The development of the new robotic FPS is a global effort built by an international team, including Ohio State University’s Imaging Sciences Laboratory, the University of Washington, École Polytechnique Fédérale de Lausanne (EPFL) and the Carnegie Observatories in Pasadena. These design teams overcame numerous challenges posed by the global pandemic by developing and constructing components wherever they were – some in their own garages and backyards – and shipping them elsewhere for further assembly. The robots were built in Switzerland and integrated into the main mechanical units in Columbus, Ohio. From there, they traveled to their final home in New Mexico — and soon, they will head to Chile as well.
Richard Pogge, the FPS Lead and a professor at Ohio State, noted, “OSU has built many exciting instruments, but this was new for us. It has been a challenging project for our team and a great success.”
The FPS will enable two of the three core science programs in SDSS-V: the Milky Way Mapper (MWM) and the Black Hole Mapper (BHM). Together, these projects will collect data from millions of objects spread across the sky, from stars in our own galactic backyard to unimaginably distant supermassive black holes.
“Developing the control software for the FPS has been a very challenging and extremely rewarding process” said Jose-Sanchez Gallego, an assistant professor at the University of Washington, who leads the controls and operations team along with graduate student Conor Sayres. “When we got the first light down the robotic fibres, we knew the last three years of teamwork had been worth it.” Solange Ramirez, an astronomer at the Carnegie Observatories and the Project Manager of SDSS-V added “This is such a major milestone for SDSS-V, its success had required a major technical and coordination effort.
The MWM will study our home galaxy in unprecedented detail. The ecosystem of stars, gas, dust and dark matter in large galaxies like our own has been shaped over billions of years by numerous physical processes that dominate on different scales in space and time. It will take advantage of our unique perspective within the Milky Way Galaxy to create a uniquely high-resolution map of the galaxy’s stars and how they are moving.
The MWM will also measure masses, ages, chemical compositions, the presence of companions, and a slew of other properties for vast samples of stars of all types — including hot massive stars, stars that are just forming, and the white dwarfs that are dead remnants of stars like our Sun. It will also target tens of thousands of multi-star and planetary systems in order to understand how often multi-companion systems form and what determines how they are structured.
“Without the observing speed and flexibility that the FPS gives us, it would be simply impossible to target so many objects across the entire sky,” said Jennifer Johnson, a professor at Ohio State and head of the MWM team.
Looking farther afield, the BHM will study quasars, which are among the most luminous objects in the universe. Powered by accretion onto supermassive black holes at the centres of galaxies, quasars can be used as beacons to trace the growth of these titans over cosmic time. SDSS-V will collect data on more than 300,000 quasars to measure the masses of their black holes, understand the physics of how they gobble up matter, and trace their growth over many billions of years.
By observing these objects many times, and combining the data with earlier SDSS observations, SDSS-V will be able to see how these systems evolve on timescales ranging from days to decades. The survey will also provide follow-up observations of hundreds of thousands of sources identified at X-ray wavelengths by the SRG/eROSITA satellite, to determine their nature and their distance. This vast sample of sources will include not only new quasars, but also distant clusters of galaxies -— the largest gravitationally bound structures in the universe — as well as nearby X-ray-emitting stars.
These vast samples of strikingly different types of targets —- millions of Milky Way stars, hundreds of thousands of distant quasars -— are among the key aspects that set SDSS-V apart from other surveys and are enabled by the new FPS system.
Hans-Walter Rix of the Max-Planck-Institute for Astronomy in Heidelberg, Germany, the SDSS-V Project Scientist, remarked, “In addition to probing even larger numbers of objects than before, the agile observing mode enabled by the FPS is the key to observing objects repeatedly, opening up the physics of changing and variable objects in the sky to systematic study.”
Added Kollmeier, “The SDSS team is an inspiration. While the world was shutting down, they were showing up. Everyone from the undergraduate students to the project leadership to our industry partners kept at it as best they could and supported each other to get here. I am so proud of this team’s perseverance and I look forward to the mysteries we both solve and uncover as the survey gets underway in full force.”