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 | IC443 NORTHWEST | 93.9975 | 22.7552 | 93.240341 | 22.772771 | 93.68801 | -0.634546 | 188.75644855 | 2.86235674 | 91.4819 | 55456.3191435185 | 2010-09-17 07:39:34 | 55458.2829050926 | 2010-09-19 06:47:23 | 505001010 | 83.1917 | 80 | 83.1917 | 83.1917 | 0 | 83.1917 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 69.6786 | 69.6786 | 169.6457 | 2 | PROCESSED | 57553.4791087963 | 2016-06-14 11:29:55 | 55836 | 2011-10-02 00:00:00 | 55469.4041087963 | 2010-09-30 09:41:55 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 050001 | Suzaku discovered the radiative recombination continua (RRC) of Si and S from the supernova remnant IC443. This new phenomenon (the RRC) would be due to either pre-ionization by X-ray flash of gamma-ray burst, or adiabatic cooling in a rarefied ambient medium, or yet-unknown process. In any case, the RRC have essential and new clues for the mechanisms, evolution and/or even the cosmic-ray acceleration of IC443. Spectra of the rim regions provide key information for the RRC origin. We thus propose the East and West periphery of IC443 for total 200 ksec. | GALACTIC DIFFUSE EMISSION | 5 | C | MIDORI OZAWA | JAP | 5 | AO5 | EXPLORING THE ORIGIN OF THE RADIATIVE RECOMBINATION CONTINUUM OF IC443 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/505001010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '505001010'
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