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 | NGC 1365 | 53.3968 | -36.1347 | 52.919388 | -36.301683 | 36.801187 | -53.032832 | 237.94662462 | -54.6022242 | 221.6565 | 54486.2300578704 | 2008-01-21 05:31:17 | 54490.0002083333 | 2008-01-25 00:00:18 | 702047010 | 160.5057 | 150 | 160.5057 | 160.5137 | 0 | 160.5137 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 146.8139 | 146.8139 | 325.6768 | 4 | PROCESSED | 57541.4786342593 | 2016-06-02 11:29:14 | 54883 | 2009-02-21 00:00:00 | 54515.5847800926 | 2008-02-19 14:02:05 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 021314 | We propose a 150 ksec observation of the Seyfert Galaxy NGC 1365. This galaxy have a unique set of properties: FeXXV and FeXXVI Kalpha and Kbeta absorption lines (the highest S/N detection so far among AGNs), rapidly varying cold absorber (nH variations of ~10^23/cm^2 in a few hours, changes from Compton-thick to Compton-thin in two days), a relativistic iron emission line. This new long observation will use at best the unique capabilities of Suzaku to constrain the dimensions of the absorbers, and, for the first time, will investigate the dynamics and physical conditions of the hot absorber responsible of the iron absorption lines. It is likely that an occultation will occur during the observation. This occultation would directly set the dimension of the X-ray source. | EXTRAGALACTIC COMPACT SOURCES | 7 | C | GUIDO RISALITI | USA | 2 | AO2 | BLACK HOLE OCCULTATION AND OUTFLOW VARIABILITY IN NGC 1365 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702047010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '702047010'
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