SMC-Last Mosaic Images
arXiv:2210.10874 · doi:10.1088/1538-3873/ac8a18
Abstract
We present mosaic images of the Small Magellanic Cloud (SMC) observed with the Spitzer IRAC 3.6 m and 4.5 m bands over two epochs, 2017 August 25 to 2017 September 13, and 2017 November 24 to 2018 February 12. The survey region comprises 30 square degrees covering the SMC and the Bridge to the Large Magellanic Cloud. The region is covered by 52 1111 tiles, with each tile including images in each band for both separate and combined epochs. The mosaics are made in individual tangent projections in J2000 coordinates. The angular pixel size is 06 with a resolution (FWHM) of 20. We describe processing to correct or mitigate residual artifacts and remove background discontinuities. The mosaic images are publicly available at the Infrared Science Archive (IRSA).
29 pages, 20 figures. Mosaics are available via the Dataverse (https://doi.org/10.7910/DVN/EF4QKP) and will be available at IRSA
References in corpus (6)
- Initial Performance of the NEOWISE Reactivation Mission
- Clustering of Local Group distances: publication bias or correlated measurements? III. The Small Magellanic Cloud
- Luminosities and mass-loss rates of Local Group AGB stars and Red Supergiants
- Photometry using the Infrared Array Camera on the Spitzer Space Telescope
- The VMC survey -- XXXIX: Mapping metallicity trends in the Small Magellanic Cloud using near-infrared passbands
- The effects of cosmic rays and solar flares on the IRAC detectors: the first two years of in-flight operation