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 G290.1-0.8 165.7447 -60.8884 165.228717 -60.618807 206.73964 -58.122992 290.11957377 -0.7436408 293.2659 55737.4551388889 2011-06-25 10:55:24 55740.5883333333 2011-06-28 14:07:12 506061010 110.5931 110 110.6091 110.5931 0 110.6011 2 2 0 2 1 0 0 99.3596 99.3596 270.6596 4 PROCESSED 57602.4993634259 2016-08-02 11:59:05 55652 2011-04-01 00:00:00 55775.3693287037 2011-08-02 08:51:50 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 066001 Suzaku found recombining plasma (RP) from the mixed-morphology SNRs (MM-SNRs). Since the standard evolution of SNR does not predict RP, the Suzaku discovery requires a dramatic change on the scenario of SNR dynamics and evolution. Suggestive facts are that all RP detected SNRs have OH masers and all RP-detected SNRs have TeV/GeV emissions. The most important issue at this stage, however, is not model making, but systematic and comprehensive observations to study which kind of SNRs, and/or which circum SN conditions, are responsible to RP. This is our primary objective. The second aim of this proposal is to provide path-finding data for the Astro-H science. GALACTIC DIFFUSE EMISSION 5 A KATSUJI KOYAMA JAP 6 AO6-KP NEW SCENARIO FOR THE THERMAL PLASMA IN SNRS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/506061010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '506061010'

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