High-Contrast Observations with an Integral Field Spectrograph
This thesis is comprised of work carried out during the commissioning phase of Project 1640, a combined coronagraph--integral field spectrograph for Palomar Observatory's adaptive optics-equipped 200'' Hale Telescope. I have divided my investigations into three chapters. First, I desc...
Main Author: | |
---|---|
Language: | English |
Published: |
2011
|
Subjects: | |
Online Access: | https://doi.org/10.7916/D8GM8F91 |
id |
ndltd-columbia.edu-oai-academiccommons.columbia.edu-10.7916-D8GM8F91 |
---|---|
record_format |
oai_dc |
spelling |
ndltd-columbia.edu-oai-academiccommons.columbia.edu-10.7916-D8GM8F912019-05-09T15:13:39ZHigh-Contrast Observations with an Integral Field SpectrographZimmerman, Neil Thomas2011ThesesAstronomyThis thesis is comprised of work carried out during the commissioning phase of Project 1640, a combined coronagraph--integral field spectrograph for Palomar Observatory's adaptive optics-equipped 200'' Hale Telescope. I have divided my investigations into three chapters. First, I describe the data reduction pipeline software, which solves a number of data extraction and calibration challenges unique to this kind of instrument. In the second chapter, I demonstrate a novel method for faint companion discovery which takes advantage of the high-precision relative astrometry enabled by a pupil plane reticle grid. This tool, in combination with the spectrophotometric capability of the integral field spectrograph, reveal that the A5V star Alcor has a heretofore unknown M-dwarf companion. In my third chapter, I explore the suitability of combining the non-redundant aperture mask interferometry technique with an integral field spectrograph. In the proof-of-concept observation of the spectroscopic binary star Beta CrB, I retrieve the first near-infrared spectrum of its F-dwarf companion.Englishhttps://doi.org/10.7916/D8GM8F91 |
collection |
NDLTD |
language |
English |
sources |
NDLTD |
topic |
Astronomy |
spellingShingle |
Astronomy Zimmerman, Neil Thomas High-Contrast Observations with an Integral Field Spectrograph |
description |
This thesis is comprised of work carried out during the commissioning phase of Project 1640, a combined coronagraph--integral field spectrograph for Palomar Observatory's adaptive optics-equipped 200'' Hale Telescope. I have divided my investigations into three chapters. First, I describe the data reduction pipeline software, which solves a number of data extraction and calibration challenges unique to this kind of instrument. In the second chapter, I demonstrate a novel method for faint companion discovery which takes advantage of the high-precision relative astrometry enabled by a pupil plane reticle grid. This tool, in combination with the spectrophotometric capability of the integral field spectrograph, reveal that the A5V star Alcor has a heretofore unknown M-dwarf companion. In my third chapter, I explore the suitability of combining the non-redundant aperture mask interferometry technique with an integral field spectrograph. In the proof-of-concept observation of the spectroscopic binary star Beta CrB, I retrieve the first near-infrared spectrum of its F-dwarf companion. |
author |
Zimmerman, Neil Thomas |
author_facet |
Zimmerman, Neil Thomas |
author_sort |
Zimmerman, Neil Thomas |
title |
High-Contrast Observations with an Integral Field Spectrograph |
title_short |
High-Contrast Observations with an Integral Field Spectrograph |
title_full |
High-Contrast Observations with an Integral Field Spectrograph |
title_fullStr |
High-Contrast Observations with an Integral Field Spectrograph |
title_full_unstemmed |
High-Contrast Observations with an Integral Field Spectrograph |
title_sort |
high-contrast observations with an integral field spectrograph |
publishDate |
2011 |
url |
https://doi.org/10.7916/D8GM8F91 |
work_keys_str_mv |
AT zimmermanneilthomas highcontrastobservationswithanintegralfieldspectrograph |
_version_ |
1719045464798527488 |