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相关论文: 3C 273 Host Galaxy with Hubble Space Telescope Cor…

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Star-forming galaxies are considered to be the leading candidate sources that dominate the cosmic reionization at z>7, and the search for analogs at moderate redshift showing Lyman continuum (LyC) leakage is currently a active line of…

Archival Hubble Space Telescope WFPC2 images were used to search for optical emission associated with the radio jets of a number of luminous quasars. From this search, we report new optical hotspot detections in the well-known blazar…

天体物理学 · 物理学 2009-11-10 C. C. Cheung , J. F. C. Wardle , T. Chen

We present new rest frame UV and visible observations of 22 high-redshift (1 < z < 2.5) 3C radio galaxies and QSOs obtained with the Hubble Space Telescope's (HST) Wide Field Camera 3 (WFC3) instrument. Using a custom data reduction…

We present an unprecedented view on the morphology and kinematics of the extended narrow-line region (ENLR) and molecular gas around the prototypical hyper-luminous quasar 3C273 ($L\sim10^{47}$ erg/s at z=0.158) based on VLT-MUSE optical 3D…

星系天体物理 · 物理学 2019-07-17 B. Husemann , V. N. Bennert , K. Jahnke , T. A. Davis , J. -H. Woo , J. Scharwächter , A. Schulze , M. Gaspari , M. Zwaan

We estimate the amount of negative feedback energy injected into the ISM of the host galaxy of 3C273, a prototypical radio loud quasar. We obtained 93, 233 and 343 GHz continuum images with the Atacama Large Millimeter/Sub-millimeter Array…

星系天体物理 · 物理学 2022-05-11 Shinya Komugi , Yoshiki Toba , Yoshiki Matsuoka , Toshiki Saito , Takuji Yamashita

We present Space-VLBI RadioAstron observations at 1.6 GHz and 4.8 GHz of the flat spectrum radio quasar 3C 273, with detections on baselines up to 4.5 and 3.3 Earth Diameters, respectively. Achieving the best angular resolution at 1.6 GHz…

We have used the F160W filter (1.4-1.8 um) and the coronagraph on the Near-InfraRed Camera and Multi-Object Spectrometer (NICMOS) on the Hubble Space Telescope (HST) to survey 45 single stars with a median age of 0.15 Gyr, an average…

We report on the discovery of an extended stellar halo surrounding the distant Galactic globular cluster NGC 5694, based on new deep (V ~ 24.5) wide-field (24' * 20') photometry acquired with VIMOS at VLT. Stars with colour and magnitude…

太阳与恒星天体物理 · 物理学 2015-05-28 M. Correnti , M. Bellazzini , E. Dalessandro , A. Mucciarelli , L. Monaco , M. Catelan

We report results from Chandra observations of the X-ray jet of 3C~273 during the calibration phase in 2000 January. The zeroeth-order images and spectra from two 40-ks exposures with the HETG and LETG+ACIS-S show a complex X-ray structure.…

天体物理学 · 物理学 2009-11-06 Rita M. Sambruna , C. Megan Urry , F. Tavecchio , L. Maraschi , R. Scarpa , G. Chartas , T. Muxlow

We present a study of the morphology and intensity of star formation in the host galaxies of eight Palomar-Green quasars using observations with the Hubble Space Telescope. Our observations are motivated by recent evidence for a close…

宇宙学与河外天体物理 · 物理学 2015-06-17 J. E. Young , M. Eracleous , O. Shemmer , H. Netzer , C. Gronwall , Dieter Lutz , R. Ciardullo , Eckhard Sturm

We show initial results from our ongoing HST GHOSTS survey of the resolved stellar envelopes of 14 nearby, massive disk galaxies. In hierarchical galaxy formation the stellar halos and thick disks of galaxies are formed by accretion of…

Context: ASPIICS is a novel externally occulted solar coronagraph, which will be launched onboard the PROBA-3 mission of the European Space Agency. The external occulter will be placed on the first satellite approximately 150 m ahead of the…

天体物理仪器与方法 · 物理学 2019-02-06 S. V. Shestov , A. N. Zhukov , D. B. Seaton

A significant minority of high redshift radio galaxy (HzRG) candidates show extremely red broad band colours and remain undetected in emission lines after optical `discovery' spectroscopy. In this paper we present deep GTC optical imaging…

In this paper we present near infrared (NIR) imaging data of the host galaxy of the broad absorption line quasar (BALQ) at z=2.169, serendipitously found close to 3C48. The data were obtained with the ESO-VLT camera ISAAC during period 67.…

天体物理学 · 物理学 2009-11-11 J. Zuther , A. Eckart

We present and discuss European VLBI Network UHF band spectral line observations, made to localise the redshifted 21cm HI absorption known to occur in the subgalactic sized compact steep spectrum galaxies 3C 49 and 3C 268.3. We have…

天体物理学 · 物理学 2009-11-11 A. Labiano , R. C. Vermeulen , P. D. Barthel , C. P. O'Dea , J. F. Gallimore , S. Baum , W. de Vries

We present the analysis of a sample of 20 bright low-redshift quasars (M_B<-23 and z < 0.35) observed spectroscopically with the VLT. The FORS1 spectra, obtained in Multi Object Spectroscopy (MOS) mode, allow to observe simultaneously the…

天体物理学 · 物理学 2008-11-26 G. Letawe , P. Magain , F. Courbin , P. Jablonka , K. Jahnke , G. Meylan , L. Wisotzki

We report on Hubble Space Telescope (HST) observations of the host galaxy of GRB 971214, about four months after the burst. The redshift of the proposed host galaxy at z=3.418, combined with optical and radio observations of the burst…

We will present the results of a NICMOS H-band imaging survey of a small sample of z ~ 2 to 3 radio-quiet quasars. We have resolved extension in at least 4 of 5 objects and find evidence for a wide range in the morphologies and magnitudes…

天体物理学 · 物理学 2009-10-31 S. Ridgway , T. Heckman , D. Calzetti , M. Lehnert

Here we present the spectropolarimetric observations of the radio loud active galaxy 3C 390.3 in the period 2009-2014 (24 epochs). The galaxy has been observed with the 6-meter telescope of SAO RAS using the SCORPIO spectropolarimeter. We…

星系天体物理 · 物理学 2015-06-23 V. L. Afanasiev , A. I. Shapovalova , L. C. Popovic , N. V. Borisov

We examine 20 diffuse and translucent Galactic sight lines and extract the column densities of the ^12CO and ^13CO isotopologues from their ultraviolet A--X absorption bands detected in archival Space Telescope Imaging Spectrograph data…

天体物理学 · 物理学 2009-11-13 Y. Sheffer , M. Rogers , S. R. Federman , D. L. Lambert , R. Gredel