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 1909+07 287.7097 7.5883 287.10413 7.505006 290.320155 29.788203 41.89273161 -0.82371888 247.9131 55502.7037847222 2010-11-02 16:53:27 55503.4337731482 2010-11-03 10:24:38 405073010 29.2982 25 29.2982 29.2982 0 29.2982 2 2 0 2 1 0 0 21.3911 21.3911 63.0519 0 PROCESSED 57553.9348958333 2016-06-14 22:26:15 55882 2011-11-17 00:00:00 55515.2869328704 2010-11-15 06:53:11 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 052024 We propose the first observation of the neutron star HMXB 4U 1909+07 with Suzaku. The aim of the proposed 25 ksec observation is to study the broadband spectrum of the source. The data will provide information about the structure and ionization state of the accreted medium, as well as of the geometry of the accretion column and the strength of the magnetic field. No high-resolution CCD spectra of this source have been published so far. The source shows flaring behavior, so the wind is expected to be strongly clumped, which could be probed by studying the evolution of N_H and the iron line with high time resolution. Furthermore we will perform phase resolved spectroscopy to study the spectral variation with pulse phase and perform a detailed search for a CRSF. GALACTIC POINT SOURCES 4 A FELIX FUERST EUR 5 AO5 STUDYING ACCRETION IN THE UNCELEBRATED HMXB 4U 1909+07 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/405073010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '405073010'

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