linear polarization of Southern bright stars measured at the parts-per-million level".Monthly Notices of the Royal Astronomical Society.455 (2):1607–1628.arXiv:1509.07221.Bibcode:2016MNRAS.455.1607C.doi:10.1093/mnras/stv2185.ISSN 0035-8711.
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