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相关论文: Dusty ERO Search behind Two Massive Clusters

200 篇论文

We present high-spatial-resolution ($\sim 0.12''$ or $\approx 800 \, {\rm pc}$ at $z = 4.5$) ALMA $870\,\mu$m dust continuum observations of a sample of 44 ultrared dusty star-forming galaxies (DSFGs) selected from the H-ATLAS and HerMES…

Galaxy clusters at high redshift present a superb opportunity to study galaxy evolution, with large galaxy samples at fixed distances. Several lines of evidence point towards large formation redshifts and passive evolution for cluster…

天体物理学 · 物理学 2009-03-02 S. C. Chapman , P. McCarthy , S. E. Persson

We present a panoramic narrow-band study of H-alpha emitters in the field of the z=2.16 proto-cluster around PKS1138-262 using MOIRCS on the Subaru Telescope. We find 83 H-alpha emitters down to a SFR(Ha)~10Msun/yr across a ~7'x7' region…

宇宙学与河外天体物理 · 物理学 2015-06-11 Yusei Koyama , Tadayuki Kodama , Ken-ichi Tadaki , Masao Hayashi , Masayuki Tanaka , Ian Smail , Ichi Tanaka , Jaron Kurk

In this paper we present deep VLT multi wavelength imaging observations of the field around the radio galaxy PKS 1138-262 aimed at detecting and studying a (potential) proto-cluster centered at this radio source. PKS 1138-262 is a massive…

天体物理学 · 物理学 2009-11-10 J. D. Kurk , L. Pentericci , H. J. A. Roettgering , G. K. Miley

During the course of a gravitational lensing survey of distant, X-ray selected, EMSS clusters of galaxies, we have studied 6 X-ray luminous (Lx > 5x10^44 h_{50}^{-2} erg s^{-1}) clusters at redshifts exceeding z=0.5. All of these clusters…

天体物理学 · 物理学 2016-08-30 G. A. Luppino , I. M. Gioia

We present the results of VLT optical spectroscopy of a complete sample of 78 EROs with R-Ks\geq5 over a field of 52 arcmin^2. About 70% of the 45 EROs with Ks\leq19.2 have been spectroscopically identified with old passively evolving and…

We present a wide-field H-alpha imaging survey of the rich cluster CL0939+4713 (Abell 851) at z=0.41 with Suprime-Cam on the Subaru Telescope, using the narrow-band filter NB921. The survey is sensitive to active galaxies with star…

宇宙学与河外天体物理 · 物理学 2015-05-27 Yusei Koyama , Tadayuki Kodama , Fumiaki Nakata , Kazuhiro Shimasaku , Sadanori Okamura

We present environmental dependence of dusty star forming activity in and around the cluster RXJ1716.4+6708 at z=0.81 based on wide-field and multi-wavelength observations with Suprime-Cam on the Subaru telescope and IRC onboard the AKARI…

We analyze the X-ray properties of a near-infrared selected (Ks < 20) sample of spectroscopically identified Extremely Red Objects (R-Ks>5) in a region of the Chandra Deep Field-South using the public 1 Ms observation. The 21 objects were…

天体物理学 · 物理学 2009-11-07 M. Brusa , A. Comastri , E. Daddi , A. Cimatti , M. Mignoli , L. Pozzetti

SMM J04542-0301 is an extended (~1 arcmin) sub-mm source located near the core of the cluster MS0451.6-0305. It has been suggested that part of its emission arises from the interaction between a LBG and two EROs at z~2.9 that are…

宇宙学与河外天体物理 · 物理学 2015-05-14 A. Berciano Alba , L. V. E. Koopmans , M. A. Garrett , O. Wucknitz , M. Limousin

We use deep near-infrared and submillimeter observations of three massive lensing cluster fields, A370, A851, and A2390, to determine the average submillimeter properties of a K'-selected sample. The 38 Extremely Red Objects (EROs; I-K'>4)…

天体物理学 · 物理学 2009-11-07 E. H. Wehner , A. J. Barger , J. -P. Kneib

This paper presents a search for high redshift galaxies from the Euclid Early Release Observations program "Magnifying Lens." The 1.5 deg$^2$ area covered by the twin Abell lensing cluster fields is comparable in size to the few other deep…

