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 | A3627CENTER | 243.5672 | -60.8499 | 242.482666 | -60.723566 | 253.815365 | -38.883288 | 325.25917104 | -7.10560665 | 129.9148 | 54905.9231597222 | 2009-03-15 22:09:21 | 54906.6072222222 | 2009-03-16 14:34:24 | 803032010 | 46.0339 | 50 | 46.0388 | 46.0419 | 0 | 46.0339 | 1 | 1 | 0 | 1 | 1 | 0 | 0 | 43.3969 | 43.3969 | 59.0959 | 0 | PROCESSED | 57545.823900463 | 2016-06-06 19:46:25 | 55330 | 2010-05-14 00:00:00 | 54917.2613657407 | 2009-03-27 06:16:22 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 030117 | We propsoe to observe the cluster of galaxies A3627, which has evidences of cluster merging, in order to detect hard X-rays from high energy particles acceralated in the cluster and also measure the doppler shift of the iron-K line. This cluster is a nearby bright cluster behind the Galactic plane, and thus so far X-ray studies have been poor. However, its proximity and relatively low temperature against other merging clusters enable us to constrain the hard X-ray emission more tightly. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | SHO NISHINO | JAP | 3 | AO3 | OBSERVATION OF MERGING CLUSTER A3627, LOCATED AROUND THE CENTER OF THE GREAT ATTRACTOR | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/803032010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '803032010'
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