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 PLCK G214.6-37.0 137.1752 14.6923 136.484307 14.895327 135.215425 -1.654352 214.5759479 36.9399481 287 56413.2455439815 2013-05-01 05:53:35 56416.322349537 2013-05-04 07:44:11 808101010 119.2637 120 119.2637 119.2637 0 119.2637 2 2 0 2 1 0 0 106.3127 106.3127 265.8039 5 PROCESSED 57611.2793981482 2016-08-11 06:42:20 56795 2014-05-18 00:00:00 56429.7933217593 2013-05-17 19:02:23 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 082007 We propose a detailed investigation of the nature of PLCK G214.6-37.0, discovered in the Planck survey. We aim at constraining the presence and properties of filamentary structures connecting and surrounding the clusters. We will unveil the overall dynamics of this complex structure and establish its detailed pressure distribution that can be used for a better estimation of YX to be compared with YSZ. Thus, we will perform a direct search for structures in between identified supercluster components from a careful comparison with the Planck results. Furthermore, the distribution of the PLCK G214.6-37.0 components suggest that it is evolving accreting sub-clusters along the filaments. That makes this supercluster one of the to search for the WHIM. EXTRAGALACTIC DIFFUSE SOURCES 8 A LORENZO LOVISARI EUR 8 AO8 TRACKING DOWN THE PLANCK SUPERCLUSTER PLCK G214.6-37.0 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808101010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '808101010'

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