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 CYGNUS X-2 326.1653 38.3323 325.647427 38.10178 346.69525 47.972917 87.3318132 -11.3049847 76.3142 53871.8636805556 2006-05-16 20:43:42 53872.7293171296 2006-05-17 17:30:13 401049010 39.3903 37 39.3903 39.4063 39.3903 39.3903 2 1 2 2 1 0 0 36.8804 36.8804 74.786 1 PROCESSED 57534.3858217593 2016-05-26 09:15:35 54401 2007-10-28 00:00:00 53927.6429166667 2006-07-11 15:25:48 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 011113 The potential well around low-magnetic field neutron stars is very similar to that around Schwarzschild black holes. Doppler shifts expected at the inner disk around such neutron stars should be very similar, and should produce relativistic FeK-alpha emission lines like those observed in some black hole systems. To date, however, relativistically broadened FeK-alpha emission lines have not been clearly detected in neutron star systems, in part because their lines are generally weaker than those found in black hole systems. We propose to observe the neutron star binaries 4U 1820-30, Cygnus X-2, and Serpens X-1 for 37 ksec each in Suzaku Cycle 1, to confirm possible evidence of relativistic broadening. Relativistic phenomena and accretion studies are central to NASA's ``SEU'' theme. GALACTIC POINT SOURCES 4 B JON MILLER USA 1 AO1 A SUZAKU STUDY OF BROAD IRON LINES IN NEUTRON STAR BINARIES XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/401049010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '401049010'

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

Go to top of this page ⏏