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Observation Date (UT) Observation Lat

Canonical Name:LS 5039
TeVCat Name:TeV J1826-148
Other Names:HESS J1826-148
2HWC J1825-134
Source Type:Binary
R.A.:18 26 15 (hh mm ss)
Dec.:-14 49 30 (dd mm ss)
Gal Long: 16.90 (deg)
Gal Lat: -1.28 (deg)
Distance: 2.5 kpc
Flux:0.03 (Crab Units)
Energy Threshold:220 GeV
Spectral Index:
Extended:No
Discovery Date:2005-07
Discovered By: H.E.S.S.
TeVCat SubCat:Default Catalog

Source Notes:


H.E.S.S. Galactic Plane Survey (HGPS, 2018):
A selection of information for each of the 78 sources in the HGPS is provided in TeVCat. For full details, visit the HGPS website.

Name: HESS J1826-148
Source Class: Binary
Identified Object: LS 5039
R.A. (J2000): 276.56 deg (18 26 15)
Dec. (J2000): -14.85 deg (-14 50 50)
Positional uncertainty: 0.012 deg
Spatial Model: Gaussian
Size: N/A
Spectral Model: power law
Integral Flux > 1 TeV: 8.35e-13 +/- 7.69e-14 cm-2 s-1
Pivot Energy, E0: 1.05 TeV
Diff. Flux at E0: 9.82e-13 +/- 7.41e-14 cm-2 s-1 TeV-1
Spectral Index: 2.32 +/- 0.07
HGPS Source Notes:
This is one of the 31 firmly-identified objects among the HGPS sources. Three possible associations are listed in Table A.9. "This is a list of astronomical objects, extracted from catalogs of plausible counterparts, which are are found to be spatially coincident with the HGPS source":
- LS 5039 (EXTRA)
- 3FGL J1826.2-1450 (3FGL)
- 2FHL J1826.3-1450 (2FHL)
"EXTRA associations: For completeness, in addition to the associations obtained through the catalog-based, automatic procedure, we add a list of 20 extra associated objects that are plausible counterparts for some HGPS sources and are not covered by the limited set of catalogs we use."


Source position and its uncertainty:

From Aharonian et al. (2005):
- R.A.(J2000): 18 26 15 +/- 32"(stat) +/- 30"(syst)
- Dec.(J2000): -14 49 30 +/- 32"(stat) +/- 30"(syst)
From Aharonian et al. (2006):
- l: 16.879 +/- 12"(stat) +/- 20"(syst) (position converts to R.A.(J2000): 18 26 13.83)
- b: -1.285 +/- 12"(stat) +/- 20"(syst) (position converts to Dec.(J2000): -14 50 55.4)
From HESS Online Catalog:
- R.A. (J2000): 18:26:15
- Dec. (J2000): -14:49:30

Source Association:

From Abeysekara et al. (2017):
- this is one of three sources potentially associated with 2HWC J1825-134

Spectral information:

From Abeysekara et al. (2020):
- "Fitting a power law to the spectrum for each orbital phase interval
gives a photon index of:
... 2.1 +/- 0.2 stat +/- 0.2 sys near inferior conjunction
and
... 2.4 +/- 0.5 stat +/- 0.2 sys near superior conjunction"

Flux:

From Abeysekara et al. (2020):
- "The flux above 1 TeV is:
... (2.5 +/- 0.4stat +/- 0.5sys) x10e-12 cm-2 s-1 near inferior conjunction
(orbital phase 0.45 < phase ≤ 0.9, 232 minutes exposure)
... and (7.8 +/- 2.8stat +/- 1.6sys) ×10e-13 cm-2 s-1 near superior conjunction
(orbital phase 0.0 ≤ phase ≤ 0.45 and 0.9 < phase ≤ 1.0, 230 minutes)"

Pevatron Candidate:

From Alfaro et al. (2025):
- "In this work, we present new observations of LS 5039 obtained with
the High Altitude Water Cherenkov (HAWC) observatory. Our data reveal
that the gamma-ray spectrum of LS 5039 extends up to 200 TeV with no
apparent spectral cut-off. Furthermore, we confirm, with a confidence
level of 4.7 sigma, that the emission between 2 TeV and 118 TeV is
modulated by the orbital motion of the system, which indicates that
these photons are likely produced within or near the binary orbit
where they can undergo absorption by the stellar photons. In a
leptonic scenario, the highest energy photons detected by HAWC can be
emitted by approx. 200 TeV electrons inverse Compton scattering
stellar photons, which would require an extremely efficient
acceleration mechanism operating within LS 5039. Alternatively, a
hadronic scenario could explain the data through proton-proton or
proton-gamma collisions of protons accelerated to peta-electronvolt
(PeV) energies."


Seen by: H.E.S.S., HAWC, VERITAS
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