237th meeting

237th AAS Meeting Exhibitors

237
Virtually Anywhere
237th meeting of the American Astronomical Society
Virtually Anywhere
10 – 15 January 2021

 

[Monday] [Tuesday] [Wednesday] [Thursday] [Friday]

**All times specified in Eastern Timezone

Monday, 11 January 2021

Exoplanet Science with the Nancy Grace Roman Space Telescope

Aki Roberge (NASA)
Monday, 11 January - 12:00pm-12:30pm ET

Join NASA Deputy Program Scientist for the Nancy Grace Roman Space Telescope, Aki Roberge, to learn how Roman will conduct the definitive survey of cold exoplanet demographics and provide the first space demonstration of active coronagraphy to study exoplanets.

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Hubble Advanced Products

Clara Brasseur (STScI), David Rodriguez (STScI)
Monday, 11 January - 12:00pm-12:30pm ET

The Hubble Advanced Products are a new generation of high level products generated from HST data with the most recent calibration and reference files. We will show how to use the MAST Portal and Astroquery to discover and access these products alongside their original HST data.

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Tools and Tutorials for the analysis of time series data from Kepler/K2 and TESS missions

Rebekah Hounsell (UMBC/NASA GSFC)
Monday, 11 January - 12:30pm-1:00pm ET

In this workshop we will teach the user how to access, analyze, and manipulate data from NASA’s exoplanet missions, Kepler/K2 and TESS. All tools presented will teach the user how to work with time series data for the purpose of scientific research. A set of Jupyter notebooks have been created via a collaboration between NumFocus, MAST, Lightkurve, and TESS GI office. They make use of python astronomical data packages to demonstrate how to analyze time series data from these NASA missions. The workshop assumes a basic knowledge of python and astronomy and will walk the user through several of the concepts outlined below, · How to obtain Kepler/K2 and TESS data products from the MAST archive · How to use LightKurve to access the various data products and create time series · How to analyze and assess various data anomalies and how you might visualize them · How to account for instrumental and noise effects within your data

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ALMA Opportunities & Status

Phil Jewell (NRAO), TBD (NRAO)
Monday, 11 January - 12:30pm-1:00pm ET

This NRAO webinar will inform the AAS membership and user community of the current status of: (a) the ALMA Observatory and science restart operations in Chile; (b) the Cycle 8 Call for Proposals and opportunities; (c) the next ALMA Development Call for Proposals opportunity; and (d) other matters of particular interest to the ALMA users community.

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The James Webb Space Telescope Science

Jonathan Gardner (NASA)
Monday, 11 January - 1:00pm-1:30pm ET

Webb has less than a year to launch. Join Jonathan Gardner, NASA's Deputy Senior Project Scientist for the James Webb Space Telescope, for an overview of Webb science goals.

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The Keck Observatory Archive

G. Bruce Berriman (Caltech/IPAC-NExScI)
Monday, 11 January - 1:00pm-1:30pm ET

New and upcoming services for KOA users.

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Chandra Source Catalog: Multiband Counterparts and SDSS-V Spectroscopic Followup

Paul J. Green (CXC), Francesca Civano (CXC)
Monday, 11 January - 1:30pm-2:00pm ET

The Chandra Source Catalog v2.0 (CSC) characterizes more than 300,000 unique X-ray sources detected in Chandra observations covering ~600deg2 of the sky. Making use of a Bayesian matching algorithm, we are finding the most likely counterparts in other wavebands (SDSS, PanSTARRs, 2MASS, Gaia). More than 100,000 optical and IR counterparts thus identified are being submitted as potential targets for spectroscopy during the latest incarnation of the Sloan Digital Sky Survey, SDSS-V between 2020 and 2025. We estimate that medium resolution optical fiber spectroscopy (R~2000) will be obtained for more than a third of submitted targets, where SDSS pointings and larger science programs allow. Such spectra will characterize tens of thousands of X-ray emitting quasars, stars and galaxies. About 3% of matched CSC sources, mostly in the Galactic plane, have no optical counterpart, yet are quite bright in the infrared, so may receive high resolution (R~22,000) IR spectroscopy. We expect this to unveil thousands of highly obscured X-ray binaries in the Milky Way. The SDSS calibrated digital spectra will be served to the public by the CXC, along with SDSS pipeline characterizations.

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NExScI's NASA Exoplanet Archive and ExoFOP

Calen B. Henderson (Caltechh/IPAC-NExScI)
Monday, 11 January - 1:30pm-2:00pm ET

Come learn about NASA's Exoplanet Archive and ExoFOP services --- serving the most comprehensive data on exoplanetary systems and supporting the community follow-up observations of TESS candidates.

