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 | A3581_CEN | 211.9083 | -27.0199 | 211.193684 | -26.782616 | 219.008869 | -13.266139 | 323.17769244 | 32.83870198 | 117.8993 | 56308.5541782407 | 2013-01-16 13:18:01 | 56310.7078356482 | 2013-01-18 16:59:17 | 807026010 | 80.408 | 80 | 80.416 | 80.416 | 0 | 80.408 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 70.1715 | 70.1715 | 186.0419 | 1 | PROCESSED | 57608.5784259259 | 2016-08-08 13:52:56 | 56711 | 2014-02-23 00:00:00 | 56345.6637384259 | 2013-02-22 15:55:47 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 070064 | We propose to study the metallicity of Abell 3581 to the outer region beyond 0.5 r180. Abell 3581 is a very useful system for investigating the history of the chemical evolution of groups and clusters, because the temperature of the intra-cluster medium is about 1.7 keV, which is intermediate between groups and clusters of galaxies. Suzaku will enable us to measure for the first time the metal distributions to such outer regions of the clusters, because of the significantly lower background level and higher sensitivity below ~1 keV. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | KOSUKE SATO | JAP | 7 | AO7 | SEARCH FOR THE METALLICITY OF ABELL 3581 TO THE OUTER REGION BEYOND 0.5 R180 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/807026010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '807026010'
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