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相关论文: Mid-Infrared Spectroscopy of Infrared Luminous Gal…

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We present a sample of low-resolution 5-38um Spitzer IRS spectra of the inner few square kiloparsecs of 59 nearby galaxies spanning a large range of star formation properties. A robust method for decomposing mid-infrared galaxy spectra is…

We present mid-infrared to optical properties of 22 representative irregular galaxies: 18 Im, 3 BCDs, and one Sm. The mid-IR is based on images from the Spitzer Space Telescope archives. The 3.6 and 4.5 micron bands and the UBVJHK images…

天体物理学 · 物理学 2008-11-26 Deidre A. Hunter , Bruce G. Elmegreen , Emily Martin

We present 5-38um mid-infrared spectra at a spectral resolution of R~65-130 of a large sample of 22 starburst nuclei taken with the Infrared Spectrograph IRS on board the Spitzer Space Telescope. The spectra show a vast range in starburst…

We present Spitzer/Infrared Spectrograph (IRS) 5-21 micron spectroscopic maps towards 12 regions in the Andromeda galaxy (M31). These regions include the nucleus, bulge, an active region in the star-forming ring, and 9 other regions chosen…

We report the initial results from a Spitzer GO-1 program to obtain low resolution, mid-infrared spectra of infrared luminous galaxies at z~1-2. This paper presents the spectra of eight sources observed with the Spitzer InfraRed…

天体物理学 · 物理学 2008-11-26 Lin Yan , R. Chary , L. Armus , H. Teplitz , G. Helou , D. Frayer , D. Fadda , J. Surace , P. Choi

We present mid-infrared spectra of sixteen optically faint sources with 70 micron fluxes in the range 19-38mJy. The sample spans a redshift range of 0.35<z<1.9, with most lying between 0.8<z<1.6, and has infrared luminosities of 10^{12} -…

宇宙学与河外天体物理 · 物理学 2014-11-18 D. Farrah , D. Weedman , C. Lonsdale , M. Polletta , M. Rowan-Robinson , J. Houck , H. Smith

We investigate the relationship between 8.44\,GHz brightness temperatures and 1.4 to 8.44\,GHz radio spectral indices with 6.2\,$\mu$m polycyclic aromatic hydrocarbon (PAH) emission and 9.7\,$\mu$m silicate absorption features for a sample…

宇宙学与河外天体物理 · 物理学 2015-06-15 E. J. Murphy , S. Stierwalt , L. Armus , J. J. Condon , A. S. Evans

We present mid-infrared spectra of 5 submillimeter galaxies at z=0.65-2.38 taken with the Spitzer Space Telescope. Four of these sources, at z<1.5, have strong PAH features and their composite spectrum is well fitted by an M82-like spectrum…

We investigate the mid-infrared radiation of galaxies that are powered by a starburst or by an AGN. For this end, we compare the spectra obtained at different spatial scales in a sample of infrared bright galaxies. ISO observations which…

天体物理学 · 物理学 2008-12-18 R. Siebenmorgen , E. Kr"ugel , H. W. W. Spoon

We present mid-infrared observations of 18 sources from a sample of 21 z~2 radio-intermediate obscured quasars. The mid-infrared spectra of the sources are continuum dominated, and 12 sources show deep silicate absorption with tau_9.7~1-2.…

天体物理学 · 物理学 2009-11-13 Alejo Martinez-Sansigre , Mark Lacy , Anna Sajina , Steve Rawlings

The study of the dominant population of high redshift IR-luminous galaxies (10^11 - 10^12 Lsun at 1<z<3), requires observation of sources at the ~0.1 mJy level in the mid-IR. We present the deepest spectra taken to date with the Infrared…

Near infrared spectra with resolution R ~ 1100 in the rest wavelength range 1.8-2.2 microns have been obtained for a complete sample of 33 ultraluminous infrared galaxies. Of the 33 objects observed, 2 show evidence of a central AGN through…

天体物理学 · 物理学 2012-08-27 T. W. Murphy, , B. T. Soifer , K. Matthews , J. R. Kiger , L. Armus

We present T-ReCS high spatial resolution N-band (8-13 micron) spectroscopy of the central regions (a few kpc) of 3 local LIRGs. The nuclear spectra show deep 9.7 micron silicate absorption feature and the high ionization [SIV]10.5 micron…

天体物理学 · 物理学 2007-05-23 T. Diaz-Santos , A. Alonso-Herrero , L. Colina , C. Packham , J. T. Radomski , C. M. Telesco

The paper is devoted to the understanding of the infrared emission of nuclear regions in galaxies. a) ISO data of NGC1808 are presented: spectro--photometry from 5.1 to 16.4 mic., a 25"x25" map at 6 mic. and 170mic. photometry. b) The data…

天体物理学 · 物理学 2009-11-06 R. Siebenmorgen , E. Kr"ugel , R. J. Laureijs

We measure IRAC colors of extended emission in several fields covering a range of Galactic latitudes and longitudes outside of star forming regions. We determine the nature of the Galactic diffuse emission in Spitzer/IRAC images by…

天体物理学 · 物理学 2009-02-24 N. Flagey , F. Boulanger , L. Verstraete , M. A. Miville Deschenes , A. Noriega Crespo , W. T. Reach

We present a catalog of mid-infrared (MIR) spectra of 150 infrared (IR) luminous galaxies in the Spitzer extragalactic first look survey obtained with IRS on board Spitzer. The sample is selected to be brighter than ~0.9 mJy at 24 micron…

宇宙学与河外天体物理 · 物理学 2009-08-05 Kalliopi M. Dasyra , Lin Yan , George Helou , Anna Sajina , Dario Fadda , Michel Zamojski , Lee Armus , Bruce Draine , David Frayer

We present results on low-resolution mid-infrared (MIR) spectra of 70 infrared-luminous galaxies obtained with the Infrared Spectrograph (IRS) onboard Spitzer. We selected sources from the European Large Area Infrared Survey (ELAIS) with…

We present the results of infrared 2.8-4.1 micron (L-band) spectroscopy of nearby infrared luminous galaxies with possible signatures of dust-obscured active galactic nuclei (AGNs) in data at other wavelengths. The samples are chosen to…

天体物理学 · 物理学 2008-11-26 Masatoshi Imanishi

We present mid-infrared spectroscopy obtained with the Spitzer Space Telescope of a sample of 11 optically faint, infrared luminous galaxies selected from a Spitzer MIPS 70um imaging survey of the NDWFS Bootes field. These are the first…

We present data from mid-infrared Keck Telescope imaging of 18 radio-selected ultra-compact HII region candidates at diffraction-limited resolution. The goal of these observations is to determine the sizes, luminosities, and morphologies of…

天体物理学 · 物理学 2008-11-26 Uriel Giveon , Matthew J. Richter , Robert H. Becker , Richard L. White
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