Results 51 to 60 of about 1,141 (166)
Stark Broadening of Se IV, Sn IV, Sb IV and Te IV Spectral Lines
Atoms, 2018 Stark broadening parameters, line width and shift, are needed for investigations, analysis and modelling of astrophysical, laboratory, laser produced and technological plasmas.
Milan S. Dimitrijević +5 more
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A near infrared laser frequency comb for high precision Doppler planet surveys
EPJ Web of Conferences, 2011 Perhaps the most exciting area of astronomical research today is the study of exoplanets and exoplanetary systems, engaging the imagination not just of the astronomical community, but of the general population. Astronomical instrumentation has matured to
Bally J. +5 more
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GRASS. II. Simulations of Potential Granulation Noise Mitigation Methods
The Astronomical JournalWe present an updated version of the GRanulation And Spectrum Simulator (GRASS) which now uses an expanded library of 22 solar lines to empirically model time-resolved spectral variations arising from solar granulation.
Michael L. Palumbo III +5 more
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The Mitchell Spectrograph: Studying Nearby Galaxies with the VIRUS Prototype
Advances in Astronomy, 2013 The Mitchell Spectrograph (a.k.a. VIRUS-P) on the 2.7 m Harlan J. Smith telescope at McDonald Observatory is currently the largest field of view (FOV) integral field unit (IFU) spectrograph in the world (1.7′×1.7′). It was designed as a prototype for the
Guillermo A. Blanc
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Turkish Journal of Orthodontics, 2008 The aim of the study was to assess the audiologic and the speech status of operated unilateral cleft preschooler patients who have no orthodontic, otologic, and speech therapy.
Fatih Ögüt +4 more
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Hamilton’s Object revisited: A challenging source redshift of a strong lensing configuration
Astronomy & AstrophysicsLow-resolution spectrographs used to have difficulties in determining redshifts of galaxies at z ≈ 1 and z ≈ 3. Spectral emission and absorption lines of magnesium and iron redshifted to z ≈ 1 fall close to hydrogen, silicon, and oxygen lines at z ≈ 3 ...
Wagner Jenny, Falco Emilio E.
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AerospaceParticle acceleration, and the thermalisation of energetic particles, are fundamental processes across the universe. Whilst the Sun is an excellent object to study this phenomenon, since it is the most energetic particle accelerator in the Solar System ...
Ariadna Calcines Rosario +14 more
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Transiting Sub-stellar companions of Intermediate-mass stars
EPJ Web of Conferences, 2015 We use the CoRoT-survey to search for transiting close-in planets of intermediate-mass stars (M* = 1.3 − 2.1 M⊙). We present recent results of our survey.
Sebastian Daniel +4 more
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Design and Commissioning of an Iodine Cell for the ESPRESSO Spectrograph
The Astronomical JournalHigh-resolution echelle spectrographs remain the backbone of precision Doppler radial velocity (RV) programs, detecting almost all known exoplanets within 50 pc. Precision Doppler RV spectrographs have traditionally fallen into two camps.
Gillian Nave, R. Paul Butler
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Radial velocity follow-up of CoRoT transiting exoplanets
EPJ Web of Conferences, 2011 We report on the results from the radial-velocity follow-up program performed to establish the planetary nature and to characterize the transiting candidates discovered by the space mission CoRoT.
Deleuil M. +5 more
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