FIG1 {fermicatsR}

1FIG (First Fermi-LAT Inner Galaxy point source Catalog)

Description

First Fermi-LAT Inner Galaxy point source Catalog (1FIG). Ajello, M. et al., The Astrophysical Journal, 819, 44 (2016).

Usage

FIG1

Format

A data frame with 31 variables on 48 gamma-ray sources.

Details

Results from Table 3 and Table 7 of the journal article.

Fields

Source_Name

1FIG JHHMM.m+DDMM, constructed according to IAU Specifications for Nomenclature; m is decimal minutes of R.A.; in the name R.A. and decl. are truncated at 0.1 decimal minutes and 1' , respectively

GLON

Galactic Longitude, degrees

GLAT

Galactic Latitude, degrees

dTH

Deltatheta, 95% confidence region, deg

TS

Test Statistic

F_PSR_INT

1-100 GeV flux, Pulsars Intensity-scaled, 10^-9 ph cm^-2 s^-1

F_PSR_IND

1-100 GeV flux, Pulsars Index-scaled, 10^-9 ph cm^-2 s^-1

F_PSR_INT

1-100 GeV flux, OBstars Intensity-scaled, 10^-9 ph cm^-2 s^-1

F_PSR_INT

1-100 GeV flux, OBstars Index-scaled, 10^-9 ph cm^-2 s^-1

TYPE

Spectral type, PowerLaw (PL) or LogParabola (LP)

A_PSR_INT

alpha, Pulsars Intensity-scaled, for spectral model dN/dE ~ (E/Eb)^-alpha -beta*log(E/Eb)

UNC_A_PSR_INT

uncertainty in alpha, Pulsars Intensity-scaled

B_PSR_INT

beta, Pulsars Intensity-scaled, for spectral model dN/dE ~ (E/Eb)^-alpha -beta*log(E/Eb)

UNC_B_PSR_INT

uncertainty in beta, Pulsars Intensity-scaled

EB_PSR_INT

Eb, Pulsars Intensity-scaled, for spectral model dN/dE ~ (E/Eb)^-alpha -beta*log(E/Eb)

A_PSR_IND

alpha, Pulsars Index-scaled, for spectral model dN/dE ~ (E/Eb)^-alpha -beta*log(E/Eb)

UNC_A_PSR_IND

uncertainty in alpha, Pulsars Index-scaled

B_PSR_IND

beta, Pulsars Index-scaled, for spectral model dN/dE ~ (E/Eb)^-alpha -beta*log(E/Eb)

UNC_B_PSR_IND

uncertainty in beta, Pulsars Index-scaled

EB_PSR_IND

Eb, Pulsars Index-scaled, for spectral model dN/dE ~ (E/Eb)^-alpha -beta*log(E/Eb)

A_OB_INT

alpha, OBstars Intensity-scaled, for spectral model dN/dE ~ (E/Eb)^-alpha -beta*log(E/Eb)

UNC_A_OB_INT

uncertainty in alpha, OBstars Intensity-scaled

B_OB_INT

beta, OBstars Intensity-scaled, for spectral model dN/dE ~ (E/Eb)^-alpha -beta*log(E/Eb)

UNC_B_OB_INT

uncertainty in beta, OBstars Intensity-scaled

EB_OB_INT

Eb, OBstars Intensity-scaled, for spectral model dN/dE ~ (E/Eb)^-alpha -beta*log(E/Eb)

A_OB_IND

alpha, OBstars Index-scaled, for spectral model dN/dE ~ (E/Eb)^-alpha -beta*log(E/Eb)

UNC_A_OB_IND

uncertainty in alpha, OBstars Index-scaled

B_OB_IND

beta, OBstars Index-scaled, for spectral model dN/dE ~ (E/Eb)^-alpha -beta*log(E/Eb)

UNC_B_OB_IND

uncertainty in beta, OBstars Index-scaled

EB_OB_IND

Eb, OBstars Index-scaled, for spectral model dN/dE ~ (E/Eb)^-alpha -beta*log(E/Eb)

ASSOC_3FGL

3FGL association

Source

http://adsabs.harvard.edu/abs/2016ApJ...819...44A