DF1: 1DF Catalog (First D3PO Fermi catalog of gamma-ray source...

Description Usage Format Details Fields Source

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

1

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/


fermicatsR documentation built on May 2, 2019, 10:48 a.m.