The ArT\'eMiS wide-field submillimeter camera: preliminary on-sky performances at 350 microns

The ArT\'eMiS wide-field submillimeter camera: preliminary on-sky performances at 350 microns

ArTeMiS is a wide-field submillimeter camera operating at three wavelengths simultaneously (200, 350 and 450 microns). A preliminary version of the instrument equipped with the 350 microns focal plane, has been successfully installed and tested on APEX telescope in Chile during the 2013 and 2014 aus...

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Main Authors: Reveret, Vincent, André, Philippe, Pennec, Jean Le, Talvard, Michel, Agnèse, Patrick, Arnaud, Agnès, Clerc, Laurent, de Breuck, Carlos, Cigna, Jean-Charles, Delisle, Cyrille, Doumayrou, Eric, Duband, Lionel, Dubreuil, Didier, Dumaye, Luc, Ercolani, Eric, Gallais, Pascal, Groult, Elodie, Jourdan, Thierry, Leriche, Bernadette, Maffei, Bruno, Lortholary, Michel, Martignac, Jérôme, Rabaud, Wilfried, Relland, Johan, Rodriguez, Louis, Vandeneynde, Aurélie, Visticot, François
Format: Journal Article
Language:English
Published: 09-07-2014
Subjects:
Physics - Instrumentation and Methods for Astrophysics
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Summary:ArTeMiS is a wide-field submillimeter camera operating at three wavelengths simultaneously (200, 350 and 450 microns). A preliminary version of the instrument equipped with the 350 microns focal plane, has been successfully installed and tested on APEX telescope in Chile during the 2013 and 2014 austral winters. This instrument is developed by CEA (Saclay and Grenoble, France), IAS (France) and University of Manchester (UK) in collaboration with ESO. We introduce the mechanical and optical design, as well as the cryogenics and electronics of the ArTeMiS camera. ArTeMiS detectors are similar to the ones developed for the Herschel PACS photometer but they are adapted to the high optical load encountered at APEX site. Ultimately, ArTeMiS will contain 4 sub-arrays at 200 microns and 2x8 sub-arrays at 350 and 450 microns. We show preliminary lab measurements like the responsivity of the instrument to hot and cold loads illumination and NEP calculation. Details on the on-sky commissioning runs made in 2013 and 2014 at APEX are shown. We used planets (Mars, Saturn, Uranus) to determine the flat-field and to get the flux calibration. A pointing model was established in the first days of the runs. The average relative pointing accuracy is 3 arcsec. The beam at 350 microns has been estimated to be 8.5 arcsec, which is in good agreement with the beam of the 12 m APEX dish. Several observing modes have been tested, like On-The-Fly for beam-maps or large maps, spirals or raster of spirals for compact sources. With this preliminary version of ArTeMiS, we concluded that the mapping speed is already more than 5 times better than the previous 350 microns instrument at APEX. The median NEFD at 350 microns is 600 mJy.s1/2, with best values at 300 mJy.s1/2. The complete instrument with 5760 pixels and optimized settings will be installed during the first half of 2015.
DOI:10.48550/arxiv.1407.2545