Mid - infrared spectroscopy of two luminous submillimeter galaxies at z ∼ 2 . 8

نویسندگان

  • D. Lutz
  • E. Valiante
  • E. Sturm
  • R. Genzel
  • L. J. Tacconi
  • M. D. Lehnert
  • A. Sternberg
  • A. J. Baker
چکیده

Using the Infrared Spectrograph (IRS) on board the Spitzer Space Telescope, we have obtained rest frame mid-infrared spectroscopy of two bright submillime-ter galaxies. SMMJ02399-0136 at z=2.81 shows a superposition of PAH emission features and a mid-infrared continuum, indicating significant and roughly equal contributions to its bolometric luminosity from star formation and from a Compton-thick AGN. We derive a new redshift of z=2.80 for MMJ154127+6616 from the IRS spectrum and find this object is dominated by starburst PAH emission. The rest frame mid-to far-infrared spectral energy distributions are consistent with these submillimeter galaxies being scaled up versions of local ultraluminous infrared galaxies. The mid-infrared spectra support the scenario that submillimeter galaxies are sites of extreme star formation and represent a key phase in the formation of massive galaxies.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

SPITZER MID-INFRARED SPECTROSCOPY OF INFRARED LUMINOUS GALAXIES AT z 2. I. THE SPECTRA

We present the mid-infrared spectra obtained with the Spitzer IRS for 52 sources, selected as infrared luminous, zk1 candidates in the Extragalactic First Look Survey. The sample selection criteria are f24 mk 0:9 mJy, f (24 m)/ f (8 m)k 3:16, and f (24 m)/ f (0:7 m)k10. Of the 52 spectra, 47 (90%) produced measurable redshifts based solely on the mid-IR spectral features, with 35/47 (74%) at 1:...

متن کامل

A mid - infrared spectroscopic study of submillimeter galaxies : luminous starbursts at high redshift

We present rest frame mid-infrared spectroscopy of a sample of 13 submillime-ter galaxies, obtained using the Infrared Spectrograph (IRS) on board the Spitzer Space Telescope. The sample includes exclusively bright objects from blank fields and cluster lens assisted surveys that have accurate interferometric positions. We find that the majority of spectra are well fitted by a starburst template...

متن کامل

OPTICALLY FAINT COUNTERPARTS TO THE ISO-FIRBACK 170μm POPULATION: THE DISCOVERY OF COLD, LUMINOUS GALAXIES AT HIGH REDSHIFT

We present Keck spectroscopy and UKIRT near-IR imaging observations of two 170μm-selected sources from the ISO-FIRBACK survey which have faint counterparts in the optical, and r − K ∼ 5. Both sources were expected to lie at z > 1 based on their far-infrared, submillimeter and radio fluxes, assuming a similar spectral energy distribution to the local ultra-luminous infrared galaxy (ULIRG) Arp 22...

متن کامل

Spitzer Detection of PAH and Silicate Dust Features in the Mid - Infrared Spectra of z ∼ 2 Ultraluminous Infrared

We report the initial results from a Spitzer GO-1 program to obtain low resolution, mid-infrared spectra of infrared luminous galaxies at z ∼ 1 − 2. This paper presents the spectra of eight sources observed with the Spitzer InfraRed Spectrograph (IRS). Of the eight spectra, six have mid-IR spectral features, either emission from Polycyclic Aromatic Hydrocarbon (PAH) or silicate absorption. Base...

متن کامل

Mid-infrared Identification of Faint Submillimeter Sources

Faint submillimeter sources detected with the Submillimeter Common-User Bolometer Array on the James Clerk Maxwell Telescope have faced an identification problem due to the telescope’s broad beam profile. Here we propose a new method to identify such submillimeter sources with a mid-infrared image having a finer point spread function. The Infrared Space Observatory has provided a very deep 6.7μ...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2005