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20022009
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

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7 papers · 1 filter

astro-ph.GA2009180 cited

Galactic masers and the Milky Way circular velocity

Jo Bovy, David W. Hogg, Hans-Walter Rix

Masers found in massive star-forming regions can be located precisely in six-dimensional phase space and therefore serve as a tool for studying Milky Way dynamics. The non-random o…

astro-ph.GA200962 cited

Eddington ratio governs the equivalent width of MgII emission line in active galactic nuclei

Xiao-Bo Dong, Ting-Gui Wang, Jian-Guo Wang +4

We have investigated the ensemble regularities of the equivalent widths (EWs) of MgII 2800 emission line of active galactic nuclei (AGNs), using a uniformly selected sample of 2092…

astro-ph.GA200967 cited

A Multi-Color Optical Survey of the Orion Nebula Cluster. Part I: the Catalog

Nicola Da Rio, Massimo Robberto, David R. Soderblom +4

We present U, B, V, I broad-band, 6200A TiO medium-band and Halpha photometry of the Orion Nebula Cluster obtained with the WFI imager at the ESO/MPI 2.2 telescope. The nearly-simu…

astro-ph.GA2009166 cited

Dynamical masses of early-type galaxies at z~2: Are they truly superdense?

Michele Cappellari, S. di Serego Alighieri, A. Cimatti +11

We measured stellar velocity dispersions sigma and dynamical masses of 9 massive (M~10^11 Msun) early-type galaxies (ETG) from the GMASS sample at redshift 1.4<z<2.0. The sigma are…

astro-ph.GA2009124 cited

Tracing Sagittarius Structure with SDSS and SEGUE Imaging and Spectroscopy

Brian Yanny, Heidi Jo Newberg, Jennifer A. Johnson +12

We show that the Sagittarius dwarf tidal stream can be traced with very red K/M-giant stars selected from SDSS photometry. A subset of these stars are spectroscopically confirmed w…

astro-ph.GA200963 cited

The velocity distribution of nearby stars from Hipparcos data I. The significance of the moving groups

Jo Bovy, David W. Hogg, Sam T. Roweis

We present a three-dimensional reconstruction of the velocity distribution of nearby stars (<~ 100 pc) using a maximum likelihood density estimation technique applied to the two-di…