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 | BD+43 3654 | 308.4185 | 44.0658 | 307.988834 | 43.893641 | 331.745866 | 59.550103 | 82.48241574 | 2.36274642 | 104.8287 | 55655.0785416667 | 2011-04-04 01:53:06 | 55657.0925231482 | 2011-04-06 02:13:14 | 506004010 | 97.0478 | 100 | 98.9638 | 97.0478 | 0 | 98.9638 | 3 | 2 | 0 | 2 | 1 | 0 | 0 | 88.9256 | 88.9256 | 173.9877 | 0 | PROCESSED | 57601.4465972222 | 2016-08-01 10:43:06 | 56037 | 2012-04-20 00:00:00 | 55670.3073842593 | 2011-04-19 07:22:38 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 060010 | It is very important to search for possible particle-acceleration sites among the astrophysical objects. Very recently, synchrotron emission has been discovered with the VLA radio observation from a bow shock region of a runaway star, BD+43 3654, having a very fast stellar wind whose velocity reaches up to 2300 km/s. The maximum energy is estimated to be about 10 TeV, and thus the emission should come to the X-ray band. Here, we propose to perform the 100 ksec observation of BD+43 3654 with Suzaku, in order to determine the strength of the shock from the temperature of the post-shock plasma and to determine the maximum energy of the accelerated electrons. | GALACTIC DIFFUSE EMISSION | 5 | A | YUKIKATSU TERADA | JAP | 6 | AO6 | SUZAKU OBSERVATION OF NON-THERMAL EMISSION FROM A BOW SHOCK REGION OF A RUNAWAY STAR, BD+43 3654 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/506004010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '506004010'
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