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 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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