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The Inevitable Ascension of sCMOS Detectors

Colin Haig (Diffraction Ltd)
Monday, 11 January - 2:00pm-2:30pm ET

Addressing the evolving landscape of detector technology and its impact on the observing community It’s undeniable: the rise of CMOS Active Pixel Sensor technology in consumer electronics and industrial machine vision has led to the demise of affordable sub-wafer CCD detectors. This in turn has greatly affected campus and mid-sized observatories through the introduction of new sCMOS cameras: gone are the affordable CCD detectors widely used in environments commonly using metre-class telescopes. In this special presentation, Diffraction Limited's leading experts in astronomy and scientific imaging solutions will provide the needed insights for observatory users, operators and investigators who wish to harness the power of new devices, while understanding their current limitations. Topics to be discussed include: • How the greater specialization and scarcity of CCDs will continue at the leading edge • How the new generation of CMOS devices will ultimately fill a widening void in the market • How the device structure of Active Pixel Sensors and on-chip analog-to-digital conversion bit depth can be used to gain control and impact dynamic range, noise, and image calibration workflow

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The Legacy of the Spitzer Space Telescope and You

Sean Carey (Caltech/IPAC)
Monday, 11 January - 2:00pm-2:30pm ET

The Spitzer Space Telescope ceased collecting science data in January 2020 after 16+ years of operations. We’ll show you to access the entire mission archive and resources that will help you use this rich dataset for your science.

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New Content and Capabilities in the NASA/IPAC Extragalactic Database

Joseph Mazzarella (Caltech/IPAC-NED)
Monday, 11 January - 2:30pm-3:00pm ET

NED is a comprehensive database of multiwavelength data for extragalactic objects, providing a systematic, ongoing fusion of information integrated from hundreds of large sky surveys and tens of thousands of research publications. We will highlight recent updates to content and user interface capabilities.

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High Level Science Products

Scott Fleming (STScI)
Monday, 11 January - 2:30pm-3:00pm ET

High Level Science Products (HLSPs) are community-contributed data products that complement or supplement MAST missions. We will explain why you may want to provide HLSPs to MAST, and highlight the new HLSPs from the past year.

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Gemini Program Platform Overview: The Next Generation Gemini Operations Software

Bryan Miller (Gemini Obs. / NSF's NOIRLab), Andrew Stephens (Gemini Obs. / NSF's NOIRLab)
Monday, 11 January - 4:00pm-4:30pm ET

The Gemini Program Platform (GPP) is a major software development initiative to rewrite and reimagine the operations software of the International Gemini Observatory. This will replace the current Phase I Tool (PIT) and Observing Tool (OT) with a web application designed to make proposal submission and observation preparation easier. It will also improve the underlying software infrastructure in order to facilitate the development of new features and to support Gemini, and potentially NOIRLab, operations for the next few decades. This webinar will give an overview and status update of the project, demo an early test version, and allow time for questions and feedback.

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Behind the Scenes at S&T

Peter Tyson (Sky & Telescope Magazine)
Monday, 11 January - 4:00pm-4:30pm ET

Take a virtual trip into the Sky & Telescope editorial offices to learn about the magazine's nearly 80-year history, meet current staff, and expand your understanding of the S&T brand, including its website, products, and tours.

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The Network for Earth-space Research Education and Innovation with Data (NEREID).

Tim Spuck (AUI), Catherine Cramer (AUI), Stephen Uzzo (AUI)
Monday, 11 January - 4:30pm-5:00pm ET

The purpose of the Network for Earth-space Research Education and Innovation with Data (NEREID) is to catalyze a network of practitioners across academia, industry and research to identify, leverage, amplify, and scale efforts to conduct research, develop tools, and engage communities of learners and policymakers in Earth and space science. NEREID recognizes the importance of interdisciplinarity, equity, and the dynamic relationship among data, modeling, and individual perspective. NEREID will facilitate development and dissemination of accessible and democratized tools and methods and work with systems of education and learning to integrate these tools into education and policy. NEREID will accomplish this through development of a community of practice: a network of practitioners who are aligned in their goals and work mutualistically toward a common purpose.

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University of Mars Video Game: Virtual Learning for Astro 101

Jane Charleton (Penn State & AstroVenture), Andrew Mshar (AstroVenture), Nahks Tr'Ehnl (Penn State & AstroVenture)
Monday, 11 January - 4:30pm-5:00pm ET

Over 25,000 students have taken Astro 101 through our self-contained video game adventure, deliberately designed for virtual learning at the college level. Try it for yourself at this interactive webinar where we will help you download and play a demo version of our University of Mars game. This game covers all the usual topics for general education Astro 101 classes, and can be used alone in a purely virtual course or combined with your own materials in a blended learning environment. Embedded mini-games teach concepts, from moon phases to early universe particle physics, and frequent questions help students to assess their learning as they progress. As well as providing an opportunity for participants to try it themselves, this webinar presentation will provide an overview of the game, discuss learning goals and student feedback, and allow you to ask questions about how you might use it in your own virtual classroom. It has been used for classes as small as 10 students and as large as 5000 students. For more information on the Astro 101 Video game please see our website http://theastroventure.com

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One Step Closer to Imaging Earth 2.0: Latest Advances in Starshades and Coronagraphs

Brendan Crill (NASA Exoplanet Exploration Program, JPL, Caltech)
Monday, 11 January - 5:00pm-5:30pm ET

Scientists and engineers around the world have made significant advances in starlight suppression technology that could enable a future NASA mission to directly image and spectrally characterize the atmosphere of Earth-sized exoplanets in the habitable zones of Sun-like stars. Join us at this webinar to hear the latest news on technology developments from NASA’s Exoplanet Exploration Program.

