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 CTB 37B 258.4918 -38.2006 257.636889 -38.143005 260.643359 -15.13191 348.64561092 0.37683278 270.1267 53974.0604976852 2006-08-27 01:27:07 53976.2398032407 2006-08-29 05:45:19 501007010 82.8151 80 82.8711 82.8151 82.8791 82.8631 2 2 2 2 1 0 0 68.8603 68.8603 188.2779 2 PROCESSED 57535.4428703704 2016-05-27 10:37:44 54526 2008-03-01 00:00:00 54053.4840162037 2006-11-14 11:36:59 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010042 The Galactic Plane Survey with HESS found several new TeV sources, called as "dark particle accelerators". They must be powerful cosmic-ray accelerators, although their origin is still unknown due to the lack of information in other wavelengths. We investigate one of the extended sample with radio SNR counterpart, CTB 37B, which is marginally detected on the edge of ASCA GIS. ASCA spectrum shows rather soft power-law feature, indicating that there are both thermal and non-thermal X-ray emission. With the low background of XISs and HXD, parameters of both components are determined with 80 ks exposure. The non-thermal component suggests the new sample of accelerators, and the thermal compopent reveals the condition of the proton acceleration site, for the first time. GALACTIC DIFFUSE EMISSION 5 A AYA BAMBA JAP 1 AO1 UNCOVERING THE NATURE OF DARK PARTICLE ACCELERATORS XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/501007010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '501007010'

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