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 J1534-571 2 233.1754 -57.1 232.193457 -56.931173 246.039407 -36.679353 323.50919975 -0.81659232 295.9986 56544.0219212963 2013-09-09 00:31:34 56544.6695949074 2013-09-09 16:04:13 508014010 38.9186 40 38.9426 38.9186 0 38.9506 2 2 0 2 1 0 0 36.8565 36.8565 55.9539 0 PROCESSED 57612.5722916667 2016-08-12 13:44:06 56990 2014-11-29 00:00:00 56622.6062268518 2013-11-26 14:32:58 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 080024 Supernova Remnants (SNRs) detected with TeV gamma-rays and synchrotron X-rays (TeV SNRs) are the most plausible acceleration sites of Galactic cosmic rays. However, the environments of such SNRs, temperature, density, and so on, are still unknown due to the lack of thermal X-ray emission in their spectra. HESS J1534-571 is a candidate of only several TeV SNRs which is located off Galactic plane. With good statistics and low background observation of Suzaku XIS, we will detect X-rays from this object for the first time, and identifying as a TeV SNR and if possible, detecting thermal X-rays from the target for the first time. Determining the thermal parameters will reveal us what kind of environment makes ordinal SNRs to TeV SNRs and how TeV SNRs accelerate cosmic rays in such condition. GALACTIC DIFFUSE EMISSION 5 A AYA BAMBA JAP 8 AO8 RESOLVING THERMAL X-RAYS FROM A TEV SNR CANDIDATE HESS J1534-571 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/508014010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '508014010'

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