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 CAS A 350.8607 58.8031 350.294827 58.528522 27.373119 54.842451 111.73599633 -2.14263527 251.3043 56281.1375115741 2012-12-20 03:18:01 56283.3466666667 2012-12-22 08:19:12 507038010 102.411 100 102.419 102.411 0 102.426 2 1 0 2 1 0 0 126.7103 126.7103 190.8458 0 PROCESSED 57608.4566435185 2016-08-08 10:57:34 56683 2014-01-26 00:00:00 56316.9831365741 2013-01-24 23:35:43 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 070050 We will propose a follow-up 120 ksec observations of a young supernova remnant Cassiopeia A. The long exposure provides us a high quality of the broad band spectrum from XIS to HXD GSO band. We will try to detect Mn-K line at 6.1 keV for the first time. The element Mn as well as Cr gives constraint on the explosion mechanism of the ejecta. We also test a predicted flux variation of a non-thermal emission in the PIN band for the first time. The variation gives critical information to solve the physical parameters in the reverse shock of the ejecta. GALACTIC DIFFUSE EMISSION 5 C YOSHITOMO MAEDA JAP 7 AO7 MN/CR-K AND HARD X-RAY EMISSION IN CASSIOPEIA A XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/507038010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '507038010'

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