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 ABEL 754 137.2113 -9.6361 136.602656 -9.432794 142.867226 -24.832228 239.25284371 24.7578079 295.1878 54249.7445833333 2007-05-29 17:52:12 54252.4495949074 2007-06-01 10:47:25 802063010 108.9779 100 108.9859 108.9859 0 108.9779 2 2 0 2 1 0 0 97.904 97.904 233.6958 2 PROCESSED 57538.8549537037 2016-05-30 20:31:08 54773 2008-11-03 00:00:00 54257.5596759259 2007-06-06 13:25:56 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021445 We propose a 100 ksec observation of Abell 754 and a 50 ksec observation of Triangulum Australis, in order to measure the spectral shape and flux of possible nonthermal emission from clusters of galaxies. They are bright clusters of galaxies in the BAT all sky survey sample, which is crucial for making good spectral measurements by the HXD. And their spectra have a significant hard excess (power-law component). We intend to constrain the power-law photon index of the nonthermal emission for the first time and to determine the size of hard X-ray emitting region by using both of the HXD and Swift BAT data. We are aiming to test the origin of the hard flux and see whether it originates from either diffuse inverse Compton scattering by relativistic cosmic-ray electrons or an AGN. EXTRAGALACTIC DIFFUSE SOURCES 8 B TAKASHI OKAJIMA USA 2 AO2 OBSERVATIONS OF NONTHERMAL EMISSION FROM CLUSTERS OF GALAXIES XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/802063010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '802063010'

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