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Exominer: A Very accurate Deep Learning Classifier to Mine Exoplanets

Hamed Valizadegan (USRA)
Monday, 11 January - 5:00pm-5:30pm ET

The Kepler and TESS (Transiting Exoplanet Survey Satellite) missions have revolutionized the study of exo-planets in astronomy by comprehensively analyzing stars outside the solar system in search for transiting planets. These telescopes work based on transit photometry and their pipelines return a list of threshold crossing events (TCEs) whose light signature resemble a planet. However, not all TCEs are planet orbiting a star and they could be due instrument noise or other astrophysical phenomena. We will talk about our advanced deep learning model, ExoMiner, that is able to very accurately classify TCEs, much better than existing methods.

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Tuesday, 12 January 2021

 

Galaxies-MDPI: Particles and Fields in Black Hole Environment; The cultivation of X-ray binaries (XRBs): how local environments influence XRB formation and evolution

Bobomurat Ahmedov (Ulugh Beg Astronomical Inst., Tashkent), Antara Basu-Zych (University of Maryland, Baltimore County, UMBC)
Tuesday, 12 January - 10:00am-10:30am ET

Presentation 1:
There has been a rapidly growing interest in the study of relativistic astrophysics of gravitational compact objects due to several recent achievements: The recent direct detection of gravitational waves from the numerous events of merging gravitational compact objects in a close black hole and neutron star binaries by LIGO-VIRGO scientific collaboration, the measurement of general relativistic effects in strong gravity regime in the environment of the supermassive black hole Sagittarius A* at the Milky Way center by the ESOs GRAVITY instrument, and the first image of a black hole shadow in the center of elliptic galaxy M87 by the Event Horizon Telescope. In light of these recent successes of the general theory of relativity, the scope of this Special Issue is to open discussion of these topics to researchers working in areas such as Mathematical and Theoretical Physics, General Relativity, and Relativistic and Observational Astrophysics.

Presentation 2:
Over the past decade, the X-ray binary (XRB) research community has dedicated significant research to addressing: How do XRBs form and evolve in different galaxy host environments? 
As the predecessors of gravitational wave sources and millisecond pulsars and as sources potentially relevant in the early Universe for heating the intergalactic medium, XRBs have become more relevant to the broader scientific community. Studies of XRB emission within nearby and distant galaxies have seen marked refinement over these years by adding more nuanced research of the relationships between XRBs and their host galaxy properties. Both theoretical and observational studies of the detailed physics, including accretion mechanisms, within XRB systems offered important constraints for models. 

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Behind the scenes of NASA’s Exoplanet Travel Bureau posters

Tiffany Kataria (NASA's JPL, Caltech), Thalia Khan (NASA's Exoplanet Exploration Program)
Tuesday, 12 January - 12:00pm-12:30pm ET

Go behind the scenes with NASA’s Exoplanet Exploration Program Office and learn the science behind the Exoplanet Travel Bureau Posters! Learn about the process of selecting and designing worlds beyond our solar system and see how we illustrate planets we cannot see based off of observations and our knowledge of physics.

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Exploring the Mid-IR Galactic Center with SOFIA Legacy Maps

Jamse Radomski (SOFIA/USRA), Nicole Karnath (SOFIA/USRA)
Tuesday, 12 January - 12:30pm-1:00pm ET

The Galactic Center legacy maps obtained with FORCAST at 25- and 37-µm provide a large-scale view of bright infrared emission in the region, with an unprecedented spatial resolution. The detected emission allows one to constrain the dust spatial distribution and temperature, and to identify compact sources, including candidate young stellar objects, hence providing unique contextual information for the study of the closest galactic nucleus. We will present this publicly available dataset and different techniques to derive information and exploit its scientific value.

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Astronomers Turned Data Scientists

Jeff Silverman
Tuesday, 12 January - 1:00-7:30pm ET

This is the third annual Astronomers Turned Data Scientists (ATDS) Splinter Meeting. This Splinter Meeting came from a desire to create a more cohesive community among former astronomers who are currently working with big data in industry and between ATDS and current astronomers (especially those who use data science tools and techniques in their research, as well as those who might be interested in transitioning from academia into a data-related career).

The Splinter Meeting will consist of a series of talks and panels that cover a wide range of topics aimed at ATDS who are currently working as data scientists (or in data-adjacent roles) in industry. The schedule (which can be found below) will include mostly technical talks by data scientists, but we also plan to include some career-related presentations from ATDS as well (aspects of which might be more applicable to current data scientists and aspects of which might be more applicable to prospective data scientists).

In addition, networking and recruiting among the current data scientists and prospective data scientists will be strongly encouraged. To this end we will have ample time for networking during our Splinter Meeting and many of our attendees and presenters will participate in various AAS Career Services events throughout the AAS Meeting. More info about recruiting and other data-related and career-related events at the AAS Meeting can be found below.

We also plan to have an official (virtual) evening event for ATDS attendees after the main ATDS meeting on the evening of January 12.

If you have any questions, please don't hesitate to contact us at Astro2Data{at}gmail{dot}com and we look forward to seeing you in January!


