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 | FORNAX A W-LOBE N | 50.5227 | -36.9675 | 50.043813 | -37.145451 | 32.738272 | -52.85468 | 239.75066849 | -56.83654313 | 27.8129 | 54991.7546875 | 2009-06-09 18:06:45 | 54992.8119675926 | 2009-06-10 19:29:14 | 804037010 | 60.7627 | 50 | 60.7707 | 60.7627 | 0 | 60.7707 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 54.817 | 54.817 | 91.3258 | 1 | PROCESSED | 57547.5602777778 | 2016-06-08 13:26:48 | 55367 | 2010-06-20 00:00:00 | 55001.1883912037 | 2009-06-19 04:31:17 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 040073 | We propose Suzaku offset mapping observations of the Fornax A west radio lobe. By measuring the inverse-Compton X-ray spectra from the radio lobe with the mapping observations, we measure the brightness profile in the non-thermal X-ray emission. The results show us the spatial distribution of the relativistic electrons independently from the magnetic field structures determining the synchrotron radio emissions. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | B | MAKOTO TASHIRO | JAP | 4 | AO4 | X-RAY MAPPING OF THE FORNAX A WEST LOBE | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/804037010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '804037010'
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