The NICMOS Polarimetric Calibration
arXiv:astro-ph/0601541 · doi:10.1086/501534
Abstract
The value of accurately knowing the absolute calibration of the polarizing elements in the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) becomes especially important when conducting studies which require measuring degrees of polarization of close to 1% in the near infrared. We present a comprehensive study of all previously observed polarimetric standards using the NIC2 camera on NICMOS. Considering both pre- and post-NICMOS Cooling System observations we find variations in the polarimetry consistent with the effects of sub-pixel mis-alignments and the point spread function. We also measure non-zero results from unpolarized standards indicating an instrumental polarization of p ~ 1.2%, theta ~ 88degrees. The lack of polarized and unpolarized standard stars with which to perform a comprehensive calibration study means we cannot be confident that the current calibration will be effective for a number of recent large NICMOS GO programs. Further observations of polarimetric standards are needed in order to fully characterize the behavior of NICMOS at around p=1%.
9 pages, 4 figures, PASP accepted
References in corpus (4)
- Analysis of the Flux and Polarization Spectra of the Type Ia Supernova SN 2001el: Exploring the Geometry of the High-velocity Ejecta
- HST/NICMOS Imaging Polarimetry of Proto-Planetary Nebulae: Probing of the Dust Shell Structure via Polarized Light
- Polarization Profiles of Scattered Emission Lines. II. Upstream Dust Scattering in the HH 1 Jet
- Acquisition and analysis of adaptive optics imaging polarimetry data
Cited by in corpus (5)
- HST/NICMOS Imaging Polarimetry of Proto-Planetary Nebulae II: Macro-morphology of the Dust Shell Structure via Polarized Light
- Hubble Space Telescope NICMOS Polarization Observations of Three Edge-on Massive YSOs
- Nicmos Polarimetry of "Polar Scattered" Seyfert 1 Galaxies
- Aligned grains and inferred toroidal magnetic fields in the envelopes of massive young stellar objects
- The Nature of the Near-IR Core Source in 3C 433