PhysCOS Activities at AAS 248 – Wednesday, 17 June 2026
16 June 2026
Dear Physics of the Cosmos (PhysCOS) community members-
If you’re attending the American Astronomical Society’s 2026 Summer Meeting (AAS 248) in Pasadena CA, please join us for the following PhysCOS-organized activities (all times Pacific):
Wednesday 17 June
11:40a ‑ 1:10p, Conference Center 212: (XR SIG Special Session)
HEAD: Toward the 2030 Decadal: Science Cases for Potential Future X-ray Mission Concepts
Additionally, the following activities may be of special interest to the PhysCOS community:
Wednesday 17 June
10a ‑ 11:30a, Conference Center 211: Time Domain and Multi-messenger Astrophysics
11a ‑ 12n, Conference Center 204: The NASA Astrophysics ROSES Program
2p ‑ 3:30p, Conference Center 211: Stellar/Compact Objects 2: HMXBs and Pulsar Phenomena
3:40p ‑ 5:10p, Conference Center 212: HEAD: Chandra: Today and Tomorrow
And please drop by the PhysCOS table in the Exhibit Hall!ll!
For more information on PhysCOS throughout the meeting, check out our meeting webpage.
Wishing you the best,
Dr Francesca Civano & Dr Brian Humensky PhysCOS Chief Scientists, NASA GSFC
Dr Bernard Kelly PhysCOS Support Scientist, NASA GSFC
American Astronomical Society
The 248th Meeting of the AAS
The 248th AAS meeting (joint with the High Energy Astrophysics and the Laboratory Astrophysics Divisions) will be held 14-18 June 2026 in Pasadena, California.
We are especially looking for early-career researchers, including graduate students, postdocs, and early-career scientists, who are broadly interested in the intersection of AI and astronomy. You do not need to be an expert across the whole field; curiosity and a willingness to help the community learn matter most.
The organizational duties are light. Council members help suggest speakers and run the remote seminars, which mainly means sending email reminders and introducing the speaker. It is a great way to meet people across the field and to help shape a series that reaches the NASA community and beyond.
Two themes will anchor next year’s series:
1. Agentic AI for Astrophysics. How LLM agents and multi-agent systems can accelerate astronomical research, from literature and data analysis to simulation and discovery workflows.
2. AI and Astronomy in the US: Initiatives, Funding, and Broader Impacts. The wider landscape of AI in astronomy, including national initiatives, funding opportunities, AI pedagogy, the ethics and philosophy of AI in science, and ways AI can support NASA priorities such as ASTRA.
Please use this Google form to nominate yourself or someone else by the end of this week (20 June 2026).
Wishing you the best,
Dr Francesca Civano & Dr Brian Humensky PhysCOS Chief Scientists, NASA GSFC
Dr Bernard Kelly PhysCOS Support Scientist, NASA GSFC
Splinter Session: NASA’s Big Science, Small Missions
Tuesday, June 16th, 1:00pm – 2:30pm ET, 10:00am -11:30am PT (Hybrid Session)
For remote participation, please look for the “Join the Session” link above the agenda on the Cosmic Origins at AAS website.
High-Impact Science Smarter, Faster, Together
Agenda
Organizers: Swara Ravindranath (NASA/GSFC), Emily Witt (JHU)
Time
Topic
Speaker
10:00am ‑ 10:05am
Welcome
Swara Ravindranath (NASA/GSFC)
10:05am ‑ 10:15am
FORTIS Sounding Rocket
Emily Witt (JHU)
10:15am ‑ 10:25am
BlackCAT CubeSat
Abe Falcone (Pennsylvania State University)
10:25am ‑ 10:35am
SunRISE CubeSat Constellation
Joseph Lazio (University of Michigan)
10:35am ‑ 10:45am
SPHEREx Medium Explorer Mission
Roberta Paladini (IPAC/Caltech)
10:45am ‑ 10:55am
Landolt Pioneer Mission
Peter Kurczynski (NASA/GSFC)
10:55am ‑ 11:05am
Non-Traditional Path to Missions
Sanchayeeta Borthakur (Arizona State University)
11:05am ‑ 11:10am
BREAK
11:10am ‑ 11:30am
Panel Discussion
Swara Ravindranath (NASA/GSFC, moderator) Panelists: Drew Miles (Caltech), Pablo Saz Parkinson (NASA HQ), Joseph Lazio (University of Michigan), Abe Falcone (Pennsylvania State University), David Ardila (JPL)
American Astronomical Society
The 248th Meeting of the AAS
The 248th AAS meeting (joint with the High Energy Astrophysics and the Laboratory Astrophysics Divisions) will be held 14-18 June 2026 in Pasadena, California.
