Derived multi-wavelength parameters for collated galaxies
Multi Wavelength Properties of Submillimeter Selected Galaxies
... fitted parameters is not Gaussian, or (3) the models used do not adequately describe the SEDs of the ...all galaxies, we use only simple star formation histories, and we assume a single extinction model for ...
241
A Multi-Wavelength Study of Luminous Infrared Galaxies across Cosmic Time.
... The IRAS name of each galaxy or galaxy system is shown at the top, along with their common names from optical catalogs. Each of the six panels are matched and have the exact same map center as well as field of view. The ...
608
Linear estimation of particle bulk parameters from multi-wavelength lidar measurements
... properties derived from lidar observa- tions performed in Turkey in May 2010 were ...the multi-wavelength lidar data, for the first time, were inverted into time-height distributions of particle pa- ...
11
Multi-wavelength properties of Type 1 and Type 2 AGN host galaxies in the Chandra-COSMOS legacy survey.
... luminosity derived from the SED fitting with respect to L bol X ray ‐ , where the one-to-one correlation is plotted as a dotted line for ...luminosities derived from the SED fitting are on average slightly ...
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The SCUBA 2 Cosmology Legacy Survey: multi wavelength properties of ALMA identified submillimeter galaxies in UKIDSS UDS
... temperature derived from an optically thin ...the derived dust mass of each SMG, with an increase in the dust temperature resulting in a lower total dust ...
16
Multi-wavelength de-blended Herschel view of the statistical properties of dusty star-forming galaxies across cosmic time
... estimates derived from UV-based studies, we find that the fraction of dust obscured SF activity is at its highest (> 80%) around z ∼ 1 which then decreases towards both low redshift and high ...
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Multi-Wavelength Facets of Galaxy Clusters
... from galaxies that do not lie in the main source ...jected galaxies, we previously showed that the dynamically-derived mass is a robust estimate of log-mean mass at a given observable, in that case ...
240
Multi-Wavelength Surveys of Extreme Infrared Populations
... be derived by a number of observational, numerical and analytical methods that can help to constrain and investigate galaxy formation and evolution ...that galaxies in dense environments lose their wind ...
265
Multi-wavelength study of the G supernova remnant
... The X–ray emission consists of a patchy disk slightly elongated in the south–north direction, dominated by a bar-like emission close but clearly off-set from the geo- metric center. The remnant is not obviously limb ...
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A multi-wavelength census of star formation at redshift z~2
... of galaxies at a given bolometric luminosity changes as function of redshift, a result that may reflect dust enrichment and/or a changing configuration of dust as galaxies ...within galaxies may also ...
295
THE HEISENBERG UNCERTAINTY RELATION DERIVED BY MULTIPLYING MATTER WAVELENGTH AND LIGHT WAVELENGTH
... In practice, E k can be calculated from the momentum through the formula E k = p 2 /2m not from the frequency through the formula E k = hν. In the wave function, ν goes to phase angle, ν = E k /h or ν = 2E k /h would not ...
9
The SCUBA-2 Cosmology Legacy Survey : multi-wavelength properties of ALMA-identified submillimeter galaxies in UKIDSS UDS.
... the multi-wavelength coverage of our ALMA-identi fied SMGs and our SED-fitting procedures before discussing the multi-wavelength properties of these SMGs in Section ...
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The coronal parameters of local Seyfert galaxies
... In a number of observations NuSTAR operated simulta- neously with XMM-Newton and Swift. The spectral resolu- tion around the iron line complex (5–10 keV) of these low- energy detectors has been paired with the ...
6
Collated by Dana Jorgensen
... target number (20 + 5 per point of LUCK spent above the first); if the skill roll succeeds, a bonus point of LUCK is thrown into the roll. a target number of 30, and if he succeeds h[r] ...
10
Multi-wavelength studies of pulsars and their companions
... We scanned a grid of models covering effective temperatures from T eff = 8000 to 25000 K with a step-size of 250 K and surface gravities ranging from log g = 5.00 to log g = 8.00 with a step-size of 0.25 dex. At each ...
168
A cosmic perspective: Multi-wavelength astrophysics
... Using multi- wavelength observations and computer simulations, astronomers have deduced that Centaurus A is the result of a violent gravitational collision and then merger between two different ...two ...
6
Stellar Populations in Compact Galaxy Groups: a Multi-wavelength Study of HCGs 16, 22, and 42, Their Star Clusters, and Dwarf Galaxies
... a multi-wavelength analysis of three compact galaxy groups, Hickson compact groups (HCGs) 16, 22, and 42, which describe a sequence in terms of gas richness, from space- (Swift, Hubble Space Telescope ...
18
Fiber Optical Parametric Oscillator with Switchable and Wavelength-Spacing Tunable Multi-Wavelength
... The wavelength spacing of the proposed MW-FOPO can be tuned by adjusting the wavelength of the pump light or the central wavelength of the FBG at the two multi-wavelength lasing ...
10
Exploiting multi-wavelength aerosol absorption coefficients in a multi-time resolution source apportionment study to retrieve source-dependent absorption parameters
... optical parameters; for example, in contrast to the more traditional approach used by optical source apportionment models, here we obtained source-dependent α values without any a priori assumption (α biomass ...
18
The phase-space parameters of the brightest halo galaxies
... cluster galaxies to argue that cDs are at rest with respect to the ...brightest galaxies in dark matter haloes are located at rest at the centre of their potential ...halo galaxies are clearly ...
13