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 M106 184.7117 47.2376 184.094273 47.515109 160.404745 44.085185 138.43381178 68.89762168 287.1938 53896.5413078704 2006-06-10 12:59:29 53898.7113425926 2006-06-12 17:04:20 701095010 99.8175 100 99.8815 99.8175 99.8815 99.8815 2 2 2 2 1 0 0 97.5229 97.5229 187.4839 1 PROCESSED 57534.6515393518 2016-05-26 15:38:13 54401 2007-10-28 00:00:00 53927.2308449074 2006-07-11 05:32:25 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 013151 We propose observations of the nearby Low Luminosity AGN, M81 and M106, for 100 ks for each target. We aim to detect both targets up to ~200 keV for the first time. We will determine the photon indices of the hard X-ray power-law continuum, with searching for other possible characteristics such as Compton hump around 10-20 keV and cutoff around 100-200 keV which would lead major discoveries. We will study the shape of Fe-K line(s) around 6-7 keV and their time variances. Our goal is to compare their hard X-ray spectra with those of SWG seyfert galaxies, with unprecedented accuracy, to study the accresion mechanism of LLAGN. EXTRAGALACTIC COMPACT SOURCES 7 A TAKESHI ITOH CHRISTOPHER REYNOLDS JUS 1 AO1 OBSERVATIONS OF HARD X-RAYS FROM LOW LUMINOSITY ACTIVE GALACTIC NUCLEI HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701095010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '701095010'

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