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 HOT BLOB 3 127.507 51.0389 126.590865 51.206602 116.529664 30.99487 167.88407696 36.01101877 263.6154 57139.1338657407 2015-04-27 03:12:46 57140.9141319444 2015-04-28 21:56:21 509009010 81.1183 80 81.1183 81.5423 0 81.5503 2 2 0 2 0 0 0 0 0 0 0 PROCESSED 57644.5780902778 2016-09-13 13:52:27 57591 2016-07-22 00:00:00 57224.4589351852 2015-07-21 11:00:52 3.0.22.44 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 090044 Hot blobs including plasma of temperature kT = 0.6 - 1.0 keV in the Milky-Way Halo were found in 1/10 of the sky by systematical analysis of the soft X-ray diffuse background in Suzaku/XIS observations. They can play a role in matter and energy transportation among the Galactic plane, the Milky-Way Halo and intergalactic space. In order to reveal origin and physical condition of them, we focus on the part of a hot blob in (ell, b) = (161.505, 40.696) and propose to observe neighboring this area to constrain its size. GALACTIC DIFFUSE EMISSION 5 C NORIO SEKIYA JAP 9 AO9 ORIGIN AND PHYSICAL CONDITION OF HOT BLOBS IN THE MILKY-WAY HALO XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/509009010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '509009010'

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