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Multimessenger Astronomy |
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7 months 1 week ago |
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Wide companions to M and L subdwarfs with Gaia and the Virtual Observatory |
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Understanding the Angular Momentum Evolution of T Tauri and Herbig Ae/Be Stars |
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The EBLM project - VIII. First results for M-dwarf mass, radius, and effective temperature measurements using CHEOPS light curves |
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Early science with the Large Millimeter Telescope: a 1.1 mm AzTEC survey of red-Herschel dusty star-forming galaxies |
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A massive open cluster hiding in full sight |
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7 months 1 week ago |
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Processing GOTO survey data with the Rubin Observatory LSST Science Pipelines II: Forced Photometry and lightcurves |
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Long Characteristics versus Short Characteristics in 3D Radiative Transfer Simulations of Polarized Radiation |
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7 months 1 week ago |
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Is the Bremer Deep Field reionized, at z ∼ 7? |
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Interstellar Extinction, Polarization, and Grain Alignment in the Sh 2-185 (IC 59 and IC 63) Region |
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Downflowing umbral flashes as evidence of standing waves in sunspot umbrae |
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7 months 1 week ago |
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Confirming new white dwarf-ultracool dwarf binary candidates |
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7 months 1 week ago |
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MASTER Transient Discovery Report for 2020-06-23 |
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Galaxy classification: deep learning on the OTELO and COSMOS databases |
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HST Survey of the Orion Nebula Cluster in the H<SUB>2</SUB>O 1.4 μm Absorption Band. III. The Population of Substellar Binary Companions |
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7 months 1 week ago |
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The age of the Hyades from the lithium depletion boundary. |
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Astrometric orbits of spectral binary brown dwarfs - I. Massive T dwarf companions to 2M1059-21 and 2M0805+48 |
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A new spectroscopic analysis of the massive O + O type binary HD 54662 AB |
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Doppler tomographic measurement of the nodal precession of WASP-33b |
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The spectroscopic properties of the Lixiaohua family, cradle of Main Belt Comets |
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Spectropolarimetry of the Solar Mg II h and k Lines |
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Spitzer Catalog of Herschel-selected Ultrared Dusty Star-forming Galaxies |
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Challenging a Newtonian prediction through Gaia wide binaries |
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The stellar host in star-forming low-mass galaxies: Evidence for two classes |
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Origin of the chromospheric three-minute oscillations in sunspot umbrae |
iacweb |
7 months 1 week ago |
