0000000000621135

AUTHOR

M. Cecconi

showing 5 related works from this author

Optical and ultraviolet pulsed emission from an accreting millisecond pulsar

2021

Ambrosino, F., et al.

Angular momentum010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaMagnetosphereFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesLuminosityNeutron starsSettore FIS/05 - Astronomia E AstrofisicaPulsarMillisecond pulsar0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Astronomy and AstrophysicsAccretion (astrophysics)Particle accelerationNeutron starAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Multi-band high resolution spectroscopy rules out the hot Jupiter BD+20 1790b - First data from the GIARPS Commissioning

2018

Context. Stellar activity is currently challenging the detection of young planets via the radial velocity (RV) technique. Aims. We attempt to definitively discriminate the nature of the RV variations for the young active K5 star BD+20 1790, for which visible (VIS) RV measurements show divergent results on the existence of a substellar companion. Methods. We compare VIS data with high precision RVs in the near infrared (NIR) range by using the GIANO - B and IGRINS spectrographs. In addition, we present for the first time simultaneous VIS-NIR observations obtained with GIARPS (GIANO - B and HARPS - N) at Telescopio Nazionale Galileo (TNG). Orbital RVs are achromatic, so the RV amplitude does …

PhysicsEarth and Planetary Astrophysics (astro-ph.EP)010308 nuclear & particles physicsFOS: Physical sciencesAstronomy and AstrophysicsContext (language use)Astrophysics01 natural sciences7. Clean energyRadial velocityPhotometry (astronomy)StarsAmplitudeAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary SciencePlanet0103 physical sciencesHot JupiterSpectroscopy010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics - Earth and Planetary Astrophysics
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Sindrome di Sotos: descrizione di un caso da ampia delezione del gene NSD1

2008

sindrome di Sotos NSD1 gene
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The PROVENT-C19 registry: A study protocol for international multicenter SIAARTI registry on the use of prone positioning in mechanically ventilated …

2022

Background The worldwide use of prone position (PP) for invasively ventilated patients with COVID-19 is progressively increasing from the first pandemic wave in everyday clinical practice. Among the suggested treatments for the management of ARDS patients, PP was recommended in the Surviving Sepsis Campaign COVID-19 guidelines as an adjuvant therapy for improving ventilation. In patients with severe classical ARDS, some authors reported that early application of prolonged PP sessions significantly decreases 28-day and 90-day mortality. Methods and analysis Since January 2021, the COVID19 Veneto ICU Network research group has developed and implemented nationally and internationally the “PRO…

Multidisciplinaryprone positionrespiratory failureCOVID-19PLOS ONE
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Erratum to: The Intensive Care Global Study on Severe Acute Respiratory Infection (IC‑GLOSSARI): a multicenter, multinational, 14-day inception coh…

2018

In both the original publication (DOI 10.1007/s00134-015-4206-2) and the first erratum (DOI 10.1007/s00134-016-4317-4), the members of the IC-GLOSSARI Investigators and the ESICM Trials Group were provided in such a way that they could not be indexed as collaborators on PubMed. The publisher apologizes for these errors and is pleased to list the members of the groups here: (Table presented.).

Critical Care and Intensive Care Medicine
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