A census of high-energy observations of Galactic supernova remnants

Authors and credits: This database is maintained by Gilles Ferrand, under the supervision of Samar Safi-Harb, in the SNR group of the Department of Physics and Astronomy at the University of Manitoba.
The list of SNRs with their basic physical properties is based on the radio Catalogue of Galactic Supernova Remnants by Dave Green (note: the list aims to be complete for Galactic SNRs, but it does not include any extragalactic object). This work also builds on the List of Galactic SNRs Interacting with Molecular Clouds maintained by Bing Jiang, and on the census of the youngest Galactic SNRs by Matthieu Renaud. Entries have also been cross-checked with the Pulsar Wind Nebula Catalog and the SGR/AXP Catalog from the McGill Pulsar Group.

More detailed information on this work (motivation, usage, statistics, future extensions) can be found in a companion paper published in Advances in Space Research: Ferrand, G., Safi-Harb, S., A Census of High-Energy Observations of Galactic Supernova Remnants, ASR, 49, 9, 1313-1319, doi:10.1016/j.asr.2012.02.004 (final draft also available at arXiv:1202.0245). When making use of this catalogue for your own research, we kindly ask you to cite this article in your publications. We also encourage all users to publicise the URL of this website in their papers, presentations, proposals, or webpages: http://www.physics.umanitoba.ca/snr/SNRcat

You can send us feedback with this form. 		Description: The table on this page is the list of all the identified SNRs. Each row corresponds to a single object. Click anywhere on the row to open the full record in a new page, with more details and references. The columns of this table summarize the properties and observational status of all the SNRs.
The first columns (with grey background) describe the SNR (identification, environment, main physical properties). Note the question marks, that denote uncertain identifications or associations, and the strikes, that denote obsolete names or discarded claims. Note also that the given ages and distances are only the best current estimates (and might be incomplete). We use the following abbreviations in the context column: NS: Neutron Star, PSR: Pulsar, AXP: Anomalous X-ray Pulsar, SGR: Soft Gamma-ray Repeater, CCO: Central Compact Object.
The last columns summarize the observations of these remnants, with various modern X-ray and gamma-ray observatories. Colours code the current view of a given instrument as follows:
 missed : the region was observed, but no significant source was detected;
 detected : a source was detected, but it is not possible to measure its extension;
 extended : the source is clearly extended, it might show structures or not.
A purely black cell merely means lack of data: it might be that the object is not observable with this instrument, or that it has not been oberved yet, or that the results have not been disclosed.
Also note that a detection does not always imply a physical connection with the remnant: check the full record to learn more about the source(s) of emission.
Manipulation: You can re-order the instrumental columns by dragging-and-dropping the header of one column (reload the page to reset the order). You can also sort all rows according to an instrument by clicking on the header of its column (click again to unsort, hold the shift key to select other columns). Finally, you can filter rows in various ways:
• by selecting an item in the drop-down list below instruments headers. Select for instance 1-HESS-extended to get all SNRs for which HESS can measure the extension.
• by typing text in the field below other headers, to filter a given column. Try for instance magnetar in the context field, or SN in the age field. Note that you can search for abbreviated names in the ID field: for instance typing G11.2-0.3 will show G011.2-00.3.
• by typing in the field just below this paragraph, to filter the whole table. Note that the resolution levels defined in the previous section are actually present in the cells as invisible text, so that you can for instance type missed to get all records of failed observations.
