High Resolution Near-Infrared Imaging and Computer Simulations of a Lunar Occultation of the Galactic Center

1989 ◽  
pp. 509-512
Author(s):  
D. A. Simons ◽  
E. E. Becklin ◽  
K. -W. Hodapp
Keyword(s):  
High Resolution ◽  
Computer Simulations ◽  
Near Infrared ◽  
Infrared Imaging ◽  
Galactic Center ◽  
Near Infrared Imaging ◽  
Lunar Occultation

scholarly journals High Resolution Near-Infrared Imaging and Computer Simulations of a Lunar Occultation of the Galactic Center

1989 ◽  
Vol 136 ◽  
pp. 509-512
Author(s):  
D. A. Simons ◽  
E. E. Becklin ◽  
K. -W Hodapp
Keyword(s):  
High Resolution ◽  
Computer Simulations ◽  
Near Infrared ◽  
Infrared Imaging ◽  
Galactic Center ◽  
Near Infrared Imaging ◽  
Lunar Occultation ◽  
Angular Extent ◽  
K Band

A high resolution K-band (2.2 μm) image of the Galactic center was acquired as part of an effort to develop computer simulations of a lunar occultation of the IRS 16 region that was previously observed in 1986 September. Through our computer simulations and recent observations of another occultation that occurred in 1988 September, confident identifications of the objects detected during the 1986 September occultation were acquired. In particular, IRS 16C, 16SW, and 16NE were all identified and found to be unresolved (<0.05″ in angular extent).

The true nucleus of NGC 253 revealed by high-resolution near-infrared imaging

1994 ◽  
Vol 430 ◽  
pp. L33 ◽  
Author(s):  
Bruce J., III Sams ◽  
R. Genzel ◽  
A. Eckart ◽  
L. Tacconi-Garman ◽  
R. Hofmann
Keyword(s):  
High Resolution ◽  
Near Infrared ◽  
Infrared Imaging ◽  
Near Infrared Imaging

scholarly journals HIGH-RESOLUTION NEAR-INFRARED IMAGING OF SUBMILLIMETER GALAXIES

2013 ◽  
Vol 768 (2) ◽  
pp. 164 ◽  
Author(s):  
Paula Aguirre ◽  
Andrew J. Baker ◽  
Felipe Menanteau ◽  
Dieter Lutz ◽  
Linda J. Tacconi
Keyword(s):  
High Resolution ◽  
Near Infrared ◽  
Infrared Imaging ◽  
Near Infrared Imaging ◽  
Submillimeter Galaxies

Diffraction Limited Near-Infrared Imaging of the Galactic Center

1994 ◽  
pp. 305-315 ◽  
Author(s):  
A. Eckart ◽  
R. Genzel ◽  
R. Hofmann ◽  
B. J. Sams ◽  
L. E. Tacconi-Garman ◽  
...  
Keyword(s):  
Near Infrared ◽  
Infrared Imaging ◽  
Galactic Center ◽  
Near Infrared Imaging

High-Resolution Near-Infrared Imaging and Polarimetry of Four Proto-Planetary Nebulae

2003 ◽  
Vol 126 (2) ◽  
pp. 848-862 ◽  
Author(s):  
Kate Y. L. Su ◽  
Bruce J. Hrivnak ◽  
Sun Kwok ◽  
Raghvendra Sahai
Keyword(s):  
High Resolution ◽  
Near Infrared ◽  
Infrared Imaging ◽  
Planetary Nebulae ◽  
Near Infrared Imaging

scholarly journals High-Resolution Near-Infrared Imaging of the Orion 114−426 Silhouette Disk

1998 ◽  
Vol 492 (2) ◽  
pp. L157-L161 ◽  
Author(s):  
Mark J. McCaughrean ◽  
Hua Chen ◽  
John Bally ◽  
Ed Erickson ◽  
Rodger Thompson ◽  
...  
Keyword(s):  
High Resolution ◽  
Near Infrared ◽  
Infrared Imaging ◽  
Near Infrared Imaging

High-Resolution Near-Infrared Imaging of DNA Microarrays with Time-Resolved Acquisition of Fluorescence Lifetimes

2000 ◽  
Vol 72 (24) ◽  
pp. 5907-5917 ◽  
Author(s):  
Emanuel Waddell ◽  
Yun Wang ◽  
Wieslaw Stryjewski ◽  
Scott McWhorter ◽  
Alyssa C. Henry ◽  
...  
Keyword(s):  
High Resolution ◽  
Dna Microarrays ◽  
Near Infrared ◽  
Infrared Imaging ◽  
Fluorescence Lifetimes ◽  
Near Infrared Imaging ◽  
Time Resolved

scholarly journals High resolution near-infrared imaging of submillimeter galaxies

2012 ◽  
Vol 8 (S295) ◽  
pp. 53-54
Author(s):  
Paula Aguirre ◽  
Andrew J. Baker ◽  
Felipe Menanteau ◽  
Dieter Lutz ◽  
Linda J. Tacconi
Keyword(s):  
High Resolution ◽  
Ir Spectroscopy ◽  
Rest Frame ◽  
Near Infrared ◽  
Infrared Imaging ◽  
Near Infrared Imaging ◽  
Submillimeter Galaxies ◽  
Multiple Component ◽  
Stellar Masses

AbstractWe have obtained high-resolution F110W (~ J) and F160W (~ H) band observations of ten submillimeter galaxies (SMGs) with the Hubble Space Telescope's NICMOS camera, in order to resolve their rest-frame optical morphologies, determine the existence of multiple-component, merger-like configurations, and estimate their stellar masses. The selected targets have redshifts in the range 2.2≤ z ≤ 2.81 confirmed with millimeter or mid-IR spectroscopy, guaranteeing that the two bands sample the galaxies' rest-frame optical light with the Balmer break falling between them.

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