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 A2029_4 228.0053 5.6496 227.385284 5.836972 223.833276 22.612919 6.60771448 50.27207577 112.9543 55225.6146180556 2010-01-29 14:45:03 55226.2501388889 2010-01-30 06:00:12 804024040 25.6584 22 25.6584 25.6824 0 25.6664 2 2 0 2 1 0 0 19.446 19.446 54.9019 0 PROCESSED 57550.4263657407 2016-06-11 10:13:58 55637 2011-03-17 00:00:00 55271.0446064815 2010-03-16 01:04:14 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 040030 Suzaku has enabled a breakthough to be made in the study of the outer parts of clusters. For the first time the gas properties have been measured in the cluster PKS 0745-19 to beyond the virial radius. This is important for understanding the properties of clusters, such as total mass and total gas mass which are required 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 breakthrough has been possible due to low background of the Suzaku FI CCD and the use of a particularly bright cluster. We propose here to exploit Suzaku's unique capability to extend this result using the 2 X-ray bright, relaxed clusters. EXTRAGALACTIC DIFFUSE SOURCES 8 C YUZURU TAWARA JAP 4 AO4 TO THE VIRIAL RADIUS IN THE BRIGHT LUMINOUS CLUSTERS, A2029 AND A478 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/804024040/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '804024040'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