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Cosmic Origins Early Career Workshop

NASA’s Cosmic Origins Program is excited to invite you to the first Early Career Workshop, designed to support and empower the next generation of astrophysics leaders and PIs. The workshop aims to provide insights to early career scientists about the wide range of work done in the Cosmic Origins Program, to explain and demonstrate the tools and opportunities available to them, and to answer any questions they may have.

Location

Virtual

Dates

21-23 October 2025
1:00 PM - 4:00 PM

Community

Cosmic Origins

Type

Workshop

Cosmic Origins Community

To Support and Empower the Next Generation of Astrophycists

This workshop will take place virtually on October 21 – 23, 2025, from 1 – 4 pm Eastern.

The three days will be focused on Science (Day 1), Missions (Day 2) and Careers (Day 3).

Registration about To Support and Empower the Next Generation of Astrophycists
Gaseous yellow-orange filaments look like a rose seen from the side and tilted slightly from upper left to lower right, slightly higher than the center of the frame. Extending from the rose to upper left and lower right are gaseous outflows that appear as red lobes that have an overall shape of tall, narrow triangles with rounded tips. Each red triangle is made up of wavy, irregular lines. Dozens of stars are scattered across the field. One particularly bright white star with eight diffraction spikes is located at the top of the yellow rose. Another bright blue star with even more prominent diffraction spikes is to its lower left. The background of space is black.
Webb’s image of the enormous stellar jet in Sh2-284 provides evidence that protostellar jets scale with the mass of their parent stars—the more massive the stellar engine driving the plasma, the larger the resulting jet.
Image: NASA, ESA, CSA, STScI, Yu Cheng (NAOJ); Image Processing: Joseph DePasquale (STScI)

On Day 1, we will provide participants with an overview of the science themes covered by Cosmic Origins and give early career scientists opportunities to share their research.

On Day 2, we will highlight the many NASA archives, data analysis tools, and upcoming proposal opportunities so that participants can see a clear path for themselves to get involved with NASA missions.

On Day 3, participants will engage with speakers who have taken a variety of career paths that have led them to NASA science and mission work.

Workshop Schedule

Day 1 Science

Workshop Connection

TimeTopicSpeakerPresentation
1:00 PMCosmic Origins OverviewS. Ravindranath (NASA/GSFC)
1:15 PMHow to be a Scientific LeaderS. Nikzad (JPL)
S. Stierwalt (Occidental)
1:30 PMDecadal Surveys and Why They MatterR. Kennicutt (Texas A&M)
1:45 PMWhere Ideas Come From: The Creative Process of Writing a Scientific ProposalP. Kurczynski (NASA/GSFC)
2:00 PMHEASARCA. Basu-Zych (NASA/GSFC)
2:15 PMNASA Data Analysis in the Cloud: the Fornax InitiativeT. Jaffe (NASA/HQ)
2:30 PMSubmitted Talk: How did that get there?B. Koplitz (Arizona State)
2:45 PMSubmitted Talk: Investigating the Effects of SMBH Feedback on Disk Formation using FIRE SimulationsP. Fofie (UC Irvine)
3:00 PMBreak
3:15 PMSubmitted Talk: Extremely Metal-Poor Galaxies and the Faint-End of the Mass-Metallicity Relation at Cosmic DawnT. Hsiao (UT Austin)
3:30 PMSubmitted Talk: The evolution of metals and chemical enrichment in the first billion years after the big bangJ. Huyan (University of South Carolina)
3:45 PMSubmitted Talk: Hot Off the Stacks: Simulated X-ray Surface Brightness Profiles & Physical Interpretations of X-Ray BrightnessN. Sanchez (Carnegie)
4:00 PMEnd

Day 2 Missions and Technology

Workshop Connection

TimeTopicSpeakerPresentation
1:00 PMAstrophysics Missions OverviewTBD
1:15 PMGuest Observer ProgramsE. Lopez-Rodrriguez (USC)
1:30 PMThe PI Launchpad and how to prepare for mission opportunities in the futureE. Hamden (U. Arizona)
1:45 PMPioneering Emission Mapping of the Circumgalactic Medium with Aspera: Mission Progress and Lessons LearnedC. Vargas (U. Arizona)
2:00 PMCreating the Future through InnovationJ. Gaskin (NASA/HQ)
2:15 PMSubmitted Talk: The STABLE Cosmic Web ImagerD. Miles (Caltech)
2:30 PMBreak
2:45 PMSubmitted Talk: Finding the Enrichment Timescale of R-Process from Neutron Star Mergers to Star Forming RegionsZ. Smith (North Carolina A&T State)
3:00 PMHow to Join Roman – A Mission for the Community by the CommunityR. Beaton (STScI)
3:15 PMHow to get involved with the Habitable Worlds ObservatoryG. Arney (NASA/GSFC)
3:30 PMChromatic Cosmos: SPHEREx’s All-Sky Spectral Map of the Near-Infrared UniverseS. Everett (CalTech)
3:45 PMSubmitted Talk: Predictive Models for Binary Formation Across MetallicitiesA. Cason (Fisk University)
4:00 PMEnd

Day 3 Careers

Workshop Connection

TimeTopicSpeakerPresentation
1:00 PMSo many paths; Each is Unique, including mine. I’m here to champion yours!J. Crooke (NASA/HQ)
1:15 PMNavigating NASA-funded graduate and postgraduate opportunitiesN. Cucchiara (NASA/HQ)
1:30 PMTBD: Science Comms Within NASAS. Roberts (NASA/GSFC)
1:45 PMFrom the Woods to the StarsM. McTier (Astrophysicist; Folklorist)
2:00 PMIt's Not a Wall: Moving Between Academia & IndustryA. Lanz (Capella Space)
2:15 PMSubmitted Talk: Disentangling the Halo: Joint Model for Measurements of the Kinetic Sunyaev-Zeldovich Effect and Galaxy-Galaxy LensingJ. Sunseri (Princeton)
2:30 PMBreak
2:45 PMBinary Stellar Evolution Across Redshift and Varying IMF: A Choose-Your-Own-Adventure TaleE. Park (UC San Diego)
3:00 PMHow AI is Changing How We Do ScienceY. Ting (OSU)
3:15 PMLeadership Outside of AcademiaD. Norman (NoirLab)
3:30 PMCareer BrandingR. Gamble (NASA/GSFC)
3:45 PMUCO Professional Development and Summer School Experiences 2026A. Metevier (ISEE),
C. Pacheco (ISEE)
4:00 PMEnd

Workshop Science Organizing Committee

Sabrina Stierwalt
Peter Kurczynski
Swara Ravindranath
Ronald Gamble

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An illustration of Sun-like star HD 181327 and its surrounding debris disk. The star is at top right. It is surrounded by a far larger debris disk that forms an incomplete ellpitical path and is cut off at right. There’s a huge cavity between the star and the disk. The debris disk is shown in shades of light gray. Toward the top and left, there are finer, more discrete points in a range of sizes. The disk appears hazier and smokier at the bottom. The star is bright white at center, with a hazy blue region around it. The background of space is black. The label Artist's Concept appears at lower left.