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 RXJ_0852-4622_NW 132.2926 -45.6157 131.862494 -45.429101 157.976747 -59.482382 265.39238743 -1.14402175 137.763 53723.4478240741 2005-12-19 10:44:52 53727.3016666667 2005-12-23 07:14:24 500010010 175.453 150 175.453 175.525 175.4608 175.461 2 2 2 2 1 0 0 230.0025 230.0025 332.9437 7 PROCESSED 57532.5654513889 2016-05-24 13:34:15 54247 2007-05-27 00:00:00 54059.902662037 2006-11-20 21:39:50 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001048 We propose to observe two lobes of X-ray and gamma-ray emission from the shell remnant RXJ 0852-4622 (Vela Jr) with HXD. The 1-10 keV spectrum of this remnant is essentially a featureless continuum attributed to synchrotron emission from accelerated electrons, with the X-ray and gamma-ray morphologies being very well matched. Observations at energies above 10 keV with HXD will probe the cut-off energy of the synchrotron spectrum, shedding light on the electron acceleration efficiency. The large size of the remnant makes it possible to observe different portions of the limb with separate HXD PIN observations. GALACTIC DIFFUSE EMISSION 5 A UNA HWANG JAP 0 SWG HXD OBSERVATION OF NONTHERMAL EMISSION FROM RXJ 0852-4622 HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500010010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '500010010'

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