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 1608-52 243.1735 -52.4241 242.21194 -52.296335 251.322253 -30.70644 330.92310685 -0.84886634 127.9983 55277.989849537 2010-03-22 23:45:23 55278.9140393518 2010-03-23 21:56:13 404044040 16.0728 30 16.0728 16.0728 0 16.0728 3 3 0 3 1 0 0 15.6557 15.6557 79.8439 2 PROCESSED 57550.9805439815 2016-06-11 23:31:59 55665 2011-04-14 00:00:00 55299.4128819444 2010-04-13 09:54:33 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 041223 The true nature of X-ray emission from neutron star X-ray binaries (NSXRBs) has not been clear for sometime and there are many possibilities for the spectral model. Recent progress has been made, but relies on RXTE data which lacks the low energy sensitivity where disk emission is most prominent. Using Suzaku we propose four 30 ksec observations of the transient 4U 1608-52 throughout an outburst. We will test how spectral parameters change with luminosity, allowing us to untangle the correct model. An essential part of this proposal is the unique ability of Suzaku to detect asymmetric broad iron emission lines in NSXRBs. We will study how the iron line varies throughout the outburst, which combined with the spectral fits will test the interaction between the accretion disk and corona. GALACTIC POINT SOURCES 4 A EDWARD CACKETT USA 4 AO4-TOO ACCRETION DISK EVOLUTION THROUGHOUT A NEUTRON STAR LMXB OUTBURST HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/404044040/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '404044040'

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