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 | E1821+643 | 275.5207 | 64.3306 | 275.456094 | 64.303959 | 318.282096 | 86.807262 | 93.98984501 | 27.40177083 | 228.4067 | 56239.7868981482 | 2012-11-08 18:53:08 | 56241.8217708333 | 2012-11-10 19:43:21 | 707016010 | 100.4132 | 100 | 100.4132 | 100.4132 | 0 | 100.4132 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 95.5411 | 95.5411 | 175.7799 | 2 | PROCESSED | 57608.0299421296 | 2016-08-08 00:43:07 | 56631 | 2013-12-05 00:00:00 | 56265.6966319444 | 2012-12-04 16:43:09 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 070089 | Central engines of AGN are considered to be generally in Multi-Zone Comptonization (MZC) condition (e.g., Noda et al. 2011a,b). To verify this thing on a high-luminosiy AGN, we suggest to observe Radio-Quiet Quasar E1821+643 By Suzaku. Utilizing a time variability of each Comptonization component, we will resolve spectral variable components, and study whether the central engine of E1821+643 is in MZC condition or not. | EXTRAGALACTIC COMPACT SOURCES | 7 | C | HIROUMI NODA | JAP | 7 | AO7 | SUZAKU STUDY OF MULTI-ZONE COMPTONIZATION PICTURE ON THE CENTRAL ENGINE OF RADIO-QUIET QUASAR E1821+643 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/707016010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '707016010'
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