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The systematic uncertainty of the GC excess cau...

The systematic uncertainty of the GC excess caused by the analysis procedures and the ba...

F. Alemanno et al, The Astrophysical Journal Supplement Series 284 1

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Upper panels: integrated intensity map of the R...

Upper panels: integrated intensity map of the ROI from (a) the observations and (b) the ...

F. Alemanno et al, The Astrophysical Journal Supplement Series 284 1

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Left panel: the mean flux of the observed data ...

Left panel: the mean flux of the observed data and the components in the baseline model ...

F. Alemanno et al, The Astrophysical Journal Supplement Series 284 1

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The change of log-likelihood value as a functio...

The change of log-likelihood value as a function of the steepness (upper), the elliptici...

F. Alemanno et al, The Astrophysical Journal Supplement Series 284 1

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The preferred DM parameters for the annihilatio...

The preferred DM parameters for the annihilation channels of (a) ...

F. Alemanno et al, The Astrophysical Journal Supplement Series 284 1

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Several spatial models for the GC excess: (a) t...

Several spatial models for the GC excess: (a) the J-factor map given the gNFW profile wi...

F. Alemanno et al, The Astrophysical Journal Supplement Series 284 1

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The SED of the GC excess (red points) for the b...

The SED of the GC excess (red points) for the baseline background and the best-fit DM an...

F. Alemanno et al, The Astrophysical Journal Supplement Series 284 1

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Alternative bubbles templates with a low-latitu...

Alternative bubbles templates with a low-latitude component for evaluating the systemati...

F. Alemanno et al, The Astrophysical Journal Supplement Series 284 1

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The average residual flux in annuli centered at...

The average residual flux in annuli centered at GC. The gray points show the residual fl...

F. Alemanno et al, The Astrophysical Journal Supplement Series 284 1

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Upper panels: intensity map from 2 to 500 GeV i...

Upper panels: intensity map from 2 to 500 GeV in the CAR projection, smoothed with a Gau...

F. Alemanno et al, The Astrophysical Journal Supplement Series 284 1

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Left panel: the average fluxes of the observed ...

Left panel: the average fluxes of the observed data (black hollow points) and various fi...

F. Alemanno et al, The Astrophysical Journal Supplement Series 284 1

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Left panel: distribution of the values in the s...

Left panel: distribution of the values in the significance map. The map, in HEALPix proj...

F. Alemanno et al, The Astrophysical Journal Supplement Series 284 1

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The average residual flux as a function of angu...

The average residual flux as a function of angular distance to the edge in the high-lati...

F. Alemanno et al, The Astrophysical Journal Supplement Series 284 1

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The SEDs of the northern (blue) and southern (o...

The SEDs of the northern (blue) and southern (orange) lobes. The points show the baselin...

F. Alemanno et al, The Astrophysical Journal Supplement Series 284 1

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(a)–(e) Maps of the components and (f) mask in ...

(a)–(e) Maps of the components and (f) mask in the analyses of the Fermi bubbles. The ma...

F. Alemanno et al, The Astrophysical Journal Supplement Series 284 1

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(a)–(e) Maps of the components and (f) mask in ...

(a)–(e) Maps of the components and (f) mask in the analyses of the GC excess. The first ...

F. Alemanno et al, The Astrophysical Journal Supplement Series 284 1

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The mean fluxes of the components within the RO...

The mean fluxes of the components within the ROI for the best-fit global null (left) and...

F. Alemanno et al, The Astrophysical Journal Supplement Series 284 1

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The mean fluxes of the components within the RO...

The mean fluxes of the components within the ROI for the best-fit global null (left) and...

F. Alemanno et al, The Astrophysical Journal Supplement Series 284 1

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Magnitude differences from three different phot...

Magnitude differences from three different photometric measurements for each source. Blu...

Connor Auge et al, The Astrophysical Journal 1002 1

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The optical/UV SEDs and Swift/XRT data fit with...

The optical/UV SEDs and Swift/XRT data fit with the XSPEC models as described in Section...

Connor Auge et al, The Astrophysical Journal 1002 1

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Cutout images of the Swift/UVOT data in the UVM...

Cutout images of the Swift/UVOT data in the UVM2 band (top) and the HST UVIS data in the...

Connor Auge et al, The Astrophysical Journal 1002 1

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Top: ratio of the flux of the UV/optical disk f...

Top: ratio of the flux of the UV/optical disk flux (1 × 10−7–0.1 keV) derived from the b...

Connor Auge et al, The Astrophysical Journal 1002 1

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Ratio of the bolometric luminosity derived from...

Ratio of the bolometric luminosity derived from the best-fit SEDs in this work using HST...

Connor Auge et al, The Astrophysical Journal 1002 1

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Difference in maximum disk temperature derived ...

Difference in maximum disk temperature derived from the best-fit SEDs in this work using...

Connor Auge et al, The Astrophysical Journal 1002 1

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Difference in the extinction magnitude derived ...

Difference in the extinction magnitude derived from the best-fit SEDs in this work using...

Connor Auge et al, The Astrophysical Journal 1002 1

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