Brian Oetiker

Observational limits on terrestrial-sized inner planets around the CM Draconis system using the photometric transit method with a matched-filter algorithm (2000)

Doyle, Laurance, Deeg, Hans, Kozhevnikov, Valerij, Oetiker, Brian, Martin, Eduardo, Blue, J. Ellen, ...

A light curve of the eclipsing binary CM Draconis has been analyzed for the presence of transits of planets of size >=2.5 Earth radii with periods of 60 days or less, and in coplanar orbits around...

Observational limits on terrestrial-sized inner planets around the CM Draconis system using the photometric transit method with a matched-filter algorithm (2000)

Doyle, Laurance, Deeg, Hans, Kozhevnikov, Valerij, Oetiker, Brian, Martin, Eduardo, Blue, Ellen, ...

Also archived in: arXiv:astro-ph/0001177 v1 11 Jan 2000AND SETI 01/2000

Observational limits on terrestrial-sized inner planets around the CM Draconis system using the photometric transit method with a matched-filter algorithm (2000)

Doyle, Laurance, Deeg, Hans, Kozhevnikov, Valerij, Oetiker, Brian, Martin, Eduardo, Blue, J. Ellen, ...

A light curve of the eclipsing binary CM Draconis has been analyzed for the presence of transits of planets of size >=2.5 Earth radii with periods of 60 days or less, and in coplanar orbits around...

Observational limits on terrestrial-sized inner planets around the CM Draconis system using the photometric transit method with a matched-filter algorithm (2000)

Doyle, Laurance, Deeg, Hans, Kozhevnikov, Valerij, Oetiker, Brian, Martin, Eduardo, Blue, Ellen, ...

Also archived in: arXiv:astro-ph/0001177 v1 11 Jan 2000AND SETI 01/2000

Observational Limits on Terrestrial-Sized Inner Planets Around the CM Draconis System Using the Photometric Transit Method with a Matched-Filter Algorithm (2000)

Doyle, Laurance R., Deeg, Hans J., Kozhevnikov, Valerij P., Oetiker, Brian, Martin, Eduardo L., Blue, J. Ellen, ...

A lightcurve of the eclipsing binary CM Draconis has been analyzed for the presence of transits of planets of size >= 2.5 Earth-radii (Re), with periods of 60 days or less, and in co-planar orbits...

A spectrophotometric method for detecting substellar companions to late-type M stars /--by Brian Oetiker. (2000)

Oetiker, Brian.

"May, 2000."

A spectrophotometric method for detecting substellar companions to late-type M stars [microform]. (2000)

Oetiker, Brian.

University Microfilms order no. 9977778.

Searching for Companions to Late Type M Stars (1999)

Brian Oetiker, Nebojsa Duric, John Mcgraw, Tom Williams, Dale Jackson, Hans-Jörg Deeg, ...

. We describe a spectro-photometric method for detecting companions to M4 and later stars. Stars are imaged with 22 Angstrom FWHM optical lters tuned to the edge of the TiO molecular feature near...

Near-term detectability of terrestrial extrasolar planets: TEP network observations of CM Draconis (1998)

Deeg, Hans, Doyle, Laurance, Kozhevnikov, Valerij, Martin, Eduardo, Oetiker, Brian, Palaiologou, Efthimious, ...

Also archived in: arXiv: astro-ph/9806371 v1 29 Jun 1998

Near-term detectability of terrestrial extrasolar planets: TEP network observations of CM Draconis (1998)

Deeg, Hans, Doyle, Laurance, Kozhevnikov, Valerij, Martin, Eduardo, Oetiker, Brian, Paleologou, Efthimious, ...

Also archived in: arXiv: astro-ph/9806371 v1 29 Jun 1998