SAGE-Spec ID Search

The life-cycle of dust and gas in the Large Magellanic Cloud (SAGE-Spec) is the spectroscopic follow-up to the SAGE-LMC Spitzer Legacy program that mapped the LMC with IRAC and MIPS. The acronym SAGE stands for Surveying the Agents of Galaxy Evolution, and thus the project aims to make an inventory of the budget of gas and dust involved in the life-cycle of matter in the Magellanic Clouds.
This dataset or service is made available by the Infrared Science Archive (IRSA) at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.