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 RCW86_SOUTH 220.8315 -62.6734 219.843557 -62.461116 241.073682 -44.079198 315.37853465 -2.53716675 96.1597 54862.1182291667 2009-01-31 02:50:15 54863.3647569445 2009-02-01 08:45:15 503003010 54.8181 50 54.8181 54.8181 0 54.8341 2 2 0 2 1 0 0 47.3483 47.3483 107.6848 1 PROCESSED 57545.4382175926 2016-06-06 10:31:02 55329 2010-05-13 00:00:00 54880.5892361111 2009-02-18 14:08:30 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 030011 Suzaku PV and AO-1 observations revealed that the 6.4 keV Fe-K line from RCW86 originates from Fe-rich ejecta heated by reverse shock very recently. We propose the mapping observations on whole RCW86 in order to find the structure of the reverse shock by investigating the morphology of the Fe-line emission. At the same time, we can perform the hard X-ray mapping. Using the wideband non-thermal X-ray spectra with great accuracy, we will determine the origin of the TeV gamma-ray emission detected by H.E.S.S. recently. GALACTIC DIFFUSE EMISSION 5 B HIROYA YAMAGUCHI JAP 3 AO3 RCW86 MAPPING OBSERVATION XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/503003010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '503003010'

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