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 CENTAURUS CLUSTER 192.2012 -41.3132 191.510497 -41.040677 209.072585 -32.853902 302.40029759 21.55583076 106.2442 53731.2579050926 2005-12-27 06:11:23 53732.1808333333 2005-12-28 04:20:24 800014010 36.5192 30 36.5192 36.5464 36.5464 36.5224 2 2 2 2 1 0 0 32.1498 32.1498 79.7399 0 PROCESSED 57532.5349652778 2016-05-24 12:50:21 54247 2007-05-27 00:00:00 54039.373900463 2006-10-31 08:58:25 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001070 A dramatic central concentration of iron and silicon is present in the Centaurus cluster. Apart from this well-recognized contribution from Type Ia supernova, enrichment process due to Type II supernova is poorly understood. Centaurus cluster is most suited for the study of large-scale oxygen distribution, for which XIS is most sensitive. The XIS data will give us a key knowledge about how past Type II supernova have affected the enrichment process. The data would also confirm that the central gas is a mixture of hot and cool components with much better sensitivity than before. EXTRAGALACTIC DIFFUSE SOURCES 8 A YASUSHI FUKAZAWA JAP 0 SWG OXYGEN DISTRIBUTION AND MIXTURE OF HOT AND COOL GAS IN THE CENTAURUS CLUSTER XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/800014010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '800014010'

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