rest frame
The LOFAR Two-metre Sky Survey. IV. First Data Release: Photometric redshifts and rest-frame magnitudes
... nous quasars with problematic high equivalent width (EW) emission lines) will produce poor results for the other pop- ulations. Furthermore, in many cases we do not necessarily know a priori the nature of a given radio ...
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The SCUBA 2 cosmology legacy survey: ALMA resolves the rest frame far infrared emission of sub millemeter galaxies
... Nearly 20 years after their discovery, there is still debate about the nature of the population of luminous, but highly dust- obscured sources detected at high redshifts in sub-millimeter and millimeter surveys. The ...
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On the nature and physical conditions of the luminous Lyα emitter CR7 and its rest frame UV components
... z = 6.606. We do not detect any line above 3 σ, but find a potential emission line just below the 3 σ level ( ∼ 2.5 − 2.9 σ) in OB3. We find it in the VIS arm (showing the negatives from offsetting along the slit; see ...
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Discovery of a Rich Cluster at z = 1.63 Using the Rest-frame 1.6 μm ''Stellar Bump Sequence'' Method
... Photometric redshifts for galaxies are typically determined by fitting the observed colors of galaxies with a range of templates for galaxy spectra. The features in galaxy spectral energy distributions (SEDs) that ...
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On the nature and physical conditions of the luminous Lyα emitter CR7 and its rest frame UV components
... CR7 has previously been discussed as being powered by very low metallicity stars (PopIII-like; Sobral et al. 2015; Visbal et al. 2016), as a candidate for being a DCBH (e.g. Sobral et al. 2015; Pallottini et al. 2015; ...
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Evidence for Non-stellar Rest-frame Near-IR Emission Associated with Increased Star Formation in Galaxies at z ~ 1
... We explore the presence of non-stellar rest-frame near-IR (2 − 5 µm) emission in galaxies at z ∼ 1. Previous studies identified this excess in relatively small samples and suggested that such non-stellar ...
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Improving SN Ia Distance Measurements Through Better Understanding of SN Ia Systematic Uncertainties
... side. Rest-frame UV response functions are more variable from telescope to telescope than in the other bands, making the accurate characterization of the UV filter response function even more ...observer ...
161
The de Broglie Wave as Evidence of a Deeper Wave Structure
... However, it has been assumed in quantum mechanics, both in its standard form and in its many reinterpretations, as it was by de Broglie and Schrödinger, that the de Broglie wave is a wave in its own right. How the de ...
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The Stellar Mass Structure of Massive Galaxies from z = 0 to z = 2.5: Surface Density Profiles and Half-mass Radii
... measure rest-frame optical light of z ∼ 2 galaxies at a resolution approaching that of the ...though rest-frame optical light is a better tracer of stellar mass than rest-frame ...
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Dispersion of low frequency plasma waves upstream of the quasi-perpendicular terrestrial bow shock
... wave vector in Eq. (1). The full wave vector can then recon- structed which allows the transformation from frequencies in the spacecraft frame to the plasma rest frame. This relation- ship can be ...
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An Evolutionary Model for Submillimeter Galaxies
... the rest-frame, as the clustering properties and relative frac- tion in the AGN demarcated region can then be directly correlated with dynamical properties of these galaxies, such as the relative amount of ...
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The Strong Gravitationally Lensed Herschel Galaxy HLock01:Optical Spectroscopy Reveals a Close Galaxy Merger with Evidence of Inflowing Gas
... Whatever the mechanisms responsible for such extremely large SFRs are, this active phase of SMGs is a clear indica- tion of intense ionizing flux from a young, massive stellar population that dominates the ...
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Ultra-deep K_S-band Imaging of the Hubble Frontier Fields
... the rest-frame optical emission of galaxies in the fi rst billion years of cosmic history, deep sub-arcsecond resolution imaging at these wavelengths will not be available until the launch of the James Webb ...
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Statistical Study of the Properties of Magnetosheath Lion Roars
... The majority of the studies have observed few cases of LRs with � kV < 45 ∘ . Wilson et al. (2013) reported no observations of whistler waves with such angles, Moullard et al. (1998) reported an average 70 ∘ , and ...
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Is the kinematics of special relativity incomplete?
... absolute rest frame of SMS to be possible basi- ...of rest to the one of motion being identical to its inverse in accord with ...the rest frame in a full ...receiver’s rest ...
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High-resolution confirmation of an extended helium atmosphere around WASP-107b
... stellar rest frame by accounting for the barycentric Earth radial velocity, the stellar reflex motion of the star and its systemic velocity (Table ...
7
The Dynamic Universe – Space as a Spherically Closed Energy System
... In present practice, the observed bolometric magnitudes are corrected with K-correction, which is said to return the observed magnitudes to the emitter’s rest frame. Originally, the K-correction was used ...
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The Strong Gravitationally Lensed Herschel Galaxy HLock01:Optical Spectroscopy Reveals a Close Galaxy Merger with Evidence of Inflowing Gas
... Whatever the mechanisms responsible for such extremely large SFRs are, this active phase of SMGs is a clear indication of intense ionizing fl ux from a young, massive stellar population that dominates the ...
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The Relation between Dynamical Mass-to-light Ratio and Color for Massive Quiescent Galaxies out to z ~ 2 and Comparison with Stellar Population Synthesis Models
... and rest-frame color, assessing SPS models, and con- straining the ...radii, rest-frame fluxes, and stellar population ...the rest-frame color over a large dynamic range for ...
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Vector Meson Photoproduction with a Linearly Polarized Beam
... The paper is organized as follows. In Section II, we define the Regge amplitudes and discuss model param- eters. In Section III, we discuss the fitting procedure. Specifically, we first isolate the unnatural exchanges in ...
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