Dear Physics of the Cosmos (PhysCOS) community members-
If you’re attending the American Astronomical Society’s 2026 Summer Meeting (AAS 248) in Pasadena CA, please note the following activities that may be of special interest to the PhysCOS community (all times Pacific):
Tuesday, 16 June
8a ‑ 9a, Ballroom DE: Warner Plenary Lecture: Kyle Kremer, Globular Clusters: Astronomical factories of gravitational-wave and electromagnetic transients
10a – 11:30a, Conference Center 204: NASA’s Big Science, Small Missions
11:40a – 12:30p, Ballroom DE: HEAD Early Career: Carolyn Kierans
12:45p – 1:45p, Ballroom A: National Science Foundation Update Town Hall
3:40p – 5:10p, Conference Center 211: HEAD: NewAthena: The Next X-ray Flagship
3:40p – 5:10p, Conference Center 212: HEAD: Exploring the MeV Gamma-ray Sky with COSI
And please drop by the PhysCOS table in the Exhibit Hall!
For more information on PhysCOS throughout the meeting, check out our meeting webpage.
Wishing you the best,
Dr Francesca Civano & Dr Brian Humensky PhysCOS Chief Scientists, NASA GSFC
Dr Bernard Kelly PhysCOS Support Scientist, NASA GSFC
American Astronomical Society
The 248th Meeting of the AAS
The 248th AAS meeting (joint with the High Energy Astrophysics and the Laboratory Astrophysics Divisions) will be held 14-18 June 2026 in Pasadena, California.
Over the next few months, our talk series will be highlighting research from PRIMA’s Working Groups, with this talk focusing on dust properties in galaxies in the nearby universe. Stay tuned as well for overview talks this fall that highlight PRIMA’s PI science in the areas of Protoplanetary Disks and the Evolution of Dust and Metals.
Our Spotlight Series highlights recent advances in AGN science, with a strong emphasis on participation from early-career researchers, and includes plenty of time for community discussion following the presentations.
Central Shocks and Metal-Enriched Outflows: A New View of AGN Feedback
Speaker
Peixin Zhu (Harvard University)
Abstract
The growth of galaxies and their central supermassive black holes (SMBHs) is tightly linked. However, the exact impact of active galactic nuclei (AGNs) feedback on the host galaxy is still uncertain, with different observations suggesting AGNs enhance, suppress, or do not affect the host galaxy star formation rate. Resolving these controversies requires proper treatment of shocks, which are known to exist with AGN-driven outflow and yet are difficult to distinguish from AGN emission. In my talk, I will present a new theoretical three-dimensional diagram built for integral-field spectroscopy that cleanly separates star formation, AGN, and shock-dominated spaxels. Furthermore, these separation results can be combined with theoretical diagnostics to map the spatial distribution of gas-phase metallicity, ionization parameter, and gas pressure within these galaxies. After applying this new technique to 8 nearby Seyfert galaxies, we reveal that AGN and star formation coexist in the galaxy center, and fast shocks are present at the base of AGN outflows in some galaxies. We also find that outflowing gas is systematically metal-enhanced relative to adjacent star-forming rings. I will discuss how these results refine the picture of AGN feedback and the implications for nuclear enrichment and gas transport.
Investigating AGN Feeding and Feedback Through Circumnuclear Gas Kinematics in NGC 3079 and NGC 1068
Speaker
Dr. Ming-Yi Lin (University of Toledo)
Abstract
Studying gas kinematics in the circumnuclear regions (< 100 pc) of nearby AGNs on spatial scales of <10 pc provides insights into gas transport toward the supermassive black hole (SMBH) and the impact of AGN feedback in both radiative and kinetic forms. The kinematics of cold molecular gas are observed with radio interferometers (ALMA and NOEMA), while the warm molecular gas in the near-IR are studied using adaptive optics (AO)-assisted integral field spectrographs (IFS; Keck/OSIRIS). In this talk, I will use NGC 1068 and NGC 3079, two nearby Compton-thick AGNs, as pilot targets to discuss two distinct types of molecular outflows located at distances of ~40 pc from the SMBH: a cooling-efficient, momentum-driven outflow and a cooling-inefficient, energy-driven outflow. I will also present the discrepancy between Bondi accretion prescriptions and observationally constrained mass accretion rates.
Everything but Exoplanets: The Transformative General Astrophysics of the Habitable Worlds Observatory
Monday, June 15th, 10:00am -11:30am PT
This is your reminder to join the Cosmic Origins community members as they present their science and talk about relevant topics of interest across the astrophysics landscape!
For Cosmic Origins at AAS, please visit the link below.
