output
19942026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations

Showing 2009Show all

67 papers · 1 filter

astro-ph.HE2009★ 1 cited

Early time optical polarization of GRB Afterglows: GRB 060418 and GRB 090102

I. A. Steele, C. G. Mundell, R. J. Smith +2

RINGO on the Liverpool Telescope has now measured the optical polarization of GRB 060418 (where a 2 sigma upper limit of P<8% was determined) and GRB 090102 (when a detection of P…

astro-ph.GA2009★ 30 cited

The RMS Survey: Far-Infrared Photometry of Young Massive Stars

J. C. Mottram, M. G. Hoare, S. L. Lumsden +5

Context: The Red MSX Source (RMS) survey is a multi-wavelength campaign of follow-up observations of a colour-selected sample of candidate massive young stellar objects (MYSOs) in…

astro-ph.GA2009★ 39 cited

The bottom of the white dwarf cooling sequence in the old open cluster NGC 2158

L. R. Bedin, M. Salaris, I. R. King +3

We use 10 orbits of Advanced Camera for Surveys observations to reach the end of the white dwarf cooling sequence in the solar-metallicity open cluster NGC 2158. Our photometry and…

astro-ph.EP2009★ 4 cited

Interpretation of Strong Short-Term Central Perturbations in the Light Curves of Moderate-Magnification Microlensing Events

C. Han, K. -H. Hwang, D. Kim +87

To improve the planet detection efficiency, current planetary microlensing experiments are focused on high-magnification events searching for planetary signals near the peak of len…

astro-ph.CO2009★ 2 cited

[The Impact of Nuclear Star Formation on Gas Inflow to AGN

R. I. Davies, E. Hicks, M. Schartmann +8

Our adaptive optics observations of nearby AGN at spatial resolutions as small as 0.085arcsec show strong evidence for recent, but no longer active, nuclear star formation. We begi…

astro-ph.HE2009★ 101 cited

Hyper Velocity Stars and the Restricted Parabolic 3-body Problem

Re'em Sari, Shiho Kobayashi, Elena M. Rossi

Motivated by detections of hypervelocity stars that may originate from the Galactic Center, we revist the problem of a binary disruption by a passage near a much more massive point…