Tomo-e Gozen

Relationship between radar cross section and optical magnitude based on radar and optical simultaneous observations of faint meteors

Radar and optical simultaneous observations of meteors are important to understand the size distribution of the interplanetary dust. However, faint meteors detected by high power large aperture radar observations, which are typically as faint as 10 …

An optical search for transients lasting a few seconds

Using a prototype of the Tomo-e Gozen wide-field CMOS mosaic camera, we acquire wide-field optical images at a cadence of 2 Hz and search them for transient sources of duration 1.5 to 11.5 seconds. Over the course of eight nights, our survey …

New Constraint on the Atmosphere of (50000) Quaoar from a Stellar Occultation

We report observations of a stellar occultation by the classical Kuiper Belt object (50000) Quaoar that occurred on 2019 June 28. A single-chord high-cadence (2Hz) photometry data set was obtained with the Tomo-e Gozen CMOS camera mounted on the 1.05 …

Luminosity function of faint sporadic meteors measured with a wide-field CMOS mosaic camera Tomo-e PM

Imaging observations of faint meteors were carried out on April 11 and 14, 2016 with a wide-field CMOS mosaic camera, Tomo-e PM, mounted on the 105-cm Schmidt telescope at Kiso Observatory, the University of Tokyo. Tomo-e PM, which is a prototype …

Evaluation of large pixel CMOS image sensors for the Tomo-e Gozen wide field camera

Tomo-e Gozen (Tomo-e) is a wide field optical camera for the Kiso 1.05 m f/3.1 Schmidt telescope operated by the University of Tokyo. Tomo-e is equipped with 84 chips of front-illuminated CMOS image sensors with a microlens array. The field of view …

The Tomo-e Gozen wide field CMOS camera for the Kiso Shmidt telescope

The Tomo-e Gozen is a wide-field high-speed camera for the Kiso 1.0-m Schmidt telescope, with a field-of-view of 20.7-deg$^2$ covered by 84 chips of 2k $\times$ 1k CMOS image sensors with 19-$\mu$m pixels. It is capable to take consecutive images at …

``Slow-scanning'' in ground-based mid-infrared observations

Chopping observations with a tip-tilt secondary mirror have conventionally been used in ground-based mid-infrared observations. However, it is not practical for next generation large telescopes to have a large tip-tilt mirror that moves at a …

Tomo-e Gozen

Optical wide-field video-survey with a mosaic CMOS camera on the Kiso Schmidt telescope, the University of Tokyo.

Data compression for the Tomo-e Gozen using low-rank matrix approximation

Optical wide-field surveys with a high cadence are expected to create a new field of astronomy, so-called "movie astronomy," in the near future. The amount of data from the observations will be huge, and hence efficient data compression will be …

Development of a prototype of the Tomo-e Gozen wide-field CMOS camera

The Tomo-e Gozen is an extremely wide-field optical camera for the Kiso 1.0-m Schmidt telescope. It is capable of taking consecutive frames with a field-of-view of 20 deg$^2$ and a sub-second time-resolution, which are achieved by 84 chips of …