activity
19952016
most citedH_alpha Emission from High-Velocity Clouds and their Distances

181 citations · 318 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.IM2016★ 9 cited

The GALAH Survey: Relative throughputs of the 2dF fibre positioner and the HERMES spectrograph from stellar targets

Jeffrey D. Simpson, G. M. De Silva, J. Bland-Hawthorn +11

We present an analysis of the relative throughputs of the 3.9-metre Anglo-Australian Telescope's 2dF/HERMES system, based upon spectra acquired during the first two years of the GA…

astro-ph.GA2015★ 4 cited

Comment on "Evidence for dark matter in the inner Milky Way"

Stacy McGaugh, Federico Lelli, Marcel Pawlowski +21

This is a brief rebuttal to arXiv:1502.03821, which claims to provide the first observational proof of dark matter interior to the solar circle. We point out that this result is no…

astro-ph2003★ 181 cited

H_alpha Emission from High-Velocity Clouds and their Distances

M. E. Putman, J. Bland-Hawthorn, S. Veilleux +3

We present deep Halpha spectroscopy towards several high-velocity clouds (HVCs) which vary in structure from compact (CHVCs) to the Magellanic Stream. The clouds range from being b…

astro-ph1999★ 119 cited

Binary Microlensing Events from the MACHO Project

MACHO, GMAN collaborations, : +1

We present the lightcurves of 21 gravitational microlensing events from the first six years of the MACHO Project gravitational microlensing survey which are likely examples of lens…

astro-ph1999

Bars and Boxy/Peanut-Shaped Bulges: An Observational Point of View

M. Bureau, K. C. Freeman, E. Athanassoula

Prompted by work on the buckling instability in barred spiral galaxies, much effort has been devoted lately to the study of boxy/peanut-shaped (B/PS) bulges. Here, we present new b…

astro-ph1997★ 4 cited

Optical identification of the LMC supersoft source RXJ0527.8-6954 from MACHO Project photometry

C. Alcock et al

We identify the likely optical counterpart to the LMC supersoft X-ray source RXJ0527.8-6954, and hence recover HV2554. This identification is based on an analysis of approximately…