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 J2218.6-0346 334.6629 -3.7693 334.013965 -4.02026 335.129241 6.290164 58.79146355 -46.71055995 71.7798 56063.8991550926 2012-05-16 21:34:47 56064.7196875 2012-05-17 17:16:21 807085010 28.629 25 28.629 28.629 0 28.629 2 2 0 2 1 0 0 26.8327 26.8327 70.8839 1 PROCESSED 57605.4341550926 2016-08-05 10:25:11 56442 2013-05-30 00:00:00 56076.0273726852 2012-05-29 00:39:25 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/ver3.0/807085010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '807085010'

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