The search in text fields supports logical expressions (AND, OR, NOT), as well as grouping with brackets () and quotes "". For instance, you can get all observations made with Chandra of remnants suspected to interact with molecular clouds, by typing below: (NOT CHANDRA-unknown) AND cloud. Note that instrument cells are all suffixed with -X for X-rays and -g for gamma-rays, so that you can for instance type extended-g to get all extended gamma-ray sources.

 Global filter:   

Number of objects displayed:
IDnamescontextSNagedistancetypeCHANDRAXMMSUZAKUROSATASCAFERMIAGILEHESSVERITASMAGICMILAGRO
G000.0+00.0 Sgr A East, 1FGL J1745.6-2900c, 2FGL J1745.6-2858, HESS J1745-290 contains NS J174545.5-285829?, close to BH Sgr A*, interacts with molecular cloud shell CHANDRA XMM SUZAKU FERMI HESS
G000.1-00.1 1FGL J1746.4-2849c PWN G0.13-0.11 filled-centre? FERMI
G000.3+00.0 G0.33+0.04, G0.4+0.1 shell FERMI
G000.9+00.1 HESS J1747-281 contains PSR candidate J1747-2809 + PWN 1900 yr
PSR: 5000 yr		 10 kpc
PSR: 13 kpc		 composite CHANDRA XMM FERMI HESS
G001.0-00.1 Sgr D SNR, G1.05-0.1, G1.05-0.15 close to star forming region Sgr D, interacts with molecular cloud shell SUZAKU FERMI
G001.4-00.1 interacts with molecular cloud shell FERMI
G001.9+00.3 110 - 170 yr 8.5 kpc shell CHANDRA FERMI
G003.7-00.2 G003.8-00.3 shell FERMI
G003.8+00.3 shell? FERMI
G004.2-03.5 shell FERMI
G004.5+06.8 Kepler, SN1604, 3C358 1604 SN: 408 yr 3 - 6.4 kpc shell CHANDRA XMM SUZAKU ROSAT ASCA FERMI HESS
G004.8+06.2 G4.5+6.2 shell FERMI
G005.2-02.6 shell ASCA FERMI
G005.4-01.2 ? Milne 56, G5.3-1.0, G5.27-0.9, 2FGL J1802.3-2445c offset PSR J1801-2451 = B1757-24 = the Duck at the tip of radio protuberance G5.27-0.9, interacts with molecular cloud 4.3 - 4.5 kpc
PSR: 5 kpc		 composite? CHANDRA FERMI
G005.5+00.3 G5.55+0.32 shell FERMI
G005.7-00.1 ? G5.71-0.08, HESS J1800-240C close to SNR G006.4-00.1 = W28, interacts with molecular cloud ? HESS
G005.9+03.1 shell FERMI
G006.1+00.5 G6.10+0.53 shell FERMI
G006.1+01.2 G6.1+1.15 filled-centre FERMI
G006.4+04.0 shell FERMI
G006.4-00.1 W28, G6.6-0.2, 0FGL J1801.6-2327, 1FGL J1801.3-2322c and J1800.5-2359c, HESS J1801-233 and HESS J1800-240[A/B/C] close to (unrelated) PSR B1758-23 = J1801-23, close to SNRs G5.7-0.1, G6.5-0.4, G7.0-0.1, interacts with molecular cloud 35000 - 150000 yr 1.8 - 1.9 kpc composite CHANDRA XMM SUZAKU ROSAT ASCA FERMI AGILE HESS
G006.5-00.4 G6.51-0.48, G6.67-0.42, HESS J1801-233 close to SNR G006.4-00.1 = W28 shell FERMI HESS
G007.0-00.1 G7.06-0.12 close to SNR G006.4-00.1 = W28 shell FERMI
G007.2+00.2 G7.20+0.20 shell FERMI
G007.5-01.7 ? contains Taz PWN ≥ 15000 yr 1.7 - 2 kpc composite CHANDRA ROSAT ASCA
G007.7-03.7 1814-24 4.5 kpc shell ASCA FERMI
G008.3-00.0 G8.31-0.09 shell FERMI
G008.7-00.1 W30, G8.6-0.1, Suzaku J1804-2142 and J1804-2140, 1FGL J1805.2-2137c and J1806.8-2109c, HESS J1804-216 inside W30 complex, contains PSR B1800-21 and PWN G8.40+0.15, interacts with molecular cloud 4 kpc
PSR: 4 kpc		 shell? CHANDRA SUZAKU ROSAT FERMI HESS
G008.7-05.0 shell FERMI
G008.9+00.4 G8.90+0.40 shell FERMI
G009.7-00.0 G9.7-0.1, G9.70-0.06 interacts with molecular cloud shell FERMI
G009.8+00.6 shell FERMI
G009.9-00.8 G9.95-0.81 shell FERMI
G010.5-00.0 G10.59-0.04 shell ASCA FERMI
G010.9-45.4 PWN G10.93-45.44 and PSR J2124-3358 PSR: 0.25 kpc filled-centre? CHANDRA XMM ASCA
G011.0-00.0 G11.0+0.0, G11.03-0.05 contains PWN? shell ASCA FERMI
G011.1+00.1 G11.18+0.11 shell FERMI
G011.1-00.7 G11.15-0.71 shell FERMI
G011.1-01.0 G11.2-1.1, G11.17-1.04 shell FERMI
G011.2-00.3 HESS J1809-193 contains PSR J1811-1925 = the Turtle + PWN G011.18-0.35, close to PSR J1809-1917 + PWN G11.09+0.08, interacts with molecular cloud 386 ? 960 - 3400 yr
PSR: 24000 yr
SN: 1626 yr ?		 ≥ 5 kpc
PSR: 5 kpc		 composite CHANDRA XMM ROSAT ASCA FERMI HESS
G011.4-00.1 2FGL J1811.1-1905c shell? FERMI
G011.8-00.2 G11.89-0.21 shell ASCA FERMI
G012.0-00.1 shell? SUZAKU ASCA FERMI
