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History of HATPI Key Science Technical Specifications Photo Gallery

Project Inception

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HATPI Building Construction Near Completion

In Spring 2016, construction of the HATPI building at Las Campanas Observatory was nearly completed. The concrete pier for the equatorial mount had been poured and aligned. Plans were in place to install interior electrical components, power, HVAC, and internet connectivity. The facility consisted of two parts: a large instrument bay with a roll-off roof to house the HATPI instrument and allow for maintenance, and a shed containing a server room with computers to operate the telescope mount, acquire and analyze image frames, and store data. The shed also featured a small "observer's lounge" for maintenance personnel. Although HATPI was intended to operate autonomously, having on-site facilities for emergencies was considered useful.

LCO Building

Finalization of HATPI Mount and Instrument Holder Design

In Summer 2016, the engineering design of the HATPI mount and instrument holder units was finalized. The plan was to use 63 lenses attached to low-profile back-illuminated CCD cameras, controlled by focus and fine-pointing actuators. The mount was designed as a stepped pyramid to allow easy access for maintenance personnel from above and below, coupled with a heavy-duty equatorial drive capable of handling several tons of moving instrument weight.

Mount and Instrument Holder Design

Completion of HATPI Mount

By Winter 2017, the HATPI mount was completed and ready for integration with the rest of the instrument.

Completion of HATPI Mount

Mount Installation and Electronics Setup

In early Summer 2017, the first stage of mount installation and electronics setup was completed, and integration of cameras and lenses into the instrument began. More installation trips were planned throughout the summer and fall as cameras and lenses continued to be delivered in batches.

On-Sky Testing Commences

In Winter 2018, on-sky testing of HATPI began. The full instrument was integrated, and IHUs were being populated with lenses and cameras as they rolled off the assembly lines. The roof and mount operations had been automated, enabling HATPI to observe autonomously.

On-Sky Testing Commences

Key Science

The HATPI project focuses on exploring the dynamic universe, observing phenomena such as transiting exoplanets, supernovae, variable stars, and near-Earth asteroids.

Transiting Exoplanets

By continuously monitoring a quarter of the full celestial sphere all night, every night, at high cadence, spatial resolution, and photometric precision, HATPI will be able to detect a large number of exoplanetary transit events. HATPI is an especially powerful tool for finding the infrequent transits of long period, cold Jupiters that can take years or more to orbit their stars.

Transient Events

The high cadence and ultra-wide field-of-view of HATPI give it a unique sensitivity to fast astronomical transient events that may be missed by other time-domain surveys that observe the full sky at a much lower cadence. HATPI is expected to observe many bright transients, like nearby supernovae, Galactic novae, or kilonovae, providing valuable observations during the rise time before they are detected by other surveys.

Variable Stars

HATPI will produce long-term, high-cadence light curves for 10s of millions of stars, enabling the study of hundreds of thousands of variable stars. HATPI will be especially useful for detecting very long period stellar eclipsing binary systems, for routinely measuring the rotation periods of a vast number of sun-like stars, for detecting stellar flares, for studying stellar activity cycles, and for studying long-term mode changes in pulsating stars.

Moving Objects

HATPI will observe 1000s of Near-Earth asteroids every year, and will be particularly sensitive to very small nearby asteroids that would otherwise go undetected. It will also be useful for providing light curves of asteroids that can be used to measure their rotation periods and characterize their shapes.

Technical Specifications