Precision pressure control for the Veloce echelle spectrograph

AAT Dome at Siding Spring Observatory, NSW, Australia Angel Lopez-Sanchez (AAO-MQU)

AAT Dome at Siding Spring Observatory, NSW, Australia – Angel Lopez-Sanchez (AAO-MQU)

This “Alicats in the Wild” blog post comes courtesy of our Australian distributor, Duff & Macintosh Pty Ltd. Dr. James Gilbert was the technical lead for the Australian National University’s development of the Veloce echelle spectrograph, which is now installed on the 3.9-meter Anglo-Australian Telescope at the Siding Spring Observatory in New South Wales, Australia. Veloce integrates a highly-customized Alicat closed-volume pressure controller to keep air pressures inside the instrument stable. In his own words, here is Dr. James Gilbert.

Veloce was built primarily to detect stars that are ‘wobbling’ due to the gravitational tug of one or more orbiting planets. Veloce is based on a technique called Precision Radial Velocity Spectroscopy – we measure the spectral content of starlight and look for minuscule colour shifts (Doppler shifts) caused by the periodic motion of the star.

It is absolutely critical to control the measurement errors of the instrument, because the signal we are looking for is so small. We are looking for changes of 1/1500 pixels on our image detector, which is a physical distance of something like ten nanometers on the detector surface. This corresponds to a radial velocity measurement of around 1 m/s, meaning we can measure the speed of a star’s motion down to slow walking pace.  This is sufficient to detect planets not too dissimilar to Earth, that may be in the so-called ‘habitable zone’ of the host star.

Veloce echelle spectrograph interior - James Gilbert (ANU)

Veloce echelle spectrograph interior – James Gilbert (ANU)

We approached Alicat because we needed industrial-grade reliability as well as science-grade performance.

Anglo-Australian Telescope at Siding Spring Observatory, NSW, Australia Angel Lopez-Sanchez (AAO-MQU)

Anglo-Australian Telescope at Siding Spring Observatory, NSW, Australia – Angel Lopez-Sanchez (AAO-MQU)

If the air pressure in the instrument changes, then the refractive index at the surface of the optics changes, and our signals are completely drowned out.  We decided to shield the instrument from atmospheric pressure variations by keeping it at a fixed positive pressure at all times. We needed a stability of 5 mbar, with a goal of 1 mbar, in an 1800-litre volume with significant leaks. We approached Alicat because we needed industrial-grade reliability as well as science-grade performance. Alicat rose to the challenge and modified one of their standard products to provide an affordable solution to our requirements. The instrument has been operating for several months already, and its internal pressure has not ventured beyond 0.3 mbar of our set point, which is fabulous.

Veloce is now fully commissioned and has already observed its first planetary systems. Initially, we are looking at known candidates found by NASA’s Transiting Exoplanet Survey Satellite (TESS). Veloce is currently the best instrument in the world for some of these targets, and may be the first to confirm the existence and accurately measure the mass of planets we previously didn’t know existed.

While there are many factors that have made the Veloce project a success, we would certainly not be able to fulfill our science goals without the tight pressure regulation provided by our Alicat pressure controller.

Alicat, through Duff & Macintosh, supplied Veloce with a dual-valve pressure controller that can detect the smallest deviation from the chosen pressure setpoint within 5 ms. Upon such a detection, it adjusts its dual inlet and outlet valves to return the volume to setpoint within 50 ms, ensuring that Veloce never sees more than a 0.3 mbar total pressure deviation across its 1800-liter volume. To prevent unwanted thermal disturbances, the pressure sensor was physically isolated from the valve and flow path, so that the controller itself could be mounted outside the spectrograph chamber. 

Do you have a challenging application? Tell us about it below.




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