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 A426 49.9554 41.5039 49.127963 41.323287 58.608686 22.329679 150.58326426 -13.26576669 260.2176 53767.568900463 2006-02-01 13:39:13 53768.5294560185 2006-02-02 12:42:25 800010010 50.3986 50 50.4066 50.4066 50.3986 50.4066 2 2 2 2 1 0 0 54.4364 54.4364 82.9758 0 PROCESSED 57532.8781365741 2016-05-24 21:04:31 54247 2007-05-27 00:00:00 54041.0862152778 2006-11-02 02:04:09 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001036 A426 is the X-ray brightest cluster in the Sky. The core is X-ray peaked, has a short radiative cooling time, a temperature drop and a central radio source which is blowing bubbles in the intracluster medium. A radio minihalo extends over the central 6 arcmin. A coincident power-law component is seen in deep Chandra data. This is likely to be inverse Compton emission from the electron population responsible for the radio emission. The region is expected to be a luminous, extended, hard X-ray source easily detectable by the Suzaku HXD. Confirmation of this hard X-ray component will enable the magnetic field to be securely determined in the intracluster gas. EXTRAGALACTIC DIFFUSE SOURCES 8 A ANDREW FABIAN JAP 0 SWG THE HARD X-RAY FLUX FROM THE CORE OF THE PERSEUS CLUSTER XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/800010010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '800010010'

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