Search Results - fixed stars
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Nonrobustness of the carryover effects of small classes in project STAR
Published 2015“…Separately for effective schools, schools other than effective schools, and ineffective schools, the academic achievement of students is regressed on variables indicating small class assignment, along with student characteristics and school-by-entry wave fixed effects. Findings: The carryover effects of CSR are not robust; they are driven mostly by effective schools, which account for at most a quarter of STAR schools. …”
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The relationship between galaxy environment and the quenching of star formation
Published 2019“…In this thesis, we explore the impact of environment on the star formation properties of galaxies across 6.5 Gyrs of cosmic time, corresponding to the redshift range 0.5<z<3.0. …”
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The effect of the environment on the structure, morphology and star-formation history of intermediate-redshift galaxies
Published 2017“…These galaxies have smoother light distributions than their star-forming counterparts. We also find that while almost all field and cluster S0s appear undisturbed, there is a relatively small population of star-forming S0s in clusters but not in the field. …”
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A multifrequency radio continuum study of the Magellanic Clouds - I. Overall structure and star formation rates
Published 2018“…Using a new 150 MHz-Ha relation as a star formation rate indicator, we estimate global star formation rates of 0.068-0.161 M? …”
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SDSS-IV MaNGA: star formation cessation in low-redshift galaxies I: dependence on stellar mass and structural properties
Published 2018“…We have further divided the sample at fixed mass by both bulge-to-total luminosity ratio and morphological type, finding that our conclusions hold regardless of these factors: it appears that the presence of a central dense object is not a driving parameter, but rather a byproduct of the star formation cessation process.…”
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AMI radio continuum observations of young stellar objects with known outflows
Published 2012“…We present 16 GHz (1.9 cm) deep radio continuum observations made with the Arcminute Microkelvin Imager (AMI) of a sample of low-mass young stars driving jets. We combine these new data with archival information from an extensive literature search to examine spectral energy distributions (SEDs) for each source and calculate both the radio and sub-mm spectral indices in two different scenarios: (1) fixing the dust temperature (Td) according to evolutionary class; and (2) allowing Td to vary. …”
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Clumpy galaxies in CANDELS. II. Physical properties of UV-bright clumps at 0.5 ≤ z < 3
Published 2018“…Studying giant star-forming clumps in distant galaxies is important to understand galaxy formation and evolution. …”
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OMEGA - OSIRIS mapping of emission-line galaxies in A901/2: III. - Galaxy properties across projected phase space in A901/2
Published 2017“…However, there remains a reduced fraction of star-forming galaxies in the centres of the clusters at fixed stellar mass, consistent with the star formation–density relation in galaxy clusters. (5) There is no change in specific Hα-derived star formation rates of star-forming galaxies at fixed mass across the cluster environment. …”
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Wideband dynamic radio spectra of two ultra-cool dwarfs
Published 2015“…A number of radio-loud ultra-cool dwarf (UCD ) stars exhibit both continuous broadband and highly polarized pulsed radio emission. …”
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Selective relaying for reliability in power line cooperative communication system
Published 2016“…The topology of the power network (star) poses challenges of attenuation and multipath to high-speed signal transmission. …”
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Development of the portable satellite laser ranging system
Published 2003“…These tests showed that the PSLR system was capable of a ranging accuracy to fixed targets of 8.5 mm with an average accuracy of 23 mm. …”
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Ionized gas discs in elliptical and S0 galaxies at z < 1
Published 2014“…At fixed stellar mass, we also find that ETGs have systematically lower specific star formation rates than spirals. …”
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Black holes and galaxy environment in cosmological simulations
Published 2013“…Fixed aperture measures are sensitive to halo mass and best probe the `large-scale environment' external to a halo. …”
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Essays on political economy, leader demographics and corporate finance: evidence from China
Published 2021“…Our finding shows that the general political connections and the board chair’s political connections are significantly negatively related to firm performance at the highest 1% level (three-star). The CEO’s political connection is also significantly negatively related to firm performance with a significance of 5% level (two-star). …”
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Study of Fractional Differential Equations Emerging in the Theory of Chemical Graphs: A Robust Approach
Published 2022“…The study of the interconnections between chemical systems is known as chemical graph theory. Through the use of star graphs, a limited group of researchers has examined the space of possible solutions for boundary-value problems. …”
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Array-Aided Precise Orbit and Attitude Determination of CubeSats using GNSS
Published 2024“…In the estimation process, multi- and affine-constrained models are used to precisely determine the attitude, and then, highly precise observations for an antenna array are reconstructed based on fixed ambiguities and a decorrelation step. Validations confirm the significance of integer ambiguities in the model, highlighting the cost-effectiveness of this model compared with star trackers for attitude determination. …”
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CEO overseas experiences and corporate financialization: evidence from China
Published 2024“…Recently, Chief Executive Officers (CEOs) with overseas experiences have shown the ―star effect‖, according to upper echelons theory, CEOs’ overseas experiences might relate to corporate financialization, but there is little evidence of whether and how CEOs’ overseas experiences affect it. …”
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A Study of Topology Characteristics on the Real Deployment of Wireless Sensor Networks
Published 2010“…In the case of centralized WSN with star topology, we discovered an interesting finding that the various transmit powers (ranging from 3.2dBm to -17dBm) do not vary the consumed power or in other word, the consumed powers across various transmit powers are almost the same for a given fixed distance value. …”
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