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 SCT X-1 278.8604 -7.62 278.182699 -7.661262 279.107683 15.540839 24.33197703 0.06047842 260.9601 56940.5300810185 2014-10-10 12:43:19 56940.854375 2014-10-10 20:30:18 409033010 15.1616 50 15.1789 15.1776 0 15.1616 2 2 0 2 0 0 0 0 0 0 0 PROCESSED 57616.6415625 2016-08-16 15:23:51 57373 2015-12-17 00:00:00 56979.4099421296 2014-11-18 09:50:19 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 091222 We propose to observe the accreting 112s pulsar Scutum X-1 with Suzaku for 50ks. The optical companion is a late type giant or supergiant, making this a rare, persistent, non-OB-type wind accreting, Symbiotic X-ray Binary (SyXB). After initial flaring in the 1970s, the source generally exhibited low flux levels and has only rarely been observed. We will constrain the broadband spectrum, check for signs of wind accretion (variable absorption, log-normal count rate distribution), search for an iron fluorescence line, update the pulse period evolution, and compare to other Suzaku observations of SyXBs, especially to a quiescent observation of the prototype SyXB 4U 1954+31. GALACTIC POINT SOURCES 4 A KATJA POTTSCHMIDT USA 9 AO9 THE SYMBIOTIC X-RAY BINARY SCUTUM X-1 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/409033010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '409033010'

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