Big Astronomy and ACEAP Programs

Renae Kerrigan (Peoria Riverfront Museum), Vivian White (Astronomical Society of the Pacific), Shannon Schmoll (Michigan State Univ.), Tim Spuck (AUI)
Tuesday, 12 January - 1:00pm-1:30pm ET

Associated Universities recognizes the importance of cultivating excellence, delivering value, enhancing education, and engaging the public. The AUI Office of Education and Public Engagement (OEPE) builds on decades of experience across formal and informal education and outreach, and the management of large complex science projects and facilities. Through the OEPE AUI works to identify and develop initiatives that are innovative and potentially transformative in STEM related education and outreach. Astronomy in Chile Educator Ambassadors Program The Astronomy in Chile Educator Ambassadors Program (ACEAP) is a collaboration between AUI, the National Radio Astronomy Observatory, AURA, National Optical Astronomy Observatory, and Gemini Observatory, and is supported by the National Science Foundation (NSF 1439408 and 1723697). The Program brings amateur astronomers, planetarium personnel, and K-16 formal and informal astronomy educators to US astronomy facilities in Chile. While at these facilities, ACEAP Ambassadors will receive extensive training about the instruments, the science, data products, and communicating science, technology, engineering, and mathematics (STEM) concepts. When they return home, the Ambassadors will share their experiences and observatory resources with schools and community groups across the US. ACEAP Website: https://astroambassadors.com/ Big Astronomy. It takes many people with diverse backgrounds, talents, and skills to run a world-class observatory. Meet a few of these people as they share the wonder of the sky—and the excitement of discovery. Explore the world-class observatories nestled in northern Chile’s mountains and learn why Chile, with its beautiful mountain ranges and clear, cloudless skies create an ideal environment for studying the cosmos. Continue discovering! Participate in live conversations with observatory staff, explore exclusive behind-the-scenes footage, educational activities, and ongoing science experiments all at bigastronomy.org Big Astronomy Website: https://www.bigastronomy.org/

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Precision Optics for Next-Generation Missions: Reducing Manufacturing Costs and Schedule

Becky Borrelli (L3Harris)
Tuesday, 12 January - 1:30pm-2:00pm ET

L3Harris Technologies will present three of our advanced optical technologies created to significantly reduce cost and schedule associated with manufacturing of precision optical systems. Replicated Composite Optics represent a first of its kind approach to creating high stiffness, low mass, low CTE mirrors that are manufactured using a highly scalable approach. L3Harris has also developed two processes that significantly streamline the fabrication of glass components, low temperature fusion and capture range replication, that have recently been used to produce 9 off-axis aspheric segments. Finally, we will present our approach to additive manufacturing of our proprietary invar for space structures. This approach facilitates invar geometries not achievable with conventional machining while maintaining the superior performance of the L3Harris proprietary invar.

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The NEID Doppler Spectrometer: a Status Report

Paul Robertson (The Univ. of California, Irvine, NEID)
Tuesday, 12 January - 2:00pm-2:30pm ET

Learn about recent results from the commissioning of the NEID Doppler spectrometer, including the instrument, port adapter, and queue scheduling system. NEID is an ultra-stable, high-resolution broadband optical spectrometer now installed at the 3.5m WIYN Telescope at Kitt Peak National Observatory. It will be available for Guest Observer proposals to the entire community, and will have an automated pipeline to provide precise radial velocities to all users.

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SOFIA: Science from the Stratosphere

James De Buizer (USRA/SOFIA)
Tuesday, 12 January - 2:30pm-3:00pm ET

Join USRA's James De Buizer, Senior Scientist on the SOFIA Airborne Infrared Observatory, to learn how SOFIA’s mid- and far-infrared observations are uncovering new clues about the birth of stars and planets, our interstellar origins and the path to life, magnetic fields and the distant universe.

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Dual-Anonymous Peer Review at NASA

Dan Evans (NASA)
Tuesday, 12 January - 4:00pm-4:30pm ET

Dual-anonymous peer review is revolutionizing the evaluation of proposals in the space sciences. Join Dan Evans, Program Scientist in NASA's Astrophysics Division, for an overview of how NASA is implementing dual-anonymous peer review and practical advice on how to prepare proposals.

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Get your Personalized Notifications and Recommendations from ADS

Alberto Accomazzi (Center for Astrophysics | Harvard & Smithsonian), Kelly Lockhart (Center for Astrophysics | Harvard & Smithsonian)
Tuesday, 12 January - 4:30pm-5:00pm ET

After reviewing recent improvements of the NASA Astrophysics Data System (ADS), we will describe and demonstrate two new features: personalized recommendations based on a user's readership history and recommendations based on a user's profile. Join us to learn how to use the ADS to stay on top of new developments in your research area.

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Jupyter Data Analysis Tools for Visualization

Brian Cherinka (STScI), Erik Tollerud (STScI)
Tuesday, 12 January - 5:00pm-5:30pm ET

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Wednesday, 13 January 2021

How to Use Infrared Science Archive (IRSA) Tools

Luisa Rebull (Caltech-IPAC/IRSAA)
Wednesday, 13 January - 12:00pm-12:30pm ET

IRSA has the data and tools to help you make your next scientific discovery! Come and learn how to use IRSA's tools and to see all our latest tools and features.

