XMM-Newton Observations of the Lockman Hole: Spectra and Time Variability of the Brightest AGN
Not Available
Mateos, S. et al.
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2006
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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XMM-Newton and Deep Optical Observations of the OTELO Fields: the Groth-Westphal StripOTELO (OSIRIS Tunable Emission Line Object Survey) will be carried out with the OSIRIS instrument at the 10 m GTC telescope at La Palma, and is aimed to be the deepest and richest survey of emission line objects to date. The deep narrow-band optical data from OSIRIS will be complemented by means of additional observations that include: (i) anSánchez-Portal, M. et al.
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X-ray Flare Modeling in the Single Giant HR 9024We analyze a Chandra-HETGS observation of the single G-type giant HR 9024. The high flux allows us to examine spectral line and continuum diagnostics at high temporal resolution, to derive plasma parameters (thermal distribution, abundances, temperature, ...). A time-dependent 1D hydrodynamic loop model with semi-length 10$^{12}$cm ($sim R_{star}$)Testa, P. et al.
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X-ray Emission of a Sample of LINER GalaxiesNot AvailableGonzález-Martin, O. et al.
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Whole Earth telescope observations of the ZZ Ceti star HL Tau 76This paper analyses the Whole Earth Telescope observations of HL Tau 76, the first discovered pulsating DA white dwarf. The star was observed during two Whole Earth Telescope campaigns. It was a second priority target during the XCOV13 campaign in 1996 and the first priority one during the XCOV18 campaign in 1999. The 1999 campaign reached 66.5%Dolez, N. et al.
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V-type asteroids: A mineralogical studyThe relation among V-type asteroids in the Main Belt, the large basaltic asteroid (4) Vesta and the HED meteorites is a long standing issue. To better constraint this relation we analysed the spectral parameter distribution of a sample of V-type asteroids, located in the vicinity of (4) Vesta, and of basaltic achondrites meteorites. Our resultsDuffard, René et al.
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