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 J1809-193E 272.0013 -19.5033 271.261943 -19.51123 271.881238 3.92439 10.71539243 0.332309 270.1011 55085.7498148148 2009-09-11 17:59:44 55087.1564351852 2009-09-13 03:45:16 504079010 51.0289 50 51.0289 51.0289 0 51.0289 2 2 0 2 1 0 0 41.8753 41.8753 121.5198 2 PROCESSED 57548.5914699074 2016-06-09 14:11:43 55465 2010-09-26 00:00:00 55098.3372337963 2009-09-24 08:05:37 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 041303 We propose a detailed study of the extended VHE source HESS J1809-193 neighboring young PSR J1809-1917 with a known X-ray pulsar-wind nebula (PWN). As the chance coincidence is very unlikely, there should be a connection between the two. Furthermore, previous short Chandra observations of this field have revealed a large-scale asymmetric PWN extending toward the center of the TeV source. Thus, this is an excellent case for testing whether the unidentified TeV sources near young pulsars are, in fact, relic PWNe crushed by the asymmetric SNR reverse shock. We will probe the nature of the X-ray emission by measuring the surface brightness and spatially-resolved spectra across the large extent of the TeV source. Suzaku XIS is ideally suited for this purpose because of its low background. GALACTIC DIFFUSE EMISSION 5 A OLEG KARGALTSEV USA 4 AO4 CRUSHED PLERION HESS J1809-193: TEV TO X-RAY CONNECTION XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/504079010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '504079010'

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