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 CENA N LOBE 3 201.1567 -39.315 200.435438 -39.054679 215.153584 -28.04573 309.90401242 23.10702351 110.949 56316.327349537 2013-01-24 07:51:23 56318.4140046296 2013-01-26 09:56:10 807134010 81.984 75 81.992 81.992 0 81.984 2 2 0 2 1 0 0 73.8838 73.8838 180.2478 2 PROCESSED 57608.6528356482 2016-08-08 15:40:05 56708 2014-02-20 00:00:00 56342.7001157407 2013-02-19 16:48:10 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 070127 Radio source Centaurus A is the closest active galaxy in the Universe (3.7 Mpc). It is surrounded by poorly known giant radio lobes extending for about 600 kpc in the N-S direction. Here we propose Chandra follow-up of four regions in the Southern and Northern lobes where Suzaku time was allocated. We also propose joint Chandra-Suzaku observation toward interacting filamentary region where ASCA found a hint of X-ray emission. The primary goal of the project is to study the filamentary structure of the lobe in X-rays, in the broader context of particle acceleration and energy dissipation processes taking place in inhomogeneous and multi-phase plasma. The obtained results are guaranteed to improve our knowledge regarding not only the Centaurus A, but all jetted active galaxies. EXTRAGALACTIC DIFFUSE SOURCES 8 S YASUYUKI TANAKA JAP 7 AO7 STUDYING GIANT FILAMENTARY LOBES OF CENTAURUS A XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/807134010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '807134010'

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