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by Abazajian, Kevork N and Adelman-McCarthy, Jennifer K and Agüeros, Marcel A and Allam, Sahar S and Allende Prieto, Carlos and An, Deokkeun and Anderson, Kurt S. J and Anderson, Scott F and Annis, James and Bahcall, Neta A and Bailer-Jones, C. A. L and Barentine, J. C and Bassett, Bruce A and Becker, Andrew C and Beers, Timothy C and Bell, Eric F and Belokurov, Vasily and Berlind, Andreas A and Berman, Eileen F and Bernardi, Mariangela and Bickerton, Steven J and Bizyaev, Dmitry and Blakeslee, John P and Blanton, Michael R and Bochanski, John J and Boroski, William N and Brewington, Howard J and Brinchmann, Jarle and Brinkmann, J and Brunner, Robert J and Budavári, Tamás and Carey, Larry N and Carliles, Samuel and Carr, Michael A and Castander, Francisco J and Cinabro, David and Connolly, A. J and Csabai, István and Cunha, Carlos E and Czarapata, Paul C and Davenport, James R. A and de Haas, Ernst and Dilday, Ben and Doi, Mamoru and Eisenstein, Daniel J and Evans, Michael L and Evans, N. W and Fan, Xiaohui and Friedman, Scott D and Frieman, Joshua A and Fukugita, Masataka and Gänsicke, Boris T and Gates, Evalyn and Gillespie, Bruce and Gilmore, G and Gonzalez, Belinda and Gonzalez, Carlos F and Grebel, Eva K and Gunn, James E and Györy, Zsuzsanna and Hall, Patrick B and Harding, Paul and Harris, Frederick H and Harvanek, Michael and Hawley, Suzanne L and Hayes, Jeffrey J. E and Heckman, Timothy M and Hendry, John S and Hennessy, Gregory S and Hindsley, Robert B and Hoblitt, J and Hogan, Craig J and Hogg, David W and Holtzman, Jon A and Hyde, Joseph B and Ichikawa, Shin-ichi and Ichikawa, Takashi and Im, Myungshin and Ivezić, Željko and Jester, Sebastian and Jiang, Linhua and Johnson, Jennifer A and Jorgensen, Anders M and Jurić, Mario and Kent, Stephen M and Kessler, R and Kleinman, S. J and Knapp, G. R and Konishi, Kohki and Kron, Richard G and Krzesinski, Jurek and Kuropatkin, Nikolay and Lampeitl, Hubert and Lebedeva, Svetlana and Lee, Myung Gyoon and Lee, Young Sun and Leger, R. French and Lépine, Sébastien and Li, Nolan and Lima, Marcos and ... and BROOKHAVEN NATIONAL LABORATORY (BNL)
The Astrophysical Journal Supplement Series, ISSN 0067-0049, 06/2009, Volume 182, Issue 2, pp. 543 - 558
Journal Article
The Astrophysical Journal Supplement Series, ISSN 1538-4365, 12/2017, Volume 233, Issue 2, p. 27
Journal Article
The Astrophysical Journal, ISSN 1538-4357, 03/2018, Volume 856, Issue 1, p. 11
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 07/2015, Volume 450, Issue 3, pp. 2692 - 2692
We use our Galactic Globular Cluster Catalog (G2C2) photometry for 111 Galactic globular clusters (GCs) in g and z, as well as r and i photometry for a subset... 
Correlation | Color | Clusters | Sky surveys (astronomy) | Mathematical models | Globular clusters | Photometry | Colour
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2017, Volume 464, Issue 1, pp. 356 - 356
We present spatially resolved two-dimensional stellar kinematics for the 41 most massive early-type galaxies (ETGs; M sub( K) ... -25.7 mag, stellar mass M*... 
Slopes | Spectrographs | Galaxies | Anisotropy | Symbols | Angular momentum | Milky Way Galaxy | Luminosity
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2015, Volume 447, Issue 1, pp. 618 - 618
Using Hubble Space Telescope (HST) Advanced Camera for Surveys/Wide Field Camera data we present the photometry and spatial distribution of resolved stellar... 
Discs | Law | Star formation | Luminosity | Main sequence stars | Disks | Constants | Photometry
Journal Article
Astrophysical Journal, ISSN 0004-637X, 06/2015, Volume 806, Issue 1, pp. 1 - 22
We present a kinematic analysis of the globular cluster (GC) systems and diffuse stellar light of four intermediate luminosity (sub-L*) early-type galaxies in... 
Amplitudes | Galaxies | Virgo galactic cluster | Kinematics | Luminosity | Diffusion | Star clusters | Photometry
Journal Article
Astrophysical Journal, ISSN 0004-637X, 02/2017, Volume 836, Issue 1, p. 67
The total mass MGCS in the globular cluster (GC) system of a galaxy is empirically a near- constant fraction of the total mass M-h equivalent to M-bary +... 
galaxies: formation | globular clusters: general | galaxies: star clusters: general | MASS BLACK-HOLE | STAR-FORMATION | DWARF GALAXIES | LUMINOSITY FUNCTION | COMA CLUSTER | ULTRA-DIFFUSE GALAXIES | ASTRONOMY & ASTROPHYSICS | FORNAX CLUSTER | VIRGO CLUSTER | TO-LIGHT RATIOS | MILKY-WAY | Physics - Astrophysics of Galaxies
Journal Article
Nature, ISSN 0028-0836, 04/2016, Volume 532, Issue 7599, pp. 340 - 342
Journal Article
Journal Article