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 W28WEST 269.8372 -23.6072 269.074768 -23.604556 269.841247 -0.166403 6.15250357 0.06606197 270.1135 55844.0583217593 2011-10-10 01:23:59 55848.1342708333 2011-10-14 03:13:21 506036010 151.0892 150 151.0972 151.0892 0 151.0923 2 2 0 2 1 0 0 128.9797 128.9797 352.1259 2 PROCESSED 57603.4758449074 2016-08-03 11:25:13 56240 2012-11-09 00:00:00 55872.5113425926 2011-11-07 12:16:20 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 060095 W28 is a mixed-morphology supernova remnant (MM SNR). Recently, GeV and TeV gamma-ray emission have been detected from the eastern edge of W28. On the other hand, we have observed the central region of W28 and have detected an over-ionized plasma, which can not be produced in the canonical evolution of SNRs. Several SNRs have been turned out to host a over-ionized plasma. All of them are MM SNR and are showing GeV and/or TeV emission. This indicates that there are some physical connections between the existence of high-energy cosmic rays and over-ionized plasma. W28 is the best place to study this possible connection due to the large apparent size. Thus, we propose Suzaku observation of western region of W28, which has not been covered by the previous mapping observations. GALACTIC DIFFUSE EMISSION 5 A MAKOTO SAWADA JAP 6 AO6 THE SNR W28 - SEARCHING FOR THE PHYSICAL CONNECTION BETWEEN HIGH-ENERGY COSMIC RAYS AND OVER-IONIZED PLASMA XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/506036010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '506036010'

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