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 | OPHIUCHUS CLUSTER 1 | 258.2981 | -23.3868 | 257.539766 | -23.328523 | 259.261866 | -0.380707 | 0.65649186 | 9.12279372 | 88.7031 | 54180.6159953704 | 2007-03-21 14:47:02 | 54181.1398611111 | 2007-03-22 03:21:24 | 801022010 | 24.067 | 15 | 24.075 | 24.067 | 0 | 24.075 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 21.8213 | 21.8213 | 45.254 | 1 | PROCESSED | 57537.7417476852 | 2016-05-29 17:48:07 | 54736 | 2008-09-27 00:00:00 | 54186.192650463 | 2007-03-27 04:37:25 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 010065 | The Ophiuchus cluster is one of the few galaxy clusters from which hard X-ray emission was detected with INTEGRAL. The confidence level is higher than that of the Coma cluster. The hard X-ray emission was also detected with BeppoSAX. Complicated temperature structure observed with ASCA indicated that the cluster is in a merger phase at present. The hard X-ray emission is possibly originated from the cluster merger and the resultant particle acceleration. We propose a Suzaku observation of the cluster to reveal the mechanism of the particle acceleration in clusters. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | YUTAKA FUJITA | JAP | 1 | AO1 | PARTICLE ACCELERATION IN THE OPHIUCHUS CLUSTER | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801022010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '801022010'
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