activity
20062026
most citedThe Near Infrared Imager and Slitless Spectrograph for the James Webb Space Telescope -- II. Wide Field Slitless Spectroscopy

106 citations · 2.1k across the 73 of their papers we have counts for

collaborators
Showing 2015Show all

6 papers · 1 filter

astro-ph.GA2015★ 27 cited

Wisps in the Galactic center: NIR triggered observations of the radio source Sgr A* at 43 GHz

C. Rauch, E. Ros, T. P. Krichbaum +4

Context. The compact radio and near-infrared (NIR) source Sagittarius A* (Sgr A*) associated with the supermassive black hole in the Galactic center was observed at 7 mm in the con…

astro-ph.SR2015★ 6 cited

Spectro-photometric characterization of high proper motion sources from WISE

J. C. Beamín, V. D. Ivanov, D. Minniti +7

The census of the solar neighborhood is almost complete for stars and becoming more complete in the brown dwarf regime. Spectroscopic, photometric and kinematic characterization of…

astro-ph.SR2015★ 53 cited

Substellar Objects in Nearby Young Clusters (SONYC) IX: The planetary-mass domain of Chamaeleon-I and updated mass function in Lupus-3

Koraljka Muzic, Alexander Scholz, Vincent C. Geers +1

Substellar Objects in Nearby Young Clusters -- SONYC -- is a survey program to investigate the frequency and properties of substellar objects in nearby star-forming regions. We pre…

astro-ph.SR2015★ 34 cited

Rotation Periods of Young Brown Dwarfs: K2 Survey in Upper Scorpius

Aleks Scholz, Veselin Kostov, Ray Jayawardhana +1

We report rotational periods for 16 young brown dwarfs in the nearby Upper Scorpius association, based on 72 days of high-cadence, high-precision photometry from the Kepler space t…

astro-ph.SR2015★ 6 cited

WISE J061213.85-303612.5: a new T-dwarf binary candidate

N. Huélamo, V. D. Ivanov, R. Kurtev +8

T and Y-dwarfs are among the coolest and least luminous objects detected, and they can help to understand the properties of giant planets. Their multiplicity properties can shed li…

astro-ph.SR2015★ 7 cited

The young low-mass star ISO-Oph-50: Extreme variability induced by a clumpy, evolving circumstellar disk

Aleks Scholz, Koraljka Muzic, Vincent Geers

ISO-Oph-50 is a young low-mass object in the ~Myr old Ophiuchus star forming region undergoing dramatic changes in its optical/near/mid-infrared brightness by 2-4 mag. We present n…