Monday, March 03, 2025
10:00 AM - 11:00 AM
Goddard Town Hall
Goddard will hold its next centerwide town hall event on the Greenbelt campus as Center Director Dr. Makenzie Lystrup and other senior leaders preview what’s ahead for Goddard. Doors open at 9:45 a.m.
Read more about this event Tuesday, March 04, 2025
03:30 PM - 05:00 PM
ASD Colloquium Series
Looking at Infrared Background Radiation Anisotropies with Spitzer: Large-scale Anisotropies and Their Implications
Sasha Kashlinsky (NASA GSFC)
We use Spitzer/IRAC deep-exposure data covering two significantly larger than before sky areas to construct maps suitable for evaluating source-subtracted fluctuations in the cosmic infrared background (CIB). The maps are constructed using the self-calibration methodology eliminating artifacts to sufficient accuracy, and subset maps are selected in each area containing approximately uniform exposures. These maps are clipped and removed of known sources and then Fourier transformed to probe the CIB anisotropies to new larger scales. The power spectrum of the resultant CIB anisotropies is measured from the data to >1°, revealing the component well above that from remaining known galaxies on scales >1′. The fluctuations are demonstrated to be free of Galactic and solar system foreground contributions out to the largest scales measured. We discuss the proposed theories for the origin of the excess CIB anisotropies in light of the new data. Out of these, the model where the CIB fluctuation excess originates from the granulation power due to LIGO-observed primordial black holes as dark matter appears most successful in accounting for all observations related to the measured CIB power amplitude and spatial structure, including the measured coherence between the CIB and unresolved cosmic X-ray background (CXB). Finally we point out the use of the data to probe the CIB-CXB cross power to new scales and higher accuracy. We also discuss the synergy of these data with future CIB programs at shorter near-IR wavelengths with deep wide surveys and subarcsecond angular resolution as provided by Euclid and Roman space missions.
Read more about this event Sasha Kashlinsky (NASA GSFC)
We use Spitzer/IRAC deep-exposure data covering two significantly larger than before sky areas to construct maps suitable for evaluating source-subtracted fluctuations in the cosmic infrared background (CIB). The maps are constructed using the self-calibration methodology eliminating artifacts to sufficient accuracy, and subset maps are selected in each area containing approximately uniform exposures. These maps are clipped and removed of known sources and then Fourier transformed to probe the CIB anisotropies to new larger scales. The power spectrum of the resultant CIB anisotropies is measured from the data to >1°, revealing the component well above that from remaining known galaxies on scales >1′. The fluctuations are demonstrated to be free of Galactic and solar system foreground contributions out to the largest scales measured. We discuss the proposed theories for the origin of the excess CIB anisotropies in light of the new data. Out of these, the model where the CIB fluctuation excess originates from the granulation power due to LIGO-observed primordial black holes as dark matter appears most successful in accounting for all observations related to the measured CIB power amplitude and spatial structure, including the measured coherence between the CIB and unresolved cosmic X-ray background (CXB). Finally we point out the use of the data to probe the CIB-CXB cross power to new scales and higher accuracy. We also discuss the synergy of these data with future CIB programs at shorter near-IR wavelengths with deep wide surveys and subarcsecond angular resolution as provided by Euclid and Roman space missions.
Wednesday, March 05, 2025
03:00 PM - 04:30 PM
Scientific Colloquium
Exploring New Worlds with Barbie and Ken
Natasha Latouf, George Mason University
Read more about this event Natasha Latouf, George Mason University
Thursday, March 06, 2025
12:00 PM - 01:00 PM
SED Director's Seminar
Hosted by Earth Sciences Division:
Implementation and Successes of JEDI Data Assimilation in GMAO’s GEOS Systems
- Ron Gelaro (GMAO)
- Doruk Ardag (GMAO/SAMDA)
- Maryam Abdi-Oskouei (JCSDA, UCAR)
Read more about this event Implementation and Successes of JEDI Data Assimilation in GMAO’s GEOS Systems
- Ron Gelaro (GMAO)
- Doruk Ardag (GMAO/SAMDA)
- Maryam Abdi-Oskouei (JCSDA, UCAR)
Tuesday, March 11, 2025
03:30 PM - 05:00 PM
ASD Colloquium Series
TBD
Renee Ludlum (Wayne State U)
Read more about this event Renee Ludlum (Wayne State U)
Thursday, March 13, 2025
12:00 PM - 01:00 PM
SED Director’s Seminar
Please join us for the SED Director’s Seminar. Hosted by the Observational Cosmology Laboratory, Code 665!
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FEATURED STORY
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