Robert W. Noyes

Refined stellar, orbital and planetary parameters of the eccentric HAT-P-2 planetary system (2009)

Pál, András, Bakos, Gáspár Á., Torres, Guillermo, Noyes, Robert W., Fischer, Debra A., Johnson, John A., ...

We present refined parameters for the extrasolar planetary system HAT-P-2 (also known as HD 147506), based on new radial velocity and photometric data. HAT-P-2b is a transiting extrasolar planet that...

HATNet Field G205: Follow-Up Observations of 28 Transiting-Planet candidates and Confirmation of the Planet HAT-P-8b (2008)

Latham, David W., Bakos, Gáspár Á., Torres, Guillermo, Stefanik, Robert P., Noyes, Robert W., Kovács, Géza, ...

We report the identification of 32 transiting-planet candidates in HATNet field G205. We describe the procedures that we have used to follow up these candidates with spectroscopic and photometric...

Determination of stellar, orbital and planetary parameters using complete Monte-Carlo analysis -- the case of HAT-P-7b (2008)

Pál, András, Bakos, Gáspár Á., Noyes, Robert W., Torres, Guillermo

The recently discovered transiting very hot Jupiter, HAT-P-7b, a planet detected by the telescopes of HATNet, turned out to be among the ones subjected to the highest irradiation from the parent...

HAT-P-9b: A Low Density Planet Transiting a Moderately Faint F star (2008)

Shporer, Avi, Bakos, Gaspar A., Bouchy, Francois, Pont, Frederic, Kovacs, Geza, Latham, Dave W., ...

We report the discovery of a planet transiting a moderately faint (V=12.3 mag) late F star, with an orbital period of 3.92289 +/- 0.00004 days. From the transit light curve and radial velocity...

Andromedae1 (2007)

R. Paul Butler, Butler Geoffrey Marcy, Debra A. Fischer, Timothy M. Brown, Adam R. Contos, Sylvain G. Korzennik, ...

The bright F8 V star t Andromedae was previously reported to have a 4.6 day Doppler velocity periodicity, consistent with having a Jupiter-mass companion orbiting at 0.059 AU. Follow-up observations...

Harvard-SmithsonianCenter for Astrophysics (2007)

Robert W. Noyes, Adam R. Contos, Sylvain G. Korzennik, Peter Nisenson, Timothy M. Brown, Scott D. Horner, ...

Continuing precise radial velocity observationsof ae Coronae Borealis have allowed the determination of updated parameters of the 40-day orbit of its Jupiter-mass companion. This confirms the...

The Astrophysical Journal, accepted 2001 November 19. Detection of an Extrasolar Planet Atmosphere 1 (2007)

David Charbonneau, Timothy M. Brown, Robert W. Noyes, Ronald L. Gilliland

We report high precision spectrophotometric observations of four planetary transits of HD 209458, in the region of the sodium resonance doublet at 589.3 nm. We find that the photometric dimming...

Using Stellar Limb-Darkening to Refine the Properties of HD 209458b (2006)

Knutson, Heather, Charbonneau, David, Noyes, Robert W., Brown, Timothy M., Gilliland, Ronald L.

We use multi-band photometry to refine estimates for the planetary radius and orbital inclination of the transiting planet system HD 209458. We gathered 1066 spectra over four distinct transits with...

A stellar companion in the HD 189733 system with a known transiting extrasolar planet (2006)

Bakos, Gaspar A., Pal, Andras, Latham, David W., Noyes, Robert W., Stefanik, Robert P.

We show that the very close-by (19 pc) K0 star HD 189733, already found to be orbited by a transiting giant planet, is the primary of a double-star system, with the secondary being a mid-M dwarf with...

Transit Photometry of the Core-Dominated Planet HD 149026b (2005)

Charbonneau, David, Winn, Joshua N., Latham, David W., Bakos, Gaspar, Falco, Emilio E., Holman, Matthew J., ...

We report g, V, and r photometric time series of HD 149026 spanning predicted times of transit of the Saturn-mass planetary companion, which was recently discovered by Sato and collaborators. We...

Measurement of Spin-Orbit Alignment in an Extrasolar Planetary System (2005)

Winn, Joshua N., Noyes, Robert W., Holman, Matthew J., Charbonneau, David, Ohta, Yasuhiro, Taruya, Atsushi, ...