星系天体物理 · 物理学 2025-04-30 J. R. Weaver , S. Taamoli , C. J. R. McPartland , L. Zalesky , N. Allen , S. Toft , D. B. Sanders , H. Atek , R. A. A. Bowler , D. Stern , C. J. Conselice , B. Mobasher , I. Szapudi , P. R. M. Eisenhardt , G. Murphree , I. Valdes , K. Ito , S. Belladitta , P. A. Oesch , S. Serjeant , D. J. Mortlock , N. A. Hatch , M. Kluge , B. Milvang-Jensen , G. Rodighiero , E. Bañados , J. M. Diego , R. Gavazzi , G. Congedo , M. Shuntov , H. Dole , P. -F. Rocci , T. Saifollahi , M. Miluzio , M. Ezziati , A. C. N. Hughes , J. -C. Cuillandre , R. Laureijs , S. Paltani , M. Schirmer , C. Stone , N. Aghanim , B. Altieri , A. Amara , S. Andreon , N. Auricchio , M. Baldi , A. Balestra , S. Bardelli , R. Bender , C. Bodendorf , D. Bonino , E. Branchini , M. Brescia , J. Brinchmann , S. Camera , V. Capobianco , C. Carbone , V. F. Cardone , J. Carretero , S. Casas , F. J. Castander , M. Castellano , S. Cavuoti , A. Cimatti , L. Conversi , Y. Copin , L. Corcione , F. Courbin , H. M. Courtois , A. Da Silva , H. Degaudenzi , A. M. Di Giorgio , J. Dinis , M. Douspis , F. Dubath , X. Dupac , A. Ealet , M. Farina , S. Farrens , S. Ferriol , S. Fotopoulou , M. Frailis , E. Franceschi , P. Franzetti , S. Galeotta , W. Gillard , B. Gillis , C. Giocoli , P. Gómez-Alvarez , A. Grazian , F. Grupp , L. Guzzo , S. V. H. Haugan , J. Hoar , H. Hoekstra , W. Holmes , I. Hook , F. Hormuth , A. Hornstrup , P. Hudelot , K. Jahnke , M. Jhabvala , E. Keihänen , S. Kermiche , A. Kiessling , T. Kitching , B. Kubik , M. Kümmel , M. Kunz , H. Kurki-Suonio , O. Lahav , D. Le Mignant , S. Ligori , P. B. Lilje , V. Lindholm , I. Lloro , D. Maino , E. Maiorano , O. Mansutti , O. Marggraf , K. Markovic , N. Martinet , F. Marulli , R. Massey , D. C. Masters , S. Maurogordato , H. J. McCracken , E. Medinaceli , S. Mei , M. Melchior , Y. Mellier , M. Meneghetti , E. Merlin , G. Meylan , J. J. Mohr , M. Moresco , L. Moscardini , R. Nakajima , R. C. Nichol , S. -M. Niemi , C. Padilla , F. Pasian , K. Pedersen , W. J. Percival , V. Pettorino , S. Pires , G. Polenta , M. Poncet , L. A. Popa , L. Pozzetti , F. Raison , A. Renzi , J. Rhodes , G. Riccio , E. Romelli , M. Roncarelli , E. Rossetti , R. Saglia , D. Sapone , P. Schneider , T. Schrabback , A. Secroun , G. Seidel , S. Serrano , C. Sirignano , G. Sirri , L. Stanco , P. Tallada-Crespí , A. N. Taylor , H. I. Teplitz , I. Tereno , R. Toledo-Moreo , I. Tutusaus , L. Valenziano , T. Vassallo , A. Veropalumbo , Y. Wang , J. Weller , E. Zucca , C. Burigana , G. Castignani , Z. Sakr , V. Scottez , M. Viel , P. Simon , J. Martín-Fleitas , D. Scott

We report the discovery of an intrinsically faint, quintuply-imaged, dusty galaxy MACS0600-z6 at a redshift $z=$6.07 viewed through the cluster MACSJ0600.1-2008 ($z$=0.46). A $\simeq4\sigma$ dust detection is seen at 1.2mm as part of the…

We present near-infrared VLT-UT1+ISAAC spectroscopy of a sample of 9 extremely red galaxies (ERGs) with R-K>5 and K<19.0. Neither strong emission lines (F_lim<1-5 10^{-16} erg s^{-1}cm^{-2}) nor continuum breaks are detected. From…

We present near-infrared observations of the environments around three radio-loud sources (MG1 J0442+0202, 3C 068.2, and MS 1426.9+1052) at redshifts z=1.10,1.57, and 1.83 (respectively), that are surrounded by near-infrared galaxy…

星系天体物理 · 物理学 2015-08-06 J. R. Franck , S. S. McGaugh , J. M. Schombert

We report a discovery of a proto-cluster in vigorous assembly and hosting strong star forming activities, associated to a radio galaxy USS 1558-003 at z=2.53, as traced by a wide-field narrow-band H_alpha imaging with MOIRCS on Subaru…

宇宙学与河外天体物理 · 物理学 2015-06-05 Masao Hayashi , Tadayuki Kodama , Ken-ichi Tadaki , Yusei Koyama , Ichi Tanaka

We present a photometric analysis of all high Galactic lattitude (|b| > 20d) broad-band parallel images taken by the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) instrument during its initial lifetime in HST Cycle 7. These…

天体物理学 · 物理学 2009-10-31 Michael R. Corbin , Earl O'Neil , Rodger I. Thompson , Marcia J. Rieke , Glenn Schneider

(abridged) We present panoramic Spitzer MIPS 24um observations covering 9x9Mpc (25'x25') fields around two massive clusters, Cl0024+16 and MS0451-03, at z=0.39 and z=0.55. Our observations cover a very wide range of environments within…

天体物理学 · 物理学 2008-11-26 J. E. Geach , Ian Smail , R. S. Ellis , S. M. Moran , G. P. Smith , T. Treu , J. -P. Kneib , A. C. Edge , T. Kodama

The Red MSX Source (RMS) survey is a multi-wavelength programme of follow-up observations designed to distinguish between genuine massive young stellar objects (MYSOs) and other embedded or dusty objects, such as ultra compact (UC) HII…

天体物理学 · 物理学 2007-05-23 J. C. Mottram , J. S. Urquhart , M. G. Hoare , S. L. Lumsden , R. D. Oudmaijer

(Abridged) We present deep Keck spectroscopy, using the DEIMOS and LRIS spectrographs, of a large and representative sample of 67 ``Extremely Red Objects'' (EROs) to H=20.5, with I-H>3.0, in three of the Las Campanas Infrared Survey fields.…

天体物理学 · 物理学 2009-11-11 M. Doherty , A. J. Bunker , R. S. Ellis , P. J. McCarthy