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 | 1150+497 | 178.3624 | 49.5318 | 177.710529 | 49.809967 | 153.770918 | 43.67464 | 145.51949415 | 64.97605225 | 131.4133 | 55512.7136805556 | 2010-11-12 17:07:42 | 55514.1042824074 | 2010-11-14 02:30:10 | 705003010 | 105.6558 | 100 | 105.7118 | 105.6558 | 0 | 105.7198 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 84.6438 | 84.6438 | 120.128 | 1 | PROCESSED | 57554.1053356482 | 2016-06-15 02:31:41 | 55892 | 2011-11-27 00:00:00 | 55524.2197337963 | 2010-11-24 05:16:25 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 050007 | A Suzaku observation of the iron line emitting blazar 1150+497 is proposed. The object is reported to exhibit a signature iron line. By measuring the equivalent width and line width, Suzaku will reveal the state of the accretion disc with the jet activity. It is notable that the blazar, aligning the jet with the line of sight, allow us to observe the jet and the accretion disc with a sufficient isochronism even with the violently variable sources. | EXTRAGALACTIC COMPACT SOURCES | 7 | C | HIROMI SETA | JAP | 5 | AO5 | SUZAKU OBSERVATION OF AN FE-LINE BLAZAR 1150+497 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/705003010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '705003010'
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