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 RXJ1713-3946-BKGD2 257.2742 -41.0338 256.397744 -40.970376 259.926088 -18.035902 345.80577047 -0.54060643 270.0033 53641.2980671296 2005-09-28 07:09:13 53642.1843055556 2005-09-29 04:25:24 100026030 37.5132 40 37.5372 37.5292 37.5132 37.5132 2 2 2 2 1 0 0 31.8982 31.8982 76.5659 0 PROCESSED 57527.4461574074 2016-05-19 10:42:28 54247 2007-05-27 00:00:00 54035.6187268518 2006-10-27 14:50:58 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000026 RXJ1713 is very important sources in which we can study particle accelerator in the universe. X-ray synchrotron spectrum suggest the existence of distribution of high energy electron. Very similar TeV and ASCA morphologies show close connection between these energy bands. The interaction with molecular cloud suggests that proton accelerator resides in this object. The photon index of RXJ1713 seems to be difficult in the frame work of standard diffusive shock scenario. To obtain precise spectrum in the hard X-ray region is therefore very important to determine the energy cut off and to study the mechanism that produce such high energy electrons. CALIBRATION 1 A SWG JAP 0 SWG Observation of RXJ1713.7-3946 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100026030/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '100026030'

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