A Test of Near Infrared Differential Photometry for Study of Extrasolar Planets

Astronomy and Astrophysics – Astronomy

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Scientific paper

We report on test observations, done through the UKIRT Service Observing Program, of the transiting extrasolar system XO-3. While optical monitoring of transiting extrasolar systems is fairly routine, extension to the near infrared (NIR) has only recently been accomplished. Since the emergent flux from close-in planets peaks in the NIR, these bands are sensitive to atmospheric temperature and energy distribution. Furthermore, molecular bands in the planetary atmospheres alter the flux across ground-observable NIR bands; observations then constrain the atmospheric molecular abundances. We used 2MASS K-band images to examine transiting systems for their suitability for differential photometry. We selected XO-3 as one of our top choices and acquired one hour of randomly-timed data in Feb 09. We used a narrowband filter centered at 2.12 microns partly to avoid saturation and also to investigate the suitability of narrowband filters for these types of observations. Using standard aperture photometry techniques and a differential photometry algorithm provided by C. Broeg, we investigated the variability of the stars in the field. We found that XO-3 varied more than stars of comparable magnitude and, after construction of a light curve and comparing it to the XO-3 ephemeris, we discovered our data included roughly the last 25% of a primary transit. We will present analysis of our data. The success of these observations motivated us to propose for multiple narrowband filter observations in 2010A in order to construct a pseudo-spectrum of an extrasolar planet's emission. The routine acquisition of narrowband data such as we seek will significantly advance our understanding of exoplanetary atmospheres.

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