GOLF in-flight commissioning and calibration was carried out during the first four months, most of which represented the cruise phase of SOHO towards its final L1 orbit. The initial performance of GOLF is shown to be within the design specification, for the entire instrument as well as for the separate sub-systems. Malfunctioning of the polarising
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Performance and Early Results from the GOLF Instrument Flown on the SOHO MissionGabriel, A. H. et al.101997
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Periodic Comet Halley (1982i)
IAUC 4115 available at Central Bureau for Astronomical Telegrams.
Landgraf, W. et al.Advertised on:
101985 -
PGos3: a database of synthesis models in the VO
We present PGos3, a database of evolutionary synthesis models and atmosphere libraries that compiles the Single Stellar Populations (SSP) results from different authors, covering more than 90% of the models used in the literature. PGos3 provides access to the models via WWW and in VOTable format accessible using TSAP protocol. Currently, a
Cerviño, M. et al.Advertised on:
102008 -
Phase Resolved Blue Spectroscopy of SS433
Despite more than 20 years of study, we still possess only limited constraints on the fundamental properties of SS433. With the exception of the 13d period, orbital parameters are ill-constrained, and hence the nature of both compact object, a neutron star or black hole, or the mass donor are still unknown. However, newly acquired high resolution
Barnes, A. D. et al.Advertised on:
102005 -
Phenomenological MSSM interpretation of CMS searches in pp collisions at √{s}=7 and 8 TeV
Searches for new physics by the CMS collaboration are interpreted in the framework of the phenomenological minimal supersymmetric standard model (pMSSM). The data samples used in this study were collected at √{s}=7 and 8 TeV and have integrated luminosities of 5.0 fb-1 and 19.5 fb-1, respectively. A global Bayesian analysis is performed
Khachatryan, V. et al.Advertised on:
102016 -
Phenomenological simulation of the total solar irradiance and its power spectrum
Not Available
Vázquez Ramió, H. et al.Advertised on:
102006