Results 31 to 40 of about 582,844 (265)

Line bisectors and radial velocity jitter from SARG spectra [PDF]

open access: yesAstron.Astrophys. 442 (2005) 775-784, 2005
We present an analysis of spectral line bisector variations for a few stars observed in the SARG high precision radial velocity planet survey, and discuss their relationship with differential radial velocities. The spectra we consider are the same used for determining radial velocities.
arxiv   +1 more source

Modeling Stellar Oscillations and Granulation in Radial Velocity Time Series: A Fourier-based Method [PDF]

open access: yesarXiv, 2022
Tens of thousands of solar-like oscillating stars have been observed by space missions. Their photometric variability in the Fourier domain can be parameterized by a sum of two super-Lorentizian functions for granulation and a Gaussian-shaped power excess for oscillation.
arxiv  

WIYN Open Cluster Study. XXXVIII. Stellar Radial Velocities in the Young Open Cluster M35 (NGC 2168)

open access: yes, 2009
We present 5201 radial-velocity measurements of 1144 stars, as part of an ongoing study of the young (150 Myr) open cluster M35 (NGC 2168). We have observed M35 since 1997, using the Hydra Multi-Object Spectrograph on the WIYN 3.5m telescope. Our stellar
Aaron M. Geller   +27 more
core   +1 more source

AAPM‐RSS Medical Physics Practice Guideline 9.b: SRS‐SBRT

open access: yesJournal of Applied Clinical Medical Physics, EarlyView.
Abstract The purpose of this Medical Physics Practice Guideline (MPPG) is to describe the minimum level of medical physics support deemed prudent for the practice of linear‐accelerator, photon‐based (linac) stereotactic radiosurgery (SRS), and stereotactic body radiation therapy (SBRT) services.
Eileen Cirino   +9 more
wiley   +1 more source

Radial Velocities of Three Poorly Studied Clusters and the Kinematics of Open Clusters [PDF]

open access: yesAJ, 147, 69 (2014), 2014
We present radial velocities for stars in the field of the open star clusters Berkeley 44, Berkeley 81, and NGC 6802 from spectra obtained using the Wisconsin-Indiana-Yale-NOAO (WIYN) 3.5 m telescope. These clusters are of intermediate age (1-3 Gyr), located within the solar Galactocentric radius, and have no previous radial velocity measurements.
arxiv   +1 more source

Searching for Planets in the Hyades V: Limits on Planet Detection in the Presence of Stellar Activity

open access: yes, 2004
We present the results of a radial velocity survey of a sample of Hyades stars, and discuss the effects of stellar activity on radial velocity measurements. The level of radial velocity scatter due to rotational modulation of stellar surface features for
Allende Prieto C.   +5 more
core   +2 more sources

Photometry as a proxy for stellar activity in radial velocity analyses

open access: yes, 2020
Stellar activity remains a limiting factor in measuring precise planet parameters from radial velocity spectroscopy, not least in the search for Earth mass planets orbiting in the habitable zones of Sun-like stars.
Crossfield, Ian J. M.   +1 more
core   +1 more source

Multi‐institutional study on image quality for a novel CBCT solution on O‐ring linac

open access: yesJournal of Applied Clinical Medical Physics, EarlyView.
Abstract Introduction This work presents a multi‐institutional study on image quality provided by a novel cone beam computed tomography (CBCT). The main goal is to investigate the consistency of imaging performance across multiple institutions.
Luis Agulles‐Pedrós   +11 more
wiley   +1 more source

Long-lived, long-period radial velocity variations in Aldebaran: A planetary companion and stellar activity

open access: yes, 2015
We investigate the nature of the long-period radial velocity variations in Alpha Tau first reported over 20 years ago. We analyzed precise stellar radial velocity measurements for Alpha Tau spanning over 30 years.
Cochran, W. D.   +16 more
core   +1 more source

Starspot-induced optical and infrared radial velocity variability in T Tauri star Hubble 4 [PDF]

open access: yes, 2011
We report optical (6150 Ang) and K-band (2.3 micron) radial velocities obtained over two years for the pre-main sequence weak-lined T Tauri star Hubble I 4.
Bean   +35 more
core   +2 more sources

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