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 | DEM L 192 | 81.4194 | -67.497 | 81.444182 | -67.538512 | 340.379487 | -86.530508 | 277.77177426 | -33.0775429 | 334.6993 | 54968.6808680556 | 2009-05-17 16:20:27 | 54971.0113310185 | 2009-05-20 00:16:19 | 804009010 | 87.3165 | 80 | 87.3245 | 87.3165 | 0 | 87.3245 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 80.0589 | 80.0589 | 201.3277 | 2 | PROCESSED | 57546.6405439815 | 2016-06-07 15:22:23 | 55356 | 2010-06-09 00:00:00 | 54987.4577314815 | 2009-06-05 10:59:08 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 040009 | The combined actions of fast stellar winds and core-collapse supernova explosions of the massive stars create large shell-like structures, called superbubbles (SBs), by sweeping up the ambient medium. Large tenuous cavities created inside the SB walls allow that the blast shocks of the interior supernova remnants (SNRs) expand rapidly without decelerating for a long time. Therefore, the timescale of efficient cosmic-ray acceleration can be much longer than that of most isolated SNRs. We propose the observations on DEM L 192 and DEM L 205, which are the SBs in the Large Magellanic Cloud, in order to search the large non-thermal SNR shells hidden inside the SBs. They are the strong candidates of the accelerators of the "knee energy" particles. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | HIROYA YAMAGUCHI | JAP | 4 | AO4 | DEM L 192 AND DEM L 205: SUPERBUBBLES IN THE LARGE MAGELLANIC CLOUD | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/804009010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '804009010'
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