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 J1837-069 279.4395 -6.8651 278.765532 -6.909152 279.755327 16.256333 25.2664546 -0.10276403 102.6144 54164.5341898148 2007-03-05 12:49:14 54165.4286342593 2007-03-06 10:17:14 401026010 42.1911 40 42.1911 42.1991 0 42.2071 2 2 0 2 1 0 0 37.7021 37.7021 77.2599 1 PROCESSED 57537.6010185185 2016-05-29 14:25:28 54750 2008-10-11 00:00:00 54171.2613425926 2007-03-12 06:16:20 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010131 The HESS (High Energy Stereoscopic System) collaboration has recently reported the TeV survey of the inner-part of the Galaxy, which revealed the existence of a new population of gamma-ray objects. Most of which are unknown, but at least two of them, HESS J1813-178 and HESS J1837-069 are point-like, and the ASCA Galactic survey and the INTEGRAL survey detected the counterparts in 0.5-10 keV and 20-100 keV, respectively. Making full use of Suzaku's wide-band spectral capability, we will study spectral characteristics of HESS J1813-178 and HESS J1837-069 in 0.5 keV to ~200 keV, and investigate for their origins. We will also carry out pulse-search to evaluate the pulsar-wind hypothesis. GALACTIC POINT SOURCES 4 B KEN EBISAWA JAP 1 AO1 INVESTIGATION OF TWO HESS SOURCES DETECTED WITH INTEGRAL HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/401026010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '401026010'

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