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 J1702-420 255.6874 -42.0709 254.803902 -41.999975 258.786548 -19.184424 344.26217794 -0.21974248 106.4451 54550.458599537 2008-03-25 11:00:23 54555.625162037 2008-03-30 15:00:14 502049010 215.6932 200 215.7053 215.6932 0 215.7053 2 2 0 2 1 0 0 140.6375 140.6375 395.7215 6 PROCESSED 57542.1678356482 2016-06-03 04:01:41 54933 2009-04-12 00:00:00 54566.9486458333 2008-04-10 22:46:03 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 020067 The Galactic Plane Survey with HESS found several new TeV sources, called as "dark particle accelerators". They must be powerful cosmic-ray accelerators, although their origin is still unknown due to the lack of information in other wavelengths. We investigate one of the most mysterious sample, HESS J1702-420, which has the brightest HESS compact source without clear counterparts. ASCA Galactic plane survey shows no evidence of X-ray emission although the exposure was too short. With the large effective area and the low background of XISs, we will be able to detect quite dim counterpart or make strong upper-limit in the hard X-ray band. This result will lead us to distinguish that HESS J1702-420 is the true "dark" protonic accelerator, or a hypothetical PWN powered by PSR J1702-4128. GALACTIC DIFFUSE EMISSION 5 B AYA BAMBA JAP 2 AO2 RESOLVING THE DARKEST DARK PARTICLE ACCELERATOR XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/502049010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '502049010'

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