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Introduction to the Universe of Astro-Fashion

Emily Rice (STARtorialist)
Wednesday, 13 January - 12:00pm-12:30pm ET

You’ve seen our pop-up shop at previous AAS, DPS, and AGU meetings, and now you can purchase your favorite science fashion and gifts in our new online shop! Come learn about all the great things we have in store for STARtorialist.com including our newest custom & exclusive products, blog, outreach, and more.⁥

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First Black Holes

Ryan Hickox (NASA/Dartmouth College)
Wednesday, 13 January - 12:30pm-1:00pm ET

The origin of supermassive black holes is one of the greatest mysteries in astronomy. Current and upcoming NASA space telescopes can probe the distant, early Universe, to uncover the formation of these monsters that lurk in the heart of every massive galaxy today. Join Ryan Hickox, Professor of Physics and Astronomy at Dartmouth College, to hear about the latest discoveries in this exciting area of research.

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Overview of USRA

Ghassem Asrar (USRA)
Wednesday, 13 January - 12:30pm-1:00pm ET

Universities Space Research Association is an independent, nonprofit research corporation where the combined efforts of in-house talent and university-based expertise merge to advance space science and technology. USRA works across disciplines including biomedicine, planetary science, astrophysics, and engineering and integrates those competencies into applications ranging from fundamental research to facility management and operations. 

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SOFIA Archive Opportunities: Science-Ready Data and Funding

Ed Chambers (SOFIA/USRA), Luisa Rebull (IPAC), B-G Andersson (SOFIA/USRA)
Wednesday, 13 January - 1:00pm-1:30pm ET

The SOFIA Archival Research Program (SARP) is now open for proposals to fund research projects primarily using SOFIA data. The purpose of this program is to encourage the use of available SOFIA archival data and to realize the full potential of the SOFIA archive. In this webinar we will present the search and visualization functionalities for SOFIA data in the IRSA archive, highlight and describe select high-potential public datasets, and discuss the mechanics of the open funding call.

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Analyzing and visualizing volumetric data with yt

John ZuHone (SAO)
Wednesday, 13 January - 1:00pm-1:30pm ET

Yt is an open-source Python package for analyzing and visualizing volumetric data. Yt supports structured, variable-resolution meshes, unstructured meshes, and discrete or sampled data such as particles. The yt project aims to produce an integrated science environment for collaboratively asking and answering astrophysical questions. This webinar will feature a 15 minute introduction to yt, followed by a 15 minute Q&A.

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Hubble ULLYSES Program

Travis Fischer (Space Telescope Science Inst.)
Wednesday, 13 January - 1:30pm-2:00pm ET

Join Travis Fischer of the Space Telescope Science Institute for an overview of the Hubble Space Telescope's Ultraviolet Legacy Library of Young Stars as Essential Standards (ULLYSES) Program. ULLYSES is a Director's Discretionary program of approximately 1,000 orbits that will produce an ultraviolet spectroscopic library of young high- and low-mass stars in the local universe.

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From Wide Field Imaging to High Resolution Spectroscopy Meet the Canada-France-Hawaii Telescope

Daniel Devost (CFHT)
Wednesday, 13 January - 1:30pm-2:00pm ET

The Canada-France-Hawaii Telescope operates a world-class, 3.6 meter optical/infrared telescope on the summit of Maunakea in Hawaii. Join CFHT's director of science, Daniel Devost, to learn more about CFHT's suite of instrumentation, queue scheduled operations, and how the US community can utilize the facility.

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Hearing The Light: How Sonification Makes Astronomy More Accessible

Clara Brasseur (STScI), Jenn Kotler (STScI)
Wednesday, 13 January - 2:00pm-2:30pm ET

Sonification is the process of representing data as sound. Astronify is Python library for sonifying light curve data from TESS and Kepler. We will describe this exciting method of studying data, listen to sonified light curves, discuss the goals of the project, and share how you can sonify your own data.

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MAST Portal Walkthrough

Chinwe Edeani (STScI)
Wednesday, 13 January - 2:00pm-2:30pm ET

Learn the basics on how to use the MAST Portal to search for data across all our missions, including HST, JWST, TESS, Kepler, High-Level Science Products, and much more!

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Student and Teacher Discoveries with High School Radio Astronomy

Glen Langston (NSF), Keviin Bandura (WVU), Sue Ann Heatherly (GBO), Pranav Sanghavi (WVU), Thaddeeus Herman (WCSDNY), Joe Wise (Wildwood HS), David Schultz
Wednesday, 13 January - 2:30pm-3:00pm ET

Radio Telescopes open a marvelous window into the Universe. Thanks to free software, lower cost amplifiers and remarkable new low cost devices available anyone can build their own radio telescope. We focus on the experience of high school students and teachers using these telescopes to build their skills in science, engineering and computer programing. Through the group projects, we learn our place in the universe and discover the incredible speeds at which we fly through the Milky Way. Using techniques we describe, both students and teachers, can build their own research equipment. We summarize our experience with building telescopes, learning electronics fundamentals and introduce the students to the thriving world of open source software development. The telescopes we describe are low cost, $300 total, including computer, and are sensitive enough to detect our Milky Way galaxy in seconds. Teachers have developed many projects. One example is measuring the speed of the Earth around the Sun. The shape of the Milky Way is clearly seen with the telescopes. The motions of the Sun through the Galaxy are deduced from the telescope observations. A radio telescope can have almost any shape or size, and the opportunities for unique student projects are as big as the universe itself.

