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相关论文: Extremely Red Objects from the NICMOS/HST Parallel…

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We present initial results from a redshift survey carried out with the Low Resolution Imaging Spectrograph on the 10~m W. M. Keck Telescope of a field 14.6 arc-min$^2$ in solid angle. In the redshift distribution of the 106 extragalactic…

天体物理学 · 物理学 2016-08-30 J. G. Cohen , D. W. Hogg , M. A. Pahre , R. Blandford

We present the first results from the HST/ACS Grism Parallel Survey, a large program obtaining deep, slitless ACS grism spectroscopy of high-latitude HST parallel fields. We report on 11 high Galactic latitude fields here, each with grism…

天体物理学 · 物理学 2009-09-29 Igor Drozdovsky , Lin Yan , Hsiao-Wen Chen , Daniel Stern , Robert Kennicutt , Hyron Spinrad , Steve Dawson

Low mass (sub)stellar objects represent the low end of the initial mass function, the transition to free-floating planets and a prominent interloper population in the search for high-redshift galaxies. Without proper motions or…

We describe an object in the Hubble Deep Field North with very unusual near-infrared properties. It is readily visible in Hubble Space Telescope NICMOS images at 1.6um and from the ground at 2.2um, but is undetected (with signal-to-noise <~…

High-resolution near-infrared HST NICMOS (F160W, F222M) images and polarization (2 um) observations were made of four bipolar proto-planetary nebulae (PPNs): IRAS 17150-3224, IRAS 17441-2411, IRAS 17245-3951, and IRAS 16594-4656. The first…

天体物理学 · 物理学 2009-11-07 Kate Y. L. Su , Bruce J. Hrivnak , Sun Kwok , Raghvendra Sahai

We present a catalog of 10718 objects in the COSMOS field observed through multi-slit spectroscopy with the Deep Imaging Multi-Object Spectrograph (DEIMOS) on the Keck II telescope in the wavelength range ~5500-9800A. The catalog contains…

At z=2.39, the cluster around 53W002 is one of the most distant groups or clusters of galaxies known to date. At this redshift the 4000A-break falls between the J and H bands, thus our infrared observations are designed to identify cluster…

天体物理学 · 物理学 2007-05-23 Ian Waddington

The LCIR Survey, using the Cambridge IR Survey Instrument (CIRSI), reaches H \~ 20-21 over ~1 deg^2. We present results for 744 arcmin^2 in which public UBVRI data exist. We compare optical-IR colours with predictions of a semi-analytic…

The paper presents the identification of the stars in the lower part of the Main Sequence among the objects of the deep survey of the equatorial region of the sky, performed by the eROSITA telescope at the SRG orbital observatory. Of the…

太阳与恒星天体物理 · 物理学 2021-09-28 Aleksey A. Shlyapnikov

Extremely red quasars, with bolometric luminosities exceeding $10^{47}$ erg s$^{-1}$, are a fascinating high-redshift population that is absent in the local universe. They are the best candidates for supermassive black holes accreting at…

We report the discovery of four extremely faint ($m_{\mathrm{F444W}}\gtrsim29$) red point sources in recent ultra-deep JWST/NIRCam images of the strong lensing galaxy cluster Abell S1063. All four sources sit in lensed arcs, on the symmetry…

We present HST NICMOS photometry of the resolved stellar population in NGC 1569. The CMD in the F110W and F160W photometric bands contains ~2400 stars with a formal photometric error < 0.1 mag down to J~23.5 and H~22.5. We describe the data…

天体物理学 · 物理学 2009-10-31 A. Aloisi , M. Clampin , E. Diolaiti , L. Greggio , Claus Leitherer , A. Nota , L. Origlia , G. Parmeggiani , M. Tosi

We present a targeted follow-up Hubble Space Telescope WFC3 F160W imaging study of very massive galaxies $(\log(M_{\rm{star}}/M_{\odot})> 11.2)$ selected from a combination of ground-based near-infrared galaxy surveys (UltraVISTA, NMBS-II,…

We report the first results from the Z-FOURGE survey: the discovery of a candidate galaxy cluster at z = 2.2 consisting of two compact overdensities with red galaxies detected at >20{\sigma} above the mean surface density. The discovery was…

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

Deep, wide, near-infrared imaging surveys provide an opportunity to study the clustering of various galaxy populations at high redshift on the largest physical scales. We have selected $1<z<2$ extremely red objects (EROs) and $1<z<3$…

宇宙学与河外天体物理 · 物理学 2015-05-19 J. -W. Kim , A. C. Edge , D. A. Wake , J. P. Stott

We have collected optical follow-up observations from the ground and the Hubble Space Telescope (HST) for 13.74 square ' of archival images taken with the Near Infrared Camera and Multi Object Spectrograph (NICMOS). We use two criteria to…

天体物理学 · 物理学 2009-10-31 Tommaso Treu , Massimo Stiavelli

Some indications for tension have long been identified between cosmological constraints obtained from galaxy clusters and primary CMB measurements. Typically, assuming the matter density and fluctuations, as parameterized with Omega_m and…

宇宙学与河外天体物理 · 物理学 2018-11-21 Weiwei Xu , Miriam E. Ramos-Ceja , Florian Pacaud , Thomas H. Reiprich , Thomas Erben

We report results from near-infrared imaging of IZw18, the most metal-poor galaxy in the local universe with NICMOS on board the Hubble Space Telescope (HST). Observations were obtained in the broad F205W filter ($\sim$ K) and in the…

天体物理学 · 物理学 2009-11-10 G. Ostlin , M. Mouhcine
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