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 | MKN 590 | 33.6477 | -0.7713 | 33.009436 | -1.003927 | 31.140057 | -13.460103 | 163.51612886 | -56.94122484 | 251.1273 | 55587.0949652778 | 2011-01-26 02:16:45 | 55588.2146990741 | 2011-01-27 05:09:10 | 705043020 | 40.9139 | 150 | 40.9219 | 40.9219 | 0 | 40.9139 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 37.8699 | 37.8699 | 96.7339 | 1 | PROCESSED | 57600.7810763889 | 2016-07-31 18:44:45 | 55988 | 2012-03-02 00:00:00 | 55621.2137731482 | 2011-03-01 05:07:50 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 051433 | We propose a 150 ks Suzaku long-look to study the Compton reflection component, soft excess, ionized emission and possible ionized reflection of the Seyfert 1.2 AGN Mkn 590, which has an unobscured line of sight or "bare nucleus" and as of yet unquantified reflection. We aim to accurately constrain the geometry of the circumnuclear material and determine the ionization states of both the Compton-thin and Compton-thick material surrounding the black hole by studying the origin of the soft excess, determining the likelihood of ionized reflection and accurately measuring the intensity of neutral, H-like and He-like Fe emission lines. | EXTRAGALACTIC COMPACT SOURCES | 7 | C | ELIZABETH RIVERS | USA | 5 | AO5 | QUANTIFYING THE COMPTON REFLECTION AND IONIZED EMISSION IN MKN 590 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/705043020/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '705043020'
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