Robert Pearson retires from microelectronic engineering program
Robert Pearson helped make history when RIT began its microelectronic engineering program in the early 1980s. An RIT alumnus of the electrical engineering program and MicroE’s first faculty hire, Pearson reflected on some of that history—and his place in it—before retiring this summer after more than 40 years.
Pearson started his RIT story with highlights that included following in the footsteps of his father, Milton ’64 (Imaging science), combining electrical engineering and imaging science and coming to campus in 1976 as a student-athlete. He took advantage of early co-op experiences at Fairchild Semiconductor International in Maine and later its R&D center in California. He eventually worked for the company after graduation, before bringing a combination of academics and industry skills to teaching.
He saw great potential in the degree program, in the growing semiconductor industry, and RIT’s commitment to building what he would describe as a first-of-its-kind program, recognized by peer universities and industry for its skilled semiconductor graduates.
How did you come to teach in the microelectronics engineering program?
I started here in fall ’76 and played soccer. Before my first co-op I didn’t have a resume and went over to see sports information director, Roger Dykes. I made copies, sent it out, and got a co-op at Fairchild in Maine because Roger typed up my resume.
When I came back, I had classes with Lynn Fuller in semiconductor physics and thick film integrated circuits. He said, ‘I’ve got some equipment here, do you want to try to make some transistors? Just come in and start working. But you’ve got to write it up as lab reports.’ A buddy and I made the first photo masks, capacitors, solar cells, and transistors in 1979. My master’s thesis was a formalized version of all those lab reports. It is basically what we teach in our sophomore course, Integrated Circuit Technology now. It has survived the test of time.
I was working at Fairchild Semiconductors after graduation. When I visited RIT at Thanksgiving ’82, they had just started the microelectronics engineering program in September. Lynn Fuller, founder of the program, said, ‘I don’t have any faculty—it’s just me and 60 freshmen. Would you like to be a teacher?’ I asked, ‘When?’ He said, ‘January.’ So I went back to Maine, quit my job and moved back home with my wife.
What are some significant milestones in the program you were involved with since it began?
When I started teaching, we were in a couple of crowded rooms on the third floor of the engineering building. People were interested in the semiconductor field, and the country was very much interested in re-shoring—just like now. Lynn put together a proposal for a new building. I think the projected cost at the time was a measly $5 million. By 1985, we were ready to open the building, and who do we invite—Jack Kilby, inventor of the integrated circuit. And we gave him an honorary Ph.D. even before he was awarded the Nobel Prize.
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Carlos Ortiz/RIT
Robert Pearson has taught numerous lab courses and trainings. Some of his early lab notes and processes from the cleanroom during the time he was a student became the basis for some of the program materials used today.
What are some of the similarities and differences of the industry and students, then and now?
The industry in the early days of our program was very much aware of what decisions they made and how it affected their bottom line. If they found they were getting good hires from RIT, and it was helping them, they did their best to encourage us. That kept us on track for teaching what they wanted. When the semiconductor industry was still emerging, it was exciting. It was one of the obvious roots to success. The students were eager, and they worked hard. They still do. Our alumni said their careers took off because of RIT. They traveled internationally, managed big departments and projects, started their own companies. It just amazes me what all our students have done.
What personal and academic accomplishments are you most proud of?
Motorola was set to build a fab in Virginia. I thought, I would love a teaching experience at a place that had a fab right next door. We did get industry support at RIT, but not in the way of having it right there. Ironically, I went to Virginia after 14 years teaching at RIT and developed a microelectronic engineering program at Virginia Commonwealth University. It’s interesting that people thought they could do what RIT did, like it was no big deal, and they could not. The uniqueness of this program is immense. I returned to teaching at RIT in 2003 and became program director in 2008.
Outside of the college, I’ve been a steering committee member of two large conferences—the University Industry Government Microelectronic Symposium since 1985 and the Advanced Semiconductor Manufacturing Conference (founded by Lynn Fuller) since 1992. It was good advertising for our programs at RIT and what we are doing. It earned us the respect of other universities, and I’m very proud of that. I wrote the history of both of the conferences so that people would know how they began—again this is my interest in history. I should teach a history class!
Academically, winning the IEEE Outstanding Teaching Award in 2023 was great and I’m proud that Ivan Puchades, a former student and now an RIT engineering faculty member, nominated me for that. I’ve also been involved in the funding and creation of three different RIT scholarship awards for our microelectronic engineering students, and I’d like to start some more.
What will you be doing in retirement?
Helping coach my grandkids’ soccer teams. I’ll be doing some gardening, woodworking, I like wood carving and getting back into kayaking. I haven’t done much but now will be able to get out more and do this. I’ll have more time to ride my bike—if my knee still works—those old soccer injuries. I live in Henrietta and will probably still be on campus, I can’t seem to stay away.