What can’t we see from Earth orbit? Dark matter signatures hidden in the Dark Ages. The magnetic fields shielding habitable worlds around nearby stars. Gravitational waves from merging intermediate-mass black holes. The surfaces of Sun-like stars at unprecedented milliarcsecond resolution.
If you’re attending the AAS Summer Meeting this week, stop by the PhysCOS table to learn more about AMMB STIG, or reach out to nmahesh@caltech.edu to get involved.
To stay up to date, you can join our mailing list by sending an email to AMMB-STIG-join@lists.nasa.gov with the subject line “subscribe.”
In accordance with Grant Information Circular 26‑02 [PDF], Research Security Training Requirements, all covered individuals named on NASA grant and cooperative agreement proposals will be required to attest that they have completed research security training prior to proposal submission beginning 5 August 2026. This attestation will be made by signing a certification included in the NASA biographical sketch and current and pending (other) support forms. To support your preparation, NASA is providing advance copies of the updated forms that will be required starting 5 August 2026. The new attestation related to research security training is highlighted within these documents.
Please note: Do not use these updated forms before August 5, 2026. Until that date, continue to use the current biographical sketch and current and pending support forms available on the NASA Grant Operations Management website under “Grant Forms.”
NASA/IPAC Extragalactic Database (NED): New APIs and Survey
15 June 2026
Respond By 31 July 2026
The NASA/IPAC Extragalactic Database (NED) aims to capture the most reliable census of extragalactic objects and provide essential data and tools to facilitate astrophysics research and exploration.
NED has new APIs which provide access to more data and services! See the new NED API specification document for details. Notice: The legacy APIs are deprecated and cannot access data ingested after January 2026.
We are currently assessing the importance of some data types in NED to the research of our users, and how to best deliver these and other data. Please help make NED better by taking this short survey (5 mins to complete) by 31 July 2026.
ROSES-25: Several Updates to the ROSES-25 Summary of Solicitation
15 June 2026
Comments Due by 13 July 2026
Research Opportunities in Space and Earth Sciences (ROSES)-2025 is an ongoing “omnibus” or “umbrella” solicitation meaning that it includes many individual program elements each with its own topics and due dates. Refer to Table 3 of ROSES-25 for a list of those program elements. The ROSES-25 “Summary of Solicitation” is the front matter that sets the default backstop rules for each of the program elements in ROSES-25.
ROSES-25 Amendment 59 makes several additions, changes, and clarifications to the ROSES-25 Summary of Solicitation [PDF] to conform with Agency and administration priorities, see Sections I, I(g), II(a), II(b), III(b), III(d), V(b)ii, VI(c) & VIII(b). New text is in bold.
Important and substantial revisions to 2 CFR 200, the government-wide guidance for grants and cooperative agreements are proposed to take effect October 1, 2026; see the proposed regulation webpage on the Federal Register. Many types of currently allowable costs, such as but not limited to publications, research or events outside the United States, and domestic conferences may be restricted, denied, or may be allowable by legal exception or special award conditions only. Public comments on the revisions to 2 CFR 200 may be submitted until 13 July 2026, using the OMB comments portal.
Questions concerning this amendment to ROSES-25 may be directed to SARA@nasa.gov.
NASA Science
NSPIRES
NASA Solicitation and Proposal Integrated Review and Evaluation System
Astrophysics Explorers Program 2026 Small Explorer (SMEX) Announcement of Opportunity Final Text Released
15 June 2026
NASA’s Science Mission Directorate (SMD) announces the release of an Announcement of Opportunity (AO) to solicit Principal Investigator (PI)-led space science investigations for the Small Explorer (SMEX) opportunity under the Astrophysics Explorers Program. The SMD strategic goal of expanding human knowledge through new scientific discoveries in astrophysics includes the broad objective: “to understand the Sun, Earth, Solar System, and Universe.” SMD addresses this objective through astrophysics investigations that address one or more of these science goals:
How does the Universe work? Probe the origin and destiny of our universe, including the nature of black holes, dark energy, dark matter and gravity.
How did we get here? Explore the origin and evolution of the galaxies, stars, and planets that make up our universe.
Are we alone? Discover and study planets around other stars and explore whether they could harbor life.
The 2026 Astrophysics SMEX (APSMEX26) Schedule is as follows:
AO Release Date: 9 June 2026
Preproposal Conference Date: 30 June 2026
Mandatory Notice of Intent Due Date: 21 July 2026
Proposal Due Date: 9 September 2026
For the full, final text of the Astrophysics Explorers Program 2026 SMEX AO, visit its NSPIRES webpage.
Prospective investigators from any category of organizations or institutions, U.S. or non-U.S. with some restrictions as specified in Section 4.2.1 of the AO, are welcome. Specific categories of organizations and institutions include, but are not limited to, educational, industrial, and not-for-profit organizations, Federally Funded Research and Development Centers (FFRDCs), University Affiliated Research Centers (UARCs), NASA Centers, and other Government agencies. Both U.S. and non-U.S. participation is subject to China restrictions described in Sections 4.2.2 and 5.8.1 of the AO.
