First High Contrast Imaging Using a Gaussian Aperture Pupil Mask

Placing a pupil mask with a gaussian aperture into the optical train of current telescopes represents a way to attain high contrast imaging that potentially improves contrast by orders of magnitude compared to current techniques. We present here the first observations ever using a gaussian aperture pupil mask (GAPM) on the Penn State near-IR Imager and Spectrograph (PIRIS) at the Mt. Wilson 100$^{\prime\prime}$ telescope. Two nearby stars were observed, $\epsilon$ Eridani and $\mu$ Her A. A faint companion was detected around $\mu$ Her A, confirming it as a proper motion companion. Furthermore, the observed H and K magnitudes of the companion were used to constrain its nature. No companions or faint structure were observed for $\epsilon$ Eridani. We found that our observations with the GAPM achieved contrast levels similar to our coronographic images, without blocking light from the central star. The mask's performance also nearly reached sensitivities reported for other ground based adaptive optics coronographs and deep HST images, but did not reach theoretically predicted contrast levels. We outline ways that could improve the performance of the GAPM by an order of magnitude or more.Comment: 8 pages, 4 figures, accepted by ApJ letter

A Tunable Lyot Filter at Prime Focus: a Method for Tracing Supercluster Scales at z ~ 1

Tunable narrow-band, emission-line surveys have begun to show the ease with which star forming galaxies can be identified in restricted redshift intervals to z ~ 5 with a 4m class telescope. These surveys have been carried out with imaging systems at the Cassegrain or Nasmyth focus and are therefore restricted to fields smaller than 10 arcmin. We now show that tunable narrowband imaging is possible over a 30 arcmin field with a high-performance Lyot filter placed directly in front of a CCD mosaic at the prime focus. Our design is intended for the f/3.3 prime focus of the AAT 3.9m, although similar devices can be envisaged for the Subaru 8m (f/2), Palomar 5m (f/3.4), VISTA 4m (f/6), Mayall 4m (f/2.6) or CFHT 3.6m (f/4). A modified Wynne doublet ensures sub-arcsecond performance over the field. In combination with the new Wide-Field Imaging 8K x 8K mosaic (WFI) at the AAT, the overall throughput (35%) of the system to unpolarised light is expected to be comparable to the TAURUS Tunable Filter (TTF). Unlike the TTF, the field is fully monochromatic and the instrumental profile has much better wing suppression. For targetted surveys of emission-line sources at z ~ 1, a low-resolution (R ~ 150 at 550nm) Lyot filter on a 4m telescope is expected to be comparable or superior to current instruments on 8-10m class telescopes. We demonstrate that the 30 arcmin field is well matched to superclusters at these redshifts such that large-scale structure should be directly observable.Comment: Astrophysical Journal, accepted. 53 pages, 16 figures, aaste

23rd IAEA Fusion Energy Conference: summary of sessions EX/C and ICC

An overview is given of recent experimental results in the areas of innovative confinement concepts, operational scenarios and confinement experiments as presented at the 2010 IAEA Fusion Energy Conference. Important new findings are presented from fusion devices worldwide, with a strong focus towards the scientific and technical issues associated with ITER and W7-X devices, presently under construction

Étude des niveaux de 3He par spectroscopie optique à très basse température

The hyperfine structure of 3He and the isotope shift Δ T(4He — 3He) in lines : λλ = 7 065 Å ; 4 713 Å ; 4 471 Å and 3 888 Å have been mesured using a double Fabry-Perot etalon spectrophotometer scanned by pressure and a hollow-cathode usually cooled by liquid helium below the λ-point ([FORMULE]). Results are as follows : [FORMULE]. Raies [FORMULE]. This work follows experiments on the fine structure of 4He which have been published recently[1].La structure hyperfine de 3He et le déplacement isotopique Δ T(4He — 3He) ont été étudiés sur les raies : λλ = 7 065 Å ; 5 875 Å ; 4 713 Å ; 4 471 Å et 3 888 Å, au moyen d'un spectrophotomètre à deux étalons de Fabry-Perot associés en série et d'une cathode creuse généralement refroidie à l'hélium liquide pompé ([FORMULE]). Les résultats sont les suivants (en mK) : [FORMULE]. Raies [FORMULE]. Ce travail fait suite à une étude récente de la structure fine de 4He [1]