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    1. http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_feb2015/AS04.html
    ... transiting exoplanets through ground-based near-UV observations PI: Jake Turner OBSERVER(S): Jake Turner (Graduate Student ...
    [ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_feb2015/AS04.html -- 5.5 Кб -- 24.01.2015
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    2. http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_may2014/AS08.html
    ... Specifically, a transiting exoplanet with a magnetic field should show an earlier transit ingress in the near-UV than in the optical, while the transit egress times would be the same. ...
    [ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_may2014/AS08.html -- 5.9 Кб -- 06.05.2014
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    3. http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_may2015/AS02.html
    ... Specifically, a transiting exoplanet with a magnetic field should show an earlier transit ingress in the near-UV than in the optical, while the transit egress times would be the same. ...
    [ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_may2015/AS02.html -- 6.0 Кб -- 06.05.2015
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    4. http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_oct2014/AS09.html
    ... Specifically, a transiting exoplanet with a magnetic field should show an earlier transit ingress in the near-UV than in the optical, while the transit egress times would be the same. ...
    [ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_oct2014/AS09.html -- 5.9 Кб -- 08.10.2014
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    5. http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_feb2015/AS03.html
    ... ARCSAT ID NUMBER: AS03 DESCRIPTIVE TITLE: Transiting Exoplanets as a Instructional Tool for Undergraduate Observational ... SCIENCE JUSTIFICATION: We propose to observe a number of transiting exoplanets using SurveyCam in order to provide a semester ...
    [ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_feb2015/AS03.html -- 2.7 Кб -- 24.01.2015
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    6. http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_jan2016/AS02.html
    ... ID NUMBER: AS02 DESCRIPTIVE TITLE: Massive emission-line stars Transiting WDs PI: John Wisniewski OBSERVER(S): John Wisniewski ... The second program we will conduct is a pilot search for transiting planets around WD stars.. ...
    [ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_jan2016/AS02.html -- 1.7 Кб -- 28.12.2015
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    7. http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_apr2016/AS05.html
    ... If a planet orbits a typical WD near the tidal disruption radius, its orbital period falls near 8-10 hours; if this planet transits, a serendipitous observer could potentially observe two transits of the planet in one night of continuous observations. ...
    [ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_apr2016/AS05.html -- 4.0 Кб -- 04.04.2016
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    8. http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_feb2015/AS02.html
    ... If a planet orbits a typical WD near the tidal disruption radius, its orbital period falls near 8-10 hours; if this planet transits, a serendipitous observer could potentially observe two transits of the planet in one night of continuous observations. ...
    [ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_feb2015/AS02.html -- 4.0 Кб -- 24.01.2015
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    9. http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_may2015/AS04.html
    ... If a planet orbits a typical WD near the tidal disruption radius, its orbital period falls near 8-10 hours; if this planet transits, a serendipitous observer could potentially observe two transits of the planet in one night of continuous observations. ...
    [ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_may2015/AS04.html -- 3.8 Кб -- 06.05.2015
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    10. http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_oct2014/AS03.html
    ... If a planet orbits a typical WD near the tidal disruption radius, its orbital period falls near 8-10 hours; if this planet transits, a serendipitous observer could potentially observe two transits of the planet in one night of continuous observations. ...
    [ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_oct2014/AS03.html -- 3.9 Кб -- 08.10.2014
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