Announcement

CTA Prototype Telescope, the Schwarzschild-Couder Telescope, Detects Crab Nebula

Guests of the pSCT inauguration in January 2019 gather in front of the telescope. Credit: Deivid Ribeiro, Columbia University

Armado, AZ — On 1 June 2020, scientists from the Cherenkov Telescope Array (CTA) Consortium announced at the 236th meeting of the American Astronomical Society (AAS) that they have detected gamma rays from the Crab Nebula using a prototype telescope proposed for CTA, the prototype Schwarzschild-Couder Telescope (pSCT), proving the viability of the novel telescope design for use in gamma-ray astrophysics.

 

“The Crab Nebula is the brightest steady source of TeV, or very-high-energy, gamma rays in the sky, so detecting it is an excellent way of proving the pSCT technology,” said Justin Vandenbroucke, Associate Professor, University of Wisconsin. “Very-high-energy gamma rays are the highest energy photons in the universe and can unveil the physics of extreme objects including black holes and possibly dark matter.”

Detecting the Crab Nebula with the pSCT is more than just proof-positive for the telescope itself. It lays the groundwork for the future of gamma-ray astrophysics. “We’ve established this new technology, which will measure gamma rays with extraordinary precision, enabling future discoveries,” said Vandenbroucke. “Gamma-ray astronomy is already at the heart of the new multi-messenger astrophysics, and the SCT technology will make it an even more important player.”

 

The use of secondary mirrors in gamma-ray telescopes is a leap forward in innovation for the relatively young field of very-high-energy gamma-ray astronomy, which has moved rapidly to the forefront of astrophysics. “Just over three decades ago, TeV gamma rays were first detected in the universe, from the Crab Nebula, on the same mountain where the pSCT sits today,” said Vandenbroucke. “That was a real breakthrough, opening a cosmic window with light that is a trillion times more energetic than we can see with our eyes. Today, we’re using two mirror surfaces instead of one, and state-of-the-art sensors and electronics to study these gamma rays with exquisite resolution.”

Animation showing 18 gamma-ray events from the Crab Nebula detected with the pSCT telescope. Credit: CTA/SCT consortium

“The initial pSCT Crab Nebula detection was made possible by leveraging key simultaneous observations with the co-located VERITAS (Very Energetic Radiation Imaging Telescope Array System) observatory.  We have successfully evolved the way gamma-ray astronomy has been done during the past 50 years, enabling studies to be performed in much less time,” said Wystan Benbow, Director, VERITAS. “Several future programs will particularly benefit, including surveys of the gamma-ray sky, studies of large objects like supernova remnants, and searches for multi-messenger counterparts to astrophysical neutrinos and gravitational wave events.”

Sky map recorded with the pSCT over a region centered on the Crab Nebula, detection of the Crab Nebula marked at center. Credit: CTA/SCT consortium


Histogram showing the detection of gamma-ray events from the Crab Nebula, with NOFF representing background and NON representing a combination of signal and background. Credit: CTA/SCT consortium

Located at the Fred Lawrence Whipple Observatory in Amado, Arizona—the largest field site of the Center for Astrophysics | Harvard & Smithsonian—the pSCT was inaugurated in January 2019 and saw first light the same week. After a year of commissioning work, scientists began observing the Crab Nebula in January 2020, but the project has been underway for more than a decade.

 

“We first proposed the idea of applying this optical system to TeV gamma-ray astronomy nearly 15 years ago, and my colleagues and I built a team in the US and internationally to prove that this technology could work,” said Prof. Vladimir Vassiliev, Principal Investigator, pSCT. “What was once a theoretical limit to this technology is now well within our grasp, and continued improvements to the technology and the electronics will further increase our capability to detect gamma rays at resolutions and rates we once only ever dreamed of.”

 

The pSCT was made possible by the contributions of thirty institutions and five critical industry partners across the United States, Italy, Germany, Japan, and Mexico, and by funding through the U.S National Science Foundation Major Research Instrumentation Program.

 

“That a prototype of a future facility can yield such a tantalizing result promises great things from the full capability, and exemplifies NSF’s interest in creating new possibilities that can enable a project to attract wide-spread support,” said Nigel Sharp, Program Manager, National Science Foundation.

 

The SCT is being proposed to cover the core of CTA’s energy range (around 80 GeV – 50 TeV). The SCT’s two-mirror optical system is designed to better focus the light for greater imaging detail and improved detection of faint sources. A total of 40 telescopes (25 in the southern hemisphere and 15 in the northern hemisphere) are planned to cover this energy range. “CTA has been exploring the dual-mirror technology since the very beginning of the project with the Small-Sized Telescope prototypes and the SCT for the Medium-Sized Telescope,” says Federico Ferrini, Managing Director of the CTA Observatory. “The results obtained by the pSCT team re-confirm the advantages of advancing the technology for Cherenkov astronomy and the great potential it will bring to CTA.”

 

“The pSCT, and its innovations, are pathfinding for the future CTA, which will detect gamma-ray sources at around 100 times faster than VERITAS, which is the current state of the art,” said Benbow. “We have demonstrated that this new technology for gamma-ray astronomy unequivocally works. The promise is there for this groundbreaking new observatory, and it opens a tremendous amount of discovery potential.”

 

About the pSCT

 

The SCT optical design was first conceptualized by U.S. members of CTA in 2006, and the construction of the pSCT was funded in 2012. Preparation of the pSCT site at the base of Mt. Hopkins in Amado, AZ, began in late 2014, and the steel structure was assembled on site in 2016. The installation of the pSCT’s 9.7-m primary mirror surface — consisting of 48 aspheric mirror panels — occurred in early 2018, and was followed by the camera installation in May 2018 and the 5.4-m secondary mirror surface installation — consisting of 24 aspheric mirror panels — in August 2018. Scientists opened the telescope’s optical surfaces and observed first light in January 2019. It began scientific operations in January 2020.  The SCT is based on a 114 year-old two-mirror optical system first proposed by Karl Schwarzschild in 1905, but only recently became possible to construct due to the essential research and development progress made at the Brera Astronomical Observatory, the Media Lario Technologies Incorporated and the Istituto Nazionale di Fisica Nucleare, all located in Italy. pSCT operations are funded by the National Science Foundation and the Smithsonian Institution.

 

For more information visit https://www.cta-observatory.org/project/technology/sct/

Project contacts:

Center for Astrophysics | Harvard & Smithsonian
Wystan Benbow
617-496-7597
wbenbow@cfa.harvard.edu

 

University of Wisconsin

Justin Vandenbroucke
608-890-1477
justin.vandenbroucke@wisc.edu

 

University of California, Los Angeles
Vladimir Vassiliev
310-267-5878
vvv@astro.ucla.edu

 

Media contacts:

Center for Astrophysics | Harvard & Smithsonian
Fred Lawrence Whipple Observatory
Amy Oliver
801-783-9067
amy.oliver@cfa.harvard.edu

 

CTA Observatory

Megan Grunewald

+49 157 58795599

mgrunewald@cta-observatory.org