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    91. Observations and Results
    ... To investigate the possibility of discovering an Cha radio star that was not in the X-ray sample, we searched for optical counterparts of six bright sources within the primary beams. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/16_3/mamajek/paper/node2.html -- 64.4 Кб -- 08.04.2016
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    92. The need for the survey
    ... Progress in other wavebands highlights the paucity of the optical counterpart for the study of Galactic gas. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/14_1/parker/paper/node1.html -- 50.5 Кб -- 08.04.2016
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    93. http://www.atnf.csiro.au/observers/memos/AT39.3_106.pdf
    ... By analogy to its optical counterpart, this phase shifter is called a Quarter- Wave Plate ("QWP"). ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/observers/memos/AT39.3_106.pdf -- 37.5 Кб -- 31.07.2002
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    94. http://www.atnf.csiro.au/people/Matthew.Whiting/thesis/ch4.ps.gz
    ... was included to exclude those sources close to the Galactic plane, where increased optical extinction by dust, as well as the increased density of sources, would pose a problem in the identi - cation and study of the optical counterparts of the sources ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Matthew.Whiting/thesis/ch4.ps.gz -- 66.3 Кб -- 29.03.2006
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    95. Discussion
    ... MRC B1234-504 : Compact steep-spectrum source, with no optical counterpart on the UK Schmidt sky survey but possible stellar identification on a CCD image obtained at the Anglo-Australian Telescope (AAT) (Burgess 1998). ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/17_1/gaensler/paper/node4.html -- 58.9 Кб -- 08.04.2016
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    96. The Instruments
    ... Become an astronomer . CSIROpedia . A Kinematical Study of Old HII Regions and Optical Counterpart to the DRAO Canadian Galactic Plane Survey . ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/godbout/paper/node2.html -- 55.2 Кб -- 08.04.2016
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    97. http://www.atnf.csiro.au/people/Ray.Norris/papers/n262.pdf
    ... redshifts, using the FRC to estimate distances to submillimeter galaxies without optical counterparts (e.g., Carilli & Yun 1999 ... 3.2. Radio, Optical and X-ray Counterparts 3.2.1. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Ray.Norris/papers/n262.pdf -- 839.3 Кб -- 08.03.2011
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    98. Intergalactic gas
    ... The only bona fide extragalactic HI cloud is the HI 1225+01 SW complex (Giovanelli & Haynes 1989); the NE cloud is now known to have a weak optical counterpart. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/14_1/hawthorn/paper/node2.html -- 55.0 Кб -- 08.04.2016
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    99. http://www.atnf.csiro.au/pasa/16_2/meliani/catalog5.htm
    ... obs.: spectra [539]; X-ray and optical obs.: optical counterpart, localization a ... 5.45s, image, light curve, optical counterpart [387], light curve, periodogram [495 ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/16_2/meliani/catalog5.htm -- 638.5 Кб -- 08.04.2016
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    100. Australia Telescope National Facility
    ... the faint possibility that infrared-selected galaxies might differ in some intrinsic way from their optically-selected counterparts, although present indications are that the infrared-selected sample has properties similar to the optically-selected sample ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Ray.Norris/papers/n80.html -- 60.9 Кб -- 08.04.2016
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