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 | J2218.8-0258 | 334.694 | -2.9598 | 334.046783 | -3.210826 | 335.453457 | 7.033577 | 59.75779093 | -46.24852305 | 49.9996 | 56072.7972685185 | 2012-05-25 19:08:04 | 56073.7370833333 | 2012-05-26 17:41:24 | 807086010 | 38.3981 | 35 | 38.4061 | 38.3981 | 0 | 38.4061 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 36.9739 | 36.9739 | 81.1958 | 1 | PROCESSED | 57605.5228703704 | 2016-08-05 12:32:56 | 56500 | 2013-07-27 00:00:00 | 56134.0402199074 | 2012-07-26 00:57:55 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 072018 | We propose to observe the three clusters of galaxies J2218.2-0350, J2218.6-0346 and J2218.8-0258 with exposure times of 15, 25 and 35 ks respectively. These clusters are part of a structure of four linearly aligned clusters, separated from each other by 4 to 10 Mpc. We will accurately determine their masses and orientation. This will allow us to fully map the tidal force field of the structure, which is the prime force behind the formation of filaments in the cosmic web. We will study the effects of cluster mass, separation and mutual orientation on the filamentary structure of the cosmic web and on the evolution of galaxies therein. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | E.G. PATRICK BOS | EUR | 7 | AO7 | CLUSTERS AND THE COSMIC WEB | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/807086010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '807086010'
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