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 J1804-216 271.1693 -21.6722 270.417896 -21.676057 271.077547 1.764239 8.44223916 -0.04647489 89.0483 53831.6120138889 2006-04-06 14:41:18 53832.4919328704 2006-04-07 11:48:23 500007010 37.5222 50 37.5222 37.5222 37.5222 37.5222 2 2 2 2 1 0 0 28.9336 28.9336 75.9901 0 PROCESSED 57533.4045138889 2016-05-25 09:42:30 54247 2007-05-27 00:00:00 54042.288900463 2006-11-03 06:56:01 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001029 HESS found several new TeV sources in the Galactic Plane Survey. Possible origin would be PWN or synchrotron X-ray SNR shell. However many of these new TeV sources (their sizes are ~10 arcmin) have no counterpart in any other wavelength. They can be main contributors to the Galactic Cosmic rays. In order to reveal the nature of these fantastic objects, we propose to observe the extended sources. HESS~J1616-508 is already observed and we found this source has quite low surface brightness in X-rays compared with TeV gamma-rays, indicating this is a dark particle accelerator Here, we point out HESS~J1804-216 which has possible counterparts in other wavelengths, then it might be the missing link between known Galactic accelerators and dark particle accelerators. GALACTIC DIFFUSE EMISSION 5 A AYA BAMBA JAP 0 SWG SEARCH FOR X-RAY COUNTERPARTS OF ``DARK PARTICLE ACCELERATORS'' XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500007010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '500007010'

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