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 HESSJ1857-A 284.2126 2.7519 283.584668 2.685017 285.744612 25.418977 35.99783049 0.0515802 269.8116 55822.9197800926 2011-09-18 22:04:29 55823.984212963 2011-09-19 23:37:16 506019010 40.9249 40 40.9249 40.9249 0 40.9249 2 2 0 2 1 0 0 35.8469 35.8469 91.9279 1 PROCESSED 57603.2046180556 2016-08-03 04:54:39 56233 2012-11-02 00:00:00 55865.2326157407 2011-10-31 05:34:58 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 060061 Many TeV gamma-ray objects discovered on the Galactic plane are classified as pulsar wind nebulae (PWNe), just because there exists a pulsar in the vicinity of them. X-ray observations can directly show the physical connection between the TeV emission and PWNe by presenting the existence of X-ray PWNe. HESSJ1857 and HESSJ1832 are unidentified TeV objects, but they may be TeV PWNe driven by pulsars close to them. We propose to observe them to study whether the pulsars have X-ray PWNe or not. GALACTIC DIFFUSE EMISSION 5 B HIRONORI MATSUMOTO JAP 6 AO6 ARE THE TEV UNIDENTIFIED OBJECTS, HESSJ1857+026 AND HESSJ1832-084, PULSAR WIND NEBULAE? XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/506019010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '506019010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