[PAE20-P03] MuSCAT and MuSCAT2: Two Multiband Cameras for Transit Observations Developed Toward the TESS Era
Keywords:transiting planet, TESS, multiband photometry, planetary atmosphere
On the other hand, there are some limitations in the TESS survey; the survey periods for most fields are only about 27 days, the image resolution of the detector is as large as 21 arcsec/pixel, and there is no filter change mechanism (single-band survey). Because of them, the planetary candidates to be detected by the TESS survey will have a high probability of false positives. Therefore, it will be essential to follow-up them from the ground to identify which are the true planetary systems. In particular, multi-band transit observations with a higher image resolution and good enough photometric precision can play important role on the planetary validation. Multi-band transit observations are also useful for roughly studying the planetary atmospheres.
In this context, we have developed an optical 3-band camera, MuSCAT, for the Okayama 188 cm telescope, and an optical 4-band camera, MuSCAT2, for the 1.52 m telescope at Teide Observatory in Spain, in preparation for the TESS era. The development of MuSCAT has been completed in 2014, and it has been in operation since 2015. So far it has produced a number of scientific results, highlighting that we validated/characterized several planets/planetary candidates detected by K2, which is the Kepler’s second mission and is considered to be the precursor of TESS. MuSCAT2 had its first light in August 2017, and started science operation in January 2018. MuSCAT2 has various advantages over MuSCAT in the site altitude (2390m), the clear-sky ratio (70%), the number of channels (4), the available telescope times (more than 160 nights), and the field of view (7.4 x 7.4 arcmin), all of which can contribute to produce outstanding scientific results in terms of quality and quantity. On the other hand, we plan to make the 188cm telescope and MuSCAT semi-robotic so that we can use it more for monitoring the activities of planetary host stars.
In this presentation, we will report the status of MuSCAT and MuSCAT2 including the science results obtained with these instruments.