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 | 3C 35 | 18.0181 | 49.4424 | 17.27928 | 49.177164 | 38.209927 | 38.103766 | 126.37585323 | -13.29131796 | 245.0044 | 55200.6165509259 | 2010-01-04 14:47:50 | 55202.466875 | 2010-01-06 11:12:18 | 704019010 | 84.7566 | 80 | 85.0286 | 84.7566 | 0 | 85.0206 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 66.3143 | 66.3143 | 147.5778 | 2 | PROCESSED | 57550.0615277778 | 2016-06-11 01:28:36 | 55584 | 2011-01-23 00:00:00 | 55218.1479050926 | 2010-01-22 03:32:59 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 040096 | Suzaku observations of two giant radio galaxies, 3C 35 and DA 240, with a total size of about 1 Mpc are proposed, in order to detect diffuse inverse Compton X-ray emission from their radio lobes. The X-ray flux from the lobes, in comparison with the radio one, provides a precise determination of electron and magnetic field energies there. A comparison of them with those in smaller radio galaxies is used to probe into the history of jets and lobes. | EXTRAGALACTIC COMPACT SOURCES | 7 | B | NAOKI ISOBE | JAP | 4 | AO4 | SUZAKU OBSERVATION OF GIANT RADIO GALAXIES AS A PROBE OF JET HISTORY | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/704019010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '704019010'
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