activity
19962007
most citedNew Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy

1.8k citations · 1.8k across the 3 of their papers we have counts for

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astro-ph200829 cited

The WFC3 Galactic Bulge Treasury Program: A First Look at Resolved Stellar Population Tools

Thomas M. Brown, Kailash Sahu, Manuela Zoccali +12

[Abridged] When WFC3 is installed on HST, the community will have powerful new tools for investigating resolved stellar populations. The WFC3 Galactic Bulge Treasury program will o…

astro-ph2008170 cited

Stellar Proper Motions in the Galactic Bulge from deep HST ACS/WFC Photometry

Will Clarkson, Kailash Sahu, Jay Anderson +11

We present stellar proper motions in the Galactic bulge from the Sagittarius Window Eclipsing Extrasolar Search (SWEEPS) project using ACS/WFC on HST. Proper motions are extracted…

astro-ph200824 cited

The Fundamental Plane of QSOs and the Relationship Between Host and Nucleus

Timothy S. Hamilton, Stefano Casertano, David A. Turnshek

We present results from an archival study of 70 medium-redshift QSOs observed with the Wide Field Planetary Camera 2 on board the Hubble Space Telescope. The QSOs have magnitudes M…

astro-ph2008140 cited

Double-blind test program for astrometric planet detection with Gaia

S. Casertano, M. G. Lattanzi, A. Sozzetti +6

We use detailed simulations of the Gaia observations of synthetic planetary systems and develop and utilize independent software codes in double-blind mode to analyze the data, inc…

astro-ph20072 cited

Testing Planet Formation Models with Gaia as Astrometry

A. Sozzetti, S. Casertano, M. G. Lattanzi +5

In this paper, we first summarize the results of a large-scale double-blind tests campaign carried out for the realistic estimation of the Gaia potential in detecting and measuring…

astro-ph20071 cited

Planets in the Galactic Bulge: Results from the SWEEPS Project

Kailash C. Sahu, Stefano Casertano, Jeff Valenti +13

The exoplanets discovered so far have been mostly around relatively nearby and bright stars. As a result, the host stars are mostly (i) in the Galactic disk, (ii) relatively massiv…