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ATLAS-TEIDE: The next generations of ATLAS units for the Teide Observatory

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arxiv 2302.07954 v1 pith:NOSJ56V4 submitted 2023-02-15 astro-ph.IM astro-ph.EP

classification astro-ph.IMastro-ph.EP
keywords atlasatlas-teidewillmoduledesignbuildingconsistfield
verification ladder T0 review T1 audit T2 compute T3 formal
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In this work we present the design of the ATLAS unit (Asteroid Terrestrial-impact Last Alert System) that will be installed at Teide Observatory in Tenerife island (Spain). ATLAS-Teide will be built by the Instituto de Astrofisica de Canarias (IAC) and will be operated as part of the ATLAS network in the framework of an operation and science exploitation agreement between the IAC and the ATLAS team at University of Hawaii. ATLAS-Teide will be the first ATLAS unit based on commercial on the shelf (COTS) components. Its design is modular, each module (building block) consist of four Celestron RASA 11 telescopes that point to the same sky field, equipped with QHY600PRO CMOS cameras on an equatorial Direct Drive mount. Each module is equivalent to a 56cm effective diameter telescope and provides a 7.3 deg^2 field of view and a 1.26 arcsec/pix plate scale. ATLAS-Teide will consist of four ATLAS modules in a roll-off roof building. This configuration allows to cover the same sky area of the actual ATLAS telescopes. The first ATLAS module was installed in November 2022 in an existing clamshell at the TO. This module (ATLAS-P) is being used as a prototype to test the system capabilities, develop the needed software (control, image processing, etc.) and complete the fully integration of ATLAS-Teide in the ATLAS network. The preliminary results of the tests are presented here, and the benefits of the new ATLAS design are discussed.

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  1. Dust production rates in Jupiter-family comets II: Trends and population insights from ATLAS photometry of 116 JFCs

    astro-ph.EP 2025-06 conditional novelty 5.0 of 10

    A four-year ATLAS photometry campaign of 116 Jupiter-family comets confirms that dust production rises faster before perihelion than it declines after, with peak activity typically slightly after perihelion.

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