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 | 4C73.08 | 147.4414 | 73.2521 | 146.291521 | 73.485172 | 114.906674 | 54.77086 | 138.04435007 | 38.07252036 | 100.3847 | 54786.9238888889 | 2008-11-16 22:10:24 | 54788.4946643518 | 2008-11-18 11:52:19 | 703018010 | 81.3752 | 80 | 81.3752 | 81.3752 | 0 | 81.3752 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 72.4533 | 72.4533 | 135.692 | 0 | PROCESSED | 57544.4300694444 | 2016-06-05 10:19:18 | 55164 | 2009-11-29 00:00:00 | 54798.0487152778 | 2008-11-28 01:10:09 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 030063 | Suzaku observation of two giant radio galaxies, 4C 73.08 and 3C 35, are proposed. In 80 ks exposure on the individual target, inverse Compton X-ray emission from their lobes is detected with high signal statistics. As a result, the energy densities of electrons and magnetic field in these lobesare precisely determined. The size of these radio galaxies are significantly lager than that of the previous sample. Therefore, the size dependence of energetics in the lobes will be investigated | EXTRAGALACTIC COMPACT SOURCES | 7 | C | YUICHI YAJI | JAP | 3 | AO3 | SUZAKU OBSERVATION OF LOBES OF GIANT RADIO GALAXIES | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/703018010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '703018010'
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