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
|
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1 | CEN_A_LOBE_N1 | 201.8136 | -42.0782 | 201.081414 | -41.819016 | 217.012441 | -30.336854 | 310.00727378 | 20.30096505 | 292.0832 | 56859.7082060185 | 2014-07-21 16:59:49 | 56861.2571990741 | 2014-07-23 06:10:22 | 809002010 | 50.3801 | 50 | 50.3881 | 50.3881 | 0 | 50.3801 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 11.4775 | 11.4775 | 24.4719 | 0 | PROCESSED | 57615.4533333333 | 2016-08-15 10:52:48 | 57242 | 2015-08-08 00:00:00 | 56875.1360185185 | 2014-08-06 03:15:52 | 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/ver3.0/809002010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '809002010'
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