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18 results with keyword: 'the stellar mass content of submillimeter selected galaxies'

The stellar mass content of submillimeter-selected galaxies.

The median of the stellar absolute H magnitude determined in this way for the z > 1.5 SMGs in our sample, including the upper limits for galaxies which had fewer than

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Volume 03  Issue 02  (2015)  Feb. 2015

Unlike previous studies on leadership and development in Nigeria, which have observed that the system has been rendered unproductive by poor leadership, this article argues that

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PORT OF SEATTLE MEMORANDUM. COMMISSION AGENDA Item No. 4d ACTION ITEM Date of Meeting September 8, 2015

GPM is a variation of Integrated Pest Management (IPM) with the goal to use fewer resources and chemicals using IPM practices. IPM focuses on pest prevention by eliminating

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Revealing the stellar mass and dust distributions of submillimeter galaxies at Redshift 2.

Taking the dust emission as a proxy for dust-obscured star formation in our sources, our results imply that the SMG population at high redshift exhibits centrally concentrated

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Revealing the Stellar Mass and Dust Distributions of Submillimeter Galaxies at Redshift 2

We assume a burst timescale of 150 Myr, although note that this gives a conservative estimate since typical burst timescales of SMGs are estimated to be around 100 Myr (e.g., Simpson

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Our Range of Engine Oils

Castrol EDGE is Castrol’s premium, most advanced range of synthetic Engine Oils designed to meet the needs.. of newer, more technologically

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A blackboard architecture for a rule-based SQL optimiser

The search strategy and cost model enabled early selection o f promising alternatives thus enhancing optimiser efficiency and quality of QEPs produced. A number o

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2019
Private Wealth Management Trust & Estate Insights

interests in a closely held business) may be subject to "valuation discounts" for gift tax purposes, using less exemption than if the whole business was transferred at

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HIghMass-High H i Mass, H i-rich Galaxies at z ~ 0: Combined H i and H2 Observations

Typical  H 2 SFEs compared with two optically selected samples: the local spiral galaxies of THINGS and COLD GASS galaxies of similar stellar mass. This comparison holds for

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Linking galaxies to dark matter halos at z ~ 1 : dependence of galaxy clustering on stellar mass and specific star formation rate.

Splitting the selected galaxies at different stellar mass thresholds, we measured the angular two-point correla- tion function and performed the halo modeling to link galaxies with

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Multi Wavelength Properties of Submillimeter Selected Galaxies

6.1 Fits of Different Star Formation History Models to the SED of a Low- z SMG 153 6.2 Fits of Different Star Formation History Models to the SED of a High- z SMG 154 6.3

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Campomanesia velutina leaves extracts exert hypouricemic effects through inhibition of xanthine oxidase and ameliorate inflammatory response triggered by MSU crystals

This way, aqueous and ethanolic extracts from Campomanesia velutina leaves can act over crucial points of gout management: decrease uric acid serum lev- els by inhibiting

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Dark Energy Survey identification of a low-mass active galactic nucleus at redshift 0.823 from optical variability

Black hole mass versus host-galaxy total stellar mass for DES J0218 − 0430 in comparison to X-ray selected intermediate-redshift AGNs and local samples of AGNs and inactive

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arxiv: v1 [astro-ph.co] 23 Jul 2010

The relation between stellar mass, Hubble type or stellar bar, and the H I content of galaxies as a function of look-back time can all be explored using both direct detections

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The VLT LEGA C spectroscopic survey : the physics of galaxies at a lookback time of 7 Gyr

Furthermore, the underlying relationships between the stellar content of galaxies and their mass, ongoing star formation, internal structure, environment, and nuclear activity can

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Compact groups of galaxies selected by stellar mass: the 2MASS compact group catalogue

Distributions of observable properties for the CGs identified in projection in the 2MASS XSC: number of members in the CG ( top-left panel ), percentage of members with

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Simulating galaxies in the reionization era with FIRE-2: galaxy scaling relations, stellar mass functions, and luminosity functions

Bottom: The stellar mass–magnitude relation for the same bands and redshifts. At fixed magnitude, the distribution of stellar mass is skewed towards low-mass galaxies, simply due to

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