Add to ORKGResults from a study of the far infrared properties of the brightest galaxies in the IRAS survey are described. There is a correlation between the infrared luminosity and the infrared to optical luminosity ratio and between the infrared luminosity and the far infrared color temperature in these galaxies. The infrared bright galaxies represent a significant component of extragalactic objects in the local universe, being comparable in space density to the Seyferts, optically identified starburst galaxies, and more numerous than quasars at the same bolometric luminosity. The far infrared luminosity in the local universe is approximately 25% of the starlight output in the same volume
There has been considerable recent interest in the properties of infrared galaxies due to the discov...
We used spectroscopic data from the Sloan Digital Sky Survey (SDSS) and photometric data from the Wi...
Galaxies from the IRAS Bright Galaxy Sample with infrared luminosities L_(IR) ⩾ 10^(11) L⊙ have been...
Results from a study of the far infrared properties of the brightest galaxies in the IRAS survey are...
A complete sample of 324 extragalactic objects with 60 μm flux densities greater than 5.4 Jy has bee...
The local space density of galaxies with 60 μm luminosity greater than VL_v (60 μm) ≳ 10^(10) L_☉ is...
The 60 µm selected IRAS Bright Galaxy Sample is used as a starting point to derive additional comple...
Researchers constructed a volume limited sample of 443 optically selected nearby galaxies from the Z...
The optical and infrared luminosity functions are determined for a 60 micron flux-limited sample of ...
The radio counterparts to the IRAS Redshift Survey galaxies are identified in the NRAO VLA Sky Surve...
Far infrared properties of Starburst galaxies were analyzed using IRAS observations at 25, 60, and 1...
The IRAS survey gives an unbiased view of the infrared properties of the active galaxies. Seyfert ga...
Forty-seven galaxies from the IRAS Bright Galaxy Sample with infrared luminosities L_(IR)⩾ 10^(11) L...
Results are presented from a redshift survey of all 72 galaxies detected by IRAS in Band 3 at flux l...
Pointed IRAS observations and ground based observations are used to determine the infrared propertie...
There has been considerable recent interest in the properties of infrared galaxies due to the discov...
We used spectroscopic data from the Sloan Digital Sky Survey (SDSS) and photometric data from the Wi...
Galaxies from the IRAS Bright Galaxy Sample with infrared luminosities L_(IR) ⩾ 10^(11) L⊙ have been...
Results from a study of the far infrared properties of the brightest galaxies in the IRAS survey are...
A complete sample of 324 extragalactic objects with 60 μm flux densities greater than 5.4 Jy has bee...
The local space density of galaxies with 60 μm luminosity greater than VL_v (60 μm) ≳ 10^(10) L_☉ is...
The 60 µm selected IRAS Bright Galaxy Sample is used as a starting point to derive additional comple...
Researchers constructed a volume limited sample of 443 optically selected nearby galaxies from the Z...
The optical and infrared luminosity functions are determined for a 60 micron flux-limited sample of ...
The radio counterparts to the IRAS Redshift Survey galaxies are identified in the NRAO VLA Sky Surve...
Far infrared properties of Starburst galaxies were analyzed using IRAS observations at 25, 60, and 1...
The IRAS survey gives an unbiased view of the infrared properties of the active galaxies. Seyfert ga...
Forty-seven galaxies from the IRAS Bright Galaxy Sample with infrared luminosities L_(IR)⩾ 10^(11) L...
Results are presented from a redshift survey of all 72 galaxies detected by IRAS in Band 3 at flux l...
Pointed IRAS observations and ground based observations are used to determine the infrared propertie...
There has been considerable recent interest in the properties of infrared galaxies due to the discov...
We used spectroscopic data from the Sloan Digital Sky Survey (SDSS) and photometric data from the Wi...
Galaxies from the IRAS Bright Galaxy Sample with infrared luminosities L_(IR) ⩾ 10^(11) L⊙ have been...