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Confronting predictions of the galaxy stellar mass function with
Confronting predictions of the galaxy stellar mass function with

A dozen new galaxies caught in the act: Gas stripping and extended
A dozen new galaxies caught in the act: Gas stripping and extended

... designed for observing Hα emitting objects in the Coma cluster at z=0.0225, and has bell-shaped transmission with a central wavelength of 6712 Å and FWHM of 120 Å (Yagi et al. 2007; ...
Sub-luminous type Ia supernovae from the mergers of equal
Sub-luminous type Ia supernovae from the mergers of equal

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erice_091014 - Astronomy & Astrophysics Group

... Already detectable by largest radio telescopes, out to few x 100 Mpc. Observable with SKA to cosmological distances. ...
PPt 19-2
PPt 19-2

... • A straight line drawn perpendicular to the center of a concave or convex mirror is called the optical axis. • Light rays that travel parallel to the optical axis and strike the mirror are reflected so that they pass through a single point of the optical axis called the focal point. • The distance ...
Merger of binary neutron stars with realistic equations of state in full
Merger of binary neutron stars with realistic equations of state in full

... the pressure and the internal energy associated with the finite thermal energy (temperature) are not still as large as those of the cold part. From this reason, we adopt a hybrid equation of state in which the finite-temperature part generated by shocks is added as a correction using a simple prescr ...
FOURTH MIDTERM - REVIEW PROBLEMS Physics 2220 Fall 2010 George Williams
FOURTH MIDTERM - REVIEW PROBLEMS Physics 2220 Fall 2010 George Williams

... refracted ray (measured from the normal) emerging from the prism at surface (A). Find the minimum angle of incidence to the base where the beam is totally internally reflected at surface (A). Find the face, (A), (B) or (C), and angle that the beam in (b) emerges from the prism. ...
Pan-Planets: Searching for hot Jupiters around cool dwarfs⋆
Pan-Planets: Searching for hot Jupiters around cool dwarfs⋆

EBL - UCSC Physics - University of California, Santa Cruz
EBL - UCSC Physics - University of California, Santa Cruz

... Joel Primack & Alberto Domínguez Data from (non-) attenuation of gamma rays from blazars and gamma ray bursts (GRBs) give upper limits on the EBL from the UV to the mid-IR that are only a little above the lower limits from observed galaxies. New data on attenuation of gamma rays from blazers now lea ...
gwpaw - DCC
gwpaw - DCC

... Deriving the significance of an event should be determined by both the sensitivity of a search and its estimated background FAD/Productivity allows for combination of multiple searches for the same source, regardless of data epoch and relative ...
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The significant contribution of minor mergers to the cosmic star

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Michelson Morley Experiment

... considering the Doppler Effect. It needs no over-emphasis that Doppler Effect had to be taken into consideration before drawing any conclusion. Now then if it is shown that notwithstanding the differences in the distances and time taken by the light pulses in traversing the two arms of the experimen ...
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Article PDF - IOPscience

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A Tale of Two Physics

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The UV properties of E+ A galaxies: constraints on feedback

ellc: A fast, flexible light curve model for detached eclipsing binary
ellc: A fast, flexible light curve model for detached eclipsing binary

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Enhancement of sensitivity and bandwidth of gravitational wave detectors using... based white light cavities
Enhancement of sensitivity and bandwidth of gravitational wave detectors using... based white light cavities

... are expected to be separated generally by less than a few kilohertz, and in some cases by only tens or hundreds of hertz, from the carrier frequency. These sidebands, then, cannot be separated out from the carrier by means of the usual techniques for filtering light. Prisms and diffraction gratings ...
Combined MASS-DIMM instrument for atmospheric turbulence studies
Combined MASS-DIMM instrument for atmospheric turbulence studies

... A standard DIMM instrument uses only two pieces of the telescope’s aperture, while the remaining portion could serve for the MASS channel. A study of the optimum aperture size (Tokovinin et al. 2003a) has shown that an outer diameter of the 4 concentric MASS apertures can be as small as 8–9 cm. Such ...
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ASTR 610 Theory of Galaxy Formation

The Efficacy of Light Therapy in the Treatment of Mood Disorders: A
The Efficacy of Light Therapy in the Treatment of Mood Disorders: A

... treatment dose (lux by time) for the experimental bright light treatment intervention was complicated by the absence of an accepted standard definition of adequate dosing. In some studies, we found that the “placebo condition” consisted of light exposure that was greater than that for the “active co ...
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SOME CONSTRAINTS ON GALAXY EVOLUTION IMPOSED BY

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stochastic star formation and a (nearly) uniform stellar
stochastic star formation and a (nearly) uniform stellar

... galaxy SFR. The IGIMF implementation follows the minimal-1 and minimal-2 formulations (Pflamm-Altenburg et al. 2007), with a Kroupa (2001) IMF and a CMF with β = 2, minimum mass of 20 M and maximum mass derived from the SFR averaged over 107 yr. In both the Kroupa fc = 1 and the IGIMF model, the IM ...
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