activity
19992011
most citedThe FIRST Bright Quasar Survey. II. 60 Nights and 1200 Spectra Later

358 citations · 420 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2011★ 11 cited

Mapping the Asymmetric Thick Disk: II Distance, Size and Mass of the Hercules Thick Disk Cloud

Jeffrey A. Larsen, Juan E. Cabanela, Roberta M. Humphreys

The Hercules Thick Disk Cloud (Larsen et al. 2008) was initially discovered as an excess in the number of faint blue stars between quadrants 1 and 4 of the Galaxy. The origin of th…

astro-ph.GA2010★ 10 cited

Mapping the Asymmetric Thick Disk: III. The Kinematics and Interaction with the Galactic Bar

Roberta M. Humphreys, Timothy C. Beers, Juan E. Cabanela +4

In the first two papers of this series, Larsen et al (2010a,b) describe our faint CCD survey in the inner Galaxy and map the over-density of Thick Disk stars in Quadrant I (Q1) to…

astro-ph.GA2009★ 5 cited

Mapping the Asymmetric Thick Disk I. A Search for Triaxiality

J. A. Larsen, J. E. Cabanela, R. M. Humphreys +1

A significant asymmetry in the distribution of faint blue stars in the inner Galaxy, Quadrant 1 (l = 20 to 45 degrees) compared to Quadrant 4 was first reported by Larsen & Humphre…

astro-ph2008★ 14 cited

Mapping the Asymmetric Thick Disk: The Hercules Thick Disk Cloud

Jeffrey A. Larsen, Roberta M. Humphreys, Juan E. Cabanela

The stellar asymmetry of faint thick disk/inner halo stars in the first quadrant first reported by Larsen & Humphreys (1996) and investigated further by Parker et al. (2003, 2004)…

astro-ph2002★ 4 cited

Galaxies on the Blue Edge

J. E. Cabanela, J. M. Dickey

We have successfully constructed a catalog of HI-rich galaxies selected from the Minnesota Automated Plate Scanner Catalog of the Palomar Observatory Sky Survey (POSS I) based sole…

astro-ph1999★ 358 cited

The FIRST Bright Quasar Survey. II. 60 Nights and 1200 Spectra Later

R. L. White, R. H. Becker, M. D. Gregg +11

We have used the VLA FIRST survey and the APM catalog of the POSS-I plates as the basis for constructing a new radio-selected sample of optically bright quasars. This is the first…