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_J1825-137_2 276.1969 -13.7002 275.488545 -13.728547 276.096187 9.609358 17.73170044 -0.43977824 271.0001 54756.4591666667 2008-10-17 11:01:12 54758.1953009259 2008-10-19 04:41:14 503029010 57.1993 50 57.1993 57.1993 0 57.1993 2 2 0 2 1 0 0 51.185 51.185 149.9858 0 PROCESSED 57544.2276157407 2016-06-05 05:27:46 55148 2009-11-13 00:00:00 54780.5081365741 2008-11-10 12:11:43 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 030044 The TeV gamma-ray source HESS J1825-137 has been discovered in a survey of the Galactic plane performed by HESS. This source is one of the most interesting source in the HESS catalog since it is the first and the only TeV gamma-ray emitter that shows energy dependent morphology. However, all the gamma-ray emitting region is not covered by X-ray observatories. We propose Suzaku observations of HESS J1825-137 region, which has not been covered by other X-ray satellites. By comparing the spectral and morphological properties of X-ray emission with those of TeV gamma-rays, we can probe the morophology and strength of the magnetic fiels, which should reveal the physical processes of acceleration, diffusion, and radiation of relativistic electrons. GALACTIC DIFFUSE EMISSION 5 B TAKAAKI TANAKA JAP 3 AO3 MAPPING OBSERVATIONS OF HESS J1825-137 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/503029010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '503029010'

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