نتایج جستجو برای: infrared source

تعداد نتایج: 517719  

2008
Chris P. Pearson Woong-Seob Jeong Shuji Matsuura Hideo Matsuhara Takao Nakagawa Hiroshi Shibai Mitsunobu Kawada Toshinobu Takagi Hyung Mok Lee Mai Shirahata

We investigate the segregation of the extragalactic population via colour criteria to produce an efficient and inexpensive methodology to select specific source populations as a function of far-infrared flux. Combining galaxy evolution scenarios and a detailed spectral library of galaxies, we produce simulated catalogues incorporating segregation of the extragalactic population into component t...

2008
Lusine Sargsyan Areg Mickaelian Daniel Weedman James Houck

Extragalactic sources from the IRAS Faint Source Catalog (FSC) which have the optically faintest magnitudes (E & 18) were selected by spatial coincidence with a source in the FIRST radio survey, and 28 of these sources have been observed with the Infrared Spectrograph on Spitzer (IRS). While an infrared source is always detected with the IRS at the FIRST position, only ∼ 50% of the infrared sou...

2004
L. J. Greenhill

We present Keck LWS images of the Orion BN/KL star forming region obtained in the first multi-wavelength study to have 0. 3-0. 5 resolution from 4.7μm to 22μm. The young stellar objects designated infrared sourcen and radio source I are believed to dominate the BN/KL region. We have detected extended emission from a probable accretion disk around sourcen but infer a stellar luminosity on the or...

2011
Charles W. Clark Luis Orozco

Title of Document: Sum-frequency Generation in Laser Safety and Quantum Telecommunications Applications Jemellie Galang Houston, Master of Science, 2011 Directed By: Dr. Charles W. Clark This thesis describes the implications of sum-frequency generation in both laser safety and quantum telecommunications applications. Green laser pointer technology uses frequency doubling of invisible 1064 nm i...

1999
R. Chary E. E. Becklin A. S. Evans G. Neugebauer N. Z. Scoville K. Matthews M. E. Ressler

We present high resolution imaging of the nucleus of NGC4258 from 1 μm to 18 μm. Our observations reveal that the previously discovered compact source of emission is unresolved even at the near-infrared resolution of ∼0.2 FWHM which corresponds to about 7 pc at the distance of the galaxy. This is consistent with the source of emission being the region in the neighborhood of the purported 3.5×10...

2001
Kirk H. Michaelian Richard S. Jackson

The use of synchrotron radiation ~SR! as a farand mid-infrared source in the measurement of photoacoustic Fourier transform infrared spectra of solids is demonstrated for the first time in this work. Initial experiments were performed at beamline U10A at the National Synchrotron Light Source, Brookhaven National Laboratory. For synchrotron photoacoustic spectroscopy to be feasible, it must yiel...

Journal: :journal of nanostructures 2015
m. mansournia f. azizi

magnetite (fe3o4) nanoparticles have been successfully prepared by a novel one-step and surfactant-free approach utilizing ferrous ion, as a single iron source. in this manner, the reaction occurs between two aqueous solutions via the spontaneous transfer of ammonia gas from one to another in room temperature. no ferric source or oxidizing specie, oxidation controlling and capping agents are ne...

1997
C. C. Dudley C. G. Wynn-Williams

New mid-infrared (10 and 20 μm) spectro-photometry of the ultraluminous infrared galaxy IRAS 08572+3915 is presented. The 10 μm spectrum reveals a deep silicate absorption feature, while the 20 μm spectrum shows no clear evidence for an 18 μm silicate absorption feature. An interstellar extinction curve is fitted to IRAS 08572+3915 and two other deep silicate infrared galaxies, NGC 4418 and Arp...

2015
Emily Wisnioski Karl Glazebrook Chris Blake A. Mark Swinbank

We present the far-infrared-derived dust properties from Herschel Spectral and Photometric Imaging Receiver of the WiggleZ kinematic sample of 13 star-forming galaxies at z ∼ 1.3, with existing ancillary ∼kpc resolution integral field spectroscopy. We detect three galaxies individually and place limits on the remainder by stacking. The detected galaxies, two clumpy discs and one merger have col...

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