The article, soon to be published in ApJ,
describes new observations of the planet candidate discovered to orbit
GJ 504 a few years ago (
Kuzuhara et al., 2013).
By measuring the thermal emission from the companion in three custom filters in the range 3.6--4.1 microns, we’ve made new inferences about the temperature, density, and composition of the atmosphere. The observations were made possible with
LMIRCam, an AO-fed infrared camera on the Large Binocular Telescope.
I was responsible for the
entirety of the data reduction, taking steps familiar to other high-contrast observers in this wavelength regime:
- Aligning and combing thousands of raw, short exposures, correcting for background sky noise and detector pattern noise
- Angular differential imaging to subtract the star (here implemented with the KLIP algorithm)
- Contrast curve calculation, PSF modeling, photometry, and error analysis
GJ 504 b is on the extreme faint end of all the planetary-mass companions imaged to date (as Figure 4 in the journal article illustrates). Fortunately, the combination of relatively high angular separation (2.5 arcsec from the host star) with the deep sensitivity of LMIRCam--as shown above in the 3.9 micron co-add--was high enough to secure a detection at each filter. The wavefront correction provided by the LBTI AO system was such that Airy rings
spanning three orders of magnitude in intensity are evident, out beyond a 1-arcsec radius. Even without PSF subtraction, the planet is evident at a
contrast of 1E-5, in the northwest corner of the co-add image.
There is a lot more we could learn from the infrared SED at wavelengths redward of 4 microns. For such a faint object, however, that part of the spectrum is not likely to be accessed from the ground. Therefore, in the future GJ 504 will make an excellent target for JWST NIRCam.
