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 CEN_A_LOBE_N5 198.8206 -42.0777 198.100689 -41.813564 214.682372 -31.301214 307.6547721 20.57528449 295.9847 56865.6873032407 2014-07-27 16:29:43 56867.2502430556 2014-07-29 06:00:21 809006010 51.9392 50 51.9392 52.5746 0 52.5746 2 2 0 2 1 0 0 10.6586 10.6586 20.936 0 PROCESSED 57615.4722916667 2016-08-15 11:20:06 57267 2015-09-02 00:00:00 56898.3358449074 2014-08-29 08:03:37 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 090021 In AO1 and AO4, we conducted mapping observations of the western radio lobe of Fornax A, from which we disconvered thermal plasma pervasive in the lobe (Seta et al. 2013). Such a plasma may trace the AGN feedback activities influencing the evolution of the host galaxy and the cluster of galaxies, but much remains to be unveiled about its observational properties. In order to derive the surface brightness profile and the matalicity of the thermal plasma, we propose a 50 ks x 5 mapping observations of the northern radio lobe of Cen A, which is the largest radio lobe in appearance in the entire whole sky. EXTRAGALACTIC DIFFUSE SOURCES 8 A HIROMI SETA JAP 9 AO9 MAPPING OBSERVATIONS OF THE NORTHERN RADIO LOBE OF THE CENTAURUS A XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/809006010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '809006010'

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