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 | 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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