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 4U1700-37 255.9894 -37.8441 255.139416 -37.774677 258.577099 -14.956185 347.75582102 2.17172645 269.6945 53991.447662037 2006-09-13 10:44:38 53992.918912037 2006-09-14 22:03:14 401058010 81.4425 80 81.4569 81.4704 81.4425 81.4544 3 3 3 3 1 0 0 82.1093 82.1093 127.109 1 PROCESSED 57535.6097916667 2016-05-27 14:38:06 54526 2008-03-01 00:00:00 54053.5428240741 2006-11-14 13:01:40 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 011135 The compact object in the massive X-ray binary 4U1700-37/HD153919 has been inferred to be a neutron star based on its spectral shape, but no pulsations have been observed. One possible explanation for the absence of observed pulsations is that the pulsed signal is beamed in directions other than our line of sight. This can be tested using Suzaku by searching for pulsations in the iron K line. This line is formed efficiently under almost all conditions of ionization and temperature, and so represents an X-ray bolometer which should respond to pulsed X-rays no matter where they are pointed. We plan to make such a search, and to probe the other properties of the wind and compact object in this system by observing with Suzaku for 80 ks away from eclipse. GALACTIC POINT SOURCES 4 A TIMOTHY KALLMAN USA 1 AO1 IRON LINE VARIABILITY IN 4U1700-37 XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/401058010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '401058010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