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
|
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1 | HESS J1534-571 4 | 233.6872 | -56.8979 | 232.705572 | -56.731059 | 246.296725 | -36.40404 | 323.85352453 | -0.81317458 | 295.9989 | 56545.1801157407 | 2013-09-10 04:19:22 | 56545.8042708333 | 2013-09-10 19:18:09 | 508016010 | 42.1696 | 40 | 42.1696 | 42.1936 | 0 | 42.1776 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 39.9419 | 39.9419 | 53.9199 | 0 | PROCESSED | 57612.5878587963 | 2016-08-12 14:06:31 | 56990 | 2014-11-29 00:00:00 | 56625.6134953704 | 2013-11-29 14:43:26 | 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/ver3.0/508016010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '508016010'
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