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
|
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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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