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 A1060 159.1744 -27.531 158.58579 -27.271265 172.752913 -33.32931 269.60056717 26.48279097 103.6438 53696.6258796296 2005-11-22 15:01:16 53697.7211111111 2005-11-23 17:18:24 800003010 39.139 40 39.139 39.147 39.155 39.155 2 2 2 2 1 0 0 34.6024 34.6024 94.6259 1 PROCESSED 57528.0675462963 2016-05-20 01:37:16 54247 2007-05-27 00:00:00 54037.8583449074 2006-10-29 20:36:01 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001021 A1060 is a bright non cD cluster and gives us a unique opportunity to study injection process of metals in the intracluster space. Reliable measurement of oxygen distribution with XIS will tell us whether the metals produced by Type-II supernova (mainly oxygen) ditributes over a different scale compared with the SN-Ia product (Fe). A1060 is the best cluster where we can directly observe distribution of metals produced by general cluster galaxies. Also, central increase of temperature by 20%, probably connected with motions of bright central galaxies, suggests that non-thermal X-rays may be produced. EXTRAGALACTIC DIFFUSE SOURCES 8 A TAKAYA OHASHI JAP 0 SWG OXYGEN DISTRIBUTION AND CENTRAL GAS FEATURES OF A1060 XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/800003010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '800003010'

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