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 S LOBE NO. 3 | 205.7514 | -45.1409 | 204.991343 | -44.889287 | 221.546575 | -31.897052 | 312.39292182 | 16.78143613 | 279.0007 | 55420.9668981482 | 2010-08-12 23:12:20 | 55421.3452777778 | 2010-08-13 08:17:12 | 705034010 | 20.0575 | 20 | 20.0815 | 20.0735 | 0 | 20.0575 | 3 | 2 | 0 | 2 | 1 | 0 | 0 | 18.9436 | 18.9436 | 32.6879 | 1 | PROCESSED | 57552.9389467593 | 2016-06-13 22:32:05 | 55803 | 2011-08-30 00:00:00 | 55435.169537037 | 2010-08-27 04:04:08 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 051401 | We propose a set of four pointings (200 ks), to study the X-ray emission from the Southern giant lobe of the radio galaxy Cen A. Those lobes clearly separated from the central source, have been detected as a source of diffuse gamma-ray emission by the Fermi Telescope. The goal of the Suzaku observations is two-fold: first, to measure the diffuse component of the non-thermal X-ray emission with both the XIS and the HXD in order to determine the details of the distribution of the radiating relativistic particles (and B field), and second, to measure the thermal emission from the lobes (using primarily the XIS), to determine temperature and density of the X-ray emitting plasma, which, via consideration of pressure balance, will determine the content of energetic protons (cosmic rays). | EXTRAGALACTIC COMPACT SOURCES | 7 | B | GRZEGORZ MADEJSKI | USA | 5 | AO5 | SUZAKU OBSERVATIONS OF THE SOUTHERN LOBE OF CEN A | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/705034010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '705034010'
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