output
20072019
most citedSpitzer SAGE Infrared Photometry of Massive Stars in the Large Magellanic Cloud

221 citations

13 papers

astro-ph.GA2019★ 24 cited

The SOFIA Massive (SOMA) Star Formation Survey. II. High Luminosity Protostars

Mengyao Liu, Jonathan C. Tan, James M. De Buizer +6

We present multi-wavelength images observed with SOFIA-FORCAST from 10 to 40 m of seven high luminosity massive protostars, as part of the SOFIA Massive (SOMA) Star Format…

astro-ph.EP2019★ 21 cited

K2-288Bb: A Small Temperate Planet in a Low-mass Binary System Discovered by Citizen Scientists

Adina D. Feinstein, Joshua E. Schlieder, John H. Livingston +23

Observations from the Kepler and K2 missions have provided the astronomical community with unprecedented amounts of data to search for transiting exoplanets and other astrophysical…

astro-ph.HE2017★ 212 cited

Follow up of GW170817 and its electromagnetic counterpart by Australian-led observing programs

I. Andreoni, K. Ackley, J. Cooke +122

The discovery of the first electromagnetic counterpart to a gravitational wave signal has generated follow-up observations by over 50 facilities world-wide, ushering in the new era…

astro-ph.SR2017★ 11 cited

Outflow-Confined HII regions. II. The Early Break-Out Phase

Kei E. I. Tanaka, Jonathan C. Tan, Jan E. Staff +1

In this series of papers, we model the formation and evolution of the photoionized region and its observational signatures during massive star formation. Here we focus on the early…

astro-ph.HE2016★ 12 cited

The Zadko Telescope: Exploring the transient Universe

D. M. Coward, B. Gendre, P. Tanga +11

The Zadko Telescope is a 1 m f/4 Cassegrain telescope, situated in the state of Western Australia about 80 km north of Perth. The facility plays a niche role in Australian astronom…

astro-ph.SR2011★ 83 cited

X-ray illumination of the ejecta of Supernova 1987A

J. Larsson, C. Fransson, G. Östlin +25

We present the late-time optical light curve of the ejecta of SN 1987A measured from HST imaging observations spanning the past 17 years. We find that the flux from the ejecta decl…