Add to ORKGThere has been considerable recent interest in the properties of infrared galaxies due to the discovery by the Infrared Astronomical Satellite (IRAS) of a class of luminous galaxies which emit the bulk of their energy in the far-infrared (Houck et al. 1984; Soifer et al. 1984). Ground-based studies of these infrared luminous galaxies have shown that they are a substantial component of the local universe (z ~ 0.1) with a space density at luminosities above 1011 L⊙ (H_o = 75 km s^(-1)Mpc^(-1)) exceeding that of Seyfert galaxies and quasars (Soifer et al. 1986)
Ground-based observations of the object IRAS 14348-1447, which was discovered with the Infrared Astr...
We present Herschel far-IR photometry and spectroscopy as well as ground-based CO observations of a...
The IRAS survey of the local universe has revealed the existence of a class of ultraluminous infrare...
There has been considerable recent interest in the properties of infrared galaxies due to the discov...
Results from a study of the far infrared properties of the brightest galaxies in the IRAS survey are...
The local space density of galaxies with 60 μm luminosity greater than VL_v (60 μm) ≳ 10^(10) L_☉ is...
The Infrared Astronomical Satellite (IRAS) has discovered a class of ultraluminous infrared galaxies...
In this paper, we examine the contribution of galaxies with different infrared (IR) spectral energy ...
We present evidence that the mid infrared (MIR, rest frame 5–30 μm) is a good tracer of the total in...
IRAS discovered a class of objects which emit most of their radiation at infrared wavelengths and wh...
The IRAS survey gives an unbiased view of the infrared properties of the active galaxies. Seyfert ga...
Ph.D. University of Hawaii at Manoa 2012.Includes bibliographical references.We present the kinemati...
Seven very luminous galaxies were examined to determine the contribution of active nuclei to their l...
IRAS observations of extragalactic objects are analyzed, supplemented by optical spectroscopy and 10...
The 60 µm selected IRAS Bright Galaxy Sample is used as a starting point to derive additional comple...
Ground-based observations of the object IRAS 14348-1447, which was discovered with the Infrared Astr...
We present Herschel far-IR photometry and spectroscopy as well as ground-based CO observations of a...
The IRAS survey of the local universe has revealed the existence of a class of ultraluminous infrare...
There has been considerable recent interest in the properties of infrared galaxies due to the discov...
Results from a study of the far infrared properties of the brightest galaxies in the IRAS survey are...
The local space density of galaxies with 60 μm luminosity greater than VL_v (60 μm) ≳ 10^(10) L_☉ is...
The Infrared Astronomical Satellite (IRAS) has discovered a class of ultraluminous infrared galaxies...
In this paper, we examine the contribution of galaxies with different infrared (IR) spectral energy ...
We present evidence that the mid infrared (MIR, rest frame 5–30 μm) is a good tracer of the total in...
IRAS discovered a class of objects which emit most of their radiation at infrared wavelengths and wh...
The IRAS survey gives an unbiased view of the infrared properties of the active galaxies. Seyfert ga...
Ph.D. University of Hawaii at Manoa 2012.Includes bibliographical references.We present the kinemati...
Seven very luminous galaxies were examined to determine the contribution of active nuclei to their l...
IRAS observations of extragalactic objects are analyzed, supplemented by optical spectroscopy and 10...
The 60 µm selected IRAS Bright Galaxy Sample is used as a starting point to derive additional comple...
Ground-based observations of the object IRAS 14348-1447, which was discovered with the Infrared Astr...
We present Herschel far-IR photometry and spectroscopy as well as ground-based CO observations of a...
The IRAS survey of the local universe has revealed the existence of a class of ultraluminous infrare...