TeV Gamma-Ray Sources from a Survey of the Galactic Plane with Milagro
arXiv:0705.0707 · doi:10.1086/520717
Abstract
A survey of Galactic gamma-ray sources at a median energy of ~20 TeV has been performed using the Milagro Gamma Ray Observatory. Eight candidate sources of TeV emission are detected with pre-trials significance in the region of Galactic longitude and latitude . Four of these sources, including the Crab nebula and the recently published MGRO J2019+37, are observed with significances after accounting for the trials involved in searching the 3800 square degree region. All four of these sources are also coincident with EGRET sources. Two of the lower significance sources are coincident with EGRET sources and one of these sources is Geminga. The other two candidates are in the Cygnus region of the Galaxy. Several of the sources appear to be spatially extended. The fluxes of the sources at 20 TeV range from ~25% of the Crab flux to nearly as bright as the Crab.
Submitted to ApJ
References in corpus (2)
Cited by in corpus (84)
- Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth
- Fermi Large Area Telescope Bright Gamma-ray Source List
- Teraelectronvolt Astronomy
- The First LHAASO Catalog of Gamma-Ray Sources
- Milagro Observations of Multi-TeV Emission from Galactic Sources in the Fermi Bright Source List
- The Large Scale Cosmic-Ray Anisotropy as Observed with Milagro
- Time-Integrated Searches for Point-like Sources of Neutrinos with the 40-String IceCube Detector
- Constraints on Galactic Neutrino Emission with Seven Years of IceCube Data
- Identification of the TeV Gamma-ray Source ARGO J2031+4157 with the Cygnus Cocoon
- Pulsar Timing for the Fermi Gamma-ray Space Telescope
- Potential PeVatron supernova remnant G106.3+2.7 seen in the highest-energy gamma rays
- The HiSCORE concept for gamma-ray and cosmic-ray astrophysics beyond 10\,TeV
- Fermi-LAT Search for Pulsar Wind Nebulae around gamma-ray Pulsars
- Gamma-ray halos around pulsars as the key to understanding cosmic ray transport in the Galaxy
- HAWC J2227+610 and its association with G106.3+2.7, a new potential Galactic PeVatron
- The High-Altitude Water Cherenkov (HAWC) Observatory in México: The Primary Detector
- Spatially Resolving the Very High Energy emission from MGRO J2019+37 with VERITAS
- Prospects for identifying the sources of the Galactic cosmic rays with IceCube
- ASTRI Mini-Array Core Science at the Observatorio del Teide
- Self-Generated Cosmic-Ray Turbulence Can Explain the Morphology of TeV Halos
- Discovery of High-Energy Gamma-Ray Pulsations from PSR J2021+3651 with AGILE
- TeV Gamma-ray Astronomy: A Summary
- Investigating the TeV Morphology of MGRO J1908+06 with VERITAS
- Very-high energy gamma-ray astronomy: A 23-year success story in high-energy astroparticle physics
- Prospects for Detecting Galactic Sources of Cosmic Neutrinos with IceCube: An Update
- On particle acceleration and transport in plasmas in the Galaxy: theory and observations
- Modelling the Galactic very-high-energy -ray source population
- MAGIC observations provide compelling evidence of the hadronic multi-TeV emission from the putative PeVatron SNR G106.3+2.7
- The GeV-TeV Connection in Galactic gamma-ray sources
- Where are Milky Way's Hadronic PeVatrons?
