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 | 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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