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NICMOS Coronagraphic Surveys-Preliminary Results
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STScI NICMOS Software
NICMOS Science
NICMOS Coronagraphic Surveys-Preliminary Results
Introduction
The EONS Coronagraphic Surveys
Anticipated and Current Coronagraphic Performance
Summary
Acknowledgments
A Coronagraphic Search for Substellar Companions to Young Stars
Introduction
Searching around young stars
Observations with NICMOS
Preliminary Results
The Stellar Population in the NICMOS Parallel Fields
The NICMOS Parallel program
Some Statistics
The Stellar Population
The Evolution of Stars seen with ISOCAM - the Need for NICMOS and VLT Follow Up.
Introduction
A Proto-Planetary Disk around BD+31 643 ?
The Protostellar Candidate HH108MMS
A Ring of Organic Molecules around HD 97300.
Results
The IEBs Carriers
Mass of Circumstellar Material
The Origin of the Ring
Summary
Unusual
Emission near a Compact Source in Orion
Introduction
Observations
Discussion
HST NICMOS Observations of Circumstellar Matter Around CYG X-3
Introduction
Prediction of Circumbinary Material
Previous Observations
NICMOS Observations
Discussion
Conclusions
NICMOS Observes the Galactic Center
Introduction
Proper Motion Studies
Variability Studies
Observations of P
Search for the Tip of the Main Sequence
NICMOS/HST H-band (F160W) Images of the 30 Dor Starburst Cluster
Introduction
Observations and Preliminary Analysis
Preliminary Results
The Formation and Evolution of LMC Rich Star Clusters: NGC 1818
LMC Project Outline
NGC 1818 Initial Results
Future Improvements
A Color Analysis of NICMOS Parallel Observations
Introduction
The NICMOS Parallel Program
Analysis
Software
Scientific Objectives and Preliminary Findings
The Old Stellar Population of NGC 1569 from NICMOS data
Cosmological Background and Astrophysical Goals
Why choose NGC 1569?
NGC 1569 as observed in the Optical Bands of HST/WFPC2
The Need for Near-Infrared NICMOS Observations
NICMOS Data in the Central Region of NGC 1569
How can we reach our Scientific Goal?
HST-NICMOS Observations of Galactic Bulges: Red Nuclei in Nearby Galaxies
Introduction
Sample and Observations
The
B
-
I
vs.
I
-
H
color-color diagram
Dust in Nuclei of Galactic Bulges
Stellar Populations
Discussion
HST
/NICMOS Observations of the Interacting System Arp 299
Introduction
Observations
Reduction of narrow-band filter images taken with NIC3
Morphology of the [Fe
II
] emission
Discussion
Conclusions
NICMOS Camera 3 Parallel Imaging Observations: Number Counts, Sizes and Red Objects
Introduction
Observations
NICMOS Imaging
Ground-based Optical Imaging
Results and Discussion
Incompleteness Modeling
Object Sizes
Implications of the Galaxy Counts
Extremely Red Objects
Summary
Acknowledgments
The Structure and Composition of High Redshift Radio Galaxies
Introduction
The Sample
Observations
Principal Results
Discussion
Investigating the Evolution of Quasar Host Galaxies with NICMOS
Introduction
Previous work
The host galaxies of low-z quasars
R
-band imaging of low-
z
quasar hosts with WFPC2
High-redshift quasars.
Motivation: host galaxies and quasar evolution
This project: studying host galaxy evolution with WFPC2 and NICMOS
Sample Design
PSF determination
Preliminary NICMOS results
NICMOS Imaging of QSO Host Galaxies at 0.1 < z < 4.4
Limits on the Star Formation Rates of
z
>2 Damped Ly
Systems from H
Spectroscopy
Introduction
Searches for Star Formation in Damped Systems
Our Near-IR Spectroscopic Survey
Testing the Large Disk Hypothesis
Future Work
Norbert Pirzkal
1998-07-09
Emission near a Compact Source in Orion
Systems from H
Spectroscopy