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".

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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 W28_SOUTH 270.2522 -23.558 269.490042 -23.557374 270.221597 -0.117322 6.38418356 -0.23955939 89.9033 56738.9940393518 2014-03-22 23:51:25 56740.1793518518 2014-03-24 04:18:16 508006010 40.8518 100 40.8838 40.8518 0 40.8942 1 1 0 2 1 0 0 35.4568 35.4568 102.4078 1 PROCESSED 57614.1110648148 2016-08-14 02:39:56 57359 2015-12-03 00:00:00 56754.6877083333 2014-04-07 16:30:18 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 080017 A series of discoveries of recombining plasma (RP) in mixed-morphology (MM) SNRs inspires us with a new scenario for SNR evolution. The observed spectra are well described by the picture that the plasma has experienced sudden cooling in the past and currently undergoes gradual recombination to ionization equilibrium. In the MM SNR W28, we found the spatial correlation between the radio brightness and the thermal evolution (recombination) phase. Hence, the radio-fainter region may have less recombined plasma. Such a plasma should emit strong Fe-K line from the He-like ions. The line flux reflects the initial temperature of RP, which brings the key information of the explosion environment of MM SNRs. For this purpose, we propose a 100-ks observation of W28 south, the possible 'youngest' RP. GALACTIC DIFFUSE EMISSION 5 A MAKOTO SAWADA JAP 8 AO8 INITIAL PARAMETERS OF RECOMBINING PLASMA IN SUPERNOVA REMNANTS EXPLORED THROUGH W28 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/508006010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '508006010'

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