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 4U 0115+63 19.6139 63.7554 18.78861 63.492562 49.805717 49.807631 125.91367385 1.04017806 82.1235 55750.053587963 2011-07-08 01:17:10 55751.0210763889 2011-07-09 00:30:21 406049010 42.2748 45 42.2748 42.3548 0 42.3548 2 2 0 2 1 0 0 42.1432 42.1432 83.5779 1 PROCESSED 57602.5577662037 2016-08-02 13:23:11 56163 2012-08-24 00:00:00 55778.4311226852 2011-08-05 10:20:49 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 061234 We propose to perform Target of Opportunity observations of one accreting neutron star that is a known cyclotron line source, out of a sample of five, in outburst. The aim is to observe the source for 50 ks at a level of >~40 mCrab and for another 45 ks at >~200 mCrab, in order to determine the properties of the cyclotron line(s) and constrain the broad band spectrum at different luminosities. These measurements have implications for the B-field strength and geometry as well as the properties of the accreted plasma. GALACTIC POINT SOURCES 4 A KATJA POTTSCHMIDT USA 6 AO6-TOO CYCLOTRON LINES IN TRANSIENT PULSARS I: PROBING THE B-FIELD XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/406049010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '406049010'

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