G012.2+00.3 G12.26+0.30 shell FERMI
G012.5+00.2 G12.58+0.22 composite? FERMI
G012.7-00.0 G12.72-0.00 shell FERMI
G012.8-00.0 W33, G12.82-0.02, G12.83-0.02, AX J1813-178, 0FGL J1814.3-1739, HESS J1813-178 close to W33 complex, contains PSR J1813-1749 + PWN, interacts with molecular cloud 1200 yr
PSR: 5000 yr		 PSR: 4.7 kpc composite? CHANDRA XMM ASCA FERMI HESS MAGIC
G013.3-01.3 G13.46+0.16 interacts with molecular cloud shell? ROSAT FERMI
G013.5+00.2 shell FERMI
G014.1-00.1 G14.18-0.12 shell FERMI
G014.3+00.1 G14.30+0.14 shell FERMI
G015.1-01.6 shell FERMI
G015.4+00.1 G15.42+0.18, HESS J1818-154 shell? FERMI HESS
G015.9+00.2 contains CCO? 1000 yr 8.5 kpc shell? CHANDRA FERMI HESS
G016.0-00.5 G16.05-0.57 shell FERMI
G016.2-02.7 shell FERMI
G016.4-00.5 G16.41-0.55 shell FERMI
G016.7+00.1 G16.73+0.08 contains PWN, interacts with molecular cloud PSR: 2000 yr 10 kpc composite CHANDRA XMM ASCA FERMI HESS
G016.8-01.1 G16.85-1.05 ? FERMI
G017.0-00.0 G17.02-0.04 shell FERMI
G017.4-00.1 G17.48-0.12 shell FERMI
G017.4-02.3 shell FERMI
G017.8-02.6 shell FERMI
G018.0-00.7 Turkey, 2FGL J1824.5-1351e, HESS J1825-137 PWN G18.00-0.69 and PSR J1826-1334 = B1823-13 PSR: 4 kpc filled-centre? CHANDRA XMM SUZAKU ROSAT FERMI HESS
G018.1-00.1 G18.1-0.2, G18.16-0.16 shell ASCA FERMI
G018.5-00.4 Eel filled-centre? CHANDRA
G018.6-00.2 G18.62-0.28 shell FERMI
G018.8+00.3 Kes 67, G18.9+0.3 in complex region near HII region W39, interacts with molecular cloud 9.5 kpc shell FERMI
G018.9-01.1 G18.95-1.1, G18.94-1.04 contains PWN?, interacts with molecular cloud?? 2 kpc composite? CHANDRA ROSAT ASCA FERMI
G019.1+00.2 G19.15+0.27 shell FERMI
G020.0-00.2 2FGL J1828.3-1124c contains PWN? filled-centre FERMI
G020.4+00.1 G20.47+0.16 shell FERMI
G021.0-00.4 G21.04-0.47 shell FERMI
G021.5-00.1 G21.56-0.10 shell ASCA FERMI
G021.5-00.9 HESS J1833-105 contains PSR J1833-1034 + PWN G021.50-0.89 720 - 1070 yr
PSR: 4800 yr		 4.3 - 5.1 kpc
PSR: 4.7 kpc		 composite CHANDRA XMM SUZAKU ROSAT ASCA FERMI HESS
G021.8-00.6 Kes 69 interacts with molecular cloud 5.5 kpc shell XMM ROSAT ASCA FERMI
G022.7-00.2 overlaps SNR G23.3-0.3, interacts with molecular cloud?? shell? FERMI HESS
G023.3-00.3 W41, 0FGL J1834.4-0841, 1FGL J1834.3-0842c, 2FGL J1834.3-0848, HESS J1834-087 overlaps SNR G22.7-0.2, contains PSR J1834-0844 + PWN?, interacts with molecular cloud?? 100000 yr 3.9 - 4.5 kpc shell? CHANDRA XMM FERMI HESS MAGIC
G023.6+00.3 in complex region ? FERMI
G024.7+00.6 1FGL J1834.7-0709c, 2FGL J1834.7-0705c contains PWN? composite? FERMI
G024.7-00.6 shell? FERMI
G025.5+00.0 HESS J1837-069 PSR J1838-0655 + PWN at the edge ? CHANDRA SUZAKU ASCA HESS
G027.4+00.0 Kes 73, 4C-04.71, G27.3-0.1, 2FGL J1841.2-0459c contains AXP 1E 1841-045 (magnetar) 1100 - 1500 yr
PSR: 4300 yr		 7.5 - 9.1 kpc shell CHANDRA XMM SUZAKU ROSAT ASCA FERMI HESS
G027.8+00.6 2FGL J1840.3-0413c contains PWN? filled-centre XMM FERMI
G028.6-00.1 AX J1843.8-0352 ≤ 2700 yr 6 - 8.5 kpc shell CHANDRA ASCA FERMI HESS
G028.8+01.5 2FGL J1839.7-0334c shell? XMM ROSAT ASCA FERMI
G029.6+00.1 contains AXP candidate AX J1845-0258 (magnetar?) shell ASCA FERMI
G029.7-00.3 Kes 75, HESS J1846-029 contains high-B PSR J1846-0258 (magnetar?) + PWN, interacts with molecular cloud 900 - 4300 yr
PSR: 723 yr		 10.6 kpc
PSR: 19 kpc		 composite CHANDRA ASCA FERMI HESS
G030.7+01.0 shell? ASCA FERMI
G030.7-02.0 contains compact source near center ? FERMI
G031.5-00.6 G31.55-0.65 shell? FERMI
G031.9+00.0 3C391, 1FGL J1849.0-0055, 2FGL J1849.3-0055 interacts with molecular cloud 3700 - 4400 yr ≥ 7.2 kpc shell CHANDRA XMM ROSAT ASCA FERMI HESS
G032.0-04.9 3C396.1 shell? FERMI
G032.1-00.9 composite? ROSAT ASCA FERMI
G032.4+00.1 G32.45+0.1, 2FGL J1850.7-0014c shell XMM FERMI
G032.8-00.1 Kes 78, G33.1-0.1, HESS J1852-000 interacts with molecular cloud 4.8 kpc shell? XMM ROSAT FERMI HESS
G033.2-00.6 shell FERMI
G033.6+00.1 Kes 79, 4C00.70, HC13, G33.7+0.0, 2FGL J1852.7+0047c contains CCO PSR J1852+0040, interacts with molecular cloud? 3000 - 15000 yr 7.1 kpc shell CHANDRA XMM ROSAT ASCA FERMI
G034.0+20.3 PWN G34.01+20.27 and PSR J1740+1000 PSR: 1.4 kpc filled-centre? CHANDRA XMM
