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 1907+09 287.4001 9.8965 286.805564 9.814618 290.343315 32.116545 43.79892996 0.51344636 85.3836 54209.4191666667 2007-04-19 10:03:36 54211.2612731482 2007-04-21 06:16:14 402067010 80.6283 65 80.6283 80.6363 0 80.6363 2 2 0 2 1 0 0 73.2685 73.2685 159.1479 2 PROCESSED 57538.4515393518 2016-05-30 10:50:13 54702 2008-08-24 00:00:00 54216.2674189815 2007-04-26 06:25:05 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021123 The HMXB 4U 1907+09 shows a rich phenomenology: two cyclotron lines, an uncommonly weak iron line, intermittent X-ray fading, and a recent torque reversal. Compared to other persistent supergiant X-ray pulsars it has been less well observed, although it is a prime target to study the interaction of the neutron star's X-rays with the stellar wind and the accretion column. The latter has been confirmed by our 60ks AO1 observation which allowed for the first detection of a soft excess below 2keV as well as the determination of the paramters of the fundamental cyclotron line with unprecedented accuracy. Due to an unusually low source state during the AO1 exposure, however, an additional observation of 65ks is needed to perform the first phase resolved analysis of this interesting source. GALACTIC POINT SOURCES 4 B KATJA POTTSCHMIDT USA 2 AO2 THE BROAD BAND SPECTRUM OF 4U 1907+09 HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/402067010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '402067010'

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