The MUSEHubbleUltra Deep Field Survey
نویسندگان
چکیده
منابع مشابه
The Chandra Deep Field - North Survey . Xvi
We present X-ray spectral analyses of the three z > 4 Active Galactic Nuclei (AGNs) thus far spectroscopically identified in the Chandra Deep Field-North Survey, at redshifts of 5.186, 4.424, and 4.137. These analyses are made possible by the extremely deep exposure (≈ 2 Ms) and the low Chandra background. The rest-frame ≈ 2.5–40 keV spectra are the first for optically faint (two of the three s...
متن کاملThe Chandra Deep Field-south Survey: 2 Ms Source Catalogs
We present point-source catalogs for the ≈ 2 Ms exposure of the Chandra Deep Field-South (CDF-S); this is one of the two most-sensitive X-ray surveys ever performed. The survey covers an area of ≈ 436 arcmin2 and reaches on-axis sensitivity limits of ≈ 1.9× 10−17 and ≈ 1.3× 10−16 ergs cm−2 s−1 for the 0.5–2.0 and 2–8 keV bands, respectively. Four hundred and sixty-two X-ray point sources are de...
متن کاملSearch is Realized in the Hubble Ultra Deep Field Survey
The Hubble Ultra Deep Field Survey has not only provided the deepest optical and near infrared views of universe, but has enabled a search for the most distant supernovae to z ∼ 2.2. We have found four supernovae by searching spans of integrations of the Ultra Deep Field and the Ultra Deep Field Parallels taken with the Hubble Space Telescope paired with the Advanced Camera for Surveys and the ...
متن کاملThe VIRMOS deep imaging survey II: CFH12K BVRI optical data for the 0226-04 deep field⋆
In this paper we describe in detail the reduction, preparation and reliability of the photometric catalogues which comprise the CFH12K-VIRMOS deep field. This region, consisting of four contiguous pointings of the CFH12K wide-field mosaic camera, covers a total area of 1.2 deg. The survey reaches a limiting magnitude of BAB ∼ 26.5, VAB ∼ 26.2, RAB ∼ 25.9 and IAB ∼ 25.0 (corresponding to the poi...
متن کاملDeep R-band photometry of the Chandra Deep Field South from the COMBO-17 survey
We report on deep multi-color imaging (R5σ = 26.0) of the Chandra Deep Field South, obtained with the Wide Field Imager (WFI) at the MPG/ESO 2.2 m telescope on La Silla as part of the COMBO-17 survey. We include an overview of the COMBO-17 project and a detailed reduction scheme for WFI survey data. We discuss particular treatment necessary for accurate flatfielding of WFI images taken in the s...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Astronomy & Astrophysics
سال: 2017
ISSN: 0004-6361,1432-0746
DOI: 10.1051/0004-6361/201731579