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 PERSEUS CL OFFSET 49.2788 41.3719 48.454118 41.188803 58.04223 22.344257 150.2212005 -13.65398882 65.9966 53980.7676273148 2006-09-02 18:25:23 53981.4543287037 2006-09-03 10:54:14 801049020 32.4646 30 32.4806 32.4646 32.4966 32.4886 1 1 1 1 1 0 0 28.2912 28.2912 59.3199 1 PROCESSED 57535.422025463 2016-05-27 10:07:43 54526 2008-03-01 00:00:00 54021.2712731482 2006-10-13 06:30:38 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010097 We propose to observe the X-ray brightest galaxy cluster, the Perseus cluster, with 4 pointings offset from the cluster center. In this observation, we will measure a nonthermal energy budget from three measurements; search for very high temperature electron deviated from the average temperature or suprathermal electrons, search for nonthermal powerlaw component, and doppler shift of Fe-K lines caused by the bulk motion of hot gas. Hot clusters, including the Perseus cluster, are believed to be now evolving, by absorbing poor groups at the cluster periphery, and thus nonthermal energy at the cluster periphery is important to probe the information of cluster evolution. Such a measurement can be performed by only Suzaku; HXD-PIN with narrow field of view, and XIS with stable low background. EXTRAGALACTIC DIFFUSE SOURCES 8 A YASUSHI FUKAZAWA JAP 1 AO1 MEASUREMENT OF NONTHERMAL ENERGY BUDGET IN THE PERSEUS CLUSTER HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801049020/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '801049020'

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