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 | MKN 3 | 93.8839 | 71.0477 | 92.433649 | 71.063052 | 91.875357 | 47.63268 | 143.2836301 | 22.71631463 | 71.8326 | 53665.0848263889 | 2005-10-22 02:02:09 | 53667.2682175926 | 2005-10-24 06:26:14 | 100040010 | 95.0265 | 100 | 95.0265 | 95.0772 | 95.0452 | 95.0345 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 91.3441 | 91.3441 | 188.6299 | 0 | PROCESSED | 57527.6643055556 | 2016-05-19 15:56:36 | 54247 | 2007-05-27 00:00:00 | 53906.4896759259 | 2006-06-20 11:45:08 | 3.0.22.43 | 5 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000040 | Mkn 3 is the second brightest Compton-thick Sy 2 currently visible with Suzaku. The broadband spectrum of Mkn 3, as probed by previous SAX and Chandra observations, is dominated by a reflection component (Compton hump strength R is near 1), but there is also evidence for a strongly absorbed hard X-ray power law that may be direct emission from the obscured nucleus, filtering through Compton-thick material (such as the molecular torus). | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | MKN 3 | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100040010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '100040010'
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