All interested parties must read the final APSMEX26 AO carefully for significant changes from the draft AO (NNH25ZDA008J) and prior years’ SMD Explorers Program AOs. Of particular importance is the change in evaluation and selection to a single-step competitive process. NASA intends to select one investigation proposal from the APSMEX26 responses to proceed into a combined Phase A&B. All proposals must comply with the requirements, constraints, and guidelines contained within the AO.
The Science Office for Mission Assessments (SOMA) will post the virtual Preproposal Conference agenda, connection information, and related information on the official 2026 Astrophysics Small Explorer (SMEX) website, which also provides further information, including the SMEX Program Library and SMEX Question & Answer (Q&A) page. Anonymity of persons/institutions who submit questions will be preserved. Proposers are encouraged to send comments and questions early so that they may be fully addressed. Questions posed at least one week before the Pre-Proposal Conference may be addressed in the Pre-Proposal Conference presentation or on the SMEX Q&A page. The deadline for other questions is two (2) weeks before the proposal due date.
Please address all questions or comments about the Astrophysics SMEX 2026 AO Daniel Moses, APSMEX26 Lead Program Scientist, dan.moses@nasa.gov; Hannah Jang-Condell, APSMEX26 Deputy Program Scientist, hannah.jang-condell@nasa.gov; and Omar Torres, Lead Acquisition Manager for the 2026 Astrophysics SMEX AO, SOMA omar.torres@nasa.gov using subject line “APSMEX26” to be properly routed.
NASA Science
NSPIRES
NASA Solicitation and Proposal Integrated Review and Evaluation System
Dear Physics of the Cosmos (PhysCOS) community members-
If you’re attending the American Astronomical Society’s 2026 Summer Meeting (AAS 248) in Pasadena CA, please join us for the following PhysCOS-organized activities (all times Pacific):
Monday 15 June
10a – 11:30a, Conference Center 204: NASA’s Future Large Gamma Ray (FLAG) Mission Concepts Working Group
Additionally, the following activities may be of special interest to the PhysCOS community:
Sunday 14 June
10a – 12n, Conference Center 102: High Energy Science Analysis with HEASARC Services
2p – 4p, Conference Center 101: An Introduction to Fornax: Scalable Data and Compute for Scientific Analysis
Monday, 15 June
12:45p ‑ 1:45p, Ballroom DE: NASA Update Town Hall
2p – 3:30p, Conference Center 211: HEAD: NuSTAR and the future of hard X-ray observations
2p – 3:30p, Ballroom F: Gamma-ray Astrophysics from Fermi to the Future
6:15p – 8:15p, Conference Center 106: NSF NOIRLab Open House
And please drop by the PhysCOS table in the Exhibit Hall!
For more information on PhysCOS throughout the meeting, check out our meeting webpage.
Wishing you the best,
Dr Francesca Civano & Dr Brian Humensky PhysCOS Chief Scientists, NASA GSFC
Dr Bernard Kelly PhysCOS Support Scientist, NASA GSFC
American Astronomical Society
The 248th Meeting of the AAS
The 248th AAS meeting (joint with the High Energy Astrophysics and the Laboratory Astrophysics Divisions) will be held 14-18 June 2026 in Pasadena, California.
Special Session: Everything but Exoplanets: The Transformative General Astrophysics of the Habitable Worlds Observatory
Monday, June 15th, 1:00pm – 2:30pm ET, 10:00am -11:30am PT
Highlights from Cosmic Origins Science Interest Groups (SIGs) and Science Analysis Groups (SAGs).
Time
Topic
Speaker
10:20am ‑ 10:30am
Spatially Resolved UV Spectroscopy Science Analysis Group in Support of HWO
Emily Witt (JHU)
10:30am ‑ 10:40am
Investigating the NIR Discovery Space of the Habitable Worlds Observatory: Updates from the Red Limit Science Analysis Group
Kyle Cooke (University of Louisville)
10:40am ‑ 10:50am
Opening the OVI Window to Reveal the Diffuse Cosmic Ecosystem with HWO
Sanchayeeta Borthakur (Arizona State University)
11:00am ‑ 11:10am
HWO Science Interest Group: Keeping the Community Connected to HWO
Jessie Christiansen (Caltech/IPAC)
Splinter Session: NASA’s Big Science, Small Missions
Tuesday, June 16th, 1:00pm – 2:30pm ET, 10:00am -11:30am PT (Hybrid Session)
For remote participation, please look for the “Join the Session” link above the agenda on the Cosmic Origins at AAS website.
