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 | MSH15-56_SW | 238.0528 | -56.3239 | 237.060386 | -56.174494 | 248.949341 | -35.191477 | 326.11105465 | -1.81589779 | 86.2015 | 56326.3325 | 2013-02-03 07:58:48 | 56327.8577314815 | 2013-02-04 20:35:08 | 507039010 | 86.0122 | 100 | 86.0122 | 86.0122 | 0 | 86.0122 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 88.3912 | 88.3912 | 131.7719 | 2 | PROCESSED | 57610.534849537 | 2016-08-10 12:50:11 | 56714 | 2014-02-26 00:00:00 | 56345.5312847222 | 2013-02-22 12:45:03 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 070055 | The magnetic field upstream the shock front of the SN blast wave is the key parameter for discussing particle acceleration. In this study we try to constrain the upstream magnetic field and its amplification based on the ionization parameter of heated ISM just behind the shock. For this purpose, we propose a 100 ks XIS observation of an middle aged SNR MSH 15-56 with non-thermal filaments and an anomalously large ionization age for its dynamical age. | GALACTIC DIFFUSE EMISSION | 5 | C | YOICHI YATSU | JAP | 7 | AO7 | A STUDY OF PARTICLE ACCELERATION BASED ON THE THERMAL PLASMA BEHIND THE SHOCK | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/507039010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '507039010'
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