DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
No. |
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
observation_id
|
exposure
|
awarded_exposure
|
xis0_exposure
|
xis1_exposure
|
xis2_exposure
|
xis3_exposure
|
xis0_observation_mode
|
xis1_observation_mode
|
xis2_observation_mode
|
xis3_observation_mode
|
hxd_observation_mode
|
hxd_coarse_clock_rate_exposure
|
hxd_first_clock_rate_exposure
|
hxd_normal_clock_rate_exposure
|
hxd_all_clock_rate_exposure
|
hxd_wam_exposure
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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1 | SNR G106.3+2.7 P2 | 336.9121 | 60.9439 | 336.468568 | 60.688281 | 21.166616 | 61.378787 | 106.34649405 | 2.79001657 | 12.2687 | 55423.4230787037 | 2010-08-15 10:09:14 | 55424.0209837963 | 2010-08-16 00:30:13 | 505072010 | 24.5562 | 50 | 24.5722 | 24.5562 | 0 | 24.5722 | 1 | 1 | 0 | 1 | 1 | 0 | 0 | 26.6147 | 26.6147 | 51.6559 | 1 | PROCESSED | 57553.084212963 | 2016-06-14 02:01:16 | 55807 | 2011-09-03 00:00:00 | 55441.2685069444 | 2010-09-02 06:26:39 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 051305 | After two decades searching for the origin of the GeV emission from 3EG J2227+6122, it is now identified with PSR J2229+6114 and its PWN.~This highly energetic young pulsar lies within the arcmin diameter Boomerang radio nebula. Now, recently discovered nearby extended TeV emission suggest a second Vela-like "cocoon" feed by relic electrons from the PWN, blowing out the vast degree-scale radio feature.~Interactions of the SNR shock front with overlapping molecular cloud material can also contribute in the gamma-ray production.~An XIS mosaic will allow us to search for soft and hard X-ray emission similar to Vela's "Cocoon" and resolve the nature of the TeV emission and its connection to the Boomerang and the radio feature. | GALACTIC DIFFUSE EMISSION | 5 | C | ESTER ALIU | USA | 5 | AO5 | ORIGIN OF THE VHE GAMMA-RAY EMISSION FROM SNR G106.3+2.7 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/505072010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '505072010'
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