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 SGR1806-20 272.1595 -20.349 271.415501 -20.357687 272.017973 3.076639 10.0481975 -0.20823053 88.7483 54189.6305555556 2007-03-30 15:08:00 54190.0627199074 2007-03-31 01:30:19 401021010 19.2889 20 19.2889 19.595 0 19.3563 1 1 0 1 1 0 0 16.5071 16.5071 37.3279 1 PROCESSED 57538.0253587963 2016-05-30 00:36:31 54561 2008-04-05 00:00:00 54209.5169212963 2007-04-19 12:24:22 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010124 We propose a study of proton cyclotron structures and broadband burst spectra of SGRs, magnetar candidate, which are believed to have very strong magnetic field of the order of 10^15 G. Although many observations have been made by different instruments in the space, their spectra and magnetic field are yet to be well understood. The first scientific goal is the detection of proton cyclotron structures. It allows us a direct measurement of a magnetic field intensity. The second scientific goal is to reveal the burst spectral shape in a wide-band and to find out common properties to magnetars, i.e., SGRs and AXPs. We will trigger the Suzaku observation when one of the following two criteria is satisfied; 1) the burst activity becomes high state, or 2) the giant flare occurs. GALACTIC POINT SOURCES 4 A YUJIN NAKAGAWA JAP 1 AO1-TOO PROTON CYCLOTRON STRUCTURE AND BROADBAND SPECTRA OF "SGR" HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/401021010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '401021010'

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