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 LMC X-4 83.221 -66.3591 83.212611 -66.392014 1.088478 -87.292124 276.32094979 -32.52452295 284.2438 54561.5523842593 2008-04-05 13:15:26 54562.3058333333 2008-04-06 07:20:24 702036020 25.3397 20 25.3425 25.3425 0 25.3397 2 2 0 2 1 0 0 24.502 24.502 65.07 0 PROCESSED 57542.2490046296 2016-06-03 05:58:34 54943 2009-04-22 00:00:00 54574.4237152778 2008-04-18 10:10:09 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021127 We propose for a series of three 20ks observations of the binary X-ray pulsar LMC X-4. This source shows 13.5 s pulsations, a 1.4 d orbital period, and a long-period (~30 d) variability due to a warped, precessing accretion disk. The proposed analysis will use pulse-phase spectroscopy with XIS to explore changes in the X-ray pulses and spectra at three different phases in the disk precession. This work will give us a detailed picture of the accretion flow, particularly for the inner regions of the accretion disk that are illuminated by the X-rays from the neutron star. This project takes advantage of the strengths of the XIS, particularly its excellent spectral resolution, sufficient (1s) time resolution in Window mode, and wide PSF that limits pile-up effects. EXTRAGALACTIC COMPACT SOURCES 7 A RYAN HICKOX USA 2 AO2 SUPERORBITAL VARIATION OF LMC X-4: EXPLORING THE ACCRETION FLOW XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702036020/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '702036020'

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