We used the Spitzer Infrared Spectrograph (IRS) to study the mid-IR properties and investigate the energetics of 24 Submillimeter Galaxies (SMGs). This is the largest sample of SMGs observed with Spitzer IRS and covers the full extent of properties of the radio-identified population of SMGs in the redshift range of z ~ 0.65-3.2. We observe broad emission features from polycyclic aromatic hydrocarbons in more than 80% of our sample. We find that the median mid-IR spectrum is well described by a starburst component with an additional power law, F ν ~ ν-2, likely representing a <32% contribution from an active galactic nucleus to the bolometric luminosity. Our results thus confirm that starburst activity dominates the bolometric luminosity in ...
The Herschel Lensing Survey (HLS) takes advantage of gravitational lensing by massive galaxy cluster...
We present deep mid-IR spectroscopy with Spitzer of 13 SMGs in the GOODS-N field.We find strong PAH ...
Submillimeter galaxies (SMGs) at $z\gtrsim 1$ are luminous in the far-infrared, and have star format...
We used the Spitzer Infrared Spectrograph (IRS) to study the mid-IR properties and investigate the e...
We present Spitzer-IRAC and MIPS mid-IR observations of a sample of 73 radio-detected submillimeter-...
Spitzer spectroscopy has revealed that sime80% of submm galaxies (SMGs) are starburst (SB)-dominated...
We present mid-infrared spectra of five submillimeter galaxies at z = 0.65-2.38 taken with the Spitz...
We present Spitzer-IRAC and MIPS mid-IR observations of a sample of 73 radio-detected submillimeter-...
We present rest frame mid-infrared spectroscopy of a sample of 13 submillimeter galaxies, obtained u...
We present mid-infrared spectra of 5 submm galaxies at redshifts z=0.65-2.38 taken with the Spitzer ...
We present mid-infrared spectra of 5 submmillimeter galaxies at redshifts z = 0.65 − 2.38 taken with...
Spitzer spectroscopy has revealed that ≃80% of submm galaxies (SMGs) are starburst (SB)-dominated in...
By using data from the Atacama Large Millimeter/submillimeter Array and near-infrared (NIR) integral...
This thesis presents a comprehensive study of high redshift submillimetre galaxies (SMGs) using the ...
We present the first integral-field spectroscopic observations of high-redshift submillimeter-select...
The Herschel Lensing Survey (HLS) takes advantage of gravitational lensing by massive galaxy cluster...
We present deep mid-IR spectroscopy with Spitzer of 13 SMGs in the GOODS-N field.We find strong PAH ...
Submillimeter galaxies (SMGs) at $z\gtrsim 1$ are luminous in the far-infrared, and have star format...
We used the Spitzer Infrared Spectrograph (IRS) to study the mid-IR properties and investigate the e...
We present Spitzer-IRAC and MIPS mid-IR observations of a sample of 73 radio-detected submillimeter-...
Spitzer spectroscopy has revealed that sime80% of submm galaxies (SMGs) are starburst (SB)-dominated...
We present mid-infrared spectra of five submillimeter galaxies at z = 0.65-2.38 taken with the Spitz...
We present Spitzer-IRAC and MIPS mid-IR observations of a sample of 73 radio-detected submillimeter-...
We present rest frame mid-infrared spectroscopy of a sample of 13 submillimeter galaxies, obtained u...
We present mid-infrared spectra of 5 submm galaxies at redshifts z=0.65-2.38 taken with the Spitzer ...
We present mid-infrared spectra of 5 submmillimeter galaxies at redshifts z = 0.65 − 2.38 taken with...
Spitzer spectroscopy has revealed that ≃80% of submm galaxies (SMGs) are starburst (SB)-dominated in...
By using data from the Atacama Large Millimeter/submillimeter Array and near-infrared (NIR) integral...
This thesis presents a comprehensive study of high redshift submillimetre galaxies (SMGs) using the ...
We present the first integral-field spectroscopic observations of high-redshift submillimeter-select...
The Herschel Lensing Survey (HLS) takes advantage of gravitational lensing by massive galaxy cluster...
We present deep mid-IR spectroscopy with Spitzer of 13 SMGs in the GOODS-N field.We find strong PAH ...
Submillimeter galaxies (SMGs) at $z\gtrsim 1$ are luminous in the far-infrared, and have star format...