G034.7-00.4 W44, 3C392, G34.6-0.5, 0FGL J1855.9+0126, 1FGL J1856.1+0122 contains PSR B1853+01 = J1856+0113 + PWN G34.56-0.50, interacts with molecular cloud ≥ 10000 yr
PSR: 20000 yr		 3 kpc
PSR: 3 kpc		 composite CHANDRA XMM ROSAT ASCA FERMI AGILE VERITAS
G035.6-00.4 ? HESS J1858+020 contains PSR B1855+02 30000 yr
PSR: 160000 yr		 3.7 - 10.5 kpc
PSR: 8 kpc		 shell FERMI HESS
G036.6+02.6 shell FERMI
G036.6-00.7 shell? FERMI
G039.2-00.3 3C396, HC24, NRAO 593 contains PWN, interacts with molecular cloud 3000 - 7000 yr 6.2 kpc composite CHANDRA ASCA FERMI
G039.7-02.0 ? W50, G40.0-3.1 adjacent to HII region S74, contains micro-quasar SS433, interacts with molecular cloud?? 5.5 - 6.5 kpc ? CHANDRA XMM ROSAT ASCA FERMI
G040.5-00.5 0FGL J1907.5+0602, HESS J1908+063, MGRO J1908+06 PSR J1907+0602 nearby, interacts with molecular cloud? PSR: 20000 yr PSR: 3.2 kpc shell CHANDRA XMM ASCA FERMI HESS VERITAS MILAGRO
G041.1-00.3 3C397 interacts with molecular cloud 5300 yr 10.3 kpc shell CHANDRA XMM ROSAT ASCA FERMI
G042.8+00.6 G42.8+0.65 SGR 1900+14 (magnetar) and NS J1907+0918 just outside the shell, interacts with molecular cloud? PSR: 6 kpc shell CHANDRA XMM SUZAKU ROSAT ASCA FERMI
G043.3-00.2 W49B, 3C398, 0FGL J1911.0+0905, 2FGL J1911.0+0905, HESS J1911+090 near HII region W49A, interacts with molecular cloud 1000 - 4000 yr 8 - 11 kpc composite CHANDRA XMM SUZAKU ROSAT ASCA FERMI HESS
G043.9+01.6 shell? FERMI
G045.7-00.4 1FGL J1916.0+1110c, 2FGL J1916.1+1106 shell FERMI
G046.8-00.3 (HC30), G46.6-0.2 6.8 - 8.8 kpc shell FERMI
G047.4-03.9 PWN G47.38-3.88 and PSR J1932+1059 = B1929+10 PSR: 0.36 kpc filled-centre? CHANDRA XMM ROSAT ASCA
G049.2-00.7 W51C, 0FGL J1923.0+1411, 1FGL J1922.9+1411, HESS J1923+141 part of W51 complex, overlaps SFR W51B, contains CXO J192318.5+1403035 + PWN, interacts with molecular cloud 10000 yr 5.5 - 6 kpc composite? CHANDRA ROSAT ASCA FERMI HESS MAGIC MILAGRO
G053.6-02.2 3C400.2, NRAO 611, G53.7-2.2 15000 yr 2.8 kpc composite ROSAT ASCA FERMI
G054.1+00.3 contains PSR J1930+1852 + PWN G054.10+0.27, interacts with molecular cloud? 2500 - 3300 yr
PSR: 2900 yr		 5.6 - 7.2 kpc
PSR: 5 kpc		 filled-centre? CHANDRA XMM SUZAKU ROSAT ASCA FERMI VERITAS
G054.4-00.3 (HC40), G54.5-0.3, 2FGL J1932.1+1913 interacts with molecular cloud shell ASCA FERMI
G055.0+00.3 G55.2+0.5 PSR J1932+2020 nearby 14 kpc shell FERMI
G055.7+03.4 contains (unrelated?) PSR B1919+21 shell FERMI
G057.2+00.8 (4C21.53) PSR B1937+214 nearby shell? FERMI
G059.2-04.7 Black Widow PWN G59.20-4.70 and PSR J1959+2048 = B1957+20 PSR: 2.5 kpc filled-centre? CHANDRA FERMI
G059.5+00.1 G59.6+0.1 shell FERMI
G059.8+01.2 G59.7+1.2 ? FERMI
G063.7+01.1 contains PWN, interacts with molecular cloud?? filled-centre FERMI
G065.1+00.6 0FGL J1954.4+2838 PSR J1957+2831 nearby 9 kpc shell FERMI MAGIC MILAGRO
G065.3+05.7 G65.2+5.7 PSR J1931+30 nearby 0.8 kpc composite? CHANDRA ROSAT FERMI
G065.7+01.2 ? DA 495, G55.7+1.2 contains PWN 1.5 kpc filled-centre CHANDRA ROSAT ASCA FERMI
G067.7+01.8 shell FERMI
G068.6-01.2 ? FERMI
G069.0+02.7 ? CTB 80, W56, G68.8+2.8 contains PSR B1951+32 = J1952+3252 + PWN G68.77+2.82, interacts with molecular cloud 1408 SN: 604 yr PSR: 2.5 kpc filled-centre? CHANDRA ROSAT ASCA FERMI MAGIC
G069.7+01.0 shell ROSAT ASCA FERMI
G073.9+00.9 10000 yr 1.3 kpc shell? FERMI
G074.0-08.5 Cygnus Loop, W78, Sh2-103, contains Veil Nebula, NGC 6960, NGC 6992, NGC 6995, NGC 6974, NGC 6979, IC 1340, 1FGL J2046.4+3041 and J2049.1+3142 and J2055.2+3144 and J2057.4+3057 contains several compact sources, interacts with molecular cloud? 14000 yr 0.46 - 0.62 kpc shell CHANDRA XMM SUZAKU ROSAT ASCA FERMI
G074.9+01.2 CTB 87, 2FGL J2015.6+3709 contains PWN, interacts with molecular cloud?? 6.1 - 12 kpc filled-centre CHANDRA ASCA FERMI VERITAS
G075.2+00.1 Cisne, MGRO J2021+37 PWN G75.23+0.12 and PSR J2021+3651 ≥ 10 kpc
PSR: 4 kpc		 filled-centre? CHANDRA VERITAS MILAGRO
G076.9+01.0 2FGL J2022.8+3843c contains PSR J2022+3842 + PWN PSR: 9000 yr 8 kpc filled-centre? CHANDRA FERMI