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The Exciting Dawn - and bright future - of Gravitational-Wave Astronomy

Martin Hendry (IGO Scientific Collab. & Univ. of Glasgow, Joey Key (LISA Consortium and University of Washington Bothell), Haley Wahl (NANOGrav Collab. & Univ. of West Virginia)
Wednesday, 13 January - 2:30pm-3:00pm ET

A new era of astronomy has dawned – with the first direct detections of gravitational waves, and the promise of many more exciting discoveries to come. Join scientists from LIGO, LISA and NANOGrav and find out more about the remarkable science and technology behind these projects – and what lies ahead for the emerging new field of gravitational-wave astronomy.

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Grant Programs within NSF's Division of Astronomical Sciences I: General research and education programs

Harshall Gupta (NSF)
Wednesday, 13 January - 4:00pm-4:30pm ET

This session will provide an overview of funding opportunities within NSF's Division of Astronomical Sciences (AST). It will include a brief presentation followed by discussion between the audience and a small panel of AST program officers.

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US Archival Science with Euclid

Harry Teplitz (Caltech/IPAC), Phil Appleton (Caltech/IPAC), James Colbert (Caltech/IPAC)
Wednesday, 13 January - 4:30pm-5:00pm ET

Euclid is an ESA mission, with NASA involvement, to study the nature and geometry of the dark universe, with launch planned in mid-2022. Euclid will survey the extragalactic sky, obtaining near-infrared and wide-band optical imaging, as well as NIR grism spectra. All Euclid data will be made public to the world-wide community within 2 years of acquisition. The Euclid NASA Science Center at IPAC (ENSCI; https://www.euclid.caltech.edu) will support Euclid research by the US community. In this Webinar, we will give an overview of the mission and the opportunity for US-based archival research.

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Using Python to access NASA Archives

David Shupe (IPAC)
Wednesday, 13 January - 4:30pm-5:00pm ET

This webinar will feature experts from the NASA Astronomical Virtual Observatories (NAVO) Python working group. There will be a short tutorial on how to access the NASA Archives using the pyvo package. Under the hood, this package uses Virtual Observatory protocols so that the user does not need to know where the data are hosted but can discover what is available and access it in standard ways. A 15 minute general Q&A session will follow. NAVO comprises elements of MAST at STScI, HEASARC at GSFC, and both IRSA and NED at IPAC.

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Wide Field Survey Science with the Nancy Grace Roman Space Telescope

Dominic Benford (NASA)
Wednesday, 13 January - 5:00pm-5:30pm ET

The Roman Space Telescope provides a groundbreaking combination of sensitivity, resolution, and coverage to serve extragalactic astronomy, cosmology, and time domain astronomy. Join Dominic Benford, NASA's Program Scientist for the Nancy Grace Roman Space Telescope, to hear the latest about this groundbreaking telescope.

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Overview of Graduate Program

Tobias Marriage (Johns Hopkins Univ.)
Wednesday, 13 January - 5:00pm-5:30pm ET

Please join us for an overview discussion of our graduate program hosted by Prof. Tobias Marriage.

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Thursday, 14 January 2021

 

Overview of the James Webb Space Telescope

John Mather (NASA)
Thursday, 14 January - 12:00pm-12:30pm ET

Join NASA's John Mather, Senior Project Scientist for the James Webb Space Telescope, for an overview of Webb. The JWST concept and technology grew from discussions in 1995 and the HST and Beyond report into the world's most powerful space telescope ever built. The design and technology have been optimized for observations from 0.6 to 28 µm with instrument contributions from the US, Europe, and Canada. Launch is planned for Oct. 2021.

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Careers for Scientists at Northrop Grumman


Thursday, 14 January - 12:00pm-12:30pm ET

Jon Arenberg (Northrop Grumman)

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How Can the NASA Exoplanet Science Institute Help YOUR Research?

Dawn Gelino (NExScI, IPAC, Caltech)
Thursday, 14 January - 12:30pm-1:00pm ET

The NASA Exoplanet Science Institute (NExScI, https://nexsci.caltech.edu) supports the broad astrophysics and planetary science communities. Listen in to learn how NExScI can support YOUR research! Do you need observational data? Learn how to apply for 10-meter Keck telescope time and use the Keck Observatory Archive (KOA) to access all data acquired with these two telescopes since they began operations over 26 years ago. Also, find out about access to southern hemisphere telescopes for exoplanet follow-up observations. Are you looking for a postdoc? Learn how to apply for an NHFP, the premier NASA Astrophysics Postdoctoral Fellowship. Do you need to learn about or better understand precision radial velocities? Join in to learn about interacting with the experts and getting hands-on data experience at this year's virtual Sagan Summer Workshop. Are you interested in exoplanet data and tools? Come learn about the NASA Exoplanet Archive which gives you access to just about any type of exoplanet data you’d like, and contribute follow-up exoplanet observations to the ExoFOP. Have more questions? Just ask or get in touch with our Help Desks!