High-impact science. Smarter, faster, together.
Agenda
Organizers: Swara Ravindranath (NASA/GSFC), Emily Witt (JHU)
Time
Topic
Speaker
10:00am ‑ 10:05am
Welcome
Swara Ravindranath (NASA/GSFC)
10:05am ‑ 10:15am
FORTIS Sounding Rocket
Emily Witt (JHU)
10:15am ‑ 10:25am
BlackCAT CubeSat
Abe Falcone (Pennsylvania State University)
10:25am ‑ 10:35am
SunRISE CubeSat Constellation
Joseph Lazio (University of Michigan)
10:35am ‑ 10:45am
SPHEREx Medium Explorer Mission
Roberta Paladini (IPAC/Caltech)
10:45am ‑ 10:55am
Landolt Pioneer Mission
Peter Kurczynski (NASA/GSFC)
10:55am ‑ 11:05am
Non-Traditional Path to Missions
Sanchayeeta Borthakur (Arizona State University)
11:05am ‑ 11:10am
BREAK
11:10am ‑ 11:30am
Panel Discussion
Swara Ravindranath (NASA/GSFC, moderator) Panelists: Drew Miles (Caltech), Pablo Saz Parkinson (NASA HQ), Joseph Lazio (University of Michigan), Abe Falcone (Pennsylvania State University), David Ardila (JPL)
Special Session: Planning for the Future of Astrophysics and the ASTRA Initiative
Thursday, June 18th, 1:00pm – 2:30pm ET, 10:00am -11:30am PT
No remote participation is available for this special session.
Agenda
Time
Topic
Speaker
10:00am ‑ 10:10am
Introduction from the NASA Astrophysics Division Director
Shawn Domagal‑Goldman (NASA HQ)
10:10am ‑ 10:25am
The ASTRA Initiative: Overview& Path Forward
Jessica Gaskin (NASA HQ)
10:25am ‑ 10:40am
Innovation for Astrophysics Workshop: Initial Findings
Kendra Short (JPL)
10:40am ‑ 10:55am
Ad ASTRA Community Science Workshop
Peter Kurczynski (NASA/GSFC)
10:55am ‑ 11:30am
Panel Discussion
Francesca Civano (NASA/GSFC)
ASTRA Office Hours at Cosmic Origins Exhibit Booth
(June 15 – 17, 2026) at 9am PT
Stop by the AAS / Cosmic Origins Exhibit booth during these times to ask questions about the ASTRA initiative, the September Ad ASTRA workshop, and developing new strategic mission concepts for astrophysics. Monday, Tuesday, Wednesday 9 am PT (Peter Kurczynski)
Best regards, Swara Ravindranath
American Astronomical Society
The 248th Meeting of the AAS
The 248th AAS meeting (joint with the High Energy Astrophysics and the Laboratory Astrophysics Divisions) will be held 14-18 June 2026 in Pasadena, California.
Habitable Worlds Observatory Detector System Development Study Request for Proposals
12 June 2026
Due by July 7th, 2026
Dear Colleagues,
The Habitable Worlds Observatory Technology Maturation Project Office and Columbus Technologies are excited to invite you to participate in a Detector System Development Study focused on developing critical detector technologies for the Habitable Worlds Observatory. This request for proposals seeks information from qualified organizations capable of supporting detector technology maturation studies to advance candidate technologies toward Technology Readiness Level 5. Specifically, we are seeking responses to address one or more of the following detectors categories: photon-counting detectors for visible and near-infrared coronagraph applications, far-ultraviolet detectors, and large-format detectors for near-ultraviolet and visible applications. Details regarding the call for proposals, eligibility, required deliverables, and study phases are available at the Columbus Technologies website here: https://columbususa.com/opportunities/hwo-detector-rfp/
Respondents located at Government agencies including the Jet Propulsion Laboratory or NASA Centers (e.g., Goddard Space Flight Center, Ames Research Center, etc.) should submit their responses directly to Daniel Kelly (daniel.p.kelly@nasa.gov).
Dear Astrophysics Strategic Technology & Research Accelerator (ASTRA) community members-
As we prepare for our Ad ASTRA Community Science workshop, we are writing to share important updates regarding the agenda structure and instructions for abstract submissions.
The Community Science (Ad ASTRA) Workshop is organized by the NASA Astrophysics Division to engage the community in identifying future large, strategic astrophysics missions. Structured over three thematic days—Science, Capabilities and Implementation, and Community Discussion—the workshop provides a comprehensive framework to connect scientific priorities with technological readiness and mission implementation. Across all three days, plenaries, panels, breakout sessions, and poster contributions are designed to maximize community interactions and discussion. The outcomes of the workshop will help NASA prioritize mission concepts and shape a balanced, forward-looking astrophysics portfolio that is consistent with the Astro2020 recommendations and existing and future science gaps.