G078.2+02.1 W66, DR4, gamma Cygni, G78.1+1.8, 1FGL J2020.0+4049, 2FGL J2019.1+4040, VER J2019+407 contains NS J2020.2+4026?, interacts with molecular cloud? 6600 yr 1.5 kpc shell CHANDRA ASCA FERMI VERITAS MAGIC
G082.2+05.3 W63, G82.5+5.3 shell ROSAT ASCA FERMI MAGIC
G083.0-00.3 shell FERMI
G084.2-00.8 interacts with molecular cloud? 11000 yr 4.5 kpc shell CHANDRA FERMI
G085.4+00.7 3.5 kpc composite CHANDRA XMM ROSAT FERMI MAGIC
G085.9-00.6 4.8 kpc composite CHANDRA XMM ROSAT FERMI MAGIC
G089.0+04.7 HB21, 1FGL J2042.3+5041 and J2046.0+4954, 2FGL J2041.5+5003 and J2043.3+5105 and J2046.0+4954 contains 4C50.52, interacts with molecular cloud 19000 yr 0.8 kpc composite ROSAT ASCA FERMI MAGIC
G093.3+06.9 DA 530, 4C(T)55.38.1, G93.2+6.7 contains PWN 5000 yr 1.7 - 2.7 kpc composite? CHANDRA XMM SUZAKU FERMI
G093.7-00.2 CTB 104A, DA 551, G93.6-0.2, G93.7-0.3 interacts with molecular cloud 1.5 kpc shell FERMI MAGIC
G094.0+01.0 3C434.1 interacts with molecular cloud?? 5.2 kpc shell FERMI
G096.0+02.0 4 kpc shell FERMI
G106.3+02.7 0FGL J2229.0+6114, 2FGL J2229.0+6114 contains PSR J2229+6114 and PWN G106.65+2.96 = the Boomerang, interacts with molecular cloud?? PSR: 10000 yr 0.8 kpc
PSR: 3 kpc		 composite? CHANDRA SUZAKU ROSAT ASCA FERMI VERITAS MAGIC MILAGRO
G107.5-01.5 ? shell XMM
G108.2-00.6 3.2 kpc shell FERMI
G108.6+06.8 Guitar nebula contains PSR J2225+6535 = B2224+65 PSR: 1 kpc filled-centre? CHANDRA XMM ROSAT
G109.1-01.0 CTB 109 contains AXP 1E 2259+586 (magnetar), interacts with molecular cloud 7900 - 9700 yr 3 - 3.4 kpc shell CHANDRA XMM ROSAT ASCA FERMI VERITAS
G111.7-02.1 Cassiopeia A (Cas A), W81, 3C461, 1FGL J2323.4+5849, 2FGL J2323.4+5849 contains CCO, interacts with molecular cloud?? 1680 316 - 352 yr
SN: 332 yr		 3.3 - 3.7 kpc shell CHANDRA XMM ROSAT ASCA FERMI VERITAS MAGIC
G113.0+00.2 contains PSR B2324+60 = J2326+6113 PSR: 10000000 yr 3.1 kpc
PSR: 4.8 kpc		 ? FERMI
G114.3+00.3 2FGL J2333.3+6237 contains HII region S165 and PSR 2334+61 41000 yr 0.7 kpc shell ROSAT FERMI
G116.5+01.1 2FGL J2358.9+6325 280000 yr 1.6 kpc shell FERMI
G116.9+00.2 CTB 1, G117.3+0.1, G116.9+0.1 contains PSR J0002+6246 44000 yr 1.6 kpc composite CHANDRA ROSAT ASCA FERMI
G119.5+10.2 CTA 1, G119.5+10.3, 0FGL J0007.4+7303 contains PSR J0007+7303 + PWN 1.4 kpc shell CHANDRA XMM ROSAT ASCA FERMI AGILE VERITAS
G120.1+01.4 Tycho, 3C10, SN1572 interacts with molecular cloud? 1572 SN: 440 yr 2.5 - 5 kpc shell CHANDRA XMM SUZAKU ROSAT ASCA FERMI VERITAS
G126.2+01.6 shell? FERMI
G127.1+00.5 R5, G127.3+0.7 associated with open cluster NGC 559? 1.2 - 1.3 kpc shell CHANDRA FERMI
G130.7+03.1 3C58, SN1181 contains PSR J0205+6449 + PWN 1181 ? ≤ 7000 yr
PSR: 5400 yr
SN: 831 yr ?		 2 - 3.2 kpc
PSR: 3.2 kpc		 filled-centre CHANDRA XMM ROSAT ASCA FERMI VERITAS MAGIC
G132.7+01.3 HB3, G132.4+2.2, 1FGL J0218.8+6158c and J0220.0+6257, 2FGL J0214.5+6251c and J0218.7+6208c and J0221.4+6257c adjacent to W3/4/5 complex, PSR J0215+6218 nearby, interacts with molecular cloud? 2.2 kpc shell XMM ROSAT ASCA FERMI
G148.1+00.8 PWN Mushroom and PSR B0355+54 filled-centre? CHANDRA XMM
G156.2+05.7 1FGL J0500.1+5237 1.3 kpc shell CHANDRA SUZAKU ROSAT ASCA FERMI
G160.9+02.6 HB9, G160.5+2.8, G160.4+2.8, 1FGL J0503.2+4526, 2FGL J0503.2+4643 contains PSR B0459+47, interacts with molecular cloud?? 1.5 - 4 kpc composite CHANDRA ROSAT FERMI MAGIC
G166.0+04.3 VRO 42.05.01, 2FGL J0526.6+4308 interacts with molecular cloud?? 4.5 kpc shell ASCA FERMI
G179.0+02.6 1FGL J0553.9+3105, 2FGL J0553.9+3104 shell? FERMI
G180.0-01.7 S147, Sh2-240, Spaghetti Nebula, 1FGL J0538.6+2717, 2FGL J0538.1+2718 contains PSR J0538+2817 and PWN G179.72-1.69 26000 - 34000 yr
PSR: 620000 yr		 0.36 - 0.88 kpc
PSR: 1.47 kpc		 shell CHANDRA XMM FERMI
G182.4+04.3 shell FERMI
G184.6-05.8 Crab Nebula, 3C144, SN1054, NGC 1952, M1, 0FGL J0534.6+2201, HESS J0534+220 contains PSR B0531+21 = J0534+2200 + PWN, interacts with molecular cloud 1054 SN: 958 yr 1.5 - 2.5 kpc
PSR: 2 kpc		 filled-centre CHANDRA XMM ROSAT FERMI AGILE HESS VERITAS MAGIC MILAGRO
