THE SPECTRUM AND MORPHOLOGY OF THE FERMI BUBBLES

By Anna Franckowiak. 2014

185 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/b220fa1a8a615cea1588167080cf1500124356cc

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The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. A. Strong
2. E. Orlando
3. Anna Franckowiak
4. Troy A. Porter
5. Igor V. Moskalenko
6. I. Grenier
7. G. Zaharijas
8. G. Jóhannesson

In Nuclear and High Energy Physics

1. A. Strong
2. E. Orlando
3. Anna Franckowiak
4. Troy A. Porter
5. I. Grenier
6. J. Black
7. Igor V. Moskalenko
8. G. Zaharijas

Citations in the corpus

• FERMI-LAT OBSERVATIONS OF HIGH-ENERGY γ-RAY EMISSION TOWARD THE GALACTIC CENTER (2015, methodology): “Without a spatial template for the Fermi bubbles over the region their contribution is tested using a model with an isotropic spatial distribution across the 15◦ × 15◦ region with intensity and spectrum as determined from analyses at higher latitudes (e.g., Ackermann et al. 2014).”
• The Fermi Galactic Center GeV Excess and Implications for Dark Matter (2017, methodology): “The statistical uncertainty is calculated by smoothing the data count maps in each energy bin, di i 2s = ˜ , to avoid bias in using either data or the model as an estimator of standard deviation (see, e.g., AppendixA in Ackermann et al. 2014).”
• DEVELOPMENT OF THE MODEL OF GALACTIC INTERSTELLAR EMISSION FOR STANDARD POINT-SOURCE ANALYSIS OF FERMI LARGE AREA TELESCOPE DATA (2016, background): “The Fermi bubbles correspond to two lobes of hard emission extending north and south from the direction of the GC (Su et al. 2010; Ackermann et al. 2014).”
• The Nine Lives of Cosmic Rays in Galaxies (2015, background): “A detailed spatial and spectral analysis is presented in Ackermann et al. (2014).”
• 2FHL: THE SECOND CATALOG OF HARD FERMI-LAT SOURCES (2015, background): “The count map reported in Figure 1 shows that Fermi-LATobserves many point-like sources and large-scale diffuse emission in the direction of our Galaxy, some of which appears coincident with the so-called Fermi bubbles (Su et al. 2010; Ackermann et al. 2014b).”
• THE SPECTRUM OF ISOTROPIC DIFFUSE GAMMA-RAY EMISSION BETWEEN 100 MeV AND 820 GeV (2014, unknown): “…break in the energy spectrum and the harder injection spectrum for helium are motivated by the results of the measurements of the proton spectrum by the PAMELA satellite (Adriani et al. 2011b), and by the CR spectrum inferred from LAT observations of Earth limb γ rays (Ackermann et al. 2014)11.”