To best serve the community and facilitate meaningful collaboration, we are splitting the mission concept presentations into two distinct focuses: Science on Day 1, and Capabilities and Implementation on Day 2. We are relying on you—the concept teams and the broader community—to submit abstracts for both days. We are also offering the option to present mission concepts as posters, and will offer the opportunity to present as posters any abstracts for which there is insufficient room in the parallel sessions.
Please review the detailed agenda structure and submission guidelines below:
Day 1: Science Focus
Science Questions: Day 1 will focus on open science priorities and questions from strategic documents (Astro 2020 Decadal Survey, Enduring Quests – Daring Visions from 2014) and more recent science questions that the mission concepts submitted to ASTRA will address.
Abstract Submission: Presentations for Day 1 are not restricted to mission concept team members. We strongly encourage other scientists in the community to submit abstracts presenting important science questions and to use this opportunity to connect with concept teams.
Breakout Sessions: These sessions will be organized by science themes (Compact Objects and Energetic Phenomena, Cosmology, Galaxies, Exoplanets & Astrobiology, Stars and Stellar Populations). Moderators will present a summary of the panel discussions at the end of Day 1.
Day 2: Mission Concepts – Capabilities and Implementation
Focus: Day 2 is focused on implementation, capabilities, and technologies (software and hardware) relevant to the ASTRA submitted mission concepts. A summary of the Innovation for Astrophysics Missions Workshop (May 2026) will inform discussions regarding industry and other capabilities and opportunities that may be leveraged.
Breakout Sessions: These sessions will be organized by capability groups, which will be determined once the submitted mission concept documents are reviewed.
Format & Goals: Breakout sessions will feature a mix of presentations and flexible discussion. The goal is for teams with concepts at varying maturity levels to collaborate, find commonalities, and strengthen their respective capability groups.
Abstract Submission Note: Teams may submit multiple abstracts for these sessions if their concept spans different capabilities (e.g., requiring both UV and X-ray technologies).
Day 3 & Workshop Outcome
A primary goal of this workshop is to refine a draft “science-to-capabilities” matrix, which will be built using inputs from your submitted ASTRA mission concept documents. During the Day 1 and 2 breakout sessions, moderators will capture key discussion points to present during end-of-day summary panels. On Day 3 of the workshop, we will hold a plenary discussion to recap the week and collaboratively revise the “science-to-capabilities” matrix. Together as a community, we will add, refine, and prioritize science questions, mapping them to mission concepts.
Key Upcoming Dates:
24 June 2026: Abstract submission deadline (link). If you have already submitted an abstract and would like to modify it based on the guidelines above, please delete your previous contribution and send another submission.
Announcement of Opportunity Astrophysics Explorers Program 2026 Small Explorer (SMEX) Final Text Released
12 June 2026
The National Aeronautics and Space Administration (NASA) Science Mission Directorate (SMD) announces the release of an Announcement of Opportunity (AO) to solicit Principal Investigator (PI)-led space science investigations for the Small Explorer (SMEX) opportunity under the Astrophysics Explorers Program. The SMD strategic goal of expanding human knowledge through new scientific discoveries in astrophysics includes the broad objective: “to understand the Sun, Earth, Solar System, and Universe.” SMD addresses this objective through astrophysics investigations that address one or more of these science goals:
How does the Universe work? Probe the origin and destiny of our universe, including the nature of black holes, dark energy, dark matter and gravity.
How did we get here? Explore the origin and evolution of the galaxies, stars, and planets that make up our universe.
Are we alone? Discover and study planets around other stars and explore whether they could harbor life.
The 2026 Astrophysics SMEX (APSMEX26) Schedule:
AO Release Date: June 9, 2026
Preproposal Conference Date: June 30, 2026
Mandatory Notice of Intent Due Date: July 21, 2026
Proposal Due Date: September 9, 2026
The NASA Solicitation and Proposal Integrated Review and Evaluation System (NSPIRES) is the official source for the full text of the Astrophysics Explorers Program 2026 SMEX AO. To find the full, final text visit https://go.nasa.gov/APSMEX26. Alternatively, visit: http://nspires.nasaprs.com/, select ‘Solicitations’ at the top of the page, and on the next page enter solicitation number NNH26ZDA011O in the search field.
Prospective investigators from any category of organizations or institutions, U.S. or non-U.S. with some restrictions as specified in Section 4.2.1 of the AO, are welcome. Specific categories of organizations and institutions include, but are not limited to, educational, industrial, and not-for-profit organizations, Federally Funded Research and Development Centers (FFRDCs), University Affiliated Research Centers (UARCs), NASA Centers, and other Government agencies. Both U.S. and non-U.S. participation is subject to China restrictions described in Sections 4.2.2 and 5.8.1 of the AO.