- Hadronic vs leptonic models for -ray emission from VER J2227+608
- Investigating the nature of MGRO J1908+06 with multiwavelength observations
- Detection of extended gamma-ray emission around the Geminga pulsar with H.E.S.S
- TeV emission of Galactic plane sources with HAWC and H.E.S.S
- X-Ray Emission from the PeVatron-candidate Supernova Remnant G106.3+2.7
- Timing of 29 Pulsars Discovered in the PALFA Survey
- Gamma-ray Observation of the Cygnus Region in the 100 TeV Energy Region
- Revealing a peculiar supernova remnant G106.3+2.7 as a petaelectronvolt proton accelerator with X-ray observations
- Constraints on the TeV source population and its contribution to the galactic diffuse TeV emission
- Fermi-type particle acceleration from magnetic reconnection at the termination shock of a relativistic striped wind
- Radio study of the extended TeV source VER J1907+062
- A Search for Pulsations from Geminga Above 100 GeV with VERITAS
- Multiwavelength investigation of the candidate Galactic PeVatron MGRO J1908+06
- Investigating the multiband nonthermal emission of the 100 TeV source eHWC J2019368 with a pulsar wind nebula scenario
- Ultra-High-Energy Gamma-Ray Astronomy
- Neutrino Observations of LHAASO Sources: Present Constraints and Future Prospects
- Modeling of GeV-TeV gamma-ray emission of Cygnus Cocoon
- The LHAASO PeVatron bright sky: what we learned
- Exploring the hadronic origin of LHAASO J1908+0621
- Gamma/Hadron Separation with the HAWC Observatory
- Neutrino Astronomy with IceCube
- Gamma-ray halos around pulsars: impact on pulsar wind physics and galactic cosmic ray transport
- Galactic and Extragalactic Sources of Very High Energy Gamma-rays
- Galactic Observatory Science with the ASTRI Mini-Array at the Observatorio del Teide
- Constraints on Hadronic Contribution to LHAASO Sources with Neutrino Observations
- Identifying Galactic Sources of High-Energy Neutrinos
- Spectral study of very high energy gamma rays from SS 433 with HAWC
- Suzaku Observation of the Fermi Cygnus Cocoon: Search for a Signature of Young Cosmic-Ray Electrons
- The diffuse GeV-TeV -ray emission of the Cygnus region
- Probing LHAASO Galactic PeVatrons through gamma-ray and neutrino correspondence
- Investigating the radiative properties of LHAASO J1908+0621
- Interpretation of the puzzling gamma-ray spectrum of the Geminga halo
- Significance in Gamma Ray Astronomy with Systematic Errors
- A Possible Hadronic Origin of TeV Photon Emission from SNR G106.3+2.7
- Gamma-ray Astronomy with Muons: Sensitivity of IceCube to PeVatrons in the Southern Sky
- Cosmic ray backgrounds for dark matter indirect detection
- Search for galactic Pevatron candidates in a population of unidentified gamma-ray sources
- Exploring the high energy frontiers of the Milky Way with ground-based gamma-ray astronomy: PeVatrons and the quest for the origin of Galactic cosmic-rays
- Gamma-rays from the binary system containing PSR J2032+4127 during its periastron passage
- Multiwavelength Investigation of -ray Source MGRO J1908+06 Emission Using Fermi-LAT, VERITAS, and HAWC
- Detecting the brightest HAWC sources with IceCube in the upcoming years
- Multi-wavelength study of the MGRO J2019+37
- Status of Very High Energy gamma-ray Astronomy as of early 2008
- Milagro Observations of Potential TeV Emitters
- Search for the Galactic accelerators of Cosmic-Rays up to the Knee with the Pevatron Test Statistic
- Cosmic Rays and Non-thermal Emission Induced by Accretion of Cool Gas onto the Galactic Disk
- The Very Energetic Radiation Imaging Telescope Array System (VERITAS)
- PHECT: A lightweight computation tool for pulsar halo emission
- Method for testing diffusive shock acceleration and diffusion propagation of 1-100 TeV cosmic electrons with multiwavelength observations of the Geminga halo and pulsar wind nebula
- Studying particle acceleration from driven magnetic reconnection at the termination shock of a relativistic striped wind using particle-in-cell simulations
- FIPSER: Performance Study of a Readout Concept With Few Digitization Levels for Fast Signals
- HAWC Study of the Ultra-High-Energy Spectrum of MGRO J1908+06
- IRAM 30 m CO-line Observation toward PeVatron Candidate G106.3+2.7: Direct Interaction between the Shock and the Molecular Cloud Remains Uncertain
- Particle Acceleration in the Cygnus Superbubble