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
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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