All interested parties must read the final APSMEX26 AO carefully for significant changes from the draft AO (NNH25ZDA008J) and prior years’ SMD Explorers Program AOs. Of particular importance is the change in evaluation and selection to a single-step competitive process. NASA intends to select one investigation proposal from the APSMEX26 responses to proceed into a combined Phase A&B. All proposals must comply with the requirements, constraints, and guidelines contained within the AO.
The Science Office for Mission Assessments (SOMA) will post the virtual Preproposal Conference agenda, connection information, and related information at: https://explorers.larc.nasa.gov/APSMEX26/SMEX. SOMA hosts the official “2026 Astrophysics Small Explorer (SMEX)” website that provides further information, including the SMEX Program Library and SMEX Question & Answer (Q&A) page. Anonymity of persons/institutions who submit questions will be preserved. Proposers are encouraged to send comments and questions early so that they may be fully addressed. Questions posed at least one week before the Pre-Proposal Conference may be addressed in the Pre-Proposal Conference presentation or on the SMEXQ&A page. The deadline for other questions is two (2) weeks before the proposal due date.
All questions or comments about the Astrophysics SMEX 2026 AO shall be addressed via email to Daniel Moses, APSMEX26 Lead Program Scientist, dan.moses@nasa.gov; Hannah JangCondell, APSMEX26 Deputy Program Scientist, hannah.jang-condell@nasa.gov; and Omar Torres, Lead Acquisition Manager for the 2026 Astrophysics SMEX AO, SOMA omar.torres@nasa.gov using subject line “APSMEX26” to be properly routed.
Any costs incurred in preparing a submission in response to this notice or the full APSMEX26 AO are solely the responsibility of the submitter.
Dear Physics of the Cosmos (PhysCOS) community members-
As we prepare for our Ad ASTRA Community Science Workshop, we are writing to share important updates regarding the agenda structure and instructions for abstract submissions.
The Community Science (Ad ASTRA) Workshop is organized by the NASA Astrophysics Division to engage the community in identifying future large, strategic astrophysics missions. Structured over three thematic days—Science, Capabilities and Implementation, and Community Discussion—the workshop provides a comprehensive framework to connect scientific priorities with technological readiness and mission implementation. Across all three days, plenaries, panels, breakout sessions, and poster contributions are designed to maximize community interactions and discussion. The outcomes of the workshop will help NASA prioritize mission concepts and shape a balanced, forward-looking astrophysics portfolio that is consistent with the Astro2020 recommendations and existing and future science gaps.
To best serve the community and facilitate meaningful collaboration, we are splitting the mission concept presentations into two distinct focuses: Science on Day 1, and Capabilities and Implementation on Day 2. We are relying on you—the concept teams and the broader community—to submit abstracts for both days. We are also offering the option to present mission concepts as posters, and will offer the opportunity to present as posters any abstracts for which there is insufficient room in the parallel sessions.
Please review the detailed agenda structure and submission guidelines below:
Day 1: Science Focus
Science Questions: Day 1 will focus on open science priorities and questions from strategic documents (Astro 2020 Decadal Survey, Enduring Quests – Daring Visions from 2014) and more recent science questions that the mission concepts submitted to ASTRA will address.
Abstract Submission: Presentations for Day 1 are not restricted to mission concept team members. We strongly encourage other scientists in the community to submit abstracts presenting important science questions and to use this opportunity to connect with concept teams.
Breakout Sessions: These sessions will be organized by science themes (Compact Objects and Energetic Phenomena, Cosmology, Galaxies, Exoplanets & Astrobiology, Stars and Stellar Populations). Moderators will present a summary of the panel discussions at the end of Day 1.
Day 2: Mission Concepts – Capabilities and Implementation
Focus: Day 2 is focused on implementation, capabilities, and technologies (software and hardware) relevant to the ASTRA submitted mission concepts. A summary of the Innovation for Astrophysics Missions Workshop (May 2026) will inform discussions regarding industry and other capabilities and opportunities that may be leveraged.
Breakout Sessions: These sessions will be organized by capability groups, which will be determined once the submitted mission concept documents are reviewed.
Format & Goals: Breakout sessions will feature a mix of presentations and flexible discussion. The goal is for teams with concepts at varying maturity levels to collaborate, find commonalities, and strengthen their respective capability groups.
Abstract Submission Note: Teams may submit multiple abstracts for these sessions if their concept spans different capabilities (e.g., requiring both UV and X-ray technologies).
