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 | 1ES 1927+654 | 291.8157 | 65.5862 | 291.743016 | 65.482913 | 3.782751 | 81.150517 | 97.0030083 | 20.97400385 | 83.4311 | 55667.8280092593 | 2011-04-16 19:52:20 | 55669.2425115741 | 2011-04-18 05:49:13 | 706006010 | 71.8889 | 100 | 71.9129 | 71.8889 | 0 | 71.9129 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 79.6647 | 79.6647 | 122.1919 | 0 | PROCESSED | 57601.5407986111 | 2016-08-01 12:58:45 | 56059 | 2012-05-12 00:00:00 | 55691.2683912037 | 2011-05-10 06:26:29 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 060008 | 1ES 1927+654, an X-ray unabsorbed optically classified type-2 AGN, challenges the standard unified model. What is known about its X-ray characteristics suggest it can provide tremendous insight. It is extremely bright and will render close to 20 ct/s in the combined XIS providing sufficient data to unambiguously detect features in the Fe~K region, distinguish absorption and reflection models, and study its rapid variability. Even in the most conservative estimates a PIN detection is expected. It is persistently variable on short time scales and in combination with the long duration of Suzaku observations, the proposed observationswill yield fruitful variability studies. It has never been observed by Suzaku thus guaranteeing significant opportunity for discovery. | EXTRAGALACTIC COMPACT SOURCES | 7 | B | LUIGI GALLO | JAP | 6 | AO6 | REVEALING THE NATURE OF AN X-RAY ABSORBED SEYFERT 2 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/706006010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '706006010'
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