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 | A222/223 BRIDGE | 24.4438 | -12.9141 | 23.829522 | -13.168194 | 17.57702 | -21.440022 | 162.54430913 | -72.12239011 | 224.9995 | 55555.161099537 | 2010-12-25 03:51:59 | 55557.4654861111 | 2010-12-27 11:10:18 | 805035010 | 101.2149 | 100 | 101.2843 | 101.2149 | 0 | 101.2843 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 88.9171 | 88.9171 | 199.0699 | 4 | PROCESSED | 57554.5537268518 | 2016-06-15 13:17:22 | 55961 | 2012-02-04 00:00:00 | 55595.1387847222 | 2011-02-03 03:19:51 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 050035 | We propose to observe the unusual X-ray bridge connecting the two clusters of galaxies Abell 222 and Abell 223 (z=0.21). XMM observation showed the temperature to be 0.9 keV, interpreted as due to WHIM. Suzaku will observe the temperature distribution over the bridge region, which will tell us the origin of the bridge to be either WHIM or merger onset. Merger process should indicate a characteristic temperature increase. Redshifted oxygen lines, if detected, will be the clear evidence of WHIM. Joint study with weak lensing analysis will show us spatial offset of the dark matter against baryons, helping us to constrain dark matter properties. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | KAORI HENMI | JAP | 5 | AO5 | ORIGIN OF THE X-RAY BRIDGE CONNECTING THE CLUSTERS OF GALAXIES ABELL 222 AND ABELL 223 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805035010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '805035010'
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