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IDENTIFICATION OF A COMPLETE 160 μm FLUX-LIMITED SAMPLE OF INFRARED GALAXIES IN THE ISO LOCKMAN HOLE 1 deg2 DEEP FIELDS: SOURCE PROPERTIES AND EVIDENCE FOR STRONG EVOLUTION IN THE FIR LUMINOSITY FUNCTION FOR ULIRGs
starburst-active galactic nucleus (AGN) composite AGN spectral types
2014/12/20
We have identified a complete, flux-limited (S 160>120 mJy) sample of 160 μm selected sources from Spitzer observations of the 1 deg2 Infrared Space Observatory (ISO) Deep Field region in the Lockman ...
An optical study of the faint end of the stellar luminosity function
Stars Photometric functions Multicolor metering Height of fuzzy Projection Molecular cloud
2014/12/9
We implement a new method by which to study the faint end of the field star luminosity function. The method relies on deep, multicolor photometry of fields projected against highly obscured, nearby mo...
Stellar populations in the calán-eso catalogue. The luminosity function and kinematics
Stellar populations luminosity function calán-eso catalogue
2009/6/25
Stellar populations in the calán-eso catalogue. The luminosity function and kinematics
of dwarfs。
Chandra monitoring observation of the antennae Galaxies：the x-ray source populations and the shape of Their luminosity function
antennae Galaxies luminosity function x-ray source
2009/6/17
Chandra monitoring observation of the antennae Galaxies：the x-ray source populations and the shape of Their luminosity function。
The Pulsar Luminosity Function。
Eegular Articles Galaxy Luminosity Function: A New Analytic Expression
a new analytic approximation the luminosity function of galaxies the Schechter function
2010/10/19
We propose a new analytic approximation for the luminosity function of galaxies. The suggested expression behaves like the Schechter function at the faint end (φ ∼ Lα) but departs considerably a...