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 | 201073010 | SERPENS_X-1 | 279.99033 | 5.03594 | 279.37364 | 4.9891 | 281.29588 | 28.08433 | 36.11839 | 4.8417 | 257.94823 | 60600.90074 | 2024-10-17 21:37:04 | 60604.98060 | 2024-10-21 23:32:04 | 172.513 | 150.000 | 172.513 | 19.212 | PX_NORMAL | N | Y | N | N | Y | Y | Y | OFF | OFF | OFF | OFF | 2 | 31300010 | 320000A0 | 153.375 | 0.000 | 0.000 | 19.212 | 11110 | 313430 | 11310 | PROCESSED | 2024-10-26 11:43:52 | 2025-10-31 00:00:00 | 2024-10-27 11:43:53 | 03.00.013.009 | gen20240315_xtd20240815_rsl20240815 | Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 | 000012057 | Serpens X-1 is a persistently accreting neutron star (NS) with the first confirmed relativistically broadened Fe line for such systems. However, there remains conflicting reports of key parameters, such as the position of the inner accretion disk and inclination. These quantities can be determined from resolving the red- and blue-wings of the Fe line profile, which are most sensitive to the gravitational redshift and Doppler effects, respectively. Further, the Fe line has a unique double-peaked profile which can be due to high disk density effects causing the Fe XXV and XXVI lines to be produced at a similar strength. We request a 300 ks observation of the source to reveal the Doppler and relativistic effects that shape the line profile and further our understanding of the accretion flow. | BH AND NS BINARIES | 2 | A | RENEE LUDLAM | USA | 1 | NOR | RESOLVING RELATIVISTIC EFFECTS IN THE ACCRETION DISK OF SERPENS X-1 | archived | https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201073010/ | WINDOW2BURST | WINDOW1 | 1 | Observation Log: No remarks ; Pre-pipeline Log: No remarks |
Used SQL
SELECT * FROM xrism_master_data WHERE observation_id = '201073010'
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