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 F_2 49.9481 41.7834 49.118842 41.602757 58.6868 22.59977 150.42037818 -13.03556783 257.3692 56324.1634259259 2013-02-01 03:55:20 56324.4342939815 2013-02-01 10:25:23 807019010 17.2086 15 17.2156 17.2156 0 17.2086 1 1 0 1 1 0 0 18.5555 18.5555 23.3999 0 PROCESSED 57610.4952314815 2016-08-10 11:53:08 56731 2014-03-15 00:00:00 56365.4862731482 2013-03-14 11:40:14 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 070056 We propose to map the central region (R<20') of the Perseus cluster of galaxies. The cluster is the X-ray brightest one at z=0.02. This unique object along with good performance of the SUZAKU XIS and HXD provides the best quality, wide-band and spatially-resolved X-ray spectroscopy of the ICM. Using the data, we will measure ICM bulk motions around the cluster core. Based on these observation, we will understand the physics of cluster formation and the distribution of dark matter. EXTRAGALACTIC DIFFUSE SOURCES 8 C TAKAYUKI TAMURA JAP 7 AO7 GAS MOTION IN THE PERSEUS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/807019010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '807019010'

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