Red-shifted chromospheric emission in 70 OPH A
Not Available
Beckman, J. E. et al.
Advertised on:
12
1991
This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..
It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/
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Redshift Measurement and Spectral Classification for eBOSS Galaxies with the redmonster SoftwareWe describe the redmonster automated redshift measurement and spectral classification software designed for the extended Baryon Oscillation Spectroscopic Survey (eBOSS) of the Sloan Digital Sky Survey IV (SDSS-IV). We describe the algorithms, the template standard and requirements, and the newly developed galaxy templates to be used on eBOSSHutchinson, T. A. et al.
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122016 -
Reflections on the discovery of pulsarsNot AvailableBell Burnell, J.
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122010 -
Relationships of Dione's physical and chemical surface properties to geological and morphological surface featuresDuring orbit DI 016 (October 2005) Cassini's Visual and Infrared Mapping Spectrometer (VIMS) [1] acquired spatially resolved spectral data of the Saturnian satellite Dione with pixel ground resolutions up to 2 km per pixel. Additionally, the Imaging Science Subsystem (ISS) [2] observed the satellite synchronously to VIMS with pixel groundStephan, K. et al.
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122007 -
Relativistic baryonic jets from an ultraluminous supersoft X-ray sourceThe formation of relativistic jets by an accreting compact object is one of the fundamental mysteries of astrophysics. Although the theory is poorly understood, observations of relativistic jets from systems known as microquasars (compact binary stars) have led to a well established phenomenology. Relativistic jets are not expected to be producedLiu, Ji-Feng et al.
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122015 -
Resolving the Innermost Region of the Accretion Disk of the Lensed Quasar Q2237+0305 through Gravitational MicrolensingWe study three high magnification microlensing events, generally recognized as probable caustic crossings, in the optical light curves of the multiply imaged quasar Q2237+0305. We model the light curve of each event as the convolution of a standard thin disk luminosity profile with a straight fold caustic. We also allow for a linear gradient thatMediavilla, E. et al.
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122015