activity
20122017
most citedThe DESI Experiment Part I: Science,Targeting, and Survey Design

1.3k citations · 4.5k across the 28 of their papers we have counts for

collaborators

28 papers

astro-ph.SR201724 cited

2MASS 0213+3648 C: A wide T3 benchmark companion to an an active, old M dwarf binary

N. R. Deacon, E. A. Magnier, Michael C. Liu +14

We present the discovery of a 360 AU separation T3 companion to the tight (3.1 AU) M4.5+M6.5 binary 2MASS J02132062+3648506. This companion was identified using Pan-STARRS1 data an…

astro-ph.HE201678 cited

Detection of Time Lags Between Quasar Continuum Emission Bands based on Pan-STARRS Light-curves

Yan-Fei Jiang, Paul J. Green, Jenny E. Greene +21

We study the time lags between the continuum emission of quasars at different wavelengths, based on more than four years of multi-band (, , , ) light-curves in the Pan-…

astro-ph.IM2016236 cited

The DESI Experiment Part II: Instrument Design

DESI Collaboration, Amir Aghamousa, Jessica Aguilar +290

DESI (Dark Energy Spectropic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations and the growth of structure through redshift…

astro-ph.IM20161.3k cited

The DESI Experiment Part I: Science,Targeting, and Survey Design

DESI Collaboration, Amir Aghamousa, Jessica Aguilar +290

DESI (Dark Energy Spectroscopic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations (BAO) and the growth of structure through…

astro-ph.SR201691 cited

A Search for L/T Transition Dwarfs With Pan-STARRS1 and WISE. II. L/T Transition Atmospheres and Young Discoveries

William M. J. Best, Michael C. Liu, Eugene A. Magnier +13

The evolution of brown dwarfs from L to T spectral types is one of the least understood aspects of the ultracool population, partly for lack of a large, well-defined, and well-char…

astro-ph.GA201618 cited

Hiding in Plain Sight - Recovering Clusters of Galaxies with the Strongest AGN in Their Cores

T. S. Green, A. C. Edge, H. Ebeling +8

A key challenge in understanding the feedback mechanism of AGN in Brightest Cluster Galaxies (BCGs) is the inherent rarity of catching an AGN during its strong outburst phase. This…