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With the Spitzer Space Telescope Infrared Spectrograph (IRS) we have observed seven powerful FR2 radio galaxies and seven quasars. Both samples, the galaxies and the quasars, are comparable in isotropic 178 MHz luminosity (10^26.5 W/Hz < P…

Astrophysics · Physics 2009-11-11 Martin Haas , Ralf Siebenmorgen , Bernhard Schulz , Endrik Kruegel , Rolf Chini

We present the 2-200 um Infrared Space Observatory (ISO) spectrum and 3.8-20 um ISAAC and TIMMI2 images of the extreme OH/IR star IRAS 16342-3814. Amorphous silicate absorption features are seen, together with crystalline silicate…

Astrophysics · Physics 2009-11-07 C. Dijkstra , L. B. F. M. Waters , F. Kemper , M. Min , M. Matsuura , A. Zijlstra , A. de Koter , C. Dominik

We present the broadband (0.5-100 keV) spectra of three heavily obscured Active Galactic Nuclei (AGNs), NGC 1106, UGC 03752, and NGC 2788A, observed with Suzaku and Swift/Burst Alert Telescope (BAT). The targets are selected from the…

Astrophysics of Galaxies · Physics 2016-03-23 Atsushi Tanimoto , Yoshihiro Ueda , Taiki Kawamuro , Claudio Ricci

We present a comprehensive study of X-ray absorption by sulfur (S), argon (Ar), and calcium (Ca) in the interstellar medium (ISM) along the line of sight to the low-mass X-ray binary MAXI J1744$-$294, using high-resolution XRISM Resolve…

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 results from a coordinated $XMM$-$Newton$+$NuSTAR$ observation of the type 1.8 Seyfert galaxy IRAS 13197-1627. This is a highly complex source, with strong contributions from relativistic reflection from the inner accretion disk,…

High Energy Astrophysical Phenomena · Physics 2017-12-06 D. J. Walton , M. Brightman , G. Risaliti , A. C. Fabian , F. Fuerst , F. A. Harrison , A. Lohfink , G. Matt , G. Miniutti , M. L. Parker , D. Stern

The fastest-rotating magnetar 1E 1547.0-5408 was observed in broad-band X-rays with Suzaku for 33 ks on 2009 January 28-29, 7 days after the onset of its latest bursting activity. After removing burst events, the absorption-uncorrected 2-10…

The extreme NLS1 galaxy IRAS 13224-3809 shows significant variability, frequency depended time lags, and strong Fe K line and Fe L features in the long 2011 XMM-Newton observation. In this work we study the spectral properties of IRAS…

High Energy Astrophysical Phenomena · Physics 2015-06-23 Chia-Ying Chiang , D. J. Walton , A. C. Fabian , D. R. Wilkins , L. C. Gallo

We model the time-variable absorption of FeII, FeIII, SiII, CII and CrII detected in UVES spectra of GRB 080310, with the afterglow radiation exciting and ionizing the interstellar medium in the host galaxy at a redshift of z=2.42743. To…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 P. M. Vreeswijk , C. Ledoux , A. J. J. Raassen , A. Smette , A. De Cia , P. R. Woźniak , A. J. Fox , W. T. Vestrand , P. Jakobsson

We report on deep XMM-Newton and NuSTAR observations of the high redshift, z=2.94, extremely red quasar (ERQ), SDSS J165202.60+172852.4, with known galactic ionized outflows detected via spatially-resolved [OIII] emission lines. X-ray…

We present new XMM-Newton and NuSTAR observations of the galaxy merger IRAS F05189-2524 which is classified as an ultra-luminous infrared galaxy (ULIRG) and optical Seyfert 2 at $z$ = 0.0426. We test a variety of spectral models which…

Astrophysics of Galaxies · Physics 2020-01-08 Robyn N. Smith , Francesco Tombesi , Sylvain Veilleux , Anne M. Lohfink , Alfredo Luminari

We report on a spectro-polarimetric analysis of four southern Ultra-Luminous Infrared Galaxies (ULIRGs), aimed at constraining the presence of hidden broad AGN lines. For IRAS 19254--7245 ({\sl The Superantennae}) we find evidence for a…

Astrophysics · Physics 2009-11-07 C. Pernechele , S. Berta , A. Marconi , C. Bonoli , A. Bressan , A. Franceschini , J. Fritz , E. Giro

We present the mid-infrared (MIR) spectra obtained with the Spitzer InfraRed Spectrograph (IRS) for a sample of 52 sources, selected as infrared luminous, z>1 candidates in the Extragalactic First Look Survey (XFLS). The sample selection…

We study the time variability of five Fe Low ionization Broad Absorption Line (FeLoBAL) QSOs using repeated spectroscopic observations with the 2m telescope at IUCAA Girawali observatory (IGO) spanning an interval of upto 10 years. We…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 M. Vivek , R. Srianand , P. Petitjean , P. Noterdaeme , V. Mohan , A. Mahabal , V. C. Kuriakose

We present a high spatial (diffraction-limited) resolution (~0.3") mid-infrared (MIR) spectroscopic study of the nuclei and star-forming regions of 4 local luminous infrared galaxies (LIRGs) using T-ReCS on the Gemini South telescope. We…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 T. Diaz-Santos , A. Alonso-Herrero , L. Colina , C. Packham , N. A. Levenson , M. Pereira-Santaella , P. F. Roche , C. M. Telesco

We report the timing and spectral properties of Be/X-ray binary pulsar GX 304-1 by using two Suzaku observations during its 2010 August and 2012 January X-ray outbursts. Pulsations at ~275 s were clearly detected in the light curves from…

Solar and Stellar Astrophysics · Physics 2016-02-16 Gaurava K. Jaisawal , Sachindra Naik , Prahlad Epili

The Infrared Spectrograph (IRS) onboard the Spitzer Space Telescope (SST) has been used to obtain low and moderate resolution spectra of the dust and gas-rich quasar APM08279+5255 (z=3.91). Broad Paschen $\alpha$ and $\beta$ recombination…

We report an analysis and modelling of new Suzaku observations of the Seyfert 1 galaxies Mrk509 and Mrk841, taken between April and November 2006,for Mrk509,and between January and July 2007,for Mrk841,for a total exposure time of ~100 ks…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-19 M. Cerruti , G. Ponti , C. Boisson , E. Costantini , A. L. Longinotti , G. Matt , M. Mouchet , P. O. Petrucci

We present Suzaku observations of five hard X-ray selected nearby Seyfert 2 galaxies. All the sources were clearly detected with the pin Hard X-ray Detector up to several tens of keV, allowing for a fairly good characterization of the…

High Energy Astrophysical Phenomena · Physics 2015-05-19 A. Comastri , K. Iwasawa , R. Gilli , C. Vignali , P. Ranalli , G. Matt , F. Fiore

This is the second paper in a series discussing the properties of ultraluminous infrared galaxies (ULIGs: L_ir > 10^{12} L_sun; Ho = 75 km s^{-1} Mpc^{-1} and qo = 0.0) from the 1-Jy sample of Kim (1995). This paper presents the first…

Astrophysics · Physics 2009-10-30 D. -C. Kim , S. Veilleux , D. B. Sanders