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Using JWST imaging, ground-based telescope data, and previous COSMOS data, the catalog makes an unprecedented amount of information freely available, opening many unexplored scientific avenues. The full COSMOS-Web color image is shown with a zoom in to the region surrounding a gravitationally lensed galaxy known as the COSMOS-Web ring (Mercier et al. 2024).Credit: Kartaltepe/Casey/Franco/COSMOS-Web “This was an ambitious undertaking that required the development of innovative technologies to simultaneously measure the photometry and morphology of nearly 800,000 galaxies across 37 images,” said Marko Shuntov, postdoctoral researcher at Cosmic DAWN Center. “Building the catalog required tremendous teamwork, and it was all worth it because ultimately it has delivered some of the highest quality redshifts and physical parameters of galaxies that will enable groundbreaking science.” The raw data retrieved during COSMOS-Web was so vast that it was difficult and incredibly time-consuming for scientists to work through it. The public availability of the catalog takes that work out of the equation for the community. The COSMOS-Web team worked to reduce the data, eliminating artifacts, subtracting backgrounds, and improving the astrometry in order to provide accurate photometric and morphological analyses. The breakthroughs already discovered through JWST’s observations have shown how essential NIRCam data is for understanding galaxies in the early universe. Ensuring that the data are science-ready is an achievement that makes COSMOS-Web the standard calibration for future, large surveys. “We combined more than 10,000 images of the sky together to form the largest contiguous image available from JWST,” explained Maximilien Franco, postdoctoral researcher at Université Paris-Saclay. “To do this, we needed to ensure that all the images were properly aligned with existing data, and also to correct for any observational biases. It was incredible to reveal galaxies that were previously invisible, and very gratifying to finally see them appear on our computers.” Likewise, MIRI plays a critical role in determining the mass of early galaxies and investigating star formation over cosmic time. It has already been instrumental in confirming some of the most distant galaxies discovered by JWST. Using longer wavelengths that are less affected by dust extinction, MIRI has the ability to detect and characterize galaxies at higher redshifts, or at earlier times in the universe. “With MIRI, we’re now accessing an unprecedented level of detail in this wavelength range, providing new insights into the processes driving galaxy evolution and the growth of black holes,” said Santosh Harish, postdoctoral research associate at RIT. “The leap in sensitivity and spatial resolution is extraordinary, and MIRI observations from COSMOS-Web are a fine example of what this instrument is capable of.” Along with the data itself and three initial papers on the catalog, near infrared imaging, and mid infrared imaging, the data release also includes an interactive viewer where users can directly search images for specific objects or click on objects to see their properties. In addition, two new COSMOS-Web studies—one examining the structural evolution of brightest group galaxies over the past 11 billion years and another applying artificial intelligence to estimate key galaxy properties from photometry—highlight the wide scientific potential of the catalog. “Thanks to JWST and the COSMOS-Web survey, we can now trace how galaxies shut down star formation, undergo morphological transformation, and how these processes are shaped by their environment across cosmic time, even predicting galaxy properties using AI-driven methods,” said Ghassem Gozaliasl, astrophysicist and researcher at Aalto University. When the JWST launched in 2021, the COSMOS-Web team of nearly 50 researchers around the world had the longest observing time during the telescope’s first year. The team set out with three primary goals: to map and build understanding of the Reionization Era (in the universe’s first billion years); to trace and identify massive galaxy evolution in the first two billion years; and to study how dark matter is linked to visible matter within galaxies. The COSMOS-Web team is made up of nearly 50 researchers from around the world. The group gathered for a conference ahead of their full data release in Marseille, France, in May. Credit: COSMOS-Web After more than 150 visits and 250 hours of observations, the JWST data from COSMOS-Web has provided the information to obtain those goals. The survey has sent scientists into a new age of space observation and data analysis, and has opened the door to a future of understanding and discovery like never before. “We have data and catalogs that we’re very sure of, that we’ve tested and put a lot of work into,” said Kartaltepe. “I can’t overstate how much the field has changed. With data from JWST, we now have a new window on the universe.” COSMOS-Web is jointly led by Kartaltepe and Caitlin Casey, professor of physics at University of California, Santa Barbara, and is part of The Cosmic Evolution Survey (COSMOS). Beginning in 2007, COSMOS joined together more than 200 scientists across the globe to study the formation and evolution of galaxies using both space-based and ground-based telescopes. The remarkable longevity of the collaboration is a testament to the importance of open, accessible science. To learn more For more information on COSMOS-Web, go to the program’s website. The COSMOS-Web images, catalog, and interactive viewer are available through the team’s data release website.
