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 | NGC2110 | 88.0489 | -7.4533 | 87.444745 | -7.464256 | 87.748433 | -30.879563 | 212.92425635 | -16.54269345 | 269.0605 | 57101.7987152778 | 2015-03-20 19:10:09 | 57103.3044328704 | 2015-03-22 07:18:23 | 709011010 | 45.6257 | 50 | 45.6257 | 49.4936 | 0 | 49.5096 | 2 | 2 | 0 | 2 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | PROCESSED | 57617.8483564815 | 2016-08-17 20:21:38 | 57558 | 2016-06-19 00:00:00 | 57190.4658333333 | 2015-06-17 11:10:48 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 090062 | We propose to observe the Seyfert galaxy NGC2110 twice every half year, which showed a big flare by a factor of around 5 against the normal state around 2012 December. We can observe the echo history following the flare in a time scale of years, and then measure the reflection spectrum very accurately to constrain the geometry of the reflection torus. | EXTRAGALACTIC COMPACT SOURCES | 7 | A | YASUSHI FUKAZAWA | JAP | 9 | AO9 | X-RAY ECHO OF THE BIG FLARE OF SEYFERT GALAXY NGC2110 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/709011010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '709011010'
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