Results 31 to 40 of about 30,122 (121)
Nowadays it is difficult to list all disciplines where stereology is applied, starting from biology and medicine, through materials science, geology and agriculture, up to military systems, biometry, meteorology, geography, physics, astronomy ...
Aneta Gądek-Moszczak
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We study the spatially resolved outflow properties of CSWA13, an intermediate-mass ( M _* = 10 ^9 M _⊙ ), gravitationally lensed star-forming galaxy at z = 1.87.
Keerthi Vasan G. C. +15 more
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Marianna Skórzewska, née Ciecierska (1741–1773), a wealthy noblewoman, wife of General Franciszek Skórzewski, shared her time between Greater Poland (palace at Margonińska Wieś) and Berlin.
Kamila Kłudkiewicz
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In response to recent observations from JWST and Atacama Large Millimeter Array, we explore a new class of dynamically self-consistent models that mimics a plausible progenitor of the Milky Way over a wide range of disk gas fractions, f _gas .
Joss Bland-Hawthorn +10 more
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Aliasing from Galactic Plane Setting in Widefield Radio Interferometry
Measurements with widefield radio interferometers often include the near-infinite gradient between the sky and the horizon. This causes aliasing inherent to the measurement itself and is purely a consequence of the Fourier basis.
N. Barry +4 more
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We explore the properties of interferometric data from high-redshift 21 cm measurements using the Murchison Widefield Array (MWA). These data contain the redshifted 21 cm signal, contamination from continuum foreground sources, and radiometric noise. The
Cathryn M. Trott +31 more
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The Galactic Disk North–South Asymmetry in Metallicity May Be a New Tracer for the Disk Warp
Galactic disk warp has been widely characterized by stellar distributions and stellar kinematics but has not been traced by stellar chemistry. Here, we use a sample with over 170,000 red clump (RC) stars selected from LAMOST and APOGEE first to establish
Weixiang Sun +3 more
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Limits on the 21 cm Power Spectrum at z = 6.5–7.0 from Murchison Widefield Array Observations
This paper presents the spherically averaged 21 cm power spectrum derived from Epoch of Reionization (EoR) observations conducted with the Murchison Widefield Array (MWA). The analysis uses EoR0-field data, centered at (R.A. = 0 h , decl.
C. D. Nunhokee +31 more
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The Kinematic Signature of the Warp and Waves in the Milky Way Disk
Using over 170,000 red clump (RC) stars selected from LAMOST and APOGEE, we conduct a detailed analysis of the stellar V _Z as a function of L _Z (or R _g ) across different ϕ bins for various disk populations.
Weixiang Sun +3 more
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Using nearly 230,000 red clump stars selected from LAMOST and Gaia, we conduct a comprehensive analysis of the stellar age–velocity dispersion relations (AVRs) for various disk populations, within 5.0 ≤ R ≤ 15.0 kpc and ∣ Z ∣ ≤ 3.0 kpc.
Weixiang Sun +3 more
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