Results 11 to 20 of about 1,426,420 (265)
SPIRE Spectroscopy of Early-type Galaxies [PDF]
The Astrophysical Journal, 2019 Abstract We present Spectral and Photometric Imaging Receiver (SPIRE) spectroscopy for nine early-type galaxies (ETGs) representing the most CO-rich and far-infrared (FIR) bright galaxies of the volume-limited Atlas3D sample. Our data include detections of mid- to high-J CO transitions (J = 4–3 to J = 13–12) and the [C i] (1–0) and (2–1)
Ryen Carl Lapham, Lisa M. Young
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The Galaxy platform for accessible, reproducible and collaborative biomedical analyses: 2022 update. [PDF]
, 2022 Galaxy is a mature, browser accessible workbench for scientific computing. It enables scientists to share, analyze and visualize their own data, with minimal technical impediments.
Galaxy Community,
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Solid-state NMR spectroscopy on complex biomolecules [PDF]
, 2010 Biomolecular applications of NMR spectroscopy are often merely associated with soluble molecules or magnetic resonance imaging. However, since the late 1970s, solid-state NMR (ssNMR) spectroscopy has demonstrated its ability to provide atomic-level ...
NMR Spectroscopy +7 more
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The Astrophysical Journal, 2023 We study the recent star formation histories (SFHs) of 575 intermediate-mass galaxies (IMGs, 10 ^9 ≤ M / M _⊙ ≤ 10 ^10 ) in COSMOS at 0.3 < z < 0.4 by comparing their H α and UV luminosities.
Shannon G. Patel +4 more
doaj +1 more source
Can Cosmological Simulations Reproduce the Spectroscopically Confirmed Galaxies Seen at z ≥ 10?
The Astrophysical Journal Letters, 2023 Recent photometric detections of extreme ( z > 10) redshift galaxies from the JWST have been shown to be in strong tension with existing simulation models for galaxy formation and in the most acute case, in tension with ΛCDM itself.
B. W. Keller +3 more
doaj +1 more source
Characterization of membrane protein function by solid-state NMR spectroscopy [PDF]
, 2014 Membrane proteins are an important class of biological molecules whose association with lipid bilayers and intrinsic molecular mobility can complicate their structural study by high-resolution methods.
Baldus, Marc +3 more
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Galaxy workflow from Galaxy 101 for everyone
, 2021 Galaxy workflow from Galaxy 101 for everyone. This workflow is used in the training "How to reproduce published Galaxy analyses" to learn how to run a published Galaxy ...
Melanie Föll, Anne Fouilloux
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GMASS ultradeep spectroscopy of galaxies atz ~ 2 [PDF]
Astronomy & Astrophysics, 2012 The populations of both quiescent and actively star-forming galaxies at 11.4, called Galaxy Mass Assembly ultra-deep Spectroscopic Survey (GMASS). To determine redshifts and physical properties, such as metallicity, dust content, dynamical masses, and star formation history, we performed ultra-deep spectroscopy with the red-sensitive optical ...
Kurk, J. +14 more
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Size and Spectroscopic Evolution of HectoMAP Quiescent Galaxies
The Astrophysical Journal, 2023 The HectoMAP survey provides a complete, mass-limited sample of 30,231 quiescent galaxies with i -band Hyper Suprime-Cam Subaru Strategic Program (HSC SSP) imaging that spans the redshift range 0.2 < z < 0.6.
Ivana Damjanov +4 more
doaj +1 more source
ISO Spectroscopy of Ultraluminous Infrared Galaxies
Astrophysics and Space Science, 1999 Spectroscopy from the Infrared Space Observatory ISO has for the first timeprovided the sensitivity to exploit the diagnostic power ofmid-infrared fine structure lines and PAH features for the study ofultraluminous infrared galaxies (LIR >1012 L ⊙). We report on observations obtainedwith SWS, ISOPHOT-S, and the CVF option of ISOCAM.
Lutz, D +7 more
openaire +1 more source