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 | RXJ1713.7-3946 | 258.074 | -39.935 | 257.205787 | -39.875387 | 260.458717 | -16.88737 | 347.05133682 | -0.37925502 | 269.9977 | 53639.6563194444 | 2005-09-26 15:45:06 | 53641.2960648148 | 2005-09-28 07:06:20 | 100026010 | 68.4959 | 80 | 68.4959 | 68.5653 | 68.5119 | 68.5253 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 56.2382 | 56.2382 | 141.6619 | 0 | PROCESSED | 57527.4561921296 | 2016-05-19 10:56:55 | 54247 | 2007-05-27 00:00:00 | 54037.0750694445 | 2006-10-29 01:48:06 | 3.0.22.43 | 4 | 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/ver3.0/100026010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '100026010'
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