G189.1+03.0 IC443, 3C157, Sh2-248, Jellyfish Nebula, 0FGL J0617.4+2234, 1FGL J0617.2+2233, MAGIC J0616+225 overlaps SNR G189.6+03.3, contains runaway NS CXOU J061705.3+222127 + trail PWN, interacts with molecular cloud 837 4000 yr
SN: 1175 yr		 0.7 - 2 kpc composite CHANDRA XMM SUZAKU ROSAT ASCA FERMI AGILE VERITAS MAGIC MILAGRO
G189.6+03.3 ? overlaps SNR G189.1+03.0 = IC443, contains PSR ≥ 30000 yr composite? CHANDRA
G192.8-01.1 PKS 0607+17, G193.3-1.5 part of Origem Loop?, interacts with molecular cloud?? shell FERMI
G195.1+04.3 Geminga contains PSR J0633+1746 PSR: 0.25 kpc filled-centre? CHANDRA XMM ROSAT ASCA FERMI AGILE VERITAS MAGIC MILAGRO
G205.5+00.5 Monoceros Loop, 1FGL J0636.0+0458c, 2FGL J0631.6+0640 and J0636.0+0554 and J0637.8+0737, HESS J0632+057 interacts with Rosette nebula, close to SNR G206.9+02.3, interacts with molecular cloud?? 0.8 - 1.6 kpc shell CHANDRA XMM FERMI HESS VERITAS
G206.9+02.3 PKS 0646+06 close to SNR G205.5+00.5 = Monoceros Nebula shell? FERMI
G230.4-01.4 PWN G230.39-1.42 and PSR J0729-1448 PSR: 4 kpc filled-centre? CHANDRA
G260.4-03.4 Puppis A, MSH 08-44, 1FGL J0823.3-4248, 2FGL J0821.0-4254 and J0823.0-4246 and J0823.4-4305 overlaps SNR G263.9-3.3 = Vela, contains CCO PSR RX J0822-4300, interacts with molecular cloud?? 3700 - 5500 yr 2 kpc shell CHANDRA XMM SUZAKU ROSAT ASCA FERMI
G261.9+05.5 shell ASCA FERMI
G263.9-03.3 Vela, contains NGC 2736 = Pencil Nebula, 1FGL J0841.9-4620, 2FGL J0842.9-4721 and J0835-4510 and J0833.1-4511e, HESS J0835-455 overlaps SNR G260.4-3.4 and SNR G266.2-1.2, contains PSR B0833-45 = J0835-4510 + PWN Vela X (unrelated to eclipsing binary Vela X-1), interacts with molecular cloud? 9000 - 27000 yr
PSR: 11400 yr		 0.25 - 0.3 kpc
PSR: 0.29 kpc		 composite CHANDRA XMM SUZAKU ROSAT ASCA FERMI AGILE HESS
G266.2-01.2 Vela Jr, RX J0852.0-4622, AX J0851.9-4617.4, 1FGL J0854.0-4632, 2FGL J0848.5-4535 and J0851.7-4635 and J0853.5-4711 and J0855.4-4625, HESS J0852-463 overlaps SNR G263.9-3.3 = Vela, contains CCO CXOU J085201.4-461753, PSR J0855-4644 + PWN at the edge 700 - 4300 yr 0.2 - 2.4 kpc shell CHANDRA XMM SUZAKU ROSAT ASCA FERMI HESS
G272.2-03.2 6000 yr 1.8 - 5 kpc composite CHANDRA XMM SUZAKU ROSAT ASCA FERMI
G279.0+01.1 shell FERMI
G284.3-01.8 MSH 10-53, G284.2-1.8, 0FGL J1018.2-5858, 1FGL J1018.6-5856 PSR J1016-5857 + PWN G284.08-1.88 nearby, interacts with molecular cloud? 10000 yr 2.9 kpc
PSR: 3 kpc		 shell CHANDRA FERMI
G286.5-01.2 shell? FERMI
G287.4+00.6 Puppy PWN G287.42+0.58 and PSR J1048-5832 = B1046-58 PSR: 3 kpc filled-centre? CHANDRA XMM FERMI
G289.7-00.3 contains compact source shell FERMI
G290.1-00.8 MSH 11-61A, 0FGL J1106.4-6055 PSR J1105-6107 nearby, interacts with molecular cloud?? 10000 - 20000 yr 6 - 8 kpc composite CHANDRA ASCA FERMI
G291.0-00.1 MSH 11-62, 2FGL J1112.1-6040 contains PWN + point source 1300 - 10000 yr 1 - 11 kpc composite CHANDRA ASCA FERMI HESS
G292.0+01.8 MSH 11-54 contains PSR J1124-5916 + PWN G292.04+1.75 2930 - 3050 yr
PSR: 2900 yr		 6 kpc
PSR: 6 kpc		 composite CHANDRA XMM ASCA FERMI HESS
G292.2-00.5 1FGL J1119.4-6127c, HESS J1119-614 contains high-B PSR J1119-6127 + PWN G292.15-0.54 ≤ 1700 yr
PSR: 1600 yr		 8 - 8.8 kpc
PSR: 8.4 kpc		 shell CHANDRA XMM ROSAT ASCA FERMI HESS
G293.8+00.6 1FGL J1134.8-6055 contains PWN 3 kpc composite CHANDRA FERMI
G294.1-00.0 shell FERMI
G296.1-00.5 G296.05-0.50, G296.1-0.7 shell XMM SUZAKU ROSAT ASCA FERMI
G296.5+10.0 PKS 1209-51/52, G296.5+9.7 contains CCO PSR J1852+0040 = 1E 1207.4-5209 shell CHANDRA XMM ROSAT ASCA FERMI
G296.8-00.3 1156-62 9.6 kpc shell ROSAT FERMI
G298.5-00.3 ? FERMI
G298.6-00.0 G298.6-0.1, 1FGL J1213.7-6240c, 2FGL J1214.0-6237 shell FERMI
G299.2-02.9 5000 yr 0.5 kpc shell CHANDRA ROSAT ASCA FERMI
G299.6-00.5 shell FERMI
G301.4-01.0 shell FERMI
G302.3+00.7 shell FERMI
G304.1-00.2 HESS J1303-631 PWN G304.10-0.24 and PSR J1301-6305 PSR: 7 kpc filled-centre? CHANDRA XMM HESS
G304.6+00.1 Kes 17 interacts with molecular cloud 9.7 kpc filled-centre? SUZAKU ASCA FERMI
G308.1-00.7 shell FERMI
G308.4-01.4 G308.3-01.4 contains CXOU J134124.22-634352.0 = CCO? 5000 - 7500 yr 10 kpc shell CHANDRA ROSAT
