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1
Extremely Red Objects in The Lockman Hole
Published 2004“…We find 17% of all galaxies detected by IRAC at 3.6 or 4.5 micron to be EROs. These percentages rise to about 40% at 5.8 micron, and about 60% at 8.0 micron. …”
Journal article -
2
Infrared power-law galaxies in the Chandra Deep Field South: AGN and ULIRGs
Published 2005“…We investigate the nature of a sample of 92 Spitzer/MIPS 24 micron selected galaxies in the CDFS, showing power law-like emission in the Spitzer/IRAC 3.6-8 micron bands. …”
Journal article -
3
Identification of luminous infrared galaxies at 1
Published 2004“…We present preliminary results on 24micron detections of luminous infrared galaxies at z>1 with the Multiband Imaging Photometer for Spitzer (MIPS). …”
Journal article -
4
Local Luminous Infrared Galaxies. III. Co-evolution of Black Hole Growth and Star Formation Activity?
Published 2013“…We estimate typical BH masses of 3x10^7 M_sun using [NeIII]15.56micron and optical [OIII]5007A gas velocity dispersions and literature stellar velocity dispersions. …”
Journal article -
5
Spitzer/IRS mapping of local luminous infrared galaxies
Published 2010“…The maps cover the central 20"x20" or 30"x 30" regions of the galaxies, and use all four IRS modules to cover the full 5-38 microns spectral range. We have built spectral maps of the main mid-IR emission lines, continuum and PAH features, and extracted 1D spectra for regions of interest in each galaxy. …”
Conference item -
6
Spectral Energy Distributions of type 2 QSOs: obscured star formation at high redshifts
Published 2009“…The submillimetre (850micron) to X-ray (2 keV) spectral indices (alpha_SX) span a wide range. …”
Journal article -
7
The nuclear and extended mid-infrared emission of Seyfert galaxies
Published 2016“…We find that the nuclear MIR emission (the inner ~70 pc) is strongly correlated with the X-ray emission (the harder the X-rays the better the correlation) and with the [O IV] lambda 25.89 micron emission line, indicating that it is AGN-dominated. …”
Journal article -
8
The Host Galaxies and Black Holes of Typical z~0.5-1.4 AGN
Published 2007“…The AGN are selected such that their rest-frame UV to near-IR SEDs are dominated by stellar emission, i.e., they show a prominent 1.6micron bump, thus minimizing the AGN emission 'contamination'. …”
Journal article -
9
A Far-Infrared Spectroscopic Survey of Intermediate Redshift (Ultra) Luminous Infrared Galaxies
Published 2014“…With these measurements we trace the dust continuum, far-IR atomic line emission, in particular [CII]\,157.7microns, as well as the molecular gas of z~0.3 (U)LIRGs and perform a detailed investigation of the interstellar medium of the population. …”
Journal article