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    1. http://www.atnf.csiro.au/research/workshops/2013/astroinformatics/talks/Whiting-ASKAP-sourcefinding-Astroinformatics2013.pdf
    ... N (e.g. Continuum) Imager Pipeline UV Data 300 Channels (1MHz) Imager (cimager) Images Source Finder/ Identifier Source Catalog Imager (cimager) Source Finder/ Identifier Source Catalog Image Cube Sky Model Service Transient Detector Pipeline Transient ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/workshops/2013/astroinformatics/talks/Whiting-ASKAP-sourcefinding-Astroinformatics2013.pdf -- 2749.0 Кб -- 13.12.2013
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    2. ATLAS Source List Export Page
    ... of multi-component sources without infrared identification, the coordinates are a ... S3ID CDFS: Data for SWIRE3 sources cross-identified against ATLAS sources are taken ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Emil.Lenc/export.php -- 22.0 Кб -- 02.10.2012
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    3. http://www.atnf.csiro.au/research/workshops/2012/ALMA/Edwards_ALMAWorkshop2012.pdf
    ... radio-loud AGN as variable gamma-ray sources (and many unidentified sources) ·Fermi (2000s) maps the sky each day with better ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/workshops/2012/ALMA/Edwards_ALMAWorkshop2012.pdf -- 1835.6 Кб -- 20.03.2012
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    4. Results
    ... Given that about 26% of our sources have identifications we expect that at most (2 ... The unidentified sources are expected to be associated with objects below the plate ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/14_3/haigh/paper/node5.html -- 51.6 Кб -- 08.04.2016
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    5. Radio to H Comparison of the Sources towards the Large Magellanic Cloud
    ... The basic criterion for positive source identification is that a source must lie within 2.5'б of its counterpart. ... defined in Paperб IV) and the H sources, and retrospectively justifies the initial identification criteria of 2.5'б (which is ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/filipovic/paper/node3.html -- 52.6 Кб -- 08.04.2016
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    6. http://www.atnf.csiro.au/outreach/education/teachers/resources/sample_astro_assess_talkv2.doc
    ... Working individually, you are to identify data sources, gather, process and present ... Identify data sources, gather, process and present information to assess the impact ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/outreach/education/teachers/resources/sample_astro_assess_talkv2.doc -- 59.0 Кб -- 22.01.2014
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    7. http://www.atnf.csiro.au/research/WALLABY/Wallaby2010/RJurek-Wallaby2010.pdf
    ... Meyer · Finding sources · · + · · Mexican hat Debauchies mirrored Coiflet Haar · Debauchies (+ mirrored) should identify double ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/WALLABY/Wallaby2010/RJurek-Wallaby2010.pdf -- 1175.1 Кб -- 08.12.2010
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    8. Optical Identification Strategies for the Molonglo Cluster Survey
    ... procedure for making optical identifications of radio sources in Abell cluster ... were essential for securing identifications for the extended sources prevalent among ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/14_3/haigh/paper/index.html -- 52.1 Кб -- 08.04.2016
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    9. http://www.atnf.csiro.au/people/rnorris/papers/n233.pdf
    ... 3.4 Source Identification and Measurement Source extraction algorithms are already ... or more) ASKAP frequency bands, the sources identified in the lowest frequency band ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/rnorris/papers/n233.pdf -- 150.4 Кб -- 15.09.2009
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    10. ATCA_mm_science
    ... Of the 574 candidate sources identified, 226 distinct sources were confirmed (with fluxes > 60 mJy) in follow-up observations ... All of the extragalactic sources could be identified in the 843-MHz SUMSS catalogue, with most also having bright optical ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/newsletter/feb03/ATCA_mm_sciencefnl.htm -- 7.6 Кб -- 23.01.2013
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