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NSF: Astronomy and Astrophysics Grants Program II: Instrumentation and infrastructure programs

Hans Krimm (NSF)
Thursday, 14 January - 12:30pm-1:00pm ET

National Science Foundation program officers will give a brief overview of the funding opportunities available in the Division of Astronomical Sciences. Then participants will be able to ask questions about the available programs.

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Presenting Effective Interactive Virtual Planetarium Programs

Karrie Berglund (Digitalis Education Solutions, Inc.)
Thursday, 14 January - 1:00pm-1:30pm ET

How can you present effective, interactive VIRTUAL planetarium shows? I will share some lessons we have learned from our own online presentations as well as from customer feedback.

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JWST for Beginners

Susan Mullaly (STScI)
Thursday, 14 January - 1:00pm-1:30pm ET

This presentation is aimed at newcomers to JWST, students, and those who'd like a reminder. We will summarize the science capabilities of the observatory and its instruments, as well as the planned science program for Cycle 1.

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A day in the life of the Chandra Operation Control Center

Sabina Hurley (Northrop Grumman & Chandra X-ray)
Thursday, 14 January - 1:30pm-2:00pm ET

Get a glimpse behind the scenes with the Chandra operations teams. Peer over the shoulder of an Operations Controller on the first contact of the day, watch a weekly schedule of observations come together, listen in as engineers and scientists tackle an emerging issue, and learn how the team responds to a spacecraft anomaly. Enhance your understanding of what it takes to keep an observatory running smoothly and gain insight into how it affects observing in this discussion with the Chandra Flight Operations Manager.

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Astronomy and Astrophysics Research at the USRA Science and Technology Institute

Linda Parker (Science and Technology Inst.), Chien-Ting Chen (USRA), Adam Goldstein (USRA)
Thursday, 14 January - 1:30pm-2:00pm ET

The USRA Science and Technology Institute (STI) works closely with the NASA Marshall Space Flight Center in Huntsville, AL in science areas of Astronomy and Astrophysics, Earth Sciences, and Heliophysics research. STI scientists participate in both science and operations of many NASA astrophysics programs. The research includes x-ray and gamma-ray support for Chandra and x-ray optics, Imaging X-ray Polarimetry Explorer (IXPE), Mikhail Pavlinsky ART-XC onboard the Spectr-Roentgen-Gamma (SRG) mission, Fermi Gamma-ray Burst Monitor (GBM), the LargE Area burst polarimeter (LEAP) mission concept study, MoonBEAM mission concept study, Extreme-ultraviolet Stellar Characterization for Atmospheric Physics and Evolution (ESCAPE) concept study. We will give an overview of the research performed at STI, as well as a deeper look into the science of two programs: Chandra and Fermi GBM.

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The Once & Future Great Observatories

Grant Tremblay (Harvard/CFA)
Thursday, 14 January - 2:00pm-2:30pm ET

Join Grant Tremblay, astrophysicist at the Harvard/Smithsonian Center for Astrophysics, for an overview of the Great Observatories missions.

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Wander with Webb: VR Edition

Quyen Hart (STScI), Alex Lockwood (STScI)
Thursday, 14 January - 2:00pm-2:30pm ET

Come explore black holes, stars, disks, exoplanets and the Solar System with Webb – all in virtual reality!’ Join us on a tour of the latest and greatest updates to our publicly available, free program: WebbVR

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RADIAL: Partnering with Minority Serving Institutions to Develop Innovations in STEM+C E-learning

Alessandra Corsi (Texas Tech University), Kevin Doran (AUI), Anja Fourie (NRAO)
Thursday, 14 January - 2:30pm-3:00pm ET

The Radio Astronomy Data Imaging and Analysis Lab (RADIAL) aims to use radio astronomy research challenges to recruit, train, sustain and accelerate the progress of under-represented minority students in fields required by the sector; and to contribute to the development of a diverse, competitive US STEM workforce with transferable skills relevant for a rapidly changing workplace and society. Project RADIAL is an authentic alliance of minority-serving institutions of higher education, supported by the National Radio Astronomy Observatory, that creates intentional networks with other IHEs, federal R&D facilities, industry and professional organizations in order to address diversity in the workforce in a systemic way. One of RADIAL’s core activities is the collaborative development of practical and relevant K-12 and college curriculum materials, delivered to faculty and students at all partner institutions through SuperKnova, an accessible and online e-learning platform built for the project. This webinar, presented by Project RADIAL partners, will explore the challenges, opportunities, lessons learnt and best practices established during the collaborative development and prototyping of curricula and an e-learning platform required to serve all institutions.

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AIP Resources for Data and Diversity in Astronomy, and the TEAM-UP project

Rachel Ivie (AIP), Arlene Modeste Knowles (AIP)
Thursday, 14 January - 2:30pm-3:00pm ET

The American Institute of Physics (AIP) is a resource for AAS members looking for data about the astronomical workforce. AIP also has new programs to support efforts to improve diversity, equity, inclusion and belonging in astronomical workplaces. In this workshop, come learn about data that are available to you on astronomers—everything from demographics of astronomers to the variety of careers where astronomers work. In addition, we’re pleased to present AIP’s latest diversity efforts and how they relate to astronomy. Learn about our efforts to increase the representation of Black students earning physics and astronomy degrees including an update on the TEAM-UP report, The Time is Now: Systemic Changes to Increase African Americans with Bachelor’s Degrees in Physics & Astronomy released at the AAS 2020 meeting and our efforts to support AAS’s diversity initiatives.