We determine the stellar, planetary, and orbital properties of the transiting planetary system HD 209458, through a joint analysis of high-precision radial velocities, photometry, and timing of the...

High Resolution Astrophysical Observations Using Speckle Imaging. (2002)

Noyes,Robert W., Nisenson,Peter, Papaliolios,Costas, Stachnik,Robert V.

This report describes progress under a contract to develop a complete astronomical speckle image reconstruction facility and to apply that facility to the solution of astronomical problems. During...

Development of a CCD Based Solar Speckle Imaging System. (2002)

Nisenson,Peter, Stachnik,Robert V., Noyes,Robert W.

This report describes the program to develop software and hardware for the purpose of obtaining high angular resolution images of the solar surface. The program included the purchase of a Charge...

Detection of an Extrasolar Planet Atmosphere (2001)

Charbonneau, David, Brown, Timothy M., Noyes, Robert W., Gilliland, Ronald L.

We report high precision spectrophotometric observations of four planetary transits of HD 209458, in the region of the sodium resonance doublet at 589.3 nm. We find that the photometric dimming...

HST Time-Series Photometry of the Transiting Planet of HD 209458 (2001)

Brown, Timothy M., Charbonneau, David, Gilliland, Ronald L., Noyes, Robert W., Burrows, Adam

We have observed 4 transits of the planet of HD 209458 using the STIS spectrograph on HST. Summing the recorded counts over wavelength between 582 nm and 638 nm yields a photometric time series with...

Present and Near-Future Reflected Light Searches for Close-In Planets (2000)

Charbonneau, David, Noyes, Robert W.

Close-in extrasolar giant planets may be directly detectable by their reflected light, due to the proximity of the planet to the illuminating star. The spectrum of the system will contain a reflected...

An Upper Limit on the Reflected Light from the Planet Orbiting the Star tau Bootis (1999)

Charbonneau, David, Noyes, Robert W., Korzennik, Sylvain G., Nisenson, Peter, Jha, Saurabh, Vogt, Steven S., ...

The planet orbiting tau Boo at a separation of 0.046 AU could produce a reflected light flux as bright as 1e-4 relative to that of the star. A spectrum of the system will contain a reflected light...

High Resolution Astrophysical Observations Using Speckle Imaging. (1998)

Noyes, Robert W., Nisenson, Peter, Stachnik, Robert V.

The reconstruction of complex solar surface features to a factor of ten finer than could normally be studied under prevailing seeing conditions has been demonstrated Previously, successful examples...

Spectral Line Distortions in the Presence of a Close-In Planet (1998)

Charbonneau, David, Jha, Saurabh, Noyes, Robert W.

We discuss the interpretation of distortions to stellar spectral lines with particular attention to line bisectors in the presence of an orbiting planetary companion. We present a simple model...

Exoplanets or Dynamic Atmospheres? The Radial Velocity and Line Shape Variations of 51 Pegasi and Tau Bootis (1998)

Brown, Timothy M., Kotak, Rubina, Horner, Scott D., Kennelly, Edward J., Korzennik, Sylvain, Nisenson, P., ...

Because of our relatively low spectral resolution, we compare our observations with Gray's line bisector data by fitting observed line profiles to an expansion in terms of orthogonal (Hermite)...

Radii and Distances of Cepheids, I., Method and Measurement Errors (1996)

Krockenberger, Martin, Sasselov, Dimitar D., Noyes, Robert W.

We develop a formulation of the Baade-Wesselink method which uses the Fourier coefficients of the observables. We derive an explicit, analytic expression to determine the mean radius from each...

STRESS INCONTINENCE IN WOMEN—Treatment by Retropubic Urethrovesical Suspension

Noyes, Robert W.

Twenty-four retropubic urethrovesical suspension operations were performed in a five-year period. Twenty-one of the patients were satisfied with the results, although the objective success of the...

STRESS INCONTINENCE IN WOMEN—Treatment by Retropubic Urethrovesical Suspension

Noyes, Robert W.

Twenty-four retropubic urethrovesical suspension operations were performed in a five-year period. Twenty-one of the patients were satisfied with the results, although the objective success of the...