Spectroscopic Observations and Analysis
Hinode EUV spectroscopic observations of coronal oscillations
... over time at each oscillation period. Cross-hatched regions indi- cate the cone of influence where edge effects become strong. Due to the limited temporal resolution, only frequencies less than 10 mHz are considered. The ...
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Spectroscopic observations of the intermediate polar EX Hydrae in quiescence
... ical analysis of King & Wynn (1999) and Wynn (2000), however, has shown that equilibrium rotation is possible if the magnetic mo- ment in EX Hya falls within the range of 10 33 μ 10 34 G cm 3 ...
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Subaru FOCAS spectroscopic observations of high-redshift supernovae
... The FOCAS 2 spectroscopic data were reduced in a mostly standard way using the Image Reduction and Analysis Facility (IRAF 3 ). The bias was removed by fitting a low-order polyno- mial to the overscan ...
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Herschel spectroscopic observations of the compact obscured nucleus in Zw 049.057
... 2012). In addition, nine transitions with upper level energies up to ∼650 K were detected primarily in emission with SPIRE as summarized in Table 2. The spectral line energy distribution of the submillimeter lines is ...
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The Shapley Supercluster. II. Spectroscopic observations in a wide area and general morphology
... The positions of the observed galaxies were taken from the Digitized Sky Survey (DSS). The galaxy selection was carried out on the DSS images displayed on a computer screen, giving priority to elliptical and bright ...
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Optimizing hydroxyl airglow retrievals from long-slit astronomical spectroscopic observations
... and analysis technique, we derive a rotational temperature distribution with v 0 that agrees with atmospheric model con- ditions and the preponderance of previous ...future observations, which are at ...
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First spectroscopic observations of the substellar companion of the young debris disk star PZ Telescopii
... This publication makes use of data products from the Two Micron All Sky Sur- vey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of ...
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Galaxy And Mass Assembly (GAMA) : spectroscopic analysis
... The GAMA spectroscopic observations use the AAOmega spectro- graph (Saunders et al. 2004; Smith et al. 2004; Sharp et al. 2006) on the 3.9 m AAT (Siding Spring Observatory, NSW, Australia) for measuring the ...
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Investigating the structure of the accretion disc in WZ Sge from multiwaveband time-resolved spectroscopic observations - II
... extended analysis of a selected sample of dwarf novae shows increasing phase offset with shorter orbital period, consistent with the idea of optically thin accretion discs in low mass transfer rate ...
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Optical spectroscopic observations of gamma-ray blazar candidates III. The 2013/2014 campaign in the Southern Hemisphere
... 3.1. Unidentified Gamma-ray Sources (UGS) The WISE selected counterparts to these UGSs show IR WISE colors similar to those of γ-ray blazars considered in the analysis performed by Massaro et al. (2013a). In ...
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Directly imaging damped Lyα galaxies at z > 2 – II. Imaging and spectroscopic observations of 32 quasar fields.
... the observations and data reduc- tion for the HST and ground-based imaging, including details on the procedures adopted for photometric calibration and the prepara- tion of the galaxy ...new spectroscopic ...
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Spectroscopic Analysis of Eclipsing Binary Stars
... In order to obtain the physical and geometric parameters of the binary components, we adjusted a numerical eclipsing binary model to the observations; the mass-ratio of ER Vul and BX And were fixed at the values ...
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Galaxy And Mass Assembly (GAMA): spectroscopic analysis
... GAMA observations, the 2dF robot fibre posi- tioner is used to configure typically 345 fibres to observe galaxies within a two degree field on the ...to spectroscopic standard ...
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SPECTROSCOPIC OBSERVATIONS OF VENUS FOR ROTATION MADE AT MOUNT WILSON IN 1956
... Thus if we accept the assumption that the bands on the ultra- violet images of Venus are parallel to the equator, it would seem that the tilt of the planet relative to the earth could [r] ...
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Frequency and mode identification of gamma Doradus from photometric and spectroscopic observations
... results also allows confirmation of photometric and spectroscopic techniques for these stars. Despite the requirement to go beyond physically possible parameter space in modelling the mass and ra- dius of the ...
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The REFLEX galaxy cluster survey: VIII. Spectroscopic observations and optical atlas
... REFLEX, together with the complete table of all galaxy redshifts. Acknowledgements. We would like to thank G. Chincarini, R. Cruddace, H. MacGillivray, T. Reiprich, K. Romer, W. Seitter, P. Vettolani, W. Voges and G. ...
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The VANDELS ESO public spectroscopic survey : observations and first data release
... individual spectroscopic exposure the wavelength calibration derived from the arc exposures is checked against the positions of bright sky lines and the local inverse disper- sion solution modified to account for ...
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Optical Spectroscopic Monitoring Observations of a T Tauri Star V409 Tau
... ~10,000) spectroscopic observations with 2-m Nayuta telescope at Ni- shi-Harima Astronomical Observatory. Spectra were obtained in 18 nights between November 2015 and March 2016. Several absorption lines ...
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High-resolution optical and infrared spectroscopic observations of Cir X-1
... rate, which in turn drives a strong matter outflow. After periastron, mass transfer from the companion ceases, but accretion continues at a near-Eddington rate as the neutron star captures the residual matter in its ...
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Spectroscopic observations of the night airglow from 3000 Å to 9200 Å.
... The large modeled intensity of the OH emissions provided an upper limit to the 0(3P) number density, while the relative weakness of the modeled atomic and molecular oxygen emissions [r] ...
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