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 VELA JR P18 133.5064 -46.0415 133.075299 -45.850566 159.830487 -59.392209 266.25968404 -0.76370949 347.0006 54291.9244444444 2007-07-10 22:11:12 54292.1668634259 2007-07-11 04:00:17 502040010 15.0123 10 15.0123 15.0362 0 15.0203 2 2 0 2 1 0 0 12.8952 12.8952 20.9439 1 PROCESSED 57539.1482407407 2016-05-31 03:33:28 54696 2008-08-18 00:00:00 54328.4716666667 2007-08-16 11:19:12 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 020049 We propose to perform mapping obervations of the SNR Vela Jr (RX J0852.0-4622). Recent HESS data have revealed a shell-like morphology in TeV gamma-rays, which motivates us to map the remnant's shell with Suzaku XIS and HXD. The sensitivity of Suzaku HXD PIN detector in the 10-50 keV range is high enough to detect the hard X-ray synchrotron emission from the northwest and north rims. With Suzaku XIS, we will measure keV-to-TeV flux ratios in a wide area of the remnant. The Suzaku X-ray data sets, combined with new HESS data, allow us to investigate the origin of TeV gamma-rays and the nature of cosmic-ray acceleration in supernova shells with an unprecedented level. GALACTIC DIFFUSE EMISSION 5 A YASUNOBU UCHIYAMA JAP 2 AO2 HARD X-RAY MAPPING OF THE BRIGHT TEV SNR VELA JR XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/502040010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '502040010'

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