Back to Main Page
Observation Date (UT) Observation Lat

Canonical Name:LHAASO J1849-0003
TeVCat Name:TeV J1849-000
Other Names:HESS J1849-000
2HWC J1849+001
PSR J1849-0001
W 43
Source Type:UNID
R.A.:18 49 24 (hh mm ss)
Dec.:-00 03 00 (dd mm ss)
Gal Long: 32.66 (deg)
Gal Lat: 0.43 (deg)
Distance:
Flux:0.74 (Crab Units)
Energy Threshold:100000 GeV
Spectral Index:
Extended:Yes
Size (X):0.00 (deg)
Size (Y):0.00 (deg)
Discovery Date:2021-05
Discovered By: LHAASO
TeVCat SubCat:Default Catalog

Source Notes:

Details of the source detection:

From Cao et al. (2021):
- "At 100 TeV, the angular and energy resolutions are about 15–20 arcmin
and better than 20%, respectively, allowing adequate spectroscopic and
morphological studies."
- "The statistical significance of the detection above 100 TeV is calculated
using a 0.3deg extension template"
- "Crab Units (CU), flux of the Crab Nebula at 100 TeV; 1 CU = 6.1 x 10-17 photons TeV-1 cm-2 s-1)"
- Significance above 100 TeV: 10.4 sigma
- E_max (PeV): 0.35 +/- 0.07
- Differential photon flux at 100 TeV (CU): 0.74 +/- 0.15
- On-source events/Off-source events: 36/4.8
- Exposure (hr): 1865.3

Source Position:

From Cao et al. (2021):
- R.A. (J2000): 282.35 = 18h 49m 24s
- Dec. (J2000): -0.05 = -00d 03m

Possible Origin:

From Cao et al. (2021):
- This list contains sources potentially at the origin of the LHAASO source, together with their class, their distance, age and luminosity
- PSR J1849-0001, Pulsar, Distance: 7 kpc, Age: 43.1 kyr, L_s: 9.8 x10e36
- W 43, Young Molecular Cloud, Distance: 5.5 kpc

Potential TeV Counterparts:

From Cao et al. (2021):
- This list contains "Nearby teraelectronvolt sources within 1deg of the centre of the LHAASO source"
- HESS J1849-000 / 2HWC J1849+001

Pevatron:

From Mitchell (2021):
- this source is included in a list of Galactic sources currently known
to produce gamma-ray emission above 100 TeV.



Seen by: LHAASO
Want a reference added? Send a bibtex entry to the TeVCat Team