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 | 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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