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 | CENTAURUS B | 206.7067 | -60.4086 | 205.850027 | -60.15889 | 231.235341 | -45.192759 | 309.7224369 | 1.73083578 | 275.5009 | 55758.843912037 | 2011-07-16 20:15:14 | 55760.4932060185 | 2011-07-18 11:50:13 | 806017010 | 93.6172 | 120 | 93.645 | 93.6172 | 0 | 93.637 | 1 | 1 | 0 | 1 | 0 | 0 | 0 | 0 | 0 | 27.6959 | 0 | PROCESSED | 57602.5915625 | 2016-08-02 14:11:51 | 56152 | 2012-08-13 00:00:00 | 55830.7256134259 | 2011-09-26 17:24:53 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 060070 | X-ray observation of radio lobe is essential to reveal the particle acceleration mechanism in the lobe, because we can obtain magnetic field and electron energy density without assumption of equipartition. The radio lobe of FR I radio galaxy Centaurus B was previously detected by ASCA. For revealing the mechanism of particle acceleration in radio lobes, detailed multi-wavelength observations are very important. We propose a deep observation of the radio lobe by Suzaku, which has the advantage of low background and high sensitivity for diffuse X-ray. Good quality Suzaku data combined with a detailed modeling reveals particle acceleration mechanism working in the radio lobe. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | B | YASUYUKI TANAKA | JAP | 6 | AO6 | X-RAY OBSERVATION OF RADIO LOBE OF FR I RADIO GALAXY CENTAURUS B | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/806017010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '806017010'
Your request has been accepted.
The download will start soon automatically.