Day 3 & Workshop Outcome
A primary goal of this workshop is to refine a draft “science-to-capabilities” matrix, which will be built using inputs from your submitted ASTRA mission concept documents. During the Day 1 and 2 breakout sessions, moderators will capture key discussion points to present during end-of-day summary panels. On Day 3 of the workshop, we will hold a plenary discussion to recap the week and collaboratively revise the “science-to-capabilities” matrix. Together as a community, we will add, refine, and prioritize science questions, mapping them to mission concepts.
Key Upcoming Dates:
24 June 2026: Abstract submission deadline (link). If you have already submitted an abstract and would like to modify it based on the guidelines above, please delete your previous contribution and send another submission.
The origins and fate of massive compact objects such as black holes, neutron stars, and white dwarfs can only be fully answered by measuring deci-Hertz (dHz) gravitational wave emission. A plethora of innovative mission concepts have been proposed motivated by this need, promising incredible potential sensitivity and requiring substantial technical development. Like COBE rather than Plank, we optimize time to first knowledge over ultimate sensitivity. We describe the highest priority science goals contained in and motivating a dHz observatory, the minimum sensitivity required to make these observations, and the fastest, least-costly mission that meets these minimum requirements. We dub this mission the Deci-hertz Interferometer Space Antenna (DISA).
Dear Astrophysics Strategic Technology & Research Accelerator (ASTRA) community members-
As we prepare for our Ad ASTRA Community Science workshop, we are writing to share important updates regarding the agenda structure and instructions for abstract submissions.
The Community Science (Ad ASTRA) Workshop is organized by the NASA Astrophysics Division to engage the community in identifying future large, strategic astrophysics missions. Structured over three thematic days—Science, Capabilities and Implementation, and Community Discussion—the workshop provides a comprehensive framework to connect scientific priorities with technological readiness and mission implementation. Across all three days, plenaries, panels, breakout sessions, and poster contributions are designed to maximize community interactions and discussion. The outcomes of the workshop will help NASA prioritize mission concepts and shape a balanced, forward-looking astrophysics portfolio that is consistent with the Astro2020 recommendations and existing and future science gaps.
To best serve the community and facilitate meaningful collaboration, we are splitting the mission concept presentations into two distinct focuses: Science on Day 1, and Capabilities and Implementation on Day 2. We are relying on you—the concept teams and the broader community—to submit abstracts for both days. We are also offering the option to present mission concepts as posters, and will offer the opportunity to present as posters any abstracts for which there is insufficient room in the parallel sessions.
Please review the detailed agenda structure and submission guidelines below:
Day 1: Science Focus
Science Questions: Day 1 will focus on open science priorities and questions from strategic documents (Astro 2020 Decadal Survey, Enduring Quests – Daring Visions from 2014) and more recent science questions that the mission concepts submitted to ASTRA will address.
Abstract Submission: Presentations for Day 1 are not restricted to mission concept team members. We strongly encourage other scientists in the community to submit abstracts presenting important science questions and to use this opportunity to connect with concept teams.
Breakout Sessions: These sessions will be organized by science themes (Compact Objects and Energetic Phenomena, Cosmology, Galaxies, Exoplanets & Astrobiology, Stars and Stellar Populations). Moderators will present a summary of the panel discussions at the end of Day 1.
Day 2: Mission Concepts – Capabilities and Implementation
Focus: Day 2 is focused on implementation, capabilities, and technologies (software and hardware) relevant to the ASTRA submitted mission concepts. A summary of the Innovation for Astrophysics Missions Workshop (May 2026) will inform discussions regarding industry and other capabilities and opportunities that may be leveraged.
Breakout Sessions: These sessions will be organized by capability groups, which will be determined once the submitted mission concept documents are reviewed.
Format & Goals: Breakout sessions will feature a mix of presentations and flexible discussion. The goal is for teams with concepts at varying maturity levels to collaborate, find commonalities, and strengthen their respective capability groups.
Abstract Submission Note: Teams may submit multiple abstracts for these sessions if their concept spans different capabilities (e.g., requiring both UV and X-ray technologies).
Day 3 & Workshop Outcome
A primary goal of this workshop is to refine a draft “science-to-capabilities” matrix, which will be built using inputs from your submitted ASTRA mission concept documents. During the Day 1 and 2 breakout sessions, moderators will capture key discussion points to present during end-of-day summary panels. On Day 3 of the workshop, we will hold a plenary discussion to recap the week and collaboratively revise the “science-to-capabilities” matrix. Together as a community, we will add, refine, and prioritize science questions, mapping them to mission concepts.
Key Upcoming Dates:
24 June 2026: Abstract submission deadline (link). If you have already submitted an abstract and would like to modify it based on the guidelines above, please delete your previous contribution and send another submission.