| DF1 {fermicatsR} | R Documentation |
1DF Catalog (First D3PO Fermi catalog of gamma-ray source candidates)
Description
The Denoised, Deconvolved, and Decomposed Fermi Gamma-ray Sky: An application of the D3PO algorithm Selig, M. et al., Astronomy and Astrophysics, 581, 126 (2015).
Usage
DF1
Format
A data frame with 48 variables on 3106 gamma-ray sources.
Details
FITS Filename: catalog_1.fits
Fields
- CandidateName
Candidate Name
- GLON
Galactic Longitude, deg.
- GLAT
Galactic Latitude, deg.
- Flux
Total flux between 1-100 GeV, photon cm^-2 s^-1
- Emid1
Contributing energy band 1, T/F, Emin=0.60 GeV, Emid=0.85 GeV, Max=1.20 GeV
- Emid2
Contributing energy band 2, T/F, Emin=1.20 GeV, Emid=1.70 GeV, Max=2.40 GeV
- Emid3
Contributing energy band 3, T/F, Emin=2.40 GeV, Emid=3.40 GeV, Max=4.80 GeV
- Emid4
Contributing energy band 4, T/F, Emin=4.80 GeV, Emid=6.79 GeV, Max=9.60 GeV
- Emid5
Contributing energy band 5, T/F, Emin=9.60 GeV, Emid=13.58 GeV, Max=19.20 GeV
- Emid6
Contributing energy band 6, T/F, Emin=19.20 GeV, Emid=27.15 GeV, Max=38.40 GeV
- Emid7
Contributing energy band 7, T/F, Emin=38.40 GeV, Emid=54.31 GeV, Max=76.80 GeV
- Emid8
Contributing energy band 8, T/F, Emin=76.80 GeV, Emid=108.61 GeV, Max=153.60 GeV
- Emid9
Contributing energy band 9, T/F, Emin=153.60 GeV, Emid=217.22 GeV, Max=307.20 GeV
- Distance1
Distance1, deg.
- Association1a
Primary association
- Association1b
Association1b
- Association1c
Association1c
- Distance2
Distance2, deg.
- Association2a
Association2a
- Association2b
Association2b
- Association2c
Association2c
- Distance3
Distance3, deg.
- Association3a
Association3a
- Association3b
Association3b
- Association3c
Association3c
- Distance4
Distance4, deg.
- Association4a
Association4a
- Association4b
Association4b
- Association4c
Association4c
- Chi2_PL
Chi-squared (power-law fit), See Equation (2) of Selig et al. (2015)
- Chi2_LP
Chi-squared (log-parabola fit), See Equation (3) of Selig et al. (2015)
- Chi2_EXP
Chi-squared (exponential cut-off fit), See Equation (4) of Selig et al. (2015)
- Gamma_PL
Spectral index (power-law fit), See Equation (2) of Selig et al. (2015)
- Unc_Gamma_PL
Uncertainty in the spectral index (power-law fit), See Equation (2) of Selig et al. (2015)
- Gamma_LP
Spectral index (log-parabola fit), See Equation (3) of Selig et al. (2015)
- Unc_Gamma_LP
Uncertainty in the spectral index (log-parabola fit), See Equation (3) of Selig et al. (2015)
- Gamma_EXP
Spectral index (exponential cut-off fit), See Equation (4) of Selig et al. (2015)
- Unc_Gamma_EXP
Uncertainty in the spectral index (exponential cut-off fit), See Equation (4) of Selig et al. (2015)
- K_PL
Normalization (power-law fit), See Equation (2) of Selig et al. (2015)
- Unc_K_PL
Uncertainty in the normalization (power-law fit), See Equation (2) of Selig et al. (2015)
- K_LP
Normalization (log-parabola fit), See Equation (3) of Selig et al. (2015)
- Unc_K_LP
Uncertainty in the normalization (log-parabola fit), See Equation (3) of Selig et al. (2015)
- K_EXP
Normalization (exponential cut-off fit), See Equation (4) of Selig et al. (2015)
- Unc_K_EXP
Uncertainty in the normalization (exponential cut-off fit), See Equation (4) of Selig et al. (2015)
- Beta_LP
Beta index (log-parabola fit), See Equation (3) of Selig et al. (2015)
- Unc_Beta_LP
Uncertainty in the Beta index (log-parabola fit), See Equation (3) of Selig et al. (2015)
- Ec_EXP
Energy cut-off (exponential cut-off fit), See Equation (4) of Selig et al. (2015)
- Unc_Ec_EXP
Uncertainty in the energy cut-off (exponential cut-off fit), See Equation (4) of Selig et al. (2015)
Source
http://wwwmpa.mpa-garching.mpg.de/ift/fermi/