Vertical structure of an exoplanet's atmospheric jet stream.

Ultra-hot Jupiters, an extreme class of planets not found in our solar system, provide a unique window into atmospheric processes. The extreme temperature contrasts between their day- and night-sides pose a fundamental climate puzzle: how is energy distributed? To address this, we must observe the 3D structure of these atmospheres, particularly their vertical circulation patterns, which can serve as a testbed for advanced Global Circulation Models (GCM) e.g.

Hand Hygiene Compliance at a Canadian provincial cancer centre - the complementary roles of nurse auditor-driven and patient auditor-driven audit processes and impact upon practice in ambulatory cancer care.

Background: We examined the patterns of hand hygiene compliance (HHC) among health care providers (HCP) as observed by trained nurse and patient auditors over time in an ambulatory care Canadian provincial cancer agency.

Methods: Nurse and volunteer patient auditors completed separate standardized forms documenting hand-cleansing opportunities during clinic visits. HHC rates were compared over time by HCP group and by specialty teams.

A Review of Possible Planetary Atmospheres in the TRAPPIST-1 System.

TRAPPIST-1 is a fantastic nearby (∼39.14 light years) planetary system made of at least seven transiting terrestrial-size, terrestrial-mass planets all receiving a moderate amount of irradiation. To date, this is the most observationally favourable system of potentially habitable planets known to exist.

Nightside condensation of iron in an ultrahot giant exoplanet.

Ultrahot giant exoplanets receive thousands of times Earth's insolation. Their high-temperature atmospheres (greater than 2,000 kelvin) are ideal laboratories for studying extreme planetary climates and chemistry. Daysides are predicted to be cloud-free, dominated by atomic species and much hotter than nightsides.

Spectrally resolved helium absorption from the extended atmosphere of a warm Neptune-mass exoplanet.

Stellar heating causes atmospheres of close-in exoplanets to expand and escape. These extended atmospheres are difficult to observe because their main spectral signature-neutral hydrogen at ultraviolet wavelengths-is strongly absorbed by interstellar medium. We report the detection of the near-infrared triplet of neutral helium in the transiting warm Neptune-mass exoplanet HAT-P-11b by using ground-based, high-resolution observations.