Selected telescopes I have observed with
(page not updated recently)
- Mirror Diameter: 2.4 meter
- Location: Low Earth Orbit
- Observing Projects:
- Stellar kinematics near the nucleus of M32: the
central black hole confirmed?
1995, Cycle 5,
GO-5847, PI, 9 orbits.
- The nuclear disk in the E4 radio galaxy NGC 7052:
evidence for a central black hole?
1995/96,
Cycle 5,
GO-5848, PI, 17 orbits.
- Black holes in kinematically decoupled cores: a study of
IC 1459
1996/97, Cycle 6,
GO-6537, CoI, 8 orbits.
- Nuclear brightness profiles of merger remnants:
do mergers form ellipticals?
1997/8, Cycle 7,
GO-7268, PI, 14 orbits.
- Nuclear structure & merger-starburst relation in the
ultraluminous IRAS galaxy NGC 6240
1999, Cycle 7,
GO-6430, PI, 4 orbits.
- Nuclear structure & merger-starburst relation in the
ultraluminous IRAS galaxy NGC 6240: II. Kinematics
1999, Cycle 8,
GO-8261, PI, 10 orbits.
- Nuclear kinematics of the dense globular cluster
M15
1999, Cycle 8,
GO-8262, PI, 25 orbits.
- Black holes and gas disks in a complete sample of radio-loud
ellipticals: II. Kinematics
1999, Cycle 8,
GO-8236, CoI, 38 orbits.
- The black hole versus bulge mass relationship in
spiral galaxies
1999, Cycle 8,
GO-8228, CoI, 54 orbits.
- Merger-driven evolution of galactic nuclei: observations
of the Toomre sequence
2000, Cycle 9,
GO-8669, PI, 43 orbits.
- Imaging of brightest cluster galaxies: the high end of the
black hole mass distribution
2000, Cycle 9,
GO-8683, PI, 111 snapshot targets.
- A Census of Nuclear Star Clusters in Late-Type Spiral
Galaxies
2000, Cycle 9,
GO-8599, CoI, 113 snapshot targets.
- A Census of Nuclear Star Clusters in Late-Type Spiral
Galaxies: II - Spectroscopy and Stellar Populations
2001, Cycle 10,
GO-9070, CoI, 40 snapshot targets.
- Kinematics of emission-line gas disks in radio-quiet
galaxies
2001, Cycle 10,
GO-9163, CoI, 8 orbits.
- Searching for Primeval Galaxies: the promising case of SBS
1415+437
2002, Cycle 11,
GO-9361, CoI, 18 orbits.
- A NICMOS Study of Merging Nuclei in the Toomre Sequence:
Finding Order Amid Chaos
2002, Cycle 11,
GO-9402, CoI, 11 orbits.
- Systemic and Internal Proper Motions of the Magellanic
Clouds from Astrometry with ACS
2002, Cycle 11,
GO-9462, CoI, 54 snapshot targets.
- Do the Most Powerful Radio Galaxies Host the Most Massive
Black Holes ?
2002, Cycle 11,
GO-9495, CoI, 15 orbits.
- ACS, NICMOS, and STIS Observations of Three Ongoing Mergers
2003, Cycle 12,
GO-9735, CoI, 30 orbits.
- The Ages of Nuclear Star Clusters in Early-type Spiral Galaxies
2003, Cycle 12,
GO-9783, CoI, 16 orbits.
- Systemic and Internal Proper Motions of the Magellanic
Clouds from Astrometry with ACS: II. Second Epoch
Images
2004, Cycle 13,
GO-10130, CoI, 40 snapshot targets.
- Black Holes in Globular Clusters
2004, Cycle 13,
GTO-10335, CoI, 8 orbits.
- A Proper Motion Search for Intermediate Mass Black Holes in Globular Clusters
2004, Cycle 13,
GO-10401, CoI, 7 orbits.
- Star Formation Driven Outflows in Actively Star Forming Edge-on Spiral Galaxies
2004, Cycle 13,
GO-10416, CoI, 16 orbits.
- Merger-Induced Populations in Early-Type Galaxy Cores
2004, Cycle 13,
GO-10435, CoI, 8 orbits.
- NGC 4449: a Testbed for Starbursts in the Low- and High-Redshift Universe
2005, Cycle 14,
GO-10585, CoI, 9 orbits.
- The Rosetta Stone without a Distance: Hunting for Cepheids in the Primordial Galaxy I Zw 18
2005, Cycle 14,
GO-10586, CoI, 24 orbits.
- Archival Projects:
- Understanding Intermediate-luminosity X-ray Objects
and their Environments
2002, Cycle 11,
AR-9545, CoI.
- Archival Study of Merger-Induced Populations in Early-Type Galaxy Cores
2004, Cycle 13,
AR-10306, CoI.
- Theory Projects:
- Stellar Dynamical Models for HST Proper Motion Datasets
2003, Cycle 12,
AR-9952, PI.
- Origin of the Globular Cluster Fundamental Plane
2003, Cycle 12,
AR-10323, CoI.
- Mirror Diameter: 10 meter
- Location: Mauna Kea,
Hawaii, USA
- Observing Projects:
- The nature and origin of nucleated dwarf elliptical
galaxies
1998, CoI, 4 nights.
- Mirror Diameter: 3.6 meter
- Location: Mauna Kea,
Hawaii, USA
- Observing Projects:
- Weak Lensing observations of the clusters of the CNOC1
redshift survey
2000, CoI, 3 nights.
- Mirror Diameter: 2.3 meter
- Location: Kitt Peak,
Arizona, USA
- Observing Projects:
- The Nuclear Star Clusters of late-type Spirals -
Probing Bulge Evolution
1999, CoI, 2 nights.
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Last modified June 11, 2005.
Roeland van der Marel,
marel@stsci.edu.
Copyright Notice.