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Gaia Data Release 2
CONTEXT. The second Gaia data release is based on 22 months of mission data with an average of 0.9 billion individual CCD observations per day. A data volume of this size and granularity requires a robust and reliable but still...
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Gaia Data Release 1
At about 1000 days after the launch of Gaia we present the first Gaia data release, Gaia DR1, consisting of astrometry and photometry for over 1 billion sources brighter than magnitude 20.7. We summarize Gaia DR1 and...
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Astrometric Search Method for Individually Resolvable Gravitational Wave Sources with Gaia.
Gravitational waves (GWs) cause the apparent position of distant stars to oscillate with a characteristic pattern on the sky. Astrometric measurements (e.g., those made by Gaia) provide a new way to search for GWs. The main...
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Standard Galactic Field RR Lyrae II
RR Lyrae stars have long been popular standard candles, but significant advances in methodology and technology have been made in recent years to increase their precision as distance indicators. We present multi-wavelength...
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Standard Galactic Field RR Lyrae II
RR Lyrae stars have long been popular standard candles, but significant advances in methodology and technology have been made in recent years to increase their precision as distance indicators. We present multi-wavelength...
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The Gaia-ESO Survey
Due to their volatile nature, when sulfur and zinc are observed in external galaxies, their determined abundances represent the gas-phase abundances in the interstellar medium. This implies that they can be used as tracers of...
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New Close Binary Central Stars of Planetary Nebulae from Gaia DR3 Epoch Photometry.
Close binary interactions perform a key role in the formation and shaping of planetary nebulae (PNe). However only a small fraction of Galactic PNe are known to host close binary systems. Many such systems are detectable through...
New Close Binary Central Stars of Planetary Nebulae from Gaia DR3 Epoch Photometry.
Close binary interactions perform a key role in the formation and shaping of planetary nebulae (PNe). However only a small fraction of Galactic PNe are known to host close binary systems. Many such systems are detectable through...
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Milky Way's Eccentric Constituents with Gaia, APOGEE, and GALAH
Abstract We report the results of an unsupervised decomposition of the local stellar halo in the chemodynamical space spanned by the abundance measurements from APOGEE DR17 and...
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The Local Group Mass in the Light of Gaia
High accuracy proper motions (PMs) of M31 and other Local Group satellites have now been provided by the {\it Gaia} satellite. We revisit the Timing Argument to compute the total mass $M$ of the Local Group from the orbit of...
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Review of Bruno Latour, Facing Gaia: Eight Lectures on the New Climate Regime. Cambridge
Shannon O'Rourke
Jan 07, 2020
Facing Gaia: Eight Lectures on the New Climate Regime (FG, 2017) in significant ways represents an ecological application of Latour’s lifelong development of an anthropology of the moderns. Latour tells us in 2008, in an...
Review of Bruno Latour, Facing Gaia: Eight Lectures on the New Climate Regime. Cambridge
Shannon O'Rourke
Jan 07, 2020
Facing Gaia: Eight Lectures on the New Climate Regime (FG, 2017) in significant ways represents an ecological application of Latour’s lifelong development of an anthropology of the moderns. Latour tells us in 2008, in an...
Achieving functional neuronal dendrite structure through sequential stochastic growth and retraction
Class I ventral posterior dendritic arborisation (c1vpda) proprioceptive sensory neurons respond to contractions in the Drosophila larval body wall during crawling. Their dendritic branches run along the direction of...
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The Carnegie RR Lyrae Program
We analysed 30 RR Lyrae stars (RRLs) located in the Large Magellanic Cloud (LMC) globular cluster Reticulum that were observed in the 3.6 and 4.5 $\mu$m passbands with the Infrared Array Camera (IRAC) on board of the Spitzer...
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The Carnegie RR Lyrae Program
We analysed 30 RR Lyrae stars (RRLs) located in the Large Magellanic Cloud (LMC) globular cluster Reticulum that were observed in the 3.6 and 4.5 $\mu$m passbands with the Infrared Array Camera (IRAC) on board of the Spitzer...
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STXBP1 -associated neurodevelopmental disorder
Abstract: Background: De novo loss of function mutations in STXBP1 are a relatively common cause of epilepsy and intellectual disability (ID). However, little is known about the types and severities of behavioural features...
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Gene functional networks and autism spectrum characteristics in young people with intellectual disability
BACKGROUND: The relationships between specific genetic aetiology and phenotype in neurodevelopmental disorders are complex and hotly contested. Genes associated with intellectual disability (ID) can be grouped into networks...
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