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Citizen Science

Marc Kuchner (NASA)
Thursday, 14 January - 4:00pm-4:30pm ET

Join Marc Kuchner, NASA astrophysicist and Citizen Science Officer, to hear the latest news and information about NASA's Citizen Science Program, which currently involves more than a million citizen science volunteers.

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Introduction to Glue for Astronomical Research

Alyssa Goodman (Harvard), Catherine Zucker (Harvard), Thomas Robitaille
Thursday, 14 January - 4:00pm-4:30pm ET

Glue is an open-source Python library for exploring the relationships within and between related datasets. With Glue, users can create 2D and 3D visualizations of their data, overlay visualizations, and propagate selections across datasets. Glue is written in Python and built on top of standard scientific computing libraries so that users can easily integrate their own python code. This webinar will feature a 15 minute demo of Glue’s features, followed by a 15 minute Q&A.

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Career profiles and opportunities at AURA

Lynda Dec (AURA)
Thursday, 14 January - 4:30pm-5:00pm ET

Come and listen to other scientists to learn how their career paths have been formed and how AURA has helped them. AURA can help you too

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Spectrum Management

David Morris (NSF AAAS Fellow), Ashley Zauderer (NSF)
Thursday, 14 January - 4:30pm-5:00pm ET

We will discuss an update of spectrum management activities at the National Science Foundation, covering the results of the 2019 World Radio Conference, impacts of NGSO activity on astronomy, and NSF's Spectrum Innovation Initiative.

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Job Opportunities within NSF's Division of Astronomical Sciences

Harshall Gupta (NSF)
Thursday, 14 January - 5:00pm-5:30pm ET

This session will give an overview of rotator positions and permanent positions at NSF's Division of Astronomical Sciences (AST). The session will include a panel of AST program officers who will share their experiences working at NSF and answer questions from community members.

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Chasing Rainbows: The Maunakea Spectroscopic Explorer

Jennifer Marshall (Maunakea Spectroscopic Explorer & Texas A&M)
Thursday, 14 January - 5:00pm-5:30pm ET

The Maunakea Spectroscopic Explorer (MSE) is a next generation massively multiplexed spectroscopic facility that is completely dedicated to optical and near-Infrared spectroscopy of samples of thousands to millions of astrophysical objects at resolutions spanning R~3,000 to R~40,000. With science goals spanning all of astronomy, from detailed chemical abundance studies of nearby stars to investigating the cosmology of the early Universe, MSE will provide key next-generation science capabilities that will revolutionize the field. MSE project scientist, Jennifer Marshall, willl share a project update and describe how to join the MSE Science Team (it's easy!).

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Friday, 15 January 2021

 

CCD Data Reduction with ccdproc

Matthewe Craig (Minnesota State Univ. - Moorhead)
Friday, 15 January - 12:00pm-12:30pm ET

The Astropy affiliated ccdproc package provides many of the necessary tools for processing of CCD images. It is built on a framework that provides error propagation and bad pixel tracking throughout the reduction process. During this webinar, you will receive an introduction to the newly created “CCD Data Reduction” guide developed as a Python analog to the standard IRAF guides by Massey & Davis.

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Northrop Grumman partnerships can enhance your mission

Cherly Reed (Northrop Grumman)
Friday, 15 January - 12:30pm-1:00pm ET

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Virtual Astro-Fashion Show

Emily Rice (STARtorialist)
Friday, 15 January - 1:30pm-2:00pm ET

Celebrate your science with Astro-Fashion! This webinar will showcase the photos and videos submitted by meeting participants during the week and provide an opportunity for a live show-and-tell of our favorite discoveries.

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JWST at Northrop Grumman

Charlie Atkinson (Northrop Grumman)
Friday, 15 January - 2:00pm-2:30pm ET

 

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A Walk Through Fermi Science

David Thompson (NASA/GSFC)
Friday, 15 January - 2:30pm-3:00pm ET

Join us for a walk through of the many exciting science topics investigated by the Fermi Gamma-Ray Space Telescope as it explores the high energy universe.

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Explorers Wanted: Using Gameplay to Engage Astro 101 Students

Jeff Bary (Colgate Univ.), Nicole Gugliucci (Saint Amselm College), Adam Frank (Univ. of Rochester), Ruth Bolster (W. W. Norton & Company)
Friday, 15 January - 4:00pm-4:30pm ET

In this online workshop, Adam Frank and Jeff Bary will discuss how you can use gameplay to get your students to participate in the process of scientific discovery. They will focus specifically on At Play in the Cosmos: The Videogame, a tool that they created to give astro 101 students hands-on opportunities to collect data and apply astronomy concepts that they are learning in class. Nicole Gugliucci, Assistant Professor of Physics at Saint Anselm College, will discuss how she uses the videogame to engage students in her lab.

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