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 | HESS J1356-645 1 | 209.4297 | -64.5068 | 208.507718 | -64.263148 | 235.862386 | -48.071536 | 309.98959301 | -2.54712319 | 106.5083 | 56318.4192939815 | 2013-01-26 10:03:47 | 56320.0002083333 | 2013-01-28 00:00:18 | 507019010 | 55.7489 | 50 | 55.762 | 55.7569 | 0 | 55.7489 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 65.1023 | 65.1023 | 136.5678 | 2 | PROCESSED | 57608.6328587963 | 2016-08-08 15:11:19 | 56708 | 2014-02-20 00:00:00 | 56342.6666319444 | 2013-02-19 15:59:57 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 070017 | Recently, pulsar wind nebulae is focused on one of the electron accelerators in our Galaxy. Especially TeV pulsar wind nebulae are supposed to have a largely extended X-ray emission. Since the X-ray emission is much larger than the size considering the typical electron lifetime, high energy electrons strangely seem to be transferred too fast or without cooling. To study the electron diffusion of young pulsar wind nebula, we propose observations of HESS J1356-645, which is off the Galactic plane and is free from the Galactic ridge X-ray emission. | GALACTIC DIFFUSE EMISSION | 5 | C | TAKAHISA FUJINAGA | JAP | 7 | AO7 | OFF-PLANE TEV GAMMA-RAY SOURCE HESS J1356-645 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/507019010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '507019010'
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