G308.8-00.1 G308.7+0.0, 1FGL J1343.7-6239c contains PSR J1341-6220 = B1338-62 composite? FERMI
G309.2-00.6 G309.2-0.7 contains X-ray source 1WGA J1346.5-6255 = unrelated star HD 119682 in the foreground open cluster NGC 5281 700 - 4000 yr 2 - 6 kpc shell CHANDRA XMM ROSAT ASCA FERMI HESS
G309.8+00.0 1FGL J1350.8-6212c shell FERMI
G309.9-02.5 PWN G309.92-2.51 and PSR J1357-6429 PSR: 2.5 kpc filled-centre? CHANDRA XMM FERMI HESS
G310.6-00.3 Kes 20B shell FERMI
G310.6-01.6 contains PSR J1400-6325 700 - 2000 yr
PSR: 12700 yr		 5 - 10 kpc
PSR: 10 kpc		 composite CHANDRA
G310.8-00.4 Kes 20A interacts with molecular cloud shell FERMI
G311.5-00.3 interacts with molecular cloud?? ≥ 6.6 kpc shell ASCA FERMI
G312.4-00.4 1FGL J1410.3-6128c PSR J1412-6145 and PSR J1413-6141 nearby PSR: 50000 yr ≥ 6 kpc shell CHANDRA ASCA FERMI
G312.5-03.0 shell FERMI
G313.3+00.1 Rabbit, 0FGL J1418.8-6058, HESS J1418-609 part of the Kookaburra complex, contains PSR candidate J1418-6058 filled-centre? CHANDRA XMM FERMI HESS
G313.6+00.3 Kookaburra, HESS J1420-607 PWN G313.54+0.23 = region K3 of the Kookaburra complex, contains PSR J1420-6048 PSR: 13000 yr PSR: 5.6 kpc filled-centre? CHANDRA XMM SUZAKU ASCA FERMI HESS
G315.1+02.7 2FGL J1411.9-5744 shell FERMI
G315.4-00.3 ? FERMI
G315.4-02.3 RCW 86, MSH 14-63, HESS J1442-624 contains several X-ray sources 185 ? 2000 - 10000 yr
SN: 1827 yr ?		 2.4 - 3.2 kpc shell CHANDRA XMM SUZAKU ROSAT ASCA FERMI HESS
G315.9-00.0 G315.8-0.0 shell ASCA FERMI
G316.3-00.0 MSH 14-57, 1FGL J1442.0-6000c, 2FGL J1441.6-5956 ≥ 7.2 kpc shell ASCA FERMI
G317.3-00.2 shell FERMI
G318.2+00.1 HESS J1457-593 3.5 - 9.2 kpc shell ROSAT FERMI HESS
G318.9+00.4 ? contains PWN?, interacts with molecular cloud?? composite ASCA FERMI
G320.0-00.6 PWN G319.97-0.62 and PSR J1509-5850 PSR: 4 kpc filled-centre? CHANDRA
G320.4-01.2 RCW 89, MSH 15-52, 1FGL J1514.7-5917, 2FGL J1514.0-5915e, HESS J1514-591 overlaps SNR G320.6-01.6, contains PSR J1513-5908 = B1509-58 = the Dragon + PWN G319.97-0.62 = the Jellyfish 185 ?? 1900 yr
PSR: 1700 yr
SN: 1827 yr ??		 3.8 - 6.6 kpc
PSR: 5 kpc		 composite CHANDRA ROSAT ASCA FERMI HESS
G320.6-01.6 overlaps SNR G320.4-1.2 shell FERMI
G321.9-00.3 1FGL J1521.8-5734c, 2FGL J1521.8-5735 shell FERMI
G321.9-01.1 shell FERMI
G322.5-00.1 contains PWN? composite FERMI
G323.5+00.1 shell FERMI
G326.3-01.8 MSH 15-56, G326.2-1.7, 1FGL J1552.4-5609, 2FGL J1552.8-5609 contains PWN ≥ 1.5 kpc composite CHANDRA ROSAT ASCA FERMI
G327.1-01.1 contains PWN? 11000 yr 9 kpc composite CHANDRA XMM ROSAT ASCA FERMI HESS
G327.2-00.1 G327.24-0.13 contains AXP 1E 1547.0-5408 (magnetar) PSR: 1400 yr 4 - 5 kpc
PSR: 9 kpc		 shell CHANDRA XMM FERMI
G327.4+00.4 Kes 27, G327.3+0.4, G327.3+0.5 interacts with molecular cloud 4.3 - 5.4 kpc composite CHANDRA ROSAT ASCA FERMI
G327.4+01.0 shell FERMI
G327.6+14.6 SN1006, PKS 1459-41, 1FGL J1501.6-4204, HESS J1502-421 and HESS J1504-418 interacts with molecular cloud 1006 SN: 1006 yr 2.1 - 2.3 kpc shell CHANDRA XMM SUZAKU ROSAT ASCA FERMI HESS
G328.4+00.2 MSH 15-57 contains NS + PWN ≤ 10000 yr ≥ 17.4 kpc filled-centre XMM ASCA FERMI
G329.7+00.4 shell FERMI
G330.0+15.0 Lupus Loop contains central possibly pulsating X-ray source 1.2 kpc shell CHANDRA FERMI
G330.2+01.0 contains CCO CXOU J160103.1-513353 1000 - 1200 yr 5 - 10 kpc shell? CHANDRA XMM ASCA FERMI
G332.0+00.2 shell FERMI
G332.4+00.1 Kes 32, MSH 16-51, G332.4+0.2, 0FGL J1615.6-5049, 2FGL J1615.0-5051 PSR B1610-50 nearby 300 - 3000 yr 7 - 11 kpc shell CHANDRA ROSAT ASCA FERMI
G332.4-00.4 RCW 103, 1FGL J1617.5-5105c contains CCO 1E 161348-5055, close to PSR AXS J1617-5055 and its PWN G332.50-0.28, interacts with molecular cloud 2000 yr
PSR: 8000 yr		 3.1 kpc shell CHANDRA XMM SUZAKU ROSAT ASCA FERMI
G332.5-00.3 HESS J1616-508 PWN G332.50-0.28 and PSR J1617-5055, close to SNR G332.4-00.4 = RCW 103 PSR: 6.5 kpc filled-centre? CHANDRA ASCA HESS
G332.5-05.6 shell ROSAT FERMI
G335.2+00.1 2FGL J1628.1-4857c, HESS J1626-490 contains PSR J1627-4845 shell XMM FERMI HESS
G336.7+00.5 2FGL J1631.7-4720c shell FERMI
