IRS spectra of two ultraluminous infrared galaxies at z=1.3

We present low-resolution (64 < R < 124) mid-infrared (8-38 mu m) spectra of two z approximate to 1:3 ultraluminous infrared galaxies (ULIRGs) with L-8-1000 mu m approximate to 10(13)L circle dot. The spectra were taken with the Infrared Spectrograph(IRS) on board the Spitzer Space Telescope. Both objects were discovered in the NOAO Deep Wide-Field Survey (NDWFS) Bootes field. MIPS J142824.0+352619 is a bright 160 mu m source with a large infrared- to-optical flux density ratio. Previous authors provided evidence for a foreground lens and estimated an amplification of <= 10, although this factor is currently poorly constrained. The 6.2, 7.7, 11.3, and 12.8 mu m polycyclic aromatic hydrocarbon (PAH) emission bands in its IRS spectrum indicate a redshift of z approximate to 1.3. The large equivalent width of the 6.2 mu m PAH feature indicates that at least 50% of the mid-infrared energy is generated in a starburst, an interpretation supported by a large [Ne II]/[Ne III] ratio and a low upper limit on the X-ray luminosity. SST24 J142827.19+354127.71 has the brightest 24 mu m flux (10.55 mJy) among optically faint (R > 20) galaxies in the NDWFS. Its mid- infrared spectrum lacks emission features, but the broad 9.7 mu m silicate absorption band places this source at z approximate to 1.3. Optical spectroscopy confirms a redshift of z = 1:293 +/- 0:001. Given this redshift, SST24 J142827.19+354127.71 has among the largest rest-frame 5 mu m luminosities known. The similarity of its SED to those of known AGN-dominated ULIRGs and its lack of either PAH features or large amounts of cool dust indicate that the mid- infrared emission is dominated by an AGN rather than a starburst.