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 A3526 192.0509 -41.0558 191.361267 -40.783129 208.811762 -32.67802 302.27518183 21.81182444 109.9986 55942.2296990741 2012-01-16 05:30:46 55942.6807291667 2012-01-16 16:20:15 806084010 16.9645 10 16.9645 16.9645 0 16.9645 2 2 0 2 1 0 0 12.6605 12.6605 38.9639 0 PROCESSED 57604.361875 2016-08-04 08:41:06 56331 2013-02-08 00:00:00 55960.1781712963 2012-02-03 04:16:34 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 062001 Suzaku has enabled a breakthrough to be made in the study of the outer parts of clusters. For the first time the gas properties have been measured in a cluster to beyond the virial radius. This is important for understanding the properties of clusters and for cosmological studies. They are also needed for understanding how clusters match to the outer Universe in their temperature and entropy profiles. Are there any large scale accretion shocks? How do filaments match to clusters? The observational breakthrough has been possible due to the combination of the low orbit and thus low background of the Suzaku FI detectors and particularly X-ray bright clusters. We propose here to exploit Suzaku's unique capability to extend this result to an X-ray bright nearby relaxed cluster. EXTRAGALACTIC DIFFUSE SOURCES 8 B ANDREW FABIAN EUR 6 AO6 TO BEYOND THE VIRIAL RADIUS IN THE NEARBY CENTAURUS CLUSTER XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/806084010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '806084010'

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