Matches in SemOpenAlex for { <https://semopenalex.org/work/W2896818977> ?p ?o ?g. }
- W2896818977 abstract "The evolution of galaxies through cosmic time is studied observationally by means of extragalactic surveys. The OTELO survey aims to provide the deepest narrow-band survey to date in terms of minimum detectable flux and emission line equivalent width in order to detect the faintest extragalactic emission line systems. In this way, OTELO data will complements other broad-band, narrow-band, and spectroscopic surveys. The red tunable filter of the OSIRIS instrument on the 10.4 m Gran Telescopio Canarias (GTC) is used to scan a spectral window centred at $9175 A$, which is free from strong sky emission lines, with a sampling interval of $6 A$ and a bandwidth of $12 A$ in the most deeply explored Extended Groth Strip region. Careful data reduction using improved techniques for sky ring subtraction, accurate astrometry, photometric calibration, and source extraction enables us to compile the OTELO catalogue. This catalogue is complemented with ancillary data ranging from deep X-ray to far-infrared, including high resolution HST images, which allow us to segregate the different types of targets, derive precise photometric redshifts, and obtain the morphological classification of the extragalactic objects detected. The OTELO multi-wavelength catalogue contains 11237 entries and is 50% complete at AB magnitude 26.38. Of these sources, 6600 have photometric redshifts with an uncertainty $z_{phot}$ better than $0.2 (1+z_{phot})$. A total of 4336 of these sources correspond to preliminary emission line candidates, which are complemented by 81 candidate stars and 483 sources that qualify as absorption line systems. The OTELO survey products were released to the public on 2019." @default.
- W2896818977 created "2018-10-26" @default.
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- W2896818977 date "2020-01-30" @default.
- W2896818977 modified "2023-10-18" @default.
- W2896818977 title "The OTELO survey. I. Description, data reduction, and multi-wavelength catalogue." @default.
- W2896818977 cites W1602234112 @default.
- W2896818977 cites W1606613558 @default.
- W2896818977 cites W1845541610 @default.
- W2896818977 cites W1909359706 @default.
- W2896818977 cites W1943651020 @default.
- W2896818977 cites W1963620316 @default.
- W2896818977 cites W1963762696 @default.
- W2896818977 cites W1967651622 @default.
- W2896818977 cites W1980113072 @default.
- W2896818977 cites W1986538355 @default.
- W2896818977 cites W1989197256 @default.
- W2896818977 cites W1992083220 @default.
- W2896818977 cites W1992333888 @default.
- W2896818977 cites W1996537612 @default.
- W2896818977 cites W1998961346 @default.
- W2896818977 cites W1999977742 @default.
- W2896818977 cites W2003368276 @default.
- W2896818977 cites W2003738313 @default.
- W2896818977 cites W2007347039 @default.
- W2896818977 cites W2007486487 @default.
- W2896818977 cites W2012056991 @default.
- W2896818977 cites W2013741966 @default.
- W2896818977 cites W2018460805 @default.
- W2896818977 cites W2018489450 @default.
- W2896818977 cites W2021330485 @default.
- W2896818977 cites W2023873184 @default.
- W2896818977 cites W2024175772 @default.
- W2896818977 cites W2024740753 @default.
- W2896818977 cites W2027297109 @default.
- W2896818977 cites W2029350434 @default.
- W2896818977 cites W2033030037 @default.
- W2896818977 cites W2033450606 @default.
- W2896818977 cites W2042420315 @default.
- W2896818977 cites W2045727862 @default.
- W2896818977 cites W2060903742 @default.
- W2896818977 cites W2070131106 @default.
- W2896818977 cites W2074747635 @default.
- W2896818977 cites W2074997007 @default.
- W2896818977 cites W2088633531 @default.
- W2896818977 cites W2090231561 @default.
- W2896818977 cites W2091306090 @default.
- W2896818977 cites W2095855161 @default.
- W2896818977 cites W2100211542 @default.
- W2896818977 cites W2100336040 @default.
- W2896818977 cites W2100833883 @default.
- W2896818977 cites W2103593181 @default.
- W2896818977 cites W2104001357 @default.
- W2896818977 cites W2104604189 @default.
- W2896818977 cites W2125512696 @default.
- W2896818977 cites W2129217551 @default.
- W2896818977 cites W2130615420 @default.
- W2896818977 cites W2135759522 @default.
- W2896818977 cites W2137380495 @default.
- W2896818977 cites W2142238829 @default.
- W2896818977 cites W2146097816 @default.
- W2896818977 cites W2147847259 @default.
- W2896818977 cites W2150772486 @default.
- W2896818977 cites W2151062050 @default.
- W2896818977 cites W2155705849 @default.
- W2896818977 cites W2157917411 @default.
- W2896818977 cites W2158354392 @default.
- W2896818977 cites W2158528198 @default.
- W2896818977 cites W2159822406 @default.
- W2896818977 cites W2160298774 @default.
- W2896818977 cites W2162125418 @default.
- W2896818977 cites W2167335950 @default.
- W2896818977 cites W2169309103 @default.
- W2896818977 cites W2171144488 @default.
- W2896818977 cites W2334088617 @default.
- W2896818977 cites W2520722502 @default.
- W2896818977 cites W2591733255 @default.