9 research outputs found

    Low Efficiency Upconversion Nanoparticles for High-Resolution Coalignment of Near-Infrared and Visible Light Paths on a Light Microscope

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    One major technical barrier in working with both NIR and visible light on an optical microscope is obtaining their precise coalignment at the imaging plane position. Current techniques require complex setups and software. Photon upconverting particles (UCPs) can bridge this gap as they are excited by NIR light but emit in the visible range. Here, two different UCPs have been identified, high-efficiency micro540-UCPs and lower efficiency nano545-UCPs are compared, and it is found that the lower efficiency nano-UCPs were superior for precise coalignment of the NIR beam with the visible light path consistent with limited particle-to-particle energy transfer, superlinear power dependence for emission, and much smaller particle size

    pydantic/pydantic: v2.5.2 2023-11-22

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    <h2>v2.5.2 (2023-11-22)</h2> <p><a href="https://github.com/pydantic/pydantic/releases/tag/v2.5.2">GitHub release</a></p> <h3>What's Changed</h3> <h4>Packaging</h4> <ul> <li>uprev <code>pydantic-core</code> to 2.14.5</li> </ul> <h4>New Features</h4> <ul> <li>Add <code>ConfigDict.ser_json_inf_nan</code> by @davidhewitt in <a href="https://github.com/pydantic/pydantic/pull/8159">#8159</a></li> </ul> <h4>Fixes</h4> <ul> <li>Fix validation of <code>Literal</code> from JSON keys when used as <code>dict</code> key by @sydney-runkle in <a href="https://github.com/pydantic/pydantic-core/pull/1075">pydantic/pydantic-core#1075</a></li> <li>Fix bug re <code>custom_init</code> on members of <code>Union</code> by @sydney-runkle in <a href="https://github.com/pydantic/pydantic-core/pull/1076">pydantic/pydantic-core#1076</a></li> <li>Fix <code>JsonValue</code> <code>bool</code> serialization by @sydney-runkle in <a href="https://github.com/pydantic/pydantic/pull/8159">#8190</a></li> <li>Fix handling of unhashable inputs with <code>Literal</code> in <code>Union</code>s by @sydney-runkle in <a href="https://github.com/pydantic/pydantic-core/pull/1089">pydantic/pydantic-core#1089</a></li> </ul> <p>https://github.com/pydantic/pydantic/compare/v2.5.1...v2.5.2/</p&gt

    pydantic/pydantic: v2.5.1 2023-11-15

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    <h2>v2.5.1 (2023-11-15)</h2> <p><a href="https://github.com/pydantic/pydantic/releases/tag/v2.5.1">GitHub release</a></p> <h3>What's Changed</h3> <h4>Packaging</h4> <ul> <li>uprev pydantic-core to 2.14.3 by @samuelcolvin in <a href="https://github.com/pydantic/pydantic/pull/8120">#8120</a></li> </ul> <h4>Fixes</h4> <ul> <li>Fix package description limit by @dmontagu in <a href="https://github.com/pydantic/pydantic/pull/8097">#8097</a></li> <li>Fix <code>ValidateCallWrapper</code> error when creating a model which has a @validate_call wrapped field annotation by @sydney-runkle in <a href="https://github.com/pydantic/pydantic/pull/8110">#8110</a></li> </ul> <p>Full Changelog: https://github.com/pydantic/pydantic/compare/v2.5.0...v2.5.1/</p&gt

    Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo

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    Advanced LIGO and Advanced Virgo are monitoring the sky and collecting gravitational-wave strain data with sufficient sensitivity to detect signals routinely. In this paper we describe the data recorded by these instruments during their first and second observing runs. The main data products are gravitational-wave strain time series sampled at 16384 Hz. The datasets that include this strain measurement can be freely accessed through the Gravitational Wave Open Science Center at http://gw-openscience.org, together with data-quality information essential for the analysis of LIGO and Virgo data, documentation, tutorials, and supporting software
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