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.
observation_id
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
exposure
awarded_exposure
resolve_exposure
xtend_exposure
resolve_data_mode
resolve_with_filter_be
resolve_with_filter_fe55
resolve_with_filter_nd
resolve_with_filter_poly
resolve_with_filter_open
resolve_with_filter_undef
is_resolve_gatevalve_closed
is_resolve_mxs1
is_resolve_mxs2
is_resolve_mxs3
is_resolve_mxs4
xtend_number_modes
xtend_dataclass_file1
xtend_dataclass_file2
xtend_window1_exposure
xtend_window2_exposure
xtend_window1_burst_exposure
xtend_window2_burst_exposure
xtend_code
resolve_code
gen_code
processing_status
processing_date
public_date
distribution_date
processing_version
caldb_version
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
proposal_type
proposal_title
observation_status
data_access_url
xtend_data_mode1
xtend_data_mode2
processing_count
remarks
1 201131010 VELA_X-1 135.52796 -40.55428 135.05441 -40.35639 157.03646 -53.92494 263.05766 3.92977 111.3438 60633.01741 2024-11-19 00:25:04 60634.31741 2024-11-20 07:37:04 61.313 40.000 61.313 5.992 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31300010 320000A0 0.000 0.000 0.000 5.992 11110 313430 11310 PROCESSED 2024-12-02 09:05:19 2025-12-11 00:00:00 2024-12-03 09:05:20 03.00.013.010 gen20241115_xtd20241115_rsl20241115 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000014062 We propose a 40-ks XRISM observation of the wind-fed High-Mass X-ray Binary (HMXB) Vela X-1 at orbital phase 0.43-0.53 where we expect the largest changes in absorption as the accretion structure crosses and obstructs our line of sight. By tracing the onset of this structure, we obtain an in-depth view of the stellar wind complexity in this source. In particular, the moderate absorption combined with strong continuum emission happening at these orbital phases will reveal emission lines below 12 keV, even with the gate valve closed. We will follow absorption variability and iron line energy shifts down to the pulse period of the neutron star to probe the onset of the accretion wake on our line of sight and radial velocities of the wind. BH AND NS BINARIES 2 A CAMILLE DIEZ EUR 1 NOR ON THE ONSET OF THE ACCRETION WAKE IN THE HIGH-MASS X-RAY BINARY VELA X-1 processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201131010/ WINDOW2BURST WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201131010'

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

Go to top of this page ⏏