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 | HB21 SOUTH | 311.2245 | 50.5821 | 310.838387 | 50.399364 | 342.625257 | 64.000491 | 88.82715261 | 4.80607932 | 6.557 | 55767.8922337963 | 2011-07-25 21:24:49 | 55768.4953819444 | 2011-07-26 11:53:21 | 506005020 | 23.4607 | 20 | 23.4687 | 23.4767 | 0 | 23.4607 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 26.2649 | 26.2649 | 52.1039 | 1 | PROCESSED | 57602.6622685185 | 2016-08-02 15:53:40 | 56159 | 2012-08-20 00:00:00 | 55792.1611458333 | 2011-08-19 03:52:03 | 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/ver3.0/506005020/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '506005020'
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