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 J1641-463 250.2616 -46.3013 249.347836 -46.205158 255.208281 -23.867274 338.52580532 0.09066192 282.4572 56900.1342939815 2014-08-31 03:13:23 56902.1166435185 2014-09-02 02:47:58 509010020 0 40 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 PROCESSED 57616.5303356482 2016-08-16 12:43:41 56748 2014-04-01 00:00:00 57122.3887268518 2015-04-10 09:19:46 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 090045 The origin of cosmic rays has been one of the biggest problems in modern astrophysics. TeV gamma-ray observations provide indirect evidences of cosmic ray acceleration, although the sources detected so far have softer spectra than what would be expected by particle accelerators to explain the observed distribution of cosmic rays at the knee. HESS J1641-463 is the hardest TeV gamma-ray source ever found. With Suzaku's large effective area, and low and stable background, we will perform the first deep X-ray observation of this source to seek for its X-ray counterpart, and to identify its nature. It will provide a direct look into the physics of the highest energy particle accelerators in our Galaxy, responsible for the cosmic ray spectrum up to the spectral knee at PeV energies. GALACTIC DIFFUSE EMISSION 5 A AYA BAMBA JAP 9 AO9 IDENTIFYING THE X-RAY COUNTERPART OF THE HARDEST SOURCE HUMAN EVER DETECTED XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/509010020/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '509010020'

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