Simultaneous measurement of the four stokes parameters, as a function of ... (calcite) Detector. E. O. Light. beam. 1 Background (cont.) Example: HPOL @ PBO ...
Linear spectropolarimetry. Jorick Vink (Armagh Observatory) Linear ... X ray emission. Questions for Star Formation. Do all stars form by disk accretion? ...
Instrumentation for high-resolution spectropolarimetry in the visible and far-ultraviolet. ... 4-mirror Spherical Aberration Corrector (SAC), 8 arcmin field of view ...
FOVs of VIR Coronagraph. at differnt S/Cs roll angles. Slit's FOV of the. UV Coronagraph (the telescope points at different heights by tilting the mirror) ...
Rule of thumb: 1% polarization corresponds to 10-15% asymmetry (if oblate) Dominant axis ... ? V ~0.05 mag (if oblate, in any event vanishing ~one week after maximum) ...
Department of Physics & Astronomy. University of Western Ontario. London, Canada West ... on Spectropolarimetry. 53 Cam Fe abundance and field maps from 3 lines ...
INSTRUMENT SCIENCE - POLARIMETRY KENNETH NORDSIECK UNIVERSITY OF WISCONSIN PROGRAM TABLE Currently no NIR spectropolarimeter available on 10m-class telescope Projects ...
Polarimetry as a clue toward the nature of FeLoBAL quasars Daniel Lawther, Dark Cosmology Centre, Uni. of Copenhagen Polarimetry as a clue toward the nature of ...
Busted Myth: BALQSOs are exclusively radio-quiet (busted years ago, Becker et al. ... Vmax & luminosity, consistent with Laor & Brandt's work (green line, open green ...
Atomic fluorescence and prospects for observing magnetic geometry using magnetic realignment of atomic ground states Magnetic realignment - Observer's perspective
and black squares are the. limb parts. 1.5'' wide slit - nearly. entire planet covered ... solid line = limb of the planet. dotted line = central part. dashed ...
Discovery of Relativistic Positrons in Solar Flares with Microwave Imaging and Polarimetry Gregory D. Fleishman, Alexander T. Altyntsev, Natalia S. Meshalkina
SN 2006gy: One of the most luminous SNe. MV ~ -22 mag? Lbol~3 1044 erg s-1; slow LC evolution, ... Likely more luminous than SN 2006gz (56Ni mass 1.2 M ...
Classical T Tauri Star (Goodson et al. 1997) ... COUP: X-ray Christmas Tree. COUP (Chandra Orion Ultra-deep Project). Time lapse movie of observations many flares. ...
1. Prime Focus Imaging Spectrograph (PFIS) SALT combined with SAC provides ... spectrographs on other telescopes. 9. Wavelength Coverage & Spectral Resolution ...
A Crab-like field of 1012 Gauss and a Crab-like rotation. of 33 ms are dynamically unimportant. ... m = 1 single spiral arm mode. Outward transport of angular ...
Upcoming SV program on Gemini North with NIFS/Altair/LGS system. All Ca II. triplet ... big symbols. are NGC 5548. Collin et al. (2006) 36. What does FWHM ...
in spherically-symmetric winds, there should be no net polarisation. ... Here there are two winds: The polarisation amplitude is the total value for both ...
Tracking stations. South Africa, Argentina. CDTI Ministerio de Industria. UCM ... ORFEUS flown on the Space Shuttle on two space shuttle flights in 1993 and 1996 ...
The telescope & polarimeter. The transfer optics. The spectrographs ... The polarimeter is located @ the telescope's (F1) Cassegrain focus ... The Polarimeter ...
... 2004B and 2005A, Optical spectroscopy and IR photometry) and the ... core-collapse (via spectroscopy or phototyping) SN, above 18.5 mag, visible from ...
Polarization Surface-State Retrieval in the Presence of Atmospheric Perturbations ... D. Diner, A. Davis, R. Chipman, 'Innovative Technology Approach for High ...
Further Progress on the. SALT 11- meter telescope ... SALT is based on the Hobby-Eberly Telescope (HET) 11 m segmented spherical primary ... Upcoming Schedule: ...
(2) Comsoft, Tucson AZ http://www.comsoft-telescope.com/ No Bid? ... West library now a useful space with historic drawings, pictures and papers. 23 Jan 2006 ...
Part I: Different polarization states of light. Light as an electromagnetic wave ... 17th 19th centuries: Huygens, Malus, Brewster, Biot, Fresnel and Arago, Nicol...
... removing magazine, using insertor to inset and remove a manually loaded slitmask ... Needs slitmask magazine, more automated acquisition procedure to be ...
These observations add to the Subaru search in building up a sample of highest ... Discoveries of 29 high redshift SNe with Subaru. HST ACS follow ups of 5 SNe ...
Panel C. Solar telescopes, in situ solar system missions and Laboratory studies ... Panel C Programme (2) Solar Telescopes. Long-term studies of solar ...
A panchromatic review of thermal and non-thermal AGNs Robert R. J. Antonucci Department of Physics University of California, Santa Barbara Santa Barbara, CA 93106-9530
Simulations taking on a new degree of realism. Beginnings of confrontation of ... Magneto-convection (both strong and weak field cases): detailed comparison of ...
Bob Fosbury ST-ECF. High redshift radio galaxies. Massive galaxy ... One cycle - 4 x 30min at standard HWP angles. Reduced to I, Q and U Stokes spectra ...
Imaging,Visible, Tunable, Narrow-Passband Filter System A Multiple Fabry-Perot Etalon Interferometer for the ATST G. Allen Gary/MSFC, K. S. Balasubramaniam/NSO ...
f/17 at F1 focus. Polarimetric analysis at F1 (no instrumental polarization at ... High-res double spectrograph allowing up to 10 (6) spectral domains observed ...
Optical Spectroscopy Introduction & Overview Ian Browne & Chris O Dea Acknowledgements: Jerry Kriss & Jeff Valenti Aims for this lecture What is Spectroscopy?
Astronomical imaging. What we in general want is. Largest possible field of ... Mounted in the Cassegrain focus, together with the filter & shutter unit (FASU) ...