G337.0-00.1 CTB 33 inside the CTB 33 complex, contains SGR 1627-41 (magnetar), interacts with molecular cloud PSR: 2200 yr 4.6 - 11 kpc shell CHANDRA XMM ASCA FERMI
G337.2+00.1 1FGL J1632.7-4733c, 2FGL J1635.4-4717c, HESS J1634-472 contains PWN? 1500 yr 14 kpc composite? XMM ASCA FERMI HESS
G337.2-00.7 750 - 3500 yr 2 - 9.3 kpc shell CHANDRA ROSAT ASCA FERMI
G337.3+01.0 Kes 40 shell ASCA FERMI
G337.8-00.1 Kes 41 interacts with molecular cloud ≥ 9.3 kpc composite XMM ASCA FERMI
G338.1+00.4 shell ASCA FERMI
G338.3-00.0 1FGL J1640.8-4634c, 2FGL J1640.5-4633, HESS J1640-465 contains PWN G338.3-0.0 4500 - 8200 yr 8 - 13 kpc composite? CHANDRA XMM ASCA FERMI HESS
G338.5+00.1 11 kpc ? FERMI
G340.4+00.4 shell FERMI
G340.6+00.3 15 kpc shell CHANDRA ASCA FERMI
G341.2+00.9 contains PSR J1646-4346 = B1643-43 + PWN composite FERMI
G341.9-00.3 shell FERMI
G342.0-00.2 shell FERMI
G342.1+00.9 shell FERMI
G343.0-06.0 RCW 114, 2FGL J1727.3-4611 shell FERMI
G343.1-00.7 shell FERMI
G343.1-02.3 HESS J1708-443 PSR J1709-4429 = B1706-44 + PWN G343.10-2.69 near the edge PSR: 17500 yr PSR: 2 kpc composite? CHANDRA ROSAT FERMI HESS
G344.7-00.1 HESS J1702-420 contains CCO CXOU J170357.8-414302, close to PSR J1702-4128 and PWN G344.74+0.12, interacts with molecular cloud?? 14 kpc
PSR: 5 kpc		 composite? CHANDRA XMM SUZAKU ASCA FERMI HESS
G345.7-00.2 HESS J1708-410 shell XMM FERMI HESS
G346.6-00.2 interacts with molecular cloud 8.2 kpc shell SUZAKU FERMI
G347.3-00.5 RX J1713.7-3946, 1FGL J1711.7-3944c, 2FGL J1712.4-3941, HESS J1713-397 contains CCO 1WGA J1713.4-3949, close to PSR J1713-3945, interacts with molecular cloud 393 ? 1000 - 10000 yr
SN: 1619 yr ?		 1 - 6 kpc shell? CHANDRA XMM SUZAKU ROSAT ASCA FERMI HESS
G348.5+00.1 CTB 37A, 0FGL J1714.7-3827, 1FGL J1714.5-3830, 2FGL J1714.5-3829, HESS J1714-385 part of CTB 37, overlaps SNR G348.5-0.0, contains PWN, interacts with molecular cloud 393 ?? 1000 - 3000 yr
SN: 1619 yr ??		 6.3 - 9.5 kpc shell CHANDRA SUZAKU FERMI HESS
G348.5-00.0 part of CTB 37, overlaps SNR G348.5+0.1 = CTB 37A, interacts with molecular cloud ≤ 6.3 kpc shell? FERMI
G348.7+00.3 CTB 37B, HESS J1713-381 part of CTB 37, contains AXP candidate CXOU J171405.7-381031 (magnetar?) 393 ?? 350 - 3150 yr
PSR: 950 yr
SN: 1619 yr ??		 13.2 kpc shell CHANDRA XMM SUZAKU FERMI HESS
G348.9-00.4 HESS J1718-385 PWN G348.95-0.43 and PSR J1718-3825 PSR: 4 kpc filled-centre? CHANDRA XMM HESS
G349.2-00.1 contains PSR J1646-4346 shell FERMI
G349.7+00.2 1FGL J1717.9-3729 interacts with molecular cloud 3500 yr 18.3 - 22.4 kpc shell CHANDRA ASCA FERMI HESS
G350.0-02.0 G350.0-1.8 shell ASCA FERMI
G350.1-00.3 2FGL J1718.1-3725 contains XMMU J172054.5-372652 probably CCO NS 900 yr 4.5 kpc shell? CHANDRA XMM ASCA FERMI
G351.2+00.1 G351.3+0.2 composite? FERMI
G351.7+00.8 PSR J1721-3532 nearby shell FERMI
G351.9-00.9 shell FERMI
G352.7-00.1 interacts with molecular cloud 5000 yr 6.8 - 8.4 kpc composite XMM ASCA FERMI
G353.6-00.7 HESS J1731-347 contains AXP or CCO candidate XMMU J173203.3-344518 (magnetar?), interacts with molecular cloud?? 27000 yr 2.4 - 4 kpc shell XMM SUZAKU ROSAT FERMI HESS
G353.9-02.0 shell FERMI
G354.1+00.1 ? PSR B1727-33 at the edge composite? FERMI
G354.8-00.8 shell FERMI
G355.4+00.7 2FGL J1731.6-3234c shell FERMI
G355.6-00.0 shell ASCA FERMI
G355.9-02.5 shell FERMI
G356.2+04.5 G356.2+4.4 shell FERMI
G356.3-00.3 2FGL J1737.2-3213 shell FERMI
G356.3-01.5 shell FERMI
G357.7+00.3 interacts with molecular cloud shell FERMI
G357.7-00.1 ? The Tornado, MSH 17-39, 2FGL J1740.4-3054c interacts with molecular cloud 11.8 kpc shell? CHANDRA ROSAT ASCA FERMI
G358.0+03.8 1FGL J1725.5-2832 shell FERMI
G358.1+00.1 shell FERMI
G358.5-00.9 2FGL J1745.5-3028c shell FERMI
G359.0-00.9 shell SUZAKU ASCA FERMI
G359.1+00.9 2FGL J1738.9-2908 shell ASCA FERMI
G359.1-00.5 HESS J1745-303 adjacent to PWN G359.23-0.82 = the Mouse, interacts with molecular cloud composite SUZAKU ROSAT ASCA FERMI HESS
G359.2-00.8 Mouse PWN G359.23-0.82 and PSR J1747-2958, adjacent to SNR G359.1-0.5 PSR: 5 kpc filled-centre? CHANDRA XMM ROSAT ASCA

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