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 HESS J1356-645 2 208.8016 -64.5041 207.885224 -64.258991 235.51443 -48.210014 309.72820731 -2.47708999 123.7329 56340.1852430556 2013-02-17 04:26:45 56341.4863425926 2013-02-18 11:40:20 507020010 51.2594 50 51.2636 51.2594 0 51.2594 2 2 0 2 1 0 0 45.1505 45.1505 112.4059 2 PROCESSED 57610.6176157407 2016-08-10 14:49:22 56718 2014-03-02 00:00:00 56352.5089930556 2013-03-01 12:12:57 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/ver3.0/507020010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '507020010'

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