This project is used to calculate flux level (uJy) at Signal-Noise-Ratio = 5 for faint objects in Spitzer IRAC images. Using IDL we simulate faint objects with IRAC PRF around target position in a grid manner, which could be a possible magnetar.

An IDL tool to coadd and extract low-resolution IRS spectra taken with the Spitzer telescope (Fadda et al. 2010 ApJ 719:425)