Results 221 to 230 of about 53,403 (252)

Modes of the Dark Ages 21 cm field accessible to a lunar radio interferometer. [PDF]

Philos Trans A Math Phys Eng Sci
Bull P, Guandalin C, Addis C.
europepmc   +1 more source

A 600 m² array of 6.5 m telescopes at the lunar pole. [PDF]

Philos Trans A Math Phys Eng Sci
Angel R.
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Copper integrative catalytic pairs with mixed-valence Cu²⁺-Cu³⁺ Species for selective alkyne conversion. [PDF]

Nat Commun
Yue Y, Yu M, Yao Z, Fang G, Wang B, Wang S, Jin C, Chang R, Sun T, Pan Z, Zhu Y, Wang FR, Li X, Zhao J.   +13 more
europepmc   +1 more source

A Faint Progenitor System for the Faint Supernova 2024vjm

Zimmerman E, Gal-Yam A, Groot P, Ofek E, Roestel Jv, Pastorello A, Valenti S, Ravi A, Chen P, Schulze S, Blagorodnova N, Wavasseur M, Gómez-Muñoz M, Tranin H, de Wet S, Leloudas G, Vreeswijk P, Kwok L, Schwab M, Jha S, Maguire K, Sand D, Stringer E, Kupfer T, Faran T, Anderson J, Andrews J, Andrews M, Badash A, Bloemen S, Bostroem K, Chen T, Valle MD, Dimitriadis G, Dong Y, Farah J, Gillanders J, Godson B, Gromadzki M, Hiramatsu D, Hoang E, Howell D, Janzen D, Kuncarayakti H, Li J, Lyman J, Maeda K, Magee M, Mehta D, Milligan A, Moran S, Ni YQ, O’Neill D, Pearson J, Pieterse D, Pignata G, Reguitti A, Reichart D, Retamal NM, Santos R, Scaringi S, Shrestha M, Srivastav S, Stoppa F, Subrayan B, Valerin G, Wang X, Wynn K, Yaron O, Zang W.   +69 more
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How Does a Low Surface Brightness Galaxy Form Spiral Arms?

Ganesh Narayanan, A. G. Anagha, Arunima Banerjee   +2 more
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StarDICE II: Calibration of an Uncooled Infrared Thermal Camera for Atmospheric Gray Extinction Characterization. [PDF]

Sensors (Basel)
Sommer K, Plez B, Cohen-Tanugi J, Dagoret-Campagne S, Moniez M, Neveu J, Betoule M, Bongard S, Feinstein F, Le Guillou L, Juramy C, Sepulveda E, Souverin T.   +12 more
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A binary merger product as the direct progenitor of a Type II-P supernova

Niu* Z, Sun* N, Zapartas* E, Souropanis D, Cui Y, Maund JR, Andrews JJ, Briel MM, Fraser M, Gossage S, Kruckow MU, Liotine C, Liu Z, Srivas PM, Teng E, Wang X, Yang Y, Liu J.   +17 more
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Black hole jets on the scale of the Cosmic Web

Oei MS, Hardcastle MJ, Timmerman R, Gast AR, Botteon A, Rodriguez AC, Stern D, Rivera GC, Weeren RJv, Röttgering HJ, Intema HT, de Gasperin F, Djorgovski S.   +12 more
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Properties of low Surface Brightness Galaxies

Symposium - International Astronomical Union, 1996
We have been working on multiband surface photometry, spectrophotometry and Hi synthesis data for 20 Low Surface Brightness (LSB) galaxies. LSB galaxies are well described by disks with an average central surface brightness of ∼ 23.4B-mag arcsec–2. They have scale lengths typical for high surface brightness (HSB) galaxies, though a large range of sizes
W. J. G. De Blok, J. M. Van Der Hulst, S. S. McGaugh   +2 more
openaire   +3 more sources

Low-Surface-Brightness Galaxies: Hidden Galaxies Revealed

Publications of the Astronomical Society of the Pacific, 1997
In twenty years, low surface brightness (LSB) galaxies have evolved from being an idiosyncratic notion to being one of the major baryonic repositories in the Universe. The story of their discovery and the characterization of their properties is told here. Their recovery from the noise of the night sky background is a strong testament to the severity of
G. Bothun, C. Impey, S. McGaugh
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