Results 91 to 100 of about 5,123 (230)
A Confirmed Deficit of Hot and Cold Dust Emission in the Most Luminous Little Red Dots
The Astrophysical Journal LettersLuminous broad H α emission and red rest-optical spectral energy distributions (SEDs) are the hallmark of compact little red dots (LRDs), implying highly attenuated dusty starbursts and/or obscured active galactic nuclei (AGN).
David J. Setton +35 more
doaj +1 more source
Geologically Recent Formation of Some Tesserae on Venus by Plains Deformation
Journal of Geophysical Research: Planets, Volume 131, Issue 6, June 2026.Abstract Tessera is a pervasively deformed terrain type on Venus generally interpreted as the oldest preserved material on the surface. Large expanses of this terrain type are typically elevated and have been hypothesized to be felsic, perhaps analogous to Earth's continents and even to date from an era with a more Earth‐like climate earlier in Venus ...
Paul K. Byrne +6 more
wiley +1 more source
Blast: the far-infrared/radio correlation in distant galaxies [PDF]
, 2010 We investigate the correlation between far-infrared (FIR) and radio luminosities in distant galaxies, a lynchpin of modern astronomy. We use data from the Balloon-borne Large Aperture Submillimetre Telescope (BLAST), Spitzer, the Large Apex BOlometer ...
David Hughes
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Martian Proton Albedo as Signature of Near‐Surface Water
Journal of Geophysical Research: Planets, Volume 131, Issue 6, June 2026.Abstract Understanding the Martian soil water budget is crucial not only for in situ resource utilization in future human missions to Mars, but also for reconstructing the geological and climatic history of the planet, as well as to assess the potential of ancient or even present microbial life.
Jan Leo Löwe +13 more
wiley +1 more source
The Laboratory Astrophysics Spectroscopy Programme at Imperial College London
Galaxies, 2018 Accurate atomic parameters, such as transition probabilities, wavelengths, and energy levels, are indispensable for the analysis of stellar spectra and the obtainment of chemical abundances.
María Teresa Belmonte +4 more
doaj +1 more source
Journal of Geophysical Research: Planets, Volume 131, Issue 6, June 2026.Abstract Seasonal CO2 and H2O ice blanket the Martian polar caps, and their spectral contributions mix during seasonal evolution. Particularly in late northern winter, the spectral signature of H2O ice obscures that of CO2 ice. Using the MARVIN chamber at York University, we produced controlled analogs of layered polar ice under Mars‐like pressure (∼6 ...
Jamie A. Isen +3 more
wiley +1 more source
A balloon-borne 1 meter telescope for far-infrared astronomy
, 1974 The flight of a balloon-borne one-meter telescope for infrared astronomy in the wavelength interval of 40 to 240 microns is discussed. The gyro-stabilized telescope mapped the intensity of the far infrared radiation from NGC 7538, Mars, the Orion Nebula,
Wright, E. L. +4 more
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First results from high redshift quasar searches in VIKING [PDF]
, 2012 This thesis presents the discovery of the first luminous z & 6.5 quasars in the VISTA kilo-degree Infrared Galaxy Survey (VIKING). After some basic quality control, quasar selection is investigated via use of initial data supplementedwith ...
Findlay, Joseph
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SOFIA and its facility Far Infrared Camera HAWC
, 2002 The Stratospheric Observatory For Infrared Astronomy (SOFIA) is a 2.5 m telescope which will fly in a Boeing 747SP, commencing operation in late summer 2004.
S. H. Moseley +9 more
core +1 more source
Far infrared supplement: Catalog of infrared observations, second edition
, 1988 The Far Infrared Supplement: Catalog of Infrared Observations summarizes all infrared astronomical observations at far infrared wavelengths (5 to 1000 microns) published in the scientific literature from 1965 through 1986.
Mead, Jaylee M. +2 more
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