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 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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