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 HB21 SOUTH 311.2512 50.6016 310.86516 50.418766 342.682858 64.005982 88.85305014 4.80482025 105.492 55660.3542361111 2011-04-09 08:30:06 55662.8155208333 2011-04-11 19:34:21 506005010 132.363 150 132.371 132.371 0 132.363 3 2 0 2 1 0 0 141.7887 141.7887 212.6359 1 PROCESSED 57601.4958564815 2016-08-01 11:54:02 56159 2012-08-20 00:00:00 55677.2811342593 2011-04-26 06:44:50 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 060011 Over-ionization in SNRs is one of the biggest mystery Suzaku discovered. It affects a lot the study on chemical and thermal evolution of universe, but the origin is still unknown. HB21 is an old SNR with molecular cloud interaction and GeV gamma-rays, which remind us typical over-ionization SNRs. On the other hand, the interacting molecular cloud is much smaller or thinner than those interacting with over-ionization SNRs, and as a result, HB21 can be the key target to study the origin of over-ionization. Suzaku deep observation of HB21 south (interacting point) will determine the condition of plasma and judge whether it is in over-ionization or not, which will show us the origin of over-ionizing plasma. GALACTIC DIFFUSE EMISSION 5 A AYA BAMBA JAP 6 AO6 ORIGIN OF OVER-IONIZATION OF SNR PLASMAS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/506005010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '506005010'

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