output
20132026
most citedThe Eighteenth Data Release of the Sloan Digital Sky Surveys: Targeting and First Spectra from SDSS-V

282 citations

researchers with a paper here

Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.

collaborating institutions
Showing astro-ph.SRShow all

5 papers · 1 filter

astro-ph.SR2026★ 1 cited

JWST-DECO: Temporal Variations in the Mid-IR Silicate Features of Two T Tauri Discs Based on Spitzer and JWST observations

N. Sameshima, T. Miyata, T. Kamizuka +9

Mid-infrared spectra of planet-forming discs commonly show prominent silicate emission, whose spectral shape is sensitive to the disc temperature distribution as well as its minera…

astro-ph.SR2024★ 5 cited

Host-star and exoplanet composition: Polluted white dwarf reveals depletion of moderately refractory elements in planetary material

Claudia Aguilera-Gómez, Laura K. Rogers, Amy Bonsor +6

Planets form from the same cloud of molecular gas and dust as their host stars. Confirming if planetary bodies acquire the same refractory element composition as their natal disc d…

astro-ph.SR2016★ 234 cited

Imaging the water-snow line during a protostellar outburst

Lucas A. Cieza, Simon Casassus, John Tobin +13

A snow-line is the region of a protoplanetary disk at which a major volatile, such as water or carbon monoxide, reaches its condensation temperature. Snow-lines play a crucial role…

astro-ph.SR2014★ 84 cited

Precession and accretion in circumbinary discs: The case of HD 104237

Alex Dunhill, Jorge Cuadra, Catherine Dougados

We present the results of smoothed particle hydrodynamics (SPH) simulations of the disc around the young, eccentric stellar binary HD 104237. We find that the binary clears out a l…

astro-ph.SR2013★ 1 cited

RR Lyrae in the LMC: Insights Into the Oosterhoff Phenomenon

Charles A Kuehn, Horace A. Smith, Marcio Catelan +8

Although more than eight decades have passed since P. Th. Oosterhoff drew attention to differences in the properties of RR Lyrae variables in globular clusters, the origin and sign…