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 | PHOENIX GALAXY | 120.9921 | 5.0644 | 120.329999 | 5.206365 | 122.073674 | -14.991802 | 216.72692126 | 18.43029643 | 304.6737 | 54222.3296296296 | 2007-05-02 07:54:40 | 54223.9585069445 | 2007-05-03 23:00:15 | 702111010 | 58.8677 | 50 | 58.8677 | 58.8677 | 0 | 58.8677 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 49.6978 | 49.6978 | 140.7239 | 5 | PROCESSED | 57538.5788078704 | 2016-05-30 13:53:29 | 54744 | 2008-10-05 00:00:00 | 54230.3771527778 | 2007-05-10 09:03:06 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 022002 | We propose a 50 ks Suzaku observation of the Seyfert galaxy UGC4203 (a.k.a. Mrk 1210), the ``Phoenix Galaxy''. It is one of the sources which have been discovered to change from Compton-thin to reflection-dominated states. The aim of the proposal is to understand the origin of this variation (i.e. as either due to flux or to NH variations) by measuring its column density and compare it to previous observations. Suzaku is unique for this task, because thanks to its broad band it may probe column densities up to several times 10^24 cm^-2 in this source, which has never been observed above 10 keV. | EXTRAGALACTIC COMPACT SOURCES | 7 | B | GIORGIO MATT | EUR | 2 | AO2 | THE NATURE OF THE VARIATIONS OF STATE IN THE PHOENIX GALAXY | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702111010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '702111010'
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