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 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'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