Improved Multi-octave 3 dB IF Hybrid for Radio Astronomy Cryogenic Receivers
Not Available
Malo, I. et al.
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4
2009
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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GRB 060605: multi-wavelength analysis of the first GRB observed using integral field spectroscopyThe long and relatively faint gamma-ray burst GRB 060605 detected by Swift/BAT lasted about 20 s. Its afterglow could be observed with Swift/XRT for nearly 1 day, while Swift/UVOT could detect the afterglow during the first 6 h after the event. Here, we report on integral field spectroscopy of its afterglow performed with PMAS/PPak mounted at theFerrero, P. et al.
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42009 -
Gamma-ray burst observations with new generation imaging atmospheric Cerenkov Telescopes in the FERMI eraAfter the launch and successful beginning of operations of the FERMI satellite, the topics related to high-energy observations of gamma-ray bursts have obtained a considerable attention by the scientific community. Undoubtedly, the diagnostic power of high-energy observations in constraining the emission processes and the physical conditions ofCovino, S. et al.
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42009 -
Evidence for sub-populations in Globular Clusters - their properties and relations with the cluster propertiesNot AvailableCassisi, S.
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42009 -
e-EVN observations of Aql X-1 in outburstThe neutron star X-ray binary Aql X-1 shows quasi-periodic outbursts about once a year. These active states are relatively well covered in optical/infrared and X-ray domains. In contrast, at radio wavelengths the observations are very scarce (IAUC #5112; ATEL #286; ATEL #491). Following the reports of a new outburst of the object (ATEL #1970; ATELTudose, V. et al.
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42009 -
Disk tomography and dynamics: a time-dependent study of known mid-infrared variable young stellar objectsMost of our knowledge on young stars comes from snapshot observations: spectra and images taken at a single epoch, or at different epochs at different wavelengths. It is, however, known that many of the systems are variable. Variability at optical and near-infrared wavelength is mostly related to the central star itself. Mid-infrared flux changesAbraham, Peter et al.
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42009