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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 ...
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 of dwarfs。
Chandra monitoring observation of the antennae Galaxies:the x-ray source populations and the shape of Their luminosity function
The Pulsar Luminosity Function     Pulsar  Luminosity Function       font style='font-size:12px;'> 2009/6/16
The Pulsar Luminosity Function
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...

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