Follow-up NIR spectroscopy of ULIRGs observed by ISO
ASTR SOC P 381 (2008) 275-278
Abstract:
We discuss low resolution near-infrared spectroscopy of an unbiased sample of 24 ultraluminous infrared galaxies (ULIRGs), selected from samples previously observed in the mid-infrared with ISO. Qualitatively, the NIR spectra of our 24 ULIRGs resemble those of starbursts. The spectroscopic classification in the NIR is in very good agreement with the MIR. For a subset of our sample for which extinction corrections can be derived from Pace and Br gamma, we find rather high Pa alpha luminosities, in accordance with the powering source of these galaxies being star formation. Furthermore, we identified two unusual objects, the first exhibiting extreme [FeII] emission and the second strong emission in H-2 rotation-vibration emission.Galactic Bulges and Inner Disks, as Seen by SAURON
FORMATION AND EVOLUTION OF GALAXY DISKS 396 (2008) 81-+
IRAC photometric analysis and the mid-IR photometric properties of Lyman-break galaxies
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 386:1 (2008) 11-21
Identifying Gravitationally Inspiraling Black Hole Binaries Using their Variable Electromagnetic Emission
PANORAMIC VIEWS OF GALAXY FORMATION AND EVOLUTION, PROCEEDINGS 399 (2008) 20-27
Improvements in the Residual OH Emission Removal in SINFONI Pipeline Spectra
ESO Astrophysics Symposia Springer Nature (2008) 443-446