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19992022
most citedImproved Cosmological Constraints from New, Old and Combined Supernova Datasets

1.6k citations · 6k across the 47 of their papers we have counts for

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Showing 2014Show all

7 papers · 1 filter

astro-ph.SR2014★ 279 cited

Weather on Other Worlds. II. Survey Results: Spots Are Ubiquitous on L and T Dwarfs

Stanimir Metchev, Aren Heinze, Dániel Apai +7

We present results from the "Weather on Other Worlds" Spitzer Exploration Science program to investigate photometric variability in L and T dwarfs, usually attributed to patchy clo…

astro-ph.SR2014★ 21 cited

Spectroscopic follow-up of L- and T-type proper-motion member candidates in the Pleiades

M. R. Zapatero Osorio, V. J. S. Béjar, E. L. Martín +9

(Abridged) We report on the near-infrared low-resolution spectroscopy and red optical (Z-band) photometry of seven proper-motion, very low-mass substellar member candidates of the…

astro-ph.SR2014★ 68 cited

Search for free-floating planetary-mass objects in the Pleiades

M. R. Zapatero Osorio, M. C. Gálvez Ortiz, G. Bihain +8

(Abridged) We aim at identifying the least massive population of the solar metallicity, young (120 Myr), nearby (133.5 pc) Pleiades star cluster with the ultimate goal of understan…

astro-ph.IM2014

VISTA Variables in the Vía Láctea (VVV): Halfway Status and Results

Maren Hempel, Dante Minniti, István Dékány +89

The VISTA Variables in the Vía Láctea (VVV) survey is one of six public ESO surveys, and is now in its 4th year of observing. Although far from being complete, the VVV survey has a…

astro-ph.SR2014★ 47 cited

New constraints on the formation and settling of dust in the atmospheres of young M and L dwarfs

E. Manjavacas, M. Bonnefoy, J. E. Schlieder +7

We obtained medium-resolution near-infrared spectra of seven young M9.5-L3 dwarfs classified in the optical. We aim to confirm the low surface gravity of the objects in the NIR. We…

astro-ph.EP2014★ 209 cited

A global cloud map of the nearest known brown dwarf

I. J. M. Crossfield, B. Biller, J. E. Schlieder +9

Brown dwarfs -- substellar bodies more massive than planets but not massive enough to initiate the sustained hydrogen fusion that powers self-luminous stars -- are born hot and slo…