activity
19992022
most citedStar Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies

2k citations · 15.3k across the 169 of their papers we have counts for

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Showing 2017Show all

6 papers · 1 filter

astro-ph.SR2017★ 29 cited

Extinction and the Dimming of KIC 8462852

Huan Y. A. Meng, George Rieke, Franky Dubois +11

To test alternative hypotheses for the behavior of KIC 8462852, we obtained measurements of the star over a wide wavelength range from the UV to the mid-infrared from October 2015…

astro-ph.EP2017★ 24 cited

What Sets the Radial Locations of Warm Debris Disks?

Nicholas P. Ballering, George H. Rieke, Kate Y. L. Su +1

The architectures of debris disks encode the history of planet formation in these systems. Studies of debris disks via their spectral energy distributions (SEDs) have found infrare…

astro-ph.GA2017★ 63 cited

The Intrinsic Far-infrared Continua of Type-1 Quasars

Jianwei Lyu, George H. Rieke

The range of currently proposed active galactic nucleus (AGN) far-infrared templates results in uncertainties in retrieving host galaxy information from infrared observations and a…

astro-ph.EP2017★ 108 cited

A Complete ALMA Map of the Fomalhaut Debris Disk

Meredith A. MacGregor, Luca Matra, Paul Kalas +14

We present ALMA mosaic observations at 1.3 mm (223 GHz) of the Fomalhaut system with a sensitivity of 14 Jy/beam. These observations provide the first millimeter map of the cont…

astro-ph.SR2017★ 35 cited

The Inner 25 AU Debris Distribution in the epsilon Eri System

Kate Y. L. Su, James M. De Buizer, George H. Rieke +6

Debris disk morphology is wavelength dependent due to the wide range of particle sizes and size-dependent dynamics influenced by various forces. Resolved images of nearby debris di…

astro-ph.SR2017★ 33 cited

The first 40 million years of circumstellar disk evolution: the signature of terrestrial planet formation

Huan Y. A. Meng, George H. Rieke, Kate Y. L. Su +1

We characterize the first 40 Myr of evolution of circumstellar disks through a unified study of the infrared properties of